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Permian palynostratigraphic schemes are used primarily to correlate coal- and hydrocarbon-bearing rocks within basins and between basins, sometimes at high levels of biostratigraphic resolution. Up to now, their main shortcoming has been the lack of correlation with schemes outside the basins, coalfields and hydrocarbon fields that they serve, and chiefly a lack of correlation with the international Permian scale. This is partly because of phytogeographical provinciality from the Guadalupian onwards, making correlation between regional palynostratigraphic schemes difficult. However, local high-resolution palynostratigraphic schemes for regions are now being linked either by assemblage-level quantitative taxonomic comparison or by the use of single well-characterized palynological taxa that occur across Permian phytogeographical provinces. Such taxa include: Scutasporites spp., Vittatina spp., Weylandites spp., Lueckisporites virkkiae, Otynisporites eotriassicus and Converrucosisporites confluens. These palynological correlations are being facilitated and supplemented with radiometric, magnetostratigraphic, independent faunal and strontium isotopic dating.

Palynostratigraphy is the use of palynomorphs (defined as organic-walled microfossils 5–500 µm in diameter) in correlating and assigning relative ages to rock strata. As such, it is a branch of biostratigraphy and follows the rules of biostratigraphic practice: for example, those set out by Rawson et al. (2002).

The Permian, falling between 252.2 and 298.9 Ma, was a period of intense change in which the giant continent of Pangea as a whole moved north, and in which, through the early part of the Period, a transition from icehouse to greenhouse conditions occurred (e.g. Fielding et al. 2008), alongside the decline in coal swamps and the establishment of widespread evaporite deposits (Henderson et al. 2012). The end of the Period saw a major extinction of fauna such as fusulinacean foraminifers, trilobites, rugose and tabulate corals, blastoids, acanthodians, placoderms, and pelycosaurs; a dramatic reduction in bryozoans, brachiopods, ammonoids, sharks, bony fish, crinoids, eurypterids, ostracodes and echinoderms (Henderson et al. 2012); and, although many conifers (e.g. glossopterids, cordaites) became extinct at the end of the Permian, there is no evidence of major extinction in the plants (Gradstein & Kerp 2012). Amongst the most important changes in land plants is the replacement, near the end of the Carboniferous, of arborescent lycophytes by arborescent tree ferns; arborescent lycophytes only persisted into the Guadalupian in China. The arborescent horsetails also declined by the end of the Carboniferous. In the Permian, a great variety of new seed plant groups appeared such as cycads, ginkgos, voltzialean conifers and glossopterids. The latter are important biostratigraphic markers for the Permian of Gondwana and include several hundred species. It is estimated that by the Lopingian about 60% of the world’s flora consisted of seed plants (Gradstein & Kerp 2012).

These large-scale evolutionary changes in plants, filtered by local and regional effects, are responsible for the palynological succession that provides opportunities for subdivision on which palynostratigraphic schemes are built. However, the pronounced phytogeographical differentiation of the Permian has a powerful effect on palynostratigraphy, such that schemes differ considerably across Pangea and correlation between schemes is even now tentative or incomplete. In the Gondwana phytogeographical province, for example, it is difficult to correlate to the standard Permian stages; and the Carboniferous–Permian and Permian–Triassic boundaries are not precisely correlateable into Gondwana basins using palynology (Stephenson 2008a).

Until recently, progress in correlation was hampered by the lack of fundamental stratigraphic standards such as stage Global Stratigraphic Sections and Points (GSSPs); however, since 1997 (Jin et al. 1997; Henderson et al. 2012) a number of GSSPs have been established within the Pennsylvanian–Permian succession, the most important of which is the basal Permian GSSP at Aidaralash Creek in the southern Urals (Jin et al. 1997; Henderson et al. 2012), and the basal Triassic GSSP at Meishan section D, Changxing County, Zhejiang Province, South China (Yin et al. 2001). Since these developments, there have also been other advances contributing to the precision and utility of palynological biostratigraphy in this interval, including radiometric and faunal dating of palynological biozones, and limited high-resolution correlation between continents using a well-defined palynological species.

Palynological research in the Permian is extensive, being partly driven by exploration for coal (e.g. in India and Australia), and oil and gas (e.g. in the Middle East, South America, Australia and the Barents Sea), but has tended to be regional or local in focus (see Truswell 1980). A number of authors (Bharadwaj 1969; Kemp 1975; Bharadwaj & Srivastava 1977; Balme 1980; Truswell 1980; Utting & Piasecki 1995; Warrington 1996; Price 1997; Playford & Dino 2005; Azcuy et al. 2007; Stephenson 2008a) have attempted to summarize the research or to correlate the main biozones across regions, but correlation has been tentative. Among the difficulties acknowledged by these previous reviewers are disparate stratigraphic and taxonomic methods practised in different parts of the world, and different standards of documentation of palynological data.

The approach taken in this paper is to survey the palynostratigraphic schemes in the main phytogeographic provinces and then to attempt synthesis; and so the focus is on palynostratigraphy not taxonomy. Given the plethora of palynological literature on this interval, the review is necessarily selective. Most recent published palynostratigraphic schemes (e.g. since 2000) have emanated from South American and Middle Eastern basins. In the following account, age assignments related to these and other schemes reflect those of the original authors but may not necessarily use modern chronostratigraphic nomenclature, thus a variety of stratigraphic stage and other nomenclature is used in this paper. For the convenience of the reader, a chart showing correlations of the main chronostratigraphic subdivisions used internationally is shown in Figure 1.

Fig. 1.

Chronostratigraphy of the Permian, modified after Henderson et al. (2012).

Fig. 1.

Chronostratigraphy of the Permian, modified after Henderson et al. (2012).

Permian palynostratigraphic schemes use pollen and spores almost exclusively. While it is recognized that marine palynomorphs (acritarchs) may be present in Permian rocks, no study has sought to produce a palynostratigraphy based purely on Permian acritarchs, although they may show future potential (e.g. Lei et al. 2013).

The range of morphology seen in palynomorphs in the Permian is illustrated simply in Figure 2. To improve readability, names of authors of taxa are excluded from the main text of the paper, but the main taxa and their authorship are listed in  Appendix A.

Fig. 2.

Range of morphology in Permian palynomorphs.

Fig. 2.

Range of morphology in Permian palynomorphs.

Phytogeographical provinciality makes correlation difficult because it tends to reduce the number of taxa in common between assemblages in different provinces. In general, it seems reasonable to expect geographical parity between palaeobotanical provinces and palynological provinces since plants and palynomorphs are biologically linked (Hart 1970). However, palynomorphs are subject to much wider distribution than plant remains; similar or identical palynomorphs may be produced by unrelated plants (Meyen 1969); and taphonomic factors may affect the preservation of palynomorphs and plant macrofossils differently (Utting & Piasecki 1995). Balme (1970), Sullivan (1965), Turnau (1978) and Van der Zwan (1981) surveyed the hazards of the reconstruction of palaeophytogeographical provinces by palynology. The value of pollen and spore taxa as indices of low-rank plant taxa is limited because the plant affinities of most Palaeozoic spore and pollen genera and species are unknown, and because botanical and palynological taxonomy are independent of one another. Despite this, the broad palynological characteristics of a region at a certain time are thought to be representative of the high-rank palaeobotanical characteristics of that region (Utting & Piasecki 1995).

In broad terms, there was a gradual diversification of phytogeographical provinces from relatively uniform palaeophytogeography in the Devonian to maximum provinciality in the Lopingian (Cleal & Thomas 1991) when four main provinces existed: Gondwana, Euramerica, Angara and Cathaysia (Fig. 3) (Utting & Piasecki 1995). Palaeobotanically, the Gondwana phytogeographical province is distinct from other provinces in the Permian because of the abundance of the glossopterids whose leaf impressions (Glossopteris and Gangamopteris) and more rare associated fruiting bodies (e.g. Plumsteadia and Scutum) are characteristic. Some conifers, sphenophytes and ferns were also present (Cleal & Thomas 1991). In the northern parts of Gondwana, marattialean ferns and lycophytes were present (Cleal & Thomas 1991). Palynologically, the Gondwana province is, perhaps, the most distinct because of its diversity of taeniate and monosaccate pollen, and the occurrence of restricted genera not yet recorded outside the province: for example, Guttulapollenites, Microbaculispora, Dulhuntyispora and Corisaccites (Truswell 1980). However, mixing of floras between Gondwana, Euramerica and Cathaysia are suggested by palaeobotanical studies (Archangelsky & Wagner 1983), and such mixing has been observed by palynologists (e.g. Kar & Jain 1975; Kaiser 1976; Eshet 1990; Nader et al. 1993a, b).

Fig. 3.

Phytogeographical provinces of the Permian on a Wordian reconstruction (from the Scotese Palaeomap Project); palaeophytogeography after Utting & Piasecki (1995).

Fig. 3.

Phytogeographical provinces of the Permian on a Wordian reconstruction (from the Scotese Palaeomap Project); palaeophytogeography after Utting & Piasecki (1995).

Palaeobotanically, the Euramerican province is distinguished by its abundant conifers, marattialean ferns and pteridosperms (Cleal & Thomas 1991). In the Lopingian, aridification caused the vegetation to become sparser and of lower diversity (Schweitzer 1986). Palynologically, a similar impoverishment of species occurs in the Lopingian (Pattison et al. 1973; Smith et al. 1974). British and west European assemblages are characterized by an abundance of conifer pollen of Lueckisporites virkkiae, and by the less abundant genera Protohaploxypinus, Striatoabieites, Striatopodocarpites, Taeniaesporites, Vittatina, Falcisporites and Klausipollenites (Smith et al. 1974).

According to Utting & Piasecki (1995), Angara was dominated by a cool-temperate flora containing diverse herbaceous sphenophytes and Cordaitales, with the most northerly part (Siberia) having a cold-temperate climate that spread to most of Angara by the Lopingian. According to Hart (1970), the palynology of Angara is characterized by the abundance of trilete spores rather than by bisaccate and taeniate bisaccate pollen, which are common in the other Permian phytogeographical provinces. Monosaccate pollen of Cordaitina is common in the lower parts of the Permian in Angara, whereas the monocolpate pollen Cycadopites is common in the upper parts.

Palaeobotanically, the Cathaysia province is distinguished by its gigantopterids, noeggerathialean-like progymnosperms and plants with cycad-like foliage; however, lycophytes, sphenophytes and pteridosperms were also present (Cleal & Thomas 1991). Both palaeobotanists and palynologists report a similarity between Cisuralian floras of Cathaysia and Pennsylvanian floras of Euramerica (Kaiser 1976; Cleal & Thomas 1991; Utting & Piasecki 1995). Kaiser (1976) interpreted the relict flora as being due to the continuing palaeotropical conditions of Cathaysia, which provided a refuge for the tropical vegetation of the Pennsylvanian swamps of Euramerica.

Apart from the Cisuralian abundance of Pennsylvanian Euramerican palynological taxa in Cathaysia, there are also endemic palynological taxa that characterize Cathaysia: for example, Nixispora and Patellisporites (Utting & Piasecki 1995). The Carboniferous ‘relict flora’ of Cathaysia appears to persist into the Lopingian in eastern Yunnan, China (Ouyang 1982), where diverse assemblages of genera such as Torispora, Crassispora, Triquitrites and Laevigatosporites occur.

The phytogeographical province of Euramerica is now represented by the areas west of the Ural Mountains, Europe, parts of North Africa and North America, and contains the historical type area for the Permian and the present type area for the Early Permian (Cisuralian) in the southern Urals, including the base Permian GSSP at Aidaralash Creek, southern Urals.

Knowledge of the palynostratigraphy of the Permian of the southern Urals is hampered by the lack of work since the 1980s. Most work before that date was published in Russian, but was conveniently summarized by Hart (1970) and Warrington (1996). However, the work was regionally based and not gathered into a Urals-wide palynostratigraphic scheme, perhaps because other palaeontological groups (e.g. ammonoids and fusulinacean foraminifers) already provided ample resolution for stratigraphic subdivision.

Only a short, preliminary palynostratigraphic study has been carried out at Aidaralash Creek (Dunn 2001). Dunn (2001) described a section of approximately 50 m of strata from 24.2 m below, to 26 m above, the Carboniferous–Permian boundary. The assemblages contain abundant Vittatina (particularly Vittatina costabilis) and taeniate bisaccate pollen. The non-taeniate bisaccate pollen Limitisporites monstruosus is common throughout and spores are rare. No marked palynological change occurs at the Carboniferous–Permian boundary at the base of Bed 19.5 where the conodont Streptognathodus isolatus first appears (Davydov et al. 1998).

Faddeeva (1980) in a larger survey of southern Urals palynology considered that Gzhelian (latest Carboniferous) and Asselian assemblages are distinguished by changes in proportions of spores and pollen, in that the Gzhelian assemblages have common spores and few Vittatina specimens and pollen, while Asselian assemblages have common saccate pollen (e.g. Cordaitina and Potonieisporites) and Vittatina. A similar distinction is apparent to the SW in the Donetz Basin according to Inosova et al. (1975).

Later assemblages from the Sakmarian of the Urals are dominated by saccate pollen, while Artinskian assemblages contain common spores including Tuberculatosporites and Granulatisporites, as well as pollen (Cordaitina and Cycadopites) (Hart 1970). According to Hart (1970), the Kungurian of the Urals is characterized by taeniate bisaccate pollen, and the Kazanian by more diverse assemblages of monosaccate and taeniate bisaccate pollen and an increase in non-taeniate bisaccate pollen. Faddeeva (1980) also noted a change at the base of the Kazanian, including an increase in taeniate and non-taeniate taxa, as well as the appearance of Lueckisporites, Taeniaesporites and Vesicaspora.

Utting et al. (1997), in an important paper that constitutes one of the few modern surveys of Russian Permian palynostratigraphy, compared assemblages from the Ufimian and Kazanian type areas in the southern Urals around Perm and west towards Kazan, with the sub-Angaran palynological biozones of the Sverdrup Basin of the Canadian Arctic. The Ufimian, an original Russian stage recently abandoned by the All Russian Stratigraphic Commission (see Henderson et al. 2012), may form part of the upper Kungurian, and the Kazanian is considered equivalent to the Roadian (Fig. 1). Well-preserved palynological assemblages occur in the Ufimian and Kazanian, but Utting et al. (1997) recovered no palynomorphs from the Tatarian of the area.

Utting et al. (1997) found that many taxa range through the Ufimian and Kazanian: for example, Florinites luberae, Cordaitina uralensis, Alisporites plicatus, Limitisporites monstruosus, Hamiapollenites tractiferinus and Weylandites striatus. Several taxa appear first in the lower Kazanian (e.g. Lueckisporites virkkiae), while Crucisaccites ornatus, Weylandites cincinnatus and Hamiapollenites bullaeformis disappear in the lower Kazanian. Taxa of note that are common in the Ufimian and Kazanian sequences include Protohaploxypinus perfectus, Weylandites striatus, Alisporites plicatus, Limitisporites monstruosus and Hamiapollenites tractiferinus (see Utting et al. 1997, fig. 7). At the suprageneric level, it appears that Ufimian assemblages are more spore-rich than those of the Kazanian; the latter is characterized by abundant taeniate bisaccate pollen, and common non-taeniate and polyplicate pollen (see Utting et al. 1997, fig. 8).

Although Utting et al. (1997) did not recover palynomorphs from the Tatarian in the southern Urals, they referred to other studies (see Utting et al. 1997, p. 5) that characterize the Tatarian as being dominated by species of Protohaploxypinus, Vittatina and Florinites luberae. Gomankov (1992) refers to the presence in the lower Tatarian of Scutasporites unicus, which is similar to Scutasporites nanuki from the Wordian of the Sverdrup Basin, Canada (see later discussion); and Utting et al. (1997) noted some similarities between the Russian and Canadian assemblages, although they also noted quantitative differences (see Utting et al. 1997, fig. 8), which they attributed to palaeoclimatic differences.

Gomankov et al. (1998) described few palynological differences between the Tatarian and Kazanian, but identified four broad assemblage zones for the Tatarian. In ascending order, Zone I is characterized by Weylandites and Lueckisporites virkkiae, and species of Protohaploxypinus, Taeniaesporites and Vittatina, as well as forms related to Vittatina (e.g. Ventralvittatina and Duplivittatina). Zone II lacks Ventralvittatina and Duplivittatina, and contains the first appearance of spore specimens similar to the distinctive Limatulasporites fossulatus, as well as Cladaitina and Cordaitina. Zone III contains fewer specimens of Cladaitina and Cordaitina, but also contains rare Scutasporites unicus. Zone IV sees the first appearance of Cedripites priscus, as well as sculptured monolete spores of the genus Punctatosporites.

Much of the European sediments of the Cisuralian to the west of the southern Urals were deposited in restricted basins and are therefore difficult to correlate with beds of similar age in Russia (Utting & Piasecki 1995). Doubinger (1974) and Clayton et al. (1977) defined biozones based in the Carboniferous–Permian rocks of France and Germany. Balme (1980) related the base of the Disaccites Striatiti (DS) Zone of Clayton et al. (1977) to the base of Unit III of Western Australia (see later discussion) due to the common expansion of the taeniate bisaccate pollen at these horizons. Doubinger et al. (1987) and Jerzykiewicz (1987) described a similar abundance of taeniate bisaccate pollen in the Autunian (latest Pennsylvanian–Cisuralian: Fig. 1) of the Lodève Basin, France, and the Intrasudetic Basin of SW Poland, respectively.

Hochuli (1985) documented four biozones based in the Carboniferous–Permian rocks of NE Switzerland. Hochuli (1985) recognized the Angulisporites splendidusLatensina trileta (ST) and the Potonieisporites novicus/bharadwajiCheiledonites major (NBM) biozones of Clayton et al. (1977), which range from late Stephanian A to Stephanian D; and two higher biozones (a lower Vittatina costabilis (VCI) Zone and an upper Vittatina costabilis (VCII) Zone) that Hochuli (1985) considered together to be equivalent to the Vittatina costabilis (VC) Zone of Clayton et al. (1977) (Fig. 4).

Fig. 4.

Correlations of western European Carboniferous–Permian palynostratigraphic schemes, after Hochuli (1985).

Fig. 4.

Correlations of western European Carboniferous–Permian palynostratigraphic schemes, after Hochuli (1985).

Visscher (1980) and Edwards et al. (1997) indicated that a long hiatus (the ‘post-Variscan interval’) exists between the Autunian and the Thuringian (Lopingian) of Europe (Fig. 1), although Schaarschmidt (1980) reported a Kungurian–Kazanian assemblage from Germany. Apart from this assemblage, palynological assemblages from the Guadalupian of Europe appear to be rare: however, palynological assemblages from the Lopingian rocks of Western Europe have been intensively studied (Visscher 1973), but have been shown to be, palynologically, rather homogeneous throughout the sequence (Grebe & Schweitzer 1962; Schaarschmidt 1963; Clarke 1965; Smith et al. 1974); the only notable change being a gradual overall impoverishment of the palynoflora occurring in the upper parts of the sequence (Pattison et al. 1973). Although several important taxonomic studies emanate from the European Lopingian (e.g. Klaus 1963; Schaarschmidt 1963), possibilities for palynostratigraphic subdivision lie with the variations within the Lueckisporites virkkiae palynodemes (lineages) of Visscher (1971) and with changes in the relative abundances of suprageneric groups in, for example, the Zechstein Sea Basin (Pattison et al. 1973). Visscher (1971) erected six biozones within the Thuringian that are based on a palynodeme of Lueckisporites virkkiae.

Recent studies of European Thuringian sedimentary rocks have concentrated on the palaeoenvironment (e.g. Bercovici et al. 2009) or on the palynological character of the Permian–Triassic boundary in the Alps (Looy et al. 2001; Twitchett et al. 2001; Spina et al. 2015). In North America, only a small number publications, which concentrate on taxonomy, emanate from the Guadalupian and Lopingian, including those of Wilson (1962), Jizba (1962), Tschudy & Kosanke (1966) and Clapham (1970).

In North Africa, a palynostratigraphic scheme for a Carboniferous–Permian transition sequence was defined by Brugman et al. (1988) from cuttings samples from borehole A1-19 in NE Libya. On the basis of the ranges of taxa, Brugman et al. (1988) proposed two assemblage biozones: a lower Assemblage Zone A and an upper Assemblage Zone B. The top of the lowest biozone was defined by Brugman et al. (1988) as the stratigraphic level of the disappearance of Lycospora pusilla, a spore type particularly characteristic of the Euramerican coal belts of the Pennsylvanian. Brugman & Visscher (1988) and Brugman et al. (1988) believed this level to approximate to the Permian–Carboniferous boundary. The main difference across the boundary between Assemblage Zone A and an upper Assemblage Zone B is the loss in the latter of taxa of Euramerican affinity, including Endosporites ornatus, Crassispora kosankei and Spelaeotriletes spp.

Brugman & Visscher (1988) also identified Sakmarian–?Ufimian assemblages in A1-19. Assemblages containing Lueckisporites virkkiae was recorded from Tunisia by Kilani-Mazraoui et al. (1990).

Angara was divided into four by Utting & Piasecki (1995), including the Sub-Angara, Far Eastern, Pechoran and Siberia subprovinces (Fig. 3). Sub-Angara occupied a more southerly position in Permian palaeogeographical reconstructions, while Siberia was to the NE, at high Permian latitudes.

The palynostratigraphy of Sub-Angara is the best studied of these subprovinces as a result of work carried out in the 1980s and 1990s in the Canadian Arctic Sverdrup Basin by the Canadian Geological Survey, and work related to oil exploration in the Barents Sea and Svalbard.

Utting (1989) established five preliminary palynological biozones in the Sverdrup Basin from shallow basin margin facies; later, Utting (1994) refined the ages and detailed characteristics of two of the biozones: the Wordian Ahrensisporites thorsteinssonii Scutasporites nanuki and the Roadian Alisporites plicatusJugasporites compactus concurrent range zones (Fig. 5). The ages of the biozones are based mainly on ammonoids, conodonts, brachiopods and foraminifers from the associated fossiliferous beds of shallow and deep basinal facies.

Fig. 5.

Sub-Angara palynostratigraphic schemes, adapted from Utting (1989, 1994) and Mangerud (1994).

Fig. 5.

Sub-Angara palynostratigraphic schemes, adapted from Utting (1989, 1994) and Mangerud (1994).

Utting (1994) considered that the two Sverdrup Basin biozones were Sub-Angaran in character and correlateable with assemblages in western Canada, Alaska, Greenland, Svalbard, the Barents Sea, the Pechora Basin and the northern Russian Platform. However, the Wordian Ahrensisporites thorsteinssoniiScutasporites nanuki Concurrent Range Zone differs from assemblages further south in the Urals in the type area of the Kazanian Stage (see the previous discussion). The Sverdrup Basin assemblages are dominated by trilete spores, non-taeniate and taeniate bisaccate pollen, and polyplicate taxa. Utting’s detailed studies do not show large differences in the overall suprageneric character of assemblages across the Roadian and Wordian (see Utting 1994, fig. 7), but a number of taxa are confined to particular biozones including Crinalites sabinensis, Cladaitina kolodae and Sverdrupollenites agluatus to the Alisporites plicatusJugasporites compactus Concurrent Range Zone, and Striatoabieites borealis and the eponymous species to the Ahrensisporites thorsteinssoniiScutasporites nanuki Current Range Zone. The latter biozone differs markedly from the succeeding Griesbachian Tympanicysta stoschianaStriatoabieites richteri Assemblage Zone, which was accounted for by Utting (1994) as being due to a sedimentary hiatus and climatic differences.

Mangerud (1994) established two biozones for the Cisuralian–Guadalupian in the offshore Norway Finnmark Platform: the Dyupetalum sp.–Hamiapollenites bullaeformis Assemblage Zone of ?Kungurian–Ufimian age, and the Kazanian–?Tatarian Scutasporites cf. unicusLunatisporites spp. Assemblage Zone, as well as recognizing an older biozone previously established in Spitsbergen by Mangerud & Konieczny (1993) – the Cisuralian Hamiapollenites tractiferinus Assemblage. The Hamiapollenites tractiferinus Assemblage is dominated by species of Vittatina including V. costabilis and V. saccata, but also contains taeniate bisaccate pollen including Protohaploxypinus and Striatopodocarpites; and distally taeniate bisaccate pollen such as Hamiapollenites tractiferinus and H. bullaeformis. The Dyupetalum sp.–Hamiapollenites bullaeformis and Scutasporites cf. unicusLunatisporites spp. assemblage zones are similar except for the occurrence in the upper biozone of Scutasporites cf. unicus and the occurrence of Hamiapollenites bullaeformis in the lower biozone. According to Mangerud (1994) and Nilsson et al. (1996), the Finnmark Platform and other Barents Sea sequences can be correlated across the northern Atlantic, to Spitsbergen, Greenland and the Canadian Arctic (Fig. 5) (Mangerud & Konieczny 1993; Utting 1994).

There is very little modern palynological work on the basins to the north of Sub-Angara. Hart (1970) and Utting & Piasecki (1995) summarized palynological work from the Taimyr, Kuznets and Tungus areas in Siberia, concluding that the main difference between the lower and upper parts of the Permian is that monosaccate pollen are replaced by monosulcate pollen such as Cycadopites. To the east of Angara, in the Far Eastern subprovince, Utting & Piasecki (1995) summarized the generalized palynology in the Xinjiang, Tianshan, Kunlun and Junggar areas. More recent work by Zhu et al. (2005) compared the Junggar Basin with the Tarim Basin, which belonged to the Euramerican Province at least prior to the Cisuralian. According to Zhu et al. (2005), the Junggar Basin Permian contains mainly terrestrial sediments and the Lower (1), Middle (2) and Upper (3) Permian palynofloras are characterized, respectively, by: (1) the overwhelming dominance of taeniate bisaccate pollen; (2) the high content of Cordaitina and taeniate bisaccate pollen; and (3) by the appearance of many newly evolved forms with a ‘Mesophytic aspect’. These latter include pollen and spores of ‘advanced conifers and ferns’ including distinctive taxa such as Lueckisporites virkkiae, Scutasporites xinjiangensis, Klausipollenites schaubergeri, Falcisporites zapfei, Eucommiidites, Dictyophyllidites and abundant small bisaccate pollen (e.g. Vitreisporites). Zhu et al. (2005, fig. 2) showed stratigraphic ranges of important taxa in the Permian sequences of the Junggar and Tarim basins.

Metcalfe et al. (2009) focused on the Permian–Triassic non-marine sequence at Dalongkou and Lucaogou in the Junggar Basin, and defined three assemblages, two of Lopingian age and an upper assemblage of probable Early Triassic age. The oldest is the Tuberculatosporites homotubercularisPotonieisporites sp. Q assemblage. Apart from the eponymous species, this assemblage contains monosaccate pollen, including Cordaitina uralensis, and rare specimens of Scutasporites cf. unicus. The youngest Permian assemblage, the Klausipollenites schaubergeriReduviasporonites chalastusSyndesmorion stellatum assemblage, is again dominated by the eponymous taxa, but also contains common non-taeniate bisaccate pollen, abundant algal remains (see Foster & Afonin 2006) and common Scutasporites cf. unicus. Other taxa include Lueckisporites virkkiae, Lunatisporites transversundatus, Lunatisporites pellucidus, Platysaccus queenslandi, Alisporites splendens and Striatoabieites richteri. Among spores making their appearance in this assemblage are Leptolepidites jonkeri, Limatulasporites fossulatus and Naumovaspora striata. The probable alga Reduviasporonites chalastus is also common.

The upper assemblage is the Lundbladispora foveotaPechorosporites disertusOtynisporites eotriassicus assemblage. Of note here is the presence of the distinctive megaspore Otynisporites eotriassicus. This taxon is considered a useful marker for the base of the Triassic because it occurs in both marine and non-marine sections in Greenland, Italy, Russia and Poland (Foster & Afonin 2005).

Tha Cathaysia province is associated with the South China and Indochina blocks of the eastern Palaeotethys Ocean, including the present-day regions of Yunnan, Shanxi, Meishan and Hunan.

In eastern Yunnan, Ouyang (1982) described a Lopingian Torispora giganteaPatellisporites meishanensis assemblage dominated by spores similar to many that characterize the Pennsylvanian of Euramerica (a so-called Carboniferous ‘relict flora’), with a rather small representation of gymnosperm pollen. The succeeding Yunnanospora radiataGardenasporites assemblage from the Lopingian Changhsing Formation contains more common taeniate bisaccate pollen and other gymnosperm pollen.

Liu et al. (2008) described palynological assemblages from the Cathaysian province of Shanxi, North China, establishing four assemblage zones, in ascending order, the Torispora securisTorispora laevigata (SL), the Torispora verrucosaPachetisporites kaipingensis (VK), the Thymospora thiesseniiStriatosporites heyleri (TH) and the Platysaccus minusGulisporites cochlearius (MC) assemblage zones. Liu et al. (2008) considered that the SL Assemblage Zone correlates approximately with the western European SL Zone of Clayton et al. (1977: Westphalian C–D). The VK Assemblage Zone is believed to span the Carboniferous–Permian boundary. According to Liu et al. (2008), the upper TH and MC assemblage zones are of Cisuralian age. Liu et al. (2011) described Pennsylvanian–Lopingian megaspores from the same sections, establishing four megaspore assemblage zones extending from the Pennsylvanian to the Lopingian. This palynostratigraphic scheme is correlated with the assemblage zones of Liu et al. (2008). The lowest biozone is Carboniferous, but the succeeding Bentzisporites margaritatusSpencerisporites radiatus (MS) assemblage zone is Kasimovian–Roadian in age based on fusulinids and conodonts. The Biharisporites grosstriletus (G) assemblage zone is of Wordian–Capitanian age, while the highest of the assemblage zones of Liu et al. (2011), the Biharisporites cf. foskettensis (F) assemblage zone, is believed to be of Wuchiapingian age. Liu et al. (2011) commented that several Carboniferous megaspores characteristic of Euramerica persist into the Guadalupian in Shanxi, North China, indicating that a warm and humid climate prevailed in this area during the Pennsylvanian–Roadian, whereas the climate of Euramerica had already become arid by the end of the Carboniferous. This warm and humid climate in northern China made it a refuge for some typically Euramerican Carboniferous plants.

The only study of the Permian–Triassic boundary sequence in the Cathaysian province and of the GSSP of the basal Triassic is that of Ouyang & Utting (1990). The Changhsing Formation yields a low-diversity assemblage dominated by acritarchs, but contains rare Klausipollenites sp., scolecodonts and Reduviasporonites chalastus. The lower part of the succeeding Griesbachian Chinglung Formation contains Lueckisporites virkkiae, Klausipollenites schaubergeri, Alisporites cf. nuthallenis, Protohaploxypinus spp., Weylandites sp., Cedripites spp. and Reduviasporonites chalastus, as well as ‘taxa of Triassic aspect’ (e.g. Aratrisporites cf. yunnanensis). Species of Aratrisporites have previously been used to correlate the base of the Triassic (e.g. see Metcalfe et al. 2009), although strong evidence for their reliability is lacking because species of Aratrisporites are known from the Carboniferous of the Middle East and North Africa (e.g. Aratrisporites saharaensis; Loboziak et al. 1986). Nevertheless, Aratrisporites cf. yunnanensis first appears 2.7 m above the base of the Triassic at Meishan according to Ouyang & Utting (1990), and thus this taxon might be taken as a local marker for the base of the Triassic.

Of the four phytogeographical provinces, Gondwana underwent the greatest changes through the Permian chiefly because the landmass of Gondwana was comprehensively ice-bound at the beginning of the period and then swiftly underwent deglaciation in the Cisuralian.

The Late Palaeozoic glaciation of Gondwana probably comprised three distinct episodes (Isbell et al. 2003); the third and last glaciation was geographically widespread and had continental ice sheets spanning the Carboniferous–Permian boundary through the Moscovian to the Artinskian (Fielding et al. 2008). The extent of palaeobotanical isolation and the poverty of flora and fauna during this glacial period mean that palynological assemblages are particularly difficult to relate to the international stages and to the Carboniferous–Permian boundary, with the result that even now Carboniferous and Permian palynological assemblages are difficult to distinguish in Gondwana (Stephenson 2008a).

The sedimentary rocks deposited at this time occur in cratonic basins that are now spread widely apart across Australia, India, Antarctica, southern and central Africa, and South America. The Permian rocks of these cratonic basins contain commercial deposits of coal (e.g. in India, Australia, southern Africa and South America), and oil and gas (in Australia, South America and the Middle East), and thus are amongst the most intensely studied Permian sequences in the world. The need in exploration to access stratigraphic sequences through borehole material (cuttings, core and sidewall core) has meant that palynology is also, by far, the most important biostratigraphic tool used in locally correlating sequences in the Gondwana Permian, mainly for resource exploitation rather than for academic study. Thus, palynostratigraphic schemes tend to be locally focused, although attempts have been made recently to correlate more widely across Gondwana, and from Gondwana to the international Permian scale. Because of this local focus, this part of the review concentrates on parts of Gondwana, and then attempts a synthesis at the end of the section.

Palynostratigraphy has progressed most recently in four regions: the Tarija and Chacoparaná basins in northern Argentina, the Paganzo and other basins in central western Argentina, the Claromecó Basin in eastern Argentina, and the Paraná and Amazonas basins in Brazil. For reviews of earlier literature pertaining to South America see Azcuy (1980) and Archangelsky et al. (1980). Referring generally to South American basins, Azcuy (1980) and Archangelsky et al. (1980) considered Pennsylvanian palynological assemblages (e.g. Palynozone I of Azcuy 1980) (Fig. 6) to be dominated by monosaccate pollen (e.g. Potonieisporites) and zonate spores (e.g. Ancistrospora and Lundbladispora), with taeniate bisaccate pollen being rare. Permian assemblages (e.g. Palynozone III of Azcuy 1980) contain more taeniate bisaccate pollen, Vittatina and Cristatisporites. Superimposed on these general trends are a large number of other more subtle changes that indicate variation between South American basins and which have allowed a number of separate basin-specific palynostratigraphic schemes to evolve (e.g. see Vergel 1993; Archangelsky & Vergel 1996; Césari & Gutiérrez 2000; Playford & Dino 2000, 2002; di Pasquo 2003; Di Pasquo et al. 2003; Souza & Marques-Toigo 2003; Souza et al. 2003; Pérez Loinaze & Césari 2004; Souza 2006; Balarino 2014) (Fig. 6).

Fig. 6.

Correlation of South American palynostratigraphic schemes after Stephenson (2008a), Balarino (2014) and di Pasquo et al. (2015). Biozone codes: Césari & Gutiérrez (2000) DM, Raistrickia densaConvolutispora muriornata; FS, Fusacolpites fususVittatina subsaccata; LW, LueckisporitesWeylandites; di Pasquo (2003) BC, Dictyotriletes bireticulatusCristatisporites chacoparanensis; MR, Granulatisporites micronodosusReticulatisporites reticulatus; TB, Marsupipollenites triradiatusLundbladispora braziliensis.

Fig. 6.

Correlation of South American palynostratigraphic schemes after Stephenson (2008a), Balarino (2014) and di Pasquo et al. (2015). Biozone codes: Césari & Gutiérrez (2000) DM, Raistrickia densaConvolutispora muriornata; FS, Fusacolpites fususVittatina subsaccata; LW, LueckisporitesWeylandites; di Pasquo (2003) BC, Dictyotriletes bireticulatusCristatisporites chacoparanensis; MR, Granulatisporites micronodosusReticulatisporites reticulatus; TB, Marsupipollenites triradiatusLundbladispora braziliensis.

In general, the biostratigraphy of the basins is difficult to relate to the international stages of the Carboniferous and Permian (Archangelsky et al. 1980) because of the scarcity of marine faunas: however, indirect comparisons with sequences containing palynomorphs and cosmopolitan faunas and floras (e.g. Marques-Toigo 1974; Cisterna et al. 2011) allow some tentative dates to be assigned. Since 2007, the most marked progress has been made in integrating radiometric dates with palynological biozones, allowing limited – not always reconcilable – calibration of the latter with the international scale. Amongst the most important of these studies are those of Césari (2007), Guerra-Sommer et al. (2008), Césari et al. (2011), Mori et al. (2012) and di Pasquo et al. (2015).

In the first of the studies, Césari (2007) noted radiometric dates in the San Rafael Basin in central western Argentina and in the Paraná Basin in southern Brazil that suggested numerical ages for biozones established by Césari & Gutiérrez (2000) and Souza & Marques-Toigo (2003) in those basins, respectively. Thus, the LueckisporitesWeylandites Assemblage Biozone of Césari & Gutiérrez (2000) in the San Rafael Basin contains a horizon dated at 266.3 ± 0.8 Ma (Wordian), while the Lueckisporites virkkiae Interval Biozone of Souza & Marques-Toigo (2003) in the Paraná Basin contains a dated horizon of 278.4 ± 2.2 Ma (Kungurian).

Guerra-Sommer et al. (2008) reported an age of 285.4 ± 8.6 Ma (Artinskian) within the Paraná Basin Faxinal coal seam, which is assigned to the Hamiapollenites karooensis Sub-biozone of the Vittatina costabilis Interval Biozone of Souza & Marques-Toigo (2003). Mori et al. (2012) noted a date of 281 ± 3.4 Ma (Artinskian) for another horizon within the Lueckisporites virkkiae Interval Biozone of the Paraná Basin in the Candiota coal mine.

Césari et al. (2011, fig. 6) produced a helpful synthesis of the palynostratigraphy and radiometric dating of the Carboniferous and Cisuralian sequence across Argentina and Brazil correlating the San Rafael and Paraná basin biozones and using radiometric dates to relate South American palynological biozones to those of Namibia and Australia.

di Pasquo et al. (2015) gave radiometric dates from five volcanic ash beds within the Cisuralian Copacabana Formation in central Bolivia (Tarija Basin). The five dates (cited as preliminary and published only in the non-peer reviewed Permian ICS Newsletter Permophiles, 53, Supplement 1) are 298, 295.4–295.1 and 293 Ma (for two ash layers approximately 25 m apart stratigraphically), and 292.1–291.3 Ma. According to di Pasquo et al. (2015), these dates suggest an Asselian age for the ‘Vittatina costabilis assemblage’ and an Asselian–Sakmarian age for the ‘Lueckisporites virkkiae assemblage’ of di Pasquo et al. (2015, fig. 4). This latter date is clearly inconsistent with other dates for the Lueckisporites virkkiae Interval Biozone of Souza & Marques-Toigo (2003) in the Paraná Basin (e.g. see Césari et al. 2011).

The accuracy of radiometric dates is important for discussion of the stratigraphic occurrence of Lueckisporites virkkiae, and inaccuracies inherent in radiometric dating may be the cause of apparent discrepancy in its first appearance, otherwise it is possible that Lueckisporites virkkiae has a diachronous first occurrence strongly reducing its value as a possible Euramerica–Gondwana ‘bridging taxon’.

Another possibility is that Lueckisporites virkkiae is being misidentified or that the conception of the taxon being used by taxonomists is too wide. The original concept of Lueckisporites virkkiaePotonié & Klaus (1954) was of a diploxylonoid bisaccate pollen grain with a wide separation of sacci (e.g. see Potonié & Klaus 1954, text-fig. 5, pl. 10, fig. 3; Klaus 1963, p. 300). Clarke (1965) allowed more haploxylonoid specimens within Lueckisporites virkkiae in his emendation of the species, referring to these as ‘variant B’. di Pasquo et al. (2015) did not illustrate the specimens that they attribute to Lueckisporites virkkiae, but the specimen illustrated by Mori et al. (2012, fig. 3j) is strongly haploxylonoid and lacks evidence of a prominent cappa or exoexinal taeniae. It appears closer to Corisaccites alutas. Haploxylonoid specimens of Lueckisporites virkkiae (using the conception of Clarke 1965) are difficult to separate from C. alutas, although Venkatachala & Kar (1966) regarded C. alutas as ‘subsaccate’, and subsequent authors have described C. alutas as having poorly inflated ‘leathery’ sacci, the exoexine of which is structurally indistinguishable from that of the corpus (see Stephenson 2008b).

To maintain the value of Lueckisporites virkkiae as a biostratigraphical marker may mean rejecting the emendation of Clarke (1965) and retaining the original concept of Lueckisporites virkkiaePotonié & Klaus, 1954 as a diploxylonoid bisaccate pollen grain with a wide separation of sacci (see Stephenson 2008b). It may also be valuable to start comparative studies between South American Gondwanan and Euramerican localities focusing on the genera Lueckisporites and Corisaccites.

Such uncertainties over correlation mean that, at present, it is not possible to accurately correlate South American biozones to the international scale (Fig. 6). However, Vergel (1993) and Playford & Dino (2002) correlated the Carboniferous–Permian boundary in the Chacoparaná Basin to the boundary between the Potonieisporites–Lundbladispora Zone and the Cristatisporites Zone.

Much palynological research in southern African Permian sequences has been aimed at the correlation of coal seams (Falcon et al. 1984; Aitken 1994; Millsteed 1999): however, more general schemes have been proposed (Hart 1969; Falcon 1975; Anderson 1977; MacRae 1988).

In the most detailed and extensive study covering more than 35 boreholes, four surface localities and more than 1000 samples, Anderson (1977) erected seven biozones for the Permian. The lowest, Zone 1 (Anderson 1977, fig. 8), contains common Microbaculispora, monosaccate pollen (grouped mainly under Vestigisporites) and non-taeniate bisaccate pollen (grouped mainly under Pityosporites). Anderson (1977) considered Zone 1 to be Sakmarian in age. The succeeding Zone 2 (Sakmarian–Artinskian), divided into four subzones, is chiefly distinguished by its higher numbers of zonate spores, although the highest subzone of Zone 2, and Zone 3 (Artinskian), are characterized by very abundant non-taeniate bisaccate pollen. Taeniate bisaccate pollen become common only in the highest subzone of Anderson’s Zone 3.

Anderson’s Zone 4 (Artinskian–Wordian) contains common taeniate bisaccate pollen with small numbers of proximal taeniae which were referred to Lueckisporites by Anderson (1977), but would be referred by modern taxonomists to Corisaccites, Guttulapollenites and, possibly, Taeniaesporites, as well as to Lueckisporites. Zone 5 (Capitanian) is marked by common Vittatina. Amongst other changes, a marked drop in Vittatina marks the base of Zone 6. Zones 6 and 7 (Lopingian) are similar, but are distinguished by the differing proportions of their constituent species (Anderson 1977).

The work of Anderson (1977) was not only based on a large palynological database, but also on extensive description, and particularly illustration, of important taxa. Backhouse (1991) used these data for a comparison and correlation with palynological biozones established in the Western Australian Collie Basin (Fig. 7). This study remains one of the most rigorous intercontinental palynological correlations yet completed for the Gondwana phytogeographical province, and, although correlation to the international stages is necessarily tentative, the correlation of lithological units between Western Australia and southern Africa is probably robust.

Fig. 7.

Correlation of Karoo and Collie Basin biozones, after Backhouse (1991).

Fig. 7.

Correlation of Karoo and Collie Basin biozones, after Backhouse (1991).

Other studies have also applied Australian palynostratigraphic schemes in southern Africa (Millsteed 1993, 1999; Stephenson & McLean 1999). In east and central Africa, palynostratigraphic schemes were developed by Hart (1965a) and Utting (1978). Extensive taxonomic studies in that region were carried out by Bose & Kar (1966, 1976) and Bose & Maheshwari (1968).

Unlike South America, only a few ash layers provided opportunities for direct dating of palynological biozones in Africa. However, Stephenson (2009) recovered palynological assemblages of the Converrucosisporites confluens Oppel Zone from the Ganigobis Shale Member of Namibia, close to Ash layer IIb, which was radiometrically dated as 302.0 ± 3.0 Ma (Pennsylvanian: Gzhelian or Kasimovian) (see Bangert 2000). Thus, the Converrucosisporites confluens Oppel Zone may range earlier than previously thought and may influence age considerations of non-calibrated palynological biozones, such as those of Backhouse (1991) discussed earlier.

Recent work on the palynology of South African coal seams (Götz & Ruckwied 2014, Ruckwied et al. 2014) concentrated on using perceived climatic changes expressed in palynological sequences to correlate across South African basins. Barbolini & Bamford (2014) established two biozones in the Mmamantswe coalfield (Lower Ecca) in Botswana.

The broad character of Cisuralian assemblages in the southern parts of the Middle East, and Pakistan and India, are similar to those of Africa and South America in that monosaccate pollen and simple trilete spores dominate the lowest glacigene horizons, and these are succeeded by horizons with more diverse assemblages containing taeniate and non-taeniate bisaccate pollen, cycad pollen, and fern spores. Above this level in the late Cisuralian and Guadalupian, the assemblages of Arabia, the Middle East and Pakistan begin to diverge from those of the more southerly part of Gondwana probably because of more rapid climate warming due to the fact that these areas were already of lower latitude and were rapidly moving north (e.g. Stephenson et al. 2008b).

In Arabia, there are palynostratigraphic schemes for Oman (Besems & Schuurman 1987; Love 1994; Stephenson & Osterloff 2002; Penney et al. 2008; Stephenson et al. 2008a) and Saudi Arabia (Stump & van der Eem 1995); and these, as well as in-house oil company schemes, have been synthesized by Stephenson et al. (2003) and Stephenson (2006) to a standard palynozonation for the entire Arabian Peninsula, which also has application in the wider Middle East (e.g. see Nader et al. 1993a; Stolle 2007; Angiolini & Stephenson 2008; Jan et al. 2009; Stephenson et al. 2013; Stephenson & Powell 2013, 2014). The chief unifying features of the standard palynozonation that occur throughout the Arabian Peninsula are, towards the base, the presence of common monosaccate pollen, as well as taxa such as Anapiculatisporites concinnus (characterizing Oman and Saudi Arabia Palynological Zone 1 (OSPZ1): ?Pennsylvanian) (Fig. 8), and above this the appearance of Microbaculispora and Horriditriletes (characterizing OSPZ2: ?Pennsylvanian–Asselian).

Fig. 8.

Palynostratigraphic schemes of the Arabian peninsula.

Fig. 8.

Palynostratigraphic schemes of the Arabian peninsula.

The base of OSPZ3 is defined chiefly by the abrupt increase in the small non-taeniate bisaccate pollen Pteruchipollenites indarraensis from approximately 10 to 50 or 60% of assemblages (Stephenson 2015). Other taxa that occur first consistently in OSPZ3 are the taeniate bisaccate pollen Striatopodocarpites cancellatus and S. fusus, and the taeniate ‘circumstriate’ pollen taxa, such as Circumstriatites talchirensis and Striasulcites tectus. Kingiacolpites subcircularis is common throughout this biozone, occasionally reaching 50% of assemblages. OSPZ3 is believed to be Sakmarian in age (Stephenson 2015).

The chief distinguishing characteristic of OSPZ4 (?Artinskian–Kungurian: Stephenson et al. 2003) is the common occurrence of Barakarites rotatus, K. subcircularis and P. limpidus, although C. alutas, P. amplus, Plicatipollenites spp., Striatopodocarpites spp., S. tectus, Strotersporites spp., Vesicaspora spp., Vittatina costabilis and Vittatina spp. are also present. OSPZ5 (?Roadian–Wordian) is characterized by, amongst others, Distriatites insolitus, Playfordiaspora cancellosa and Thymospora opaqua; and OSPZ6 (?Wordian–Capitanian: Stephenson 2008b) is characterized by ?Florinites balmei and Protohaploxypinus uttingii. A high-resolution palynozonation mainly aimed at correlation in hydrocarbon basins of Oman can be correlated with the OSPZ scheme (Penney et al. 2008) (Fig. 8)

Palynological data on higher parts of the sequence to the Permian–Triassic transition is not available in the western part of the Middle East because lithologies are not suitable for palynomorph preservation. However, to the east of the region in the Salt Range of Pakistan, this part of the Permian sequence is represented by rocks that contain both palynomorphs and well-preserved fauna. Balme (1970), in a pioneering taxonomic work on the Salt Range, defined many of the taxa of value in palynostratigraphy of Permian–Triassic Tethyan and Gondwanan palynostratigraphy, although Balme (1970) did not define biozones himself. More recently, Hermann et al. (2012) defined two latest Permian assemblages in the Salt Range (‘Chhidru 1’ and ‘Chhidru 2’) present in the uppermost Chhidru Formation (Changhsingian). Chhidru 1 (the Protohaploxypinus spp.–Weylandites spp. Association) is dominated by gymnosperm pollen, including common Klausipollenites spp. (including K. schaubergeri) and Protohaploxypinus spp., (including P. limpidus), as well as Weylandites lucifer and Alisporites spp. Spores are very rare. Chhidru 2 (the Kraeuselisporites wargalensisProtohaploxypinus spp. Association) is characterized by abundant cavate trilete spores such as Kraeuselisporites wargalensis and Kraeuselisporites spp. According to Hermann et al. (2012), the range of K. wargalensis is restricted to Chhidru 2. The top of Chhidru 2 is characterized by the last occurrences of Klausipollenites schaubergeri and Lueckisporites spp. (including Lueckisporites virkkiae).

In India, much of the taxonomic work in the 1960s was directed at correlation between coal seams, and not at correlation with other Gondwana sequences or international stages of the Permian. Major taxonomic studies were confined mainly to one or other of the ‘lithostratigraphic stages’ of the peninsular Indian Permian (in ascending order: Talchir, Karharbari, Barakar, Barren Measures and Raniganj) and did not span larger parts of the sequence (Truswell 1980). However, attempts have been made to synthesize data into palynostratigraphic schemes for the entire Indian Permian (e.g. Tiwari & Tripathi 1992) and some limited correlations of Indian palynostratigraphy with international stages have been made (Tiwari 1996; Vijaya 1996).

The biozones of Tiwari & Tripathi (1992) are well defined, but are not dated using the international scale. The earliest of these biozones, the Potonieisporites neglectus Biozone, from the lowest glacigene sediments of the Talchir Formation is dominated by monosaccate pollen, but lacks taeniate bisaccate pollen. The base of the succeeding Plicatipollenites gondwanensis Biozone is marked by diversification and the appearance of taeniate bisaccate pollen, and the biozone above (Parasaccites korbaensis Biozone) in the upper Talchir Formation by fern spores such as Microbaculispora tentula. The base of the succeeding Crucisaccites monoletus Biozone of the Karhabari Formation is marked by the first appearances of the eponymous taxon, as well as taxa such as Marsupipollenites. The ages of these biozones are considered to range from the Asselian to Sakmarian (Vijaya 1996). The succeeding biozones of Tiwari & Tripathi (1992) are, in order of deceasing age, the Scheuringipollenites barakarensis, Faunipollenites varius, Densipollenites indicus, Gondisporites raniganjensis and Densipollenites magnicorpus biozones. Tiwari (1996) attempted to date ‘palynoevents’ through the Indian Permian: for example, the decline of monosaccates (Palynoevent 3) was considered to be late Artinskian, and the first appearance of Densipollenites (Palynoevent 4) as Kungurian–Ufimian – although these were not related to the biozones of Tiwari & Tripathi (1992).

Despite the fact that there has been some consolidation of schemes in India, local palynostratigraphic schemes continue to be developed in the cratonic basins. In Andhra Pradesh, Aggarwal & Jha (2013) defined eight Permian palynological biozones for the Godavari Graben, linking these with climate changes, although not to the international Permian scale. Jha et al. (2014), also working in the Andhra Pradesh Godavari Graben, identified two assemblages (Palynoassemblage-I and -II) dated as Lopingian. In northern India in Kashmir, Tewari et al. (2015) identified Permian–Triassic assemblages broadly correlated to the Densipollenites magnicorpus and Klausipollenites decipiens biozones of peninsular India (see Tiwari & Tripathi 1992).

Australia has the best-documented Cisuralian sequences of Gondwana and, owing to the presence of rare marine intervals, some calibration of palynological biozones with international stages has been possible using marine macrofaunas (e.g. Leonova 1998; Archbold 1999). Later palynological biozones in the Guadalupian and Lopingian are more difficult to date due to the lack of marine fauna (in coal and red beds), although there are tie points (Foster & Archbold 2001): for example, the record of a single specimen of the ammonoid Cyclolobus persulcatus, from the Cherrabum Member of the Hardman Formation, in the Canning Basin, Western Australia (Foster & Archbold 2001), dated as ‘post-Guadalupian’ by Glenister et al. (1990) and ‘Capitanian–Dzhulfian’ by Leonova (1998). Such tie points allow spot dates to be applied to the otherwise well-developed palynostratigraphy.

A feature of palynostratigraphy in the Australian Permian is significant endemism, with the result that separate palynozonations developed in western and eastern Australian basins in the earliest period of palynological investigation (Fig. 9). In the west, eight assemblage biozones (units I–VIII), ranging in age from Pennsylvanian to Lopingian, were recognized; while, in the east, five assemblage biozones (stages 1–5) encompass the same interval (Evans 1969; Kemp et al. 1977; Foster 1979; Truswell 1980; Price 1983, 1997). The precise relationship between these schemes, and the ages of the biozones, remains speculative (see Jones & Truswell 1992) (Fig. 9), but there are broad similarities across the continent (see Balme 1980, text-fig. 4).

Fig. 9.

Correlation of eastern and western Australian palynostratigraphic schemes, after Kemp et al. (1977), Foster (1979), Balme (1980), Backhouse (1991) and Price (1983, 1997).

Fig. 9.

Correlation of eastern and western Australian palynostratigraphic schemes, after Kemp et al. (1977), Foster (1979), Balme (1980), Backhouse (1991) and Price (1983, 1997).

In the lower parts of the glacigene sequence (Stage 1), radially and bilaterally symmetrical monosaccate pollen is dominant, and taeniate and non-taeniate bisaccate pollen is subordinate. In Stage 2 above, small triangular fern spores (cheilocardioid spores) and Cycadopites become common; while, around the bases of Stage 3, taeniate and non-taeniate bisaccate pollen become common. In Stage 4, a diversity of pollen and spores develops, including distinctive colpate pollen such as Praecolpatites sinuosus; while Stage 5 is partly characterized by the very distinctive spore genus Dulhuntyispora, which is distinguished by expanded blister-like exoexine in each of the inter-radial areas.

Early work in Antarctica was carried out by Balme & Playford (1967) and Kemp (1973). Kyle (1977) erected two informal palynological biozones from study of a wide range of Antarctica localities. Her Parasaccites Zone is dominated by monosaccate pollen, along with rare bisaccate taeniate pollen, and, locally, high frequencies of Microbaculispora tentula and Cycadopites cymbatus. According to Truswell (1980), this biozone compares closely with the upper part of Stage 2 in Australia. The succeeding Protohaploxypinus Zone of Kyle (1977) is distinguished by abundant bisaccate pollen, including many taeniate taxa. In gross composition and species content, this biozone resembles Stage 4 assemblages from eastern Australia. Work following that of Kyle (1977) has tended to apply Australian palynostratigraphy to Antarctica, rather than develop more sophisticated local palynostratigraphic schemes (e.g. Farabee et al. 1990; Larrsson et al. 1990; Lindström 1995a, b; Lindström & McLoughlin 2007).

It is clear that there are quantitative and qualitative similarities in the late Pennsylvanian and Cisuralian that allow correlation across Gondwana with reasonable accuracy; after this period, however, palynological characteristics of the various parts of Gondwana begin to diverge. For example, Guadalupian and Lopingian palynological assemblages from Oman and Saudi Arabia are very different to those of Australia. Similarly, the Guadalupian palynology of South America differs considerably to that of Australia. These palynological differences, generated in the late Cisuralian following deglaciation of the Gondwana continent, are probably due to the northwards drift of Gondwana through the Permian, and the different order in which the various parts of Gondwana moved through latitudinal belts.

For the Cisuralian, the main palynological events that can be tracked with reasonable certainty through all basins of Gondwana appear to be the appearance and diversification patterns of: (1) monosaccate pollen; (2) cheilocardioid spores (such as Microbaculispora); (3) Cycadopites pollen; and (4) taeniate and non-taeniate bisaccate pollen. The precise ages of these events in relation to the international scale are not known, and recent data from radiometric dating are still being collected and assimilated (e.g. Stephenson 2009; Césari et al. 2011; di Pasquo et al. 2015) (Fig. 10).

Fig. 10.

Main trends in palynomorph types across the Gondwana phytogeographical province from the Pennsylvanian to the Cisuralian, after Stephenson (2008a). Correlation of events to the international scale is approximate.

Fig. 10.

Main trends in palynomorph types across the Gondwana phytogeographical province from the Pennsylvanian to the Cisuralian, after Stephenson (2008a). Correlation of events to the international scale is approximate.

Having said this, a few high-resolution correlations within Gondwana that involve younger Permian rocks have been possible based on close taxonomic comparison and accurate stratigraphic information: for example, the correlation of the Collie Basin, Western Australia by Backhouse (1991) with the South African biozones of Anderson (1977) (see Fig. 7). Dino & Playford (2002) and Stephenson (2008a) identified taxa that are common to South America and Australia in the Carboniferous–Permian. Converrucosisporites confluens occurs across most Gondwana sequences: Australia (Foster & Waterhouse 1988), India (Srivastava & Bhattacharyya 1996), Argentina (Archangelsky & Gamerro 1979), Uruguay (Beri & Goso 1996), Antarctica (Lindström 1995b), and Oman and Saudi Arabia (Stephenson et al. 2003). Ahrensisporites cristatus is considered to have a near-synchronous first appearance in the early Pennsylvanian, while the last appearances of Psomospora detecta, Spelaeotriletes ybertii and Rattiganispora apiculata were also considered to be possibly coeval in both continents (Dino & Playford 2002).

The purpose of palynostratigraphy, like biostratigraphy generally, is to provide correlation. Correlation helps palynologists, stratigraphers and geologists to relate sedimentary rocks deposited in one place to those in another, and to relate geological resources or events to each other and to other important geological or scientific phenomena.

In the Permian, the most important reasons for correlation related to resource extraction are to describe coal and hydrocarbon resources, to place them into a regional framework, and to help to understand how to find more coal and hydrocarbons. Probably, the bulk of work that has been done on Permian rocks in palynostratigraphy has been in this area. There have been several tens of palynostratigraphy papers published on coal measures stratigraphy in India, South America, Australia and southern Africa, with the result that coal measures sequences (e.g. Foster 1979), and even individual coal seams, can be correlated (e.g. Aitken 1994). Perhaps the work that has led to the highest-resolution palynostratigraphy (in terms of being able to recognize and distinguish the smallest divisions of stratigraphy and time) has been for the hydrocarbons industry, particularly in the Middle East where very large accumulations of oil and gas occur in the Permian. These schemes are capable of biostratigraphically characterizing rock units of only a few metres in thickness across oil and gas fields or even basins (e.g. Stephenson & Osterloff 2002; Penney et al. 2008; Stephenson et al. 2008a). In Australia also, the work of Price (1983, 1997) has been widely used for Permian onshore oil, gas, unconventional hydrocarbons and coal exploration.

Although these palynostratigraphic schemes related to resource extraction have been very successful, their main shortcoming has been a lack of correlation with schemes outside the basins, coalfields and hydrocarbon fields that they serve, and chiefly a lack of correlation with the international Permian scale. In the past, a lack of fundamental stratigraphic standards (e.g. GSSPs) for the Permian hampered this kind of correlation, but these now substantially exist (see Henderson et al. 2012) and local and regional palynostratigraphic schemes should be fitted into the wider Permian scale.

In general, also, standards of recording of palynological data and accessibility of data are higher, allowing easier comparison between palynostratigraphic schemes. Some problems still exist in the precision of taxonomic classification in different areas such that the utility of potentially useful widely correlateable palynological taxa are reduced (e.g. Lueckisporites virkkiae).

The benefits of a better integrated general palynostratigraphy are very great scientifically because there are numerous events of global scientific interest in the Permian: for example, the timing and order of deglaciation events across the continent of Gondwana that can, arguably, only be established through a Gondwana-wide palynostratigraphic scheme (see Stephenson et al. 2007), large-scale patterns of floral migration across continents, and the detailed characteristics and timing of mass extinction events within the Permian and at the Permian–Triassic boundary.

Perhaps the most important generalization that can be made about the palynostratigraphy of the Permian is that phytogeographical provinciality is strong throughout the Permian and particularly from the Guadalupian onwards, as predicted by palaeobotanical studies. This makes correlation between regional palynostratigraphic schemes difficult. These differences appear to be more than could be accounted for by differing taxonomic concepts, although these may contribute to the extent of the apparent differences between phytogeographical provinces. For these reasons, it is unlikely that a single comprehensive palynostratigraphic scheme for the Permian globally will ever be developed, or at least not one that contains inherent precision that will be valuable for resolving Earth events. This paper does not, therefore, suggest such a scheme, nor even suggest unified schemes, for the phytogeographical provinces of the Permian.

What are likely to be possible are high-resolution palynostratigraphic schemes for regions (which substantially already exist) that can be linked by tie points. These tie points will be provided by precise assemblage-level quantitative taxonomic comparison or by the use of single well-characterized palynological taxa (‘bridging taxa’) that occur across Permian phytogeographical provinces.

Perhaps the most important of these taxa for the Permian include (Fig. 11): (1) Scutasporites spp., Vittatina spp., Weylandites spp. and Lueckisporites virkkiae (for correlation between the Euramerican and Angaran provinces); and (2) Vittatina spp., Weylandites spp. and Lueckisporites virkkiae (for correlation between the Euramerican and Gondwana provinces). Correlation between the Cathaysian and other phytogeographical provinces remains a problem because few ‘bridging taxa’ have been identified. This may represent a lack of effort in palynological studies in linking Cathaysian and other phytogeographical provinces, and the isolation of much Chinese palynology in that it is published only in Chinese.

Fig. 11.

Photomicrographs of taxa of possible biostratigraphical value between and within phytogeographical provinces of the Permian. (1) Lueckisporites virkkiae, F46, V-619, 2187; from the basal Khuff clastics, Saudi Arabia; width of specimen approximately 50 µm. (2) Lueckisporites virkkiae, E42, V-619, 2187; from the basal Khuff clastics, Saudi Arabia; width of specimen approximately 50 µm. (3) Converrucosisporites confluens, V42, MM-151, 3167, distal focus; from the Al Khlata Formation, Oman; width of specimen approximately 40 µm. (4) Converrucosisporites confluens, V42, MM-151, 3167, proximal focus; from the Al Khlata Formation, Oman; width of specimen approximately 40 µm. (5) Weylandites sp. slide: 1563, EF: V30.3; from the Lower Karoo sequence, Kalahari Karoo Basin, Botswana; courtesy Alain Le Hérissé; specimen featured in Modie & Le Hérissé (2009); width of specimen approximately 35 µm. (6) Vittatina sp., M27, RA-2, 4256; from the Al Khlata Formation, Oman; width of specimen approximately 35 µm. (7) Vittatina sp., M27, TL-16, 982, from the Al Khlata Formation, Oman; width of specimen approximately 35 µm; (8) Scutasporites unicus , collection number GBA 2010/013/0027 (holotype); single grain preparation, slide No. 404, England-finder K34r; Gröden Formation = Grödner Sandstein (Arenaria di Val Gardena); courtesy of Prof. Hans Egger; specimen featured in Draxler (2010); width of specimen approximately 50 µm. (9) Otynisporites eotriassicus; Otyn IG 1 borehole, depth 817.5 m; Balic Formation (Lower Buntsandstein), Induan; courtesy of Dr Teresa Marcinkiewicz; specimen featured in Marcinkiewicz et al. (2014); width of specimen approximately 400 µm.

Fig. 11.

Photomicrographs of taxa of possible biostratigraphical value between and within phytogeographical provinces of the Permian. (1) Lueckisporites virkkiae, F46, V-619, 2187; from the basal Khuff clastics, Saudi Arabia; width of specimen approximately 50 µm. (2) Lueckisporites virkkiae, E42, V-619, 2187; from the basal Khuff clastics, Saudi Arabia; width of specimen approximately 50 µm. (3) Converrucosisporites confluens, V42, MM-151, 3167, distal focus; from the Al Khlata Formation, Oman; width of specimen approximately 40 µm. (4) Converrucosisporites confluens, V42, MM-151, 3167, proximal focus; from the Al Khlata Formation, Oman; width of specimen approximately 40 µm. (5) Weylandites sp. slide: 1563, EF: V30.3; from the Lower Karoo sequence, Kalahari Karoo Basin, Botswana; courtesy Alain Le Hérissé; specimen featured in Modie & Le Hérissé (2009); width of specimen approximately 35 µm. (6) Vittatina sp., M27, RA-2, 4256; from the Al Khlata Formation, Oman; width of specimen approximately 35 µm. (7) Vittatina sp., M27, TL-16, 982, from the Al Khlata Formation, Oman; width of specimen approximately 35 µm; (8) Scutasporites unicus , collection number GBA 2010/013/0027 (holotype); single grain preparation, slide No. 404, England-finder K34r; Gröden Formation = Grödner Sandstein (Arenaria di Val Gardena); courtesy of Prof. Hans Egger; specimen featured in Draxler (2010); width of specimen approximately 50 µm. (9) Otynisporites eotriassicus; Otyn IG 1 borehole, depth 817.5 m; Balic Formation (Lower Buntsandstein), Induan; courtesy of Dr Teresa Marcinkiewicz; specimen featured in Marcinkiewicz et al. (2014); width of specimen approximately 400 µm.

None of the Permian GSSPs involve palynological definitions, which may be problematic given the importance of palynology in correlation in the commercial and academic worlds. However, there appear to be taxa that occur at GSSPs or well-dated boundary sections that could be used to correlate those boundaries. For example, Aratrisporites spp. and Otynisporites eotriassicus may be useful to correlate the Permian–Triassic boundary into non-marine sections or sections without radiometric dates. Converrucosisporites confluens may be useful in correlating the Carboniferous–Permian boundary (Fig. 11).

The Director of the British Geological Survey (NERC) is thanked for permission to publish this paper. Dr Mercedes di Pasquo is acknowledged for providing access to valuable reference materials. Prof. Clinton Foster and an anonymous reviewer provided constructive comments. Dr Alain Le Hérissé (University of Brest), Prof. Hans Egger (Geological Survey of Austria) and Dr Teresa Marcinkiewicz are thanked for providing images of specimens in Figure 11.

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Figures & Tables

Fig. 1.

Chronostratigraphy of the Permian, modified after Henderson et al. (2012).

Fig. 1.

Chronostratigraphy of the Permian, modified after Henderson et al. (2012).

Fig. 2.

Range of morphology in Permian palynomorphs.

Fig. 2.

Range of morphology in Permian palynomorphs.

Fig. 3.

Phytogeographical provinces of the Permian on a Wordian reconstruction (from the Scotese Palaeomap Project); palaeophytogeography after Utting & Piasecki (1995).

Fig. 3.

Phytogeographical provinces of the Permian on a Wordian reconstruction (from the Scotese Palaeomap Project); palaeophytogeography after Utting & Piasecki (1995).

Fig. 4.

Correlations of western European Carboniferous–Permian palynostratigraphic schemes, after Hochuli (1985).

Fig. 4.

Correlations of western European Carboniferous–Permian palynostratigraphic schemes, after Hochuli (1985).

Fig. 5.

Sub-Angara palynostratigraphic schemes, adapted from Utting (1989, 1994) and Mangerud (1994).

Fig. 5.

Sub-Angara palynostratigraphic schemes, adapted from Utting (1989, 1994) and Mangerud (1994).

Fig. 6.

Correlation of South American palynostratigraphic schemes after Stephenson (2008a), Balarino (2014) and di Pasquo et al. (2015). Biozone codes: Césari & Gutiérrez (2000) DM, Raistrickia densaConvolutispora muriornata; FS, Fusacolpites fususVittatina subsaccata; LW, LueckisporitesWeylandites; di Pasquo (2003) BC, Dictyotriletes bireticulatusCristatisporites chacoparanensis; MR, Granulatisporites micronodosusReticulatisporites reticulatus; TB, Marsupipollenites triradiatusLundbladispora braziliensis.

Fig. 6.

Correlation of South American palynostratigraphic schemes after Stephenson (2008a), Balarino (2014) and di Pasquo et al. (2015). Biozone codes: Césari & Gutiérrez (2000) DM, Raistrickia densaConvolutispora muriornata; FS, Fusacolpites fususVittatina subsaccata; LW, LueckisporitesWeylandites; di Pasquo (2003) BC, Dictyotriletes bireticulatusCristatisporites chacoparanensis; MR, Granulatisporites micronodosusReticulatisporites reticulatus; TB, Marsupipollenites triradiatusLundbladispora braziliensis.

Fig. 7.

Correlation of Karoo and Collie Basin biozones, after Backhouse (1991).

Fig. 7.

Correlation of Karoo and Collie Basin biozones, after Backhouse (1991).

Fig. 8.

Palynostratigraphic schemes of the Arabian peninsula.

Fig. 8.

Palynostratigraphic schemes of the Arabian peninsula.

Fig. 9.

Correlation of eastern and western Australian palynostratigraphic schemes, after Kemp et al. (1977), Foster (1979), Balme (1980), Backhouse (1991) and Price (1983, 1997).

Fig. 9.

Correlation of eastern and western Australian palynostratigraphic schemes, after Kemp et al. (1977), Foster (1979), Balme (1980), Backhouse (1991) and Price (1983, 1997).

Fig. 10.

Main trends in palynomorph types across the Gondwana phytogeographical province from the Pennsylvanian to the Cisuralian, after Stephenson (2008a). Correlation of events to the international scale is approximate.

Fig. 10.

Main trends in palynomorph types across the Gondwana phytogeographical province from the Pennsylvanian to the Cisuralian, after Stephenson (2008a). Correlation of events to the international scale is approximate.

Fig. 11.

Photomicrographs of taxa of possible biostratigraphical value between and within phytogeographical provinces of the Permian. (1) Lueckisporites virkkiae, F46, V-619, 2187; from the basal Khuff clastics, Saudi Arabia; width of specimen approximately 50 µm. (2) Lueckisporites virkkiae, E42, V-619, 2187; from the basal Khuff clastics, Saudi Arabia; width of specimen approximately 50 µm. (3) Converrucosisporites confluens, V42, MM-151, 3167, distal focus; from the Al Khlata Formation, Oman; width of specimen approximately 40 µm. (4) Converrucosisporites confluens, V42, MM-151, 3167, proximal focus; from the Al Khlata Formation, Oman; width of specimen approximately 40 µm. (5) Weylandites sp. slide: 1563, EF: V30.3; from the Lower Karoo sequence, Kalahari Karoo Basin, Botswana; courtesy Alain Le Hérissé; specimen featured in Modie & Le Hérissé (2009); width of specimen approximately 35 µm. (6) Vittatina sp., M27, RA-2, 4256; from the Al Khlata Formation, Oman; width of specimen approximately 35 µm. (7) Vittatina sp., M27, TL-16, 982, from the Al Khlata Formation, Oman; width of specimen approximately 35 µm; (8) Scutasporites unicus , collection number GBA 2010/013/0027 (holotype); single grain preparation, slide No. 404, England-finder K34r; Gröden Formation = Grödner Sandstein (Arenaria di Val Gardena); courtesy of Prof. Hans Egger; specimen featured in Draxler (2010); width of specimen approximately 50 µm. (9) Otynisporites eotriassicus; Otyn IG 1 borehole, depth 817.5 m; Balic Formation (Lower Buntsandstein), Induan; courtesy of Dr Teresa Marcinkiewicz; specimen featured in Marcinkiewicz et al. (2014); width of specimen approximately 400 µm.

Fig. 11.

Photomicrographs of taxa of possible biostratigraphical value between and within phytogeographical provinces of the Permian. (1) Lueckisporites virkkiae, F46, V-619, 2187; from the basal Khuff clastics, Saudi Arabia; width of specimen approximately 50 µm. (2) Lueckisporites virkkiae, E42, V-619, 2187; from the basal Khuff clastics, Saudi Arabia; width of specimen approximately 50 µm. (3) Converrucosisporites confluens, V42, MM-151, 3167, distal focus; from the Al Khlata Formation, Oman; width of specimen approximately 40 µm. (4) Converrucosisporites confluens, V42, MM-151, 3167, proximal focus; from the Al Khlata Formation, Oman; width of specimen approximately 40 µm. (5) Weylandites sp. slide: 1563, EF: V30.3; from the Lower Karoo sequence, Kalahari Karoo Basin, Botswana; courtesy Alain Le Hérissé; specimen featured in Modie & Le Hérissé (2009); width of specimen approximately 35 µm. (6) Vittatina sp., M27, RA-2, 4256; from the Al Khlata Formation, Oman; width of specimen approximately 35 µm. (7) Vittatina sp., M27, TL-16, 982, from the Al Khlata Formation, Oman; width of specimen approximately 35 µm; (8) Scutasporites unicus , collection number GBA 2010/013/0027 (holotype); single grain preparation, slide No. 404, England-finder K34r; Gröden Formation = Grödner Sandstein (Arenaria di Val Gardena); courtesy of Prof. Hans Egger; specimen featured in Draxler (2010); width of specimen approximately 50 µm. (9) Otynisporites eotriassicus; Otyn IG 1 borehole, depth 817.5 m; Balic Formation (Lower Buntsandstein), Induan; courtesy of Dr Teresa Marcinkiewicz; specimen featured in Marcinkiewicz et al. (2014); width of specimen approximately 400 µm.

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