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parasequences (2–5 m thick), with stacking <strong>of</strong> upwardly thicker parasequences. Micr<strong>of</strong>acies range from wackestones to packstones (occasionally crinoidal grainstones) with crinoids, along with thin-shelled bivalves (“filaments”), radiolaria, benthic <strong>and</strong> planktonic foraminifers, <strong>and</strong> o<strong>the</strong>r macroinvertebrate fragments. Apart from disarticulated crinoid ossicles, benthic macr<strong>of</strong>auna are almost absent in <strong>the</strong> Middle <strong>Jurassic</strong>, in contrast to <strong>the</strong> Lower <strong>Jurassic</strong>. Planktonic macr<strong>of</strong>auna is also scarce, but in <strong>the</strong> top <strong>of</strong> some levels, especially toward <strong>the</strong> upper part, cephalopods proved widespread (ammonites <strong>and</strong> belemnites). In <strong>the</strong>se levels, better developed in <strong>the</strong> Malvariche section, ammonites assemblages were collected, enabling recognition <strong>of</strong> <strong>the</strong> Lower Bajocian, based on <strong>the</strong> record <strong>of</strong> a specimen <strong>of</strong> Skirroceras sp. Also recognized were <strong>the</strong> Lower Callovian [Bullatus Zone; based on <strong>the</strong> record <strong>of</strong> Homoeoplanulites sp., Macrocephalites sp., <strong>and</strong> Kheraiceras cf. bullatus (d’Orbigny)], <strong>and</strong> <strong>the</strong> Gracilis Zone (Patina Zone sensu Sequeiros, 1974) with abundant <strong>and</strong> significant ammonites, especially Macrocephalinae <strong>and</strong> Reineckeidae. No o<strong>the</strong>r ammonite faunas were found in <strong>the</strong> Middle <strong>Jurassic</strong>. 4.3. Upper <strong>Jurassic</strong> The Upper <strong>Jurassic</strong> features at Malvariche <strong>and</strong> Prat Mayor differ somewhat with regard to lith<strong>of</strong>acies <strong>and</strong> faunal assemblages, although <strong>the</strong> thicknesses are quite similar, 80 <strong>and</strong> 90 m, respectively (Fig. 2). As a whole, <strong>the</strong> succession is composed by finely stratified marl <strong>and</strong> marly limestones which evolved to stratified limestones stacked in thickening upward parasequences (1–2 m thick). Then, massive nodular limestones (sometimes brecciated) alternate with stratified limestones <strong>and</strong> marls, arranged in upwardly thinning parasequences. Textures <strong>and</strong> micr<strong>of</strong>acies are highly variable, ranging from pelloidal mudstones to intraclastic packstones (occasionally crinoidal grainstones) with Globuligerina (at <strong>the</strong> base), filaments, Saccocoma, radiolaria, Globochaete, Stomiosphaera, Cadosina, macroinvertebrate fragments (mainly ammonites <strong>and</strong> belemnites) <strong>and</strong> calpionellids (in <strong>the</strong> upper part). In both sections (Fig. 2), above <strong>the</strong> multiple Fe–Mn crusts dated as Lower Callovian (Gracilis Zone) outcrops a 5–10 m thick interval <strong>of</strong> marly limestones <strong>and</strong> marls, finely stratified, <strong>and</strong> texturally mudstones to wackestones rich in Globuligerina, attributed to <strong>the</strong> Callovian?–Oxfordian. In <strong>the</strong> Malvariche section,7m<strong>of</strong>slightly nodular marly limestones appear in upwardly thickening parasequences. Towards <strong>the</strong> top, <strong>the</strong>re is an irregular massive breccioid bank,4m<strong>of</strong>slightly nodular marly limestones organized in upwardly thinning parasequences, <strong>and</strong> a characteristic crinoidal bank with an erosive base. Just below this crinoidal bank, ammonite assemblages were collected from <strong>the</strong> uppermost Kimmeridgian (Beckeri Zone). These slightly nodular marly limestones stacked in Fig. 2. Correlation <strong>of</strong> <strong>the</strong> <strong>Jurassic</strong> sections at Malvariche <strong>and</strong> Prat Mayor. Fig. 2. Corrélation des sections jurassiques de Malvariche et Prat Mayor. J.E. Caracuel et al. / Geobios 39 (2006) 25–42 upwardly thinning parasequences continues 15 m more over <strong>the</strong> encrinitic bank, <strong>and</strong> <strong>the</strong>n change to upwardly thickening parasequences; <strong>the</strong> facies change gradually to alternating marly/calcareous nodular limestones, <strong>of</strong>ten brecciated. The upper 20 m are composed <strong>of</strong> crinoidal levels <strong>and</strong> marly intervals with micr<strong>of</strong>acies enriched in hyaline calpionellids which characterized <strong>the</strong> Upper Tithonian. In <strong>the</strong> Prat Mayor section above <strong>the</strong> marly limestones with Globuligerina, outcrop 50 m <strong>of</strong> ammonitico rosso nodular limestones alternating with thick breccioids banks, organized in upwardly coarsening <strong>and</strong> thickening parasequences (2–4 m thick). In this interval, ammonite assemblages characterizing <strong>the</strong> Middle–Upper Oxfordian <strong>and</strong> <strong>the</strong> Lower– Middle? Kimmeridgian were collected. In contrast to <strong>the</strong> Malvariche section, no ammonites from <strong>the</strong> Upper Kimmeridgian were found. The upper part <strong>of</strong> section at Prat Mayor appears similar to Malvariche, although more reduced <strong>and</strong> with characteristic breccioid banks. In both sections, <strong>the</strong> calpionellids Zones <strong>of</strong> Chitinoidella, Crassicollaria <strong>and</strong> Calpionella were recorded. 5. Ammonite <strong>biostratigraphy</strong> <strong>Jurassic</strong> ammonite faunas belonging to <strong>the</strong> Internal Zone <strong>of</strong> <strong>the</strong> Betic Cordillera has been rarely <strong>and</strong> discontinuously reported, <strong>and</strong> in all cases from <strong>the</strong> non-metamorphosed Malaguide <strong>and</strong> “Dorsal” domains (Fallot, 1929, 1931–1934, 1945; Peyre <strong>and</strong> Peyre, 1960; Azema, 1960, 1961; Paquet, 1969; Geyer <strong>and</strong> Hinkelbein, 1971, 1974; Seyfried, 1978 <strong>and</strong> Caracuel et al., 2001). Biostratigraphic data from Sierra Espuña come mainly from Geyer <strong>and</strong> Hinkelbein (1974); Seyfried (1978) <strong>and</strong> Caracuel et al. (2001), who described ammonite assemblages belonging to <strong>the</strong> Domerian, Middle–Upper Toarcian, Upper Bajocian, Oxfordian <strong>and</strong> Upper Kimmeridgian. For <strong>the</strong> present paper, more than 500 macroinvertebrates, mainly ammonites, were collected in order to complete <strong>and</strong> to revise <strong>the</strong> biostratigraphic framework from <strong>the</strong> Domerian to <strong>the</strong> Kimmeridgian in <strong>the</strong> three previously studied <strong>and</strong> two new <strong>Jurassic</strong> sections at Sierra Espuña. The ammonite zonal/subzonal scheme in Cariou <strong>and</strong> Hantzpergue (1997) for <strong>the</strong> Mediterranean Domain was used in <strong>the</strong> Domerian, Toarcian <strong>and</strong> Callovian stages. Domerian ammonites show good preservation with neomorphosed shells, sometimes ferruginous, <strong>and</strong> mostly with preserved living chambers; phragmocone septa are consistently preserved (Figs. 4 <strong>and</strong> 5). There appears to be no taphonomic size bias, although <strong>the</strong> smaller ammonoids (occasionally fragments) are sometimes found in <strong>the</strong> interior <strong>of</strong> Fe–Mn oncoids, with a variable mode <strong>of</strong> preservation. 31