<?xml version="1.0" encoding="UTF-8"?><!DOCTYPE article  PUBLIC "-//NLM//DTD Journal Publishing DTD v3.0 20080202//EN" "http://dtd.nlm.nih.gov/publishing/3.0/journalpublishing3.dtd"><article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" dtd-version="3.0" xml:lang="en" article-type="research article"><front><journal-meta><journal-id journal-id-type="publisher-id">OJG</journal-id><journal-title-group><journal-title>Open Journal of Geology</journal-title></journal-title-group><issn pub-type="epub">2161-7570</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/ojg.2022.126023</article-id><article-id pub-id-type="publisher-id">OJG-118251</article-id><article-categories><subj-group subj-group-type="heading"><subject>Articles</subject></subj-group><subj-group subj-group-type="Discipline-v2"><subject>Earth&amp;Environmental Sciences</subject></subj-group></article-categories><title-group><article-title>
 
 
  The Permian-Triassic Transitional Zone: Jordan, Arabian Plate; Linked to Siberian Large Igneous Province and Neo-Tethys Breakup Degassing via Climate Forcing, Atmospheric Hazard and Metal Toxicity
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Werner</surname><given-names>Schneider</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Elias</surname><given-names>Salameh</given-names></name><xref ref-type="aff" rid="aff2"><sup>2</sup></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib></contrib-group><aff id="aff1"><addr-line>Formerly Braunschweig Technical University, Braunschweig, Germany</addr-line></aff><aff id="aff2"><addr-line>University of Jordan, Amman, Jordan</addr-line></aff><pub-date pub-type="epub"><day>02</day><month>06</month><year>2022</year></pub-date><volume>12</volume><issue>06</issue><fpage>472</fpage><lpage>503</lpage><history><date date-type="received"><day>9,</day>	<month>October</month>	<year>2021</year></date><date date-type="rev-recd"><day>27,</day>	<month>June</month>	<year>2022</year>	</date><date date-type="accepted"><day>30,</day>	<month>June</month>	<year>2022</year></date></history><permissions><copyright-statement>&#169; Copyright  2014 by authors and Scientific Research Publishing Inc. </copyright-statement><copyright-year>2014</copyright-year><license><license-p>This work is licensed under the Creative Commons Attribution-NonCommercial International License (CC BY-NC).http://creativecommons.org/licenses/by-nc/4.0/</license-p></license></permissions><abstract><p>
 
 
  End-Permian Gondwana siliciclastics (50 - 70 m) of the Um Irna F exposed along the NE Dead Sea, exhibit carbonate-free fining upward cycles (FUC) deposited during acid flash flood events under tropical climate. Several ferruginous paleosol intercalations cover periods of drying upward formation (DUP) under semiarid/arid climates. Thin grey pelite beds interbedded between paleosol and overlying FUC, are interpreted as tephra deposits sourced in Siberian LIP- and Neo-Tethys (NT)-Degassing. The Wadi Bassat en Nimra-section exhibits the P-T transitional zone where flash flood deposits meet supra-/intertidal sediments of the southward-directed transgressive NT. Decreasing flash-flooding continued through the Lower Scythian (Ma’in F.) during transgression, reworking, and resedimentation. Two euryhaline foraminifera-bearing limestone beds are discussed as indicators for the end of mass extinction (recovery phase: ca. 250.8 - 250.4 Ma) possibly correlating with the Maximum Flooding Surface MFS Tr 10 (ca. 250.5 Ma) on the Arabian Shelf (Khuff cycles B; A). Comparable data from the Germanic Basin as FUC/DUP-cycles, tephrasuspicious “Grey Beds” with high concentrations of As, Co, Pb, Zn, and Cu as well as the U-Pb Age data of the Siberian LIP meet the PTB-Zone between the MFSs Intervals P 40 (ca. 254 Ma)/Tr 10 (ca 250.5 Ma) on the Arabian Shelf. MFS (Tr 10, 20, 30) and SBs resp. on the Arabian Plate, as well as Scythian Substage boundaries correlate with 
  &amp;#8706
  <sup>13</sup> C-excursions recorded at Musandam, UAE. Thereby, the ratio of greenhouse gases (+climate forcing)/aerosols und tephra (-climate forcing) takes a significant influence on the 
  &amp;#8706
  <sup>13</sup>C-Variation.
 
</p></abstract><kwd-group><kwd>P-T Transition Zone</kwd><kwd> Jordan</kwd><kwd> Arabian Plate</kwd><kwd> Siliciclastics</kwd><kwd> Flash Flood Deposits</kwd><kwd> Neo-Tethys Transgression</kwd><kwd> Siberian LIP Degassing: Acid Rain</kwd><kwd> Tuffs</kwd><kwd> Metal Toxcicity</kwd><kwd> Climate Forcing</kwd><kwd> Milankovitch Croll Cycles</kwd><kwd> Germanic Basin (Correlation)</kwd><kwd> Earth/Moon Interplay</kwd><kwd> Self-Regulation (Autopoiesis)</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>Myths</p><p>… and rain came on Earth 40 days and 40 nights (1. Mose 7, 12).</p><p>… and the water remained150 days on Earth (1. Mose 7, 24).</p><p>… there get drowned all flesh, all animals creeping on Earth, the birds, the cattle and all that has moved on Earth, and all human beings (1. Mose 7, 21).</p><p>… and the water became abundant and rose so much on Earth that all high mountains were covered beneath the sky (1. Mose 7, 19).</p><p>… and all the water in the stream changed into “blood” (2. Mose 7, 20).</p><p>… and the fish in the stream died and the stream owned a strong smell (2. Mose 7, 21).</p><p>… and oh heaven, keep back your rain (Koran 11, 45).</p><p>From W. Jens [<xref ref-type="bibr" rid="scirp.118251-ref1">1</xref>], transl. Sch.</p><p>These citations reconfirmed by some 180 Ethnic Groups [<xref ref-type="bibr" rid="scirp.118251-ref2">2</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref3">3</xref>], may throw a glimpse at innumerable hazardous “rare events” that have occurred throughout Earth’s History.</p><p>Throughout the last decade, the authors have been dealing with: whether “rare events” (major impacting magmatic degassing), may affect apart mass extinction-sedimentologic/sequence-analytical patterns and the mineralogy of siliciclastic sediments as well?</p><p>One subject concerned Early Paleozoic and Lower Cretaceous quartz arenite fining upward cyclothems (FUC) on the Jordanian platform [<xref ref-type="bibr" rid="scirp.118251-ref4">4</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref5">5</xref>], and another one focuses on end-Cretaceous transitional quartz arenite deposited in N Germany, northern Harz-foreland with regard to Deccan volcanism, India, Chicxulub impact, Mexico and volcanic arc origination (Lesser Antilles, Seychelles, Scotia) [<xref ref-type="bibr" rid="scirp.118251-ref6">6</xref>]; furthermore, at the latter locality (Uhry, Braunschweig County), the Eocene/Oligocene boundary in connection with both impact cratersPopigai, Russia and Chesapeake, USA [<xref ref-type="bibr" rid="scirp.118251-ref7">7</xref>].</p><p>To all subjects, the Atlas System, Version 3 of Price [<xref ref-type="bibr" rid="scirp.118251-ref8">8</xref>] was applied, telling that an abrupt change of both direction and speed of plates along their tracks would imply a major impact.</p><p>However, no definite major impact craters are known throughout the relevant Early Paleozoic (Middle Cambrian to Ordovician)! In the case of the Lower Cretaceous, we are faced with the Paraňa/Etendeka Plume Province and the opening of the S Atlantic [<xref ref-type="bibr" rid="scirp.118251-ref9">9</xref>] while the Cretaceous/Tertiary boundary (KPgB) relates to both Deccan Traps and the Chicxulub impact [<xref ref-type="bibr" rid="scirp.118251-ref10">10</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref11">11</xref>].</p><p>Nevertheless, Price’s concept appears to be inviting and helpful in order to build a bridge between “rare events”, plate tectonics, and Sedimentary Geology/Mineralogy; yet the results obtained caused doubt on the main driving force by impacting versus indirect effects of plume degassing; in particular, since Deccan volcanism caused a significantly higher temperature pulse than the Chicxulub meteorite did [<xref ref-type="bibr" rid="scirp.118251-ref10">10</xref>].</p><p>Thus this paper stresses the main role of magmatic degassing causing climate change, atmospheric hazards, acid flash flooding (sturz rain), and global metal toxicity with regard to both biotic and abiotic “vulnerability” throughout the P-T transitional zone.</p><p>After Hercynian tectonics (Devonian-Carboniferous), following rifting and block faulting across the Near/Middle East led to splitting of this northern part of Gondwana, creating a passive margin of the Arabian Plata fronting the newly opened Neo-Tethys [<xref ref-type="bibr" rid="scirp.118251-ref12">12</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref13">13</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref14">14</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref15">15</xref>]. Throughout the Upper Permian, the Jordanian Platform exhibited low relief plains where fluvial clastics prograded northward into the transgressive shallow Neo-Tethys [<xref ref-type="bibr" rid="scirp.118251-ref12">12</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref16">16</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref17">17</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref18">18</xref>].</p><p>The paleogeographic position of the Arabian Platform was situated in the equatorial zone ~15˚ - 20˚ south of the paleo-equator ( [<xref ref-type="bibr" rid="scirp.118251-ref19">19</xref>], <xref ref-type="fig" rid="fig1">Figure 1</xref>).</p><p>The P-T transitional zone falls in Jordan into the time span between both Maximum Flooding Surfaces (MFSs) P 40 (~Wuchiapingian: 254 Ma) and Tr 10 (Induan: ~250.5 Ma) established on the Arabian Plate [<xref ref-type="bibr" rid="scirp.118251-ref14">14</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref15">15</xref>].</p><p>The biostratigraphic age of the late Permian Um Irna F., NE of the Dead Sea was determined by a low diversity assemblage of macroplants and palynomorphs [<xref ref-type="bibr" rid="scirp.118251-ref12">12</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref16">16</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref18">18</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref20">20</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref21">21</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref22">22</xref>] with conodonts and euryhaline foraminifera indicating an early Induan age (early Triassic) [<xref ref-type="bibr" rid="scirp.118251-ref12">12</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref16">16</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref23">23</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref24">24</xref>], after the P-T boundary events’ recovery phase.</p><p>The Um Irna F. and its transitional zone to the Himara M. (lowermost Triassic) are well exposed along the NE margin of the Dead Sea some 50 - 70 m thick, along the road outcrops and several W/E-striking wadis cutting the Jordan Rift shoulder north of Wadi Mujib ( [<xref ref-type="bibr" rid="scirp.118251-ref17">17</xref>], <xref ref-type="fig" rid="fig2">Figure 2</xref>).</p><p>Because of the low paleo-platform dipping the sections become seaward more complete, thicker and more fine-grained. Therefore, lithofacies correlation from wadi to wadi (Zarqa Ma’in, Bassat en Nimra, Himara) owns uncertainties [<xref ref-type="bibr" rid="scirp.118251-ref12">12</xref>].</p><p>Nevertheless, we are in the comfortable position to applying the biostratigraphic and sedimentologic data recovered throughout the last four decades [<xref ref-type="bibr" rid="scirp.118251-ref12">12</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref16">16</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref17">17</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref18">18</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref25">25</xref>] to confront them with the most recent data about the Siberian Large Igneous Province (LIP) evidence and with relating indirect effects [<xref ref-type="bibr" rid="scirp.118251-ref26">26</xref>].</p><p>So there does exist a general agreement on the following sedimentologic features of the P-T in Jordan transition zone [<xref ref-type="bibr" rid="scirp.118251-ref12">12</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref16">16</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref17">17</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref18">18</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref25">25</xref>].</p><p>&#173; The siliciclastic fining upward cyclothems (FUC) and paleosol intercalations of the Um Irna F. were deposited on unconfined braid plains of a northwestward smoothly dipping platform of low relief close to the Tethys coastline under tropical climate by fluvial flash flood conditions.</p><p>&#173; Each cycle originates from one single atmospheric event (sturz rain) that caused mass flow conditions to deposit complete/incomplete FUCs, nomenclature (see [<xref ref-type="bibr" rid="scirp.118251-ref27">27</xref>]).</p><p>&#173; Around the Lower/Upper Member boundary of the Um Irna F., the transport direction changed from N/NW towards W/SW indicating a reorganization of nearly located source areas [<xref ref-type="bibr" rid="scirp.118251-ref17">17</xref>].</p><p>&#173; The cyclic Fe-glabule/pisolite-bearing paleosols initially developedunder humid/tropical climate (hydromorphic) and then continuously changed towards semiarid/arid conditions (ascending pore water) for drying upward paleosol formation (DUP).</p><p>&#173; Because of paleo-platform dipping and possible pre-Cretaceous down-faulting, the Upper Permian, Triassic and Jurassic sequences became thicker, more complete and faster marine, tracing northward along the Dead Sea which is most relevant for the “PTB”-interpretation (SP or hiatus-free!) [<xref ref-type="bibr" rid="scirp.118251-ref12">12</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref16">16</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref25">25</xref>].</p><p>&#173; In contrast to other outcrops measured, the Wadi Bassat en Nimra-Section obviously exposes a hiatus-free diachronous P-T transition to the lowermost Triassic Himara M. (Fluvial → supratidal → intertidal), ( [<xref ref-type="bibr" rid="scirp.118251-ref28">28</xref>], <xref ref-type="fig" rid="fig3">Figure 3</xref>, for comparison see [<xref ref-type="bibr" rid="scirp.118251-ref17">17</xref>], <xref ref-type="fig" rid="fig4">Figure 4</xref>).</p><p>&#173; The overlying Nimra M. yields increasingly carbonate cement, ichnofacies, and two thin subtidal limestone beds bearing fully marine conodonts and euryhaline foraminifera [<xref ref-type="bibr" rid="scirp.118251-ref12">12</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref16">16</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref18">18</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref23">23</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref24">24</xref>] that may coincide with MFS Tr 10 (250.5 Ma) on the Arabian Shelf [<xref ref-type="bibr" rid="scirp.118251-ref14">14</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref15">15</xref>].</p></sec><sec id="s2"><title>2. Flash Flood Deposits’ Architecture, Lithofacies and Mineralogic Implications</title><p>Dealing with the outcrops of both Wadis Bassat en Nimra and Himara, Miall’s nomenclature ( [<xref ref-type="bibr" rid="scirp.118251-ref27">27</xref>], <xref ref-type="table" rid="table1">Table 1</xref>) is applied to the carbonate-free lithofacies types of the siliciclastic cyclothems (mostly quartz arenite) while the sequence architecture relates tro liquefied/fluidized flow processes caused by flash flooding as driving transport force, hitherto applied for deep sea clastics ( [<xref ref-type="bibr" rid="scirp.118251-ref29">29</xref>], <xref ref-type="fig" rid="fig5">Figure 5</xref>). Thereby, resedimentary processes develop from elastics via plastic to viscose-fluidal flowing mechanism between proximal and distal destination.</p><p>Atmospheric hazardous events generated, in case of the Um Irna F., five major FUCs each overlain with a kaolinitic ferruginous paleosol (0.5 - 6 m); however, all in all some 20 subordinate cycles [<xref ref-type="bibr" rid="scirp.118251-ref16">16</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref17">17</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref18">18</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref28">28</xref>] encountered in Wadi Bassat en Nimra, as follows (<xref ref-type="fig" rid="fig3">Figure 3</xref> and <xref ref-type="fig" rid="fig4">Figure 4</xref>).</p><p>&#173; Gmm → Sm → St → Fm → Fl → Paleosol (complete);</p><p>&#173; Gmm → Sm → St (partially amalgamation);</p><p>&#173; Sm → Fm → F1 → Paleosols (or missing, eroded);</p><p>&#173; St → Fm → F1;</p><p>&#173; Fm → F1 → Paleosols (or missing, eroded);</p><p>&#173; Sm → Paleosols.</p><p>According to the model represented in <xref ref-type="fig" rid="fig6">Figure 6</xref> for vertical and lateral lithofacies distribution during the single flash flood, the next one may erode more or less all other preceding lithofacies units.</p><p>When finally tailings of a flash flood passed into the intertidal environment during southward Tethys transgression, the silty/sandy clastics were sorted by wave and tidal current activity and thin-bedded deposited which concerns most portions of both Himara and Nimra M. Figures 7(a)-(c), may illustrate such processes by using recent intertidal conditions on Amrum Island, North Sea as a model for the UmIrna F./Himara M. transional zone (paleo-aerial photograph on the braid plains of the Jordanian Platform).</p><p>Siliciclastic transport and deposition occurred in short cyclic intervals. Tectonic activity at the Lower/Upper B. of the UmIrna F. led not only to a modification of the near hinterland [<xref ref-type="bibr" rid="scirp.118251-ref17">17</xref>] but also to a change of mineral composition ( [<xref ref-type="bibr" rid="scirp.118251-ref30">30</xref>], <xref ref-type="fig" rid="fig3">Figure 3</xref>). In contrast to the poorly sorted quartz arenite of the Lower M., biotite and feldspars (alkali-feldspars, plagioclase, and microcline) give evidence for an additional mica-granite source area.</p><p>Plant-bearing pelite deposited in swamps of the Upper M. provided not only palynologic age determination but also verification for paleo-wildfire [<xref ref-type="bibr" rid="scirp.118251-ref31">31</xref>]. Quartz grains generally angular, broken, strongly corroded, with relicts ofsyntaxial overgrowth, give hint on a manifold reworking and change of chemical//physical weathering (Figures 8(a)-(c)).</p><table-wrap id="table1" ><label><xref ref-type="table" rid="table1">Table 1</xref></label><caption><title> Light minerals, heavy minerals and cement minerals of the Um Irna F. and Ma. in F. from grain mounts and thin sections [<xref ref-type="bibr" rid="scirp.118251-ref17">17</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref28">28</xref>]. Grain-%, from grain mounts and thin sections, Wadi Basset en Nimra</title></caption><table><tbody><thead><tr><th align="center" valign="middle" >Light minerals</th><th align="center" valign="middle" >Um Irna F.</th><th align="center" valign="middle" >Ma’in F.</th></tr></thead><tr><td align="center" valign="middle" >Particles</td><td align="center" valign="middle" >72 - 81</td><td align="center" valign="middle" >72 - 83</td></tr><tr><td align="center" valign="middle" >Quartz</td><td align="center" valign="middle" >76 - 100</td><td align="center" valign="middle" >86 - 99</td></tr><tr><td align="center" valign="middle" >K-feldspar</td><td align="center" valign="middle" >1 - 15</td><td align="center" valign="middle" >1 - 10</td></tr><tr><td align="center" valign="middle" >Plagioclase</td><td align="center" valign="middle" >0 - 3</td><td align="center" valign="middle" >0 - 2</td></tr><tr><td align="center" valign="middle" >Muscovite</td><td align="center" valign="middle" >0 - 1</td><td align="center" valign="middle" >-</td></tr><tr><td align="center" valign="middle" >Biotite</td><td align="center" valign="middle" >0 - 4</td><td align="center" valign="middle" >-</td></tr><tr><td align="center" valign="middle" >Detrital matrix</td><td align="center" valign="middle" >7 - 12</td><td align="center" valign="middle" >0 - 10</td></tr><tr><td align="center" valign="middle" >Cement</td><td align="center" valign="middle" >8 - 16</td><td align="center" valign="middle" >10 - 26</td></tr><tr><td align="center" valign="middle" >Qz/F</td><td align="center" valign="middle" >4 -</td><td align="center" valign="middle" >7 - 99</td></tr><tr><td align="center" valign="middle" >Heavy minerals</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" >Zircon</td><td align="center" valign="middle" >48 - 81</td><td align="center" valign="middle" >14 - 61</td></tr><tr><td align="center" valign="middle" >Tourmaline</td><td align="center" valign="middle" >4 - 33</td><td align="center" valign="middle" >13 - 76</td></tr><tr><td align="center" valign="middle" >Rutile</td><td align="center" valign="middle" >13 - 22</td><td align="center" valign="middle" >3 - 25</td></tr><tr><td align="center" valign="middle" >Anatase, Brookite</td><td align="center" valign="middle" >2 - 4</td><td align="center" valign="middle" >3 - 6</td></tr><tr><td align="center" valign="middle" >Epidote (aggreg.)</td><td align="center" valign="middle" >0 - 1</td><td align="center" valign="middle" >0 - 3</td></tr><tr><td align="center" valign="middle" >Opaque</td><td align="center" valign="middle" >0 - 1</td><td align="center" valign="middle" >0 - 3</td></tr><tr><td align="center" valign="middle"  rowspan="6"  >Cement minerals</td><td align="center" valign="middle" >Quartz syntaxial overgrowth</td><td align="center" valign="middle" >Quartz syntaxial overgrowth</td></tr><tr><td align="center" valign="middle" >Kaolinite</td><td align="center" valign="middle" >Calcite, dolomite</td></tr><tr><td align="center" valign="middle" >Illite/smectite mixed l.</td><td align="center" valign="middle" >kaolinite</td></tr><tr><td align="center" valign="middle" >Hematite</td><td align="center" valign="middle" >Hematite</td></tr><tr><td align="center" valign="middle" >Chlorite</td><td align="center" valign="middle" >Chlorite</td></tr><tr><td align="center" valign="middle" >Kaol./Ill. = 2.5</td><td align="center" valign="middle" >Kaol./Ill. = 7.3</td></tr></tbody></table></table-wrap><p>The ferruginous glaebule/pisolite-bearing kaolinite paleosol exposes desiccation features [<xref ref-type="bibr" rid="scirp.118251-ref12">12</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref17">17</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref28">28</xref>], (<xref ref-type="fig" rid="fig9">Figure 9</xref>(c)). The data demand short-term atmospheric hazards (days, weeks) for building up the FUCs; however, 10<sup>3</sup> - 10<sup>4</sup> a for paleosol formation. So the architectural cyclicity of FUCs was accompanied by a cyclic tropical → arid climate change (FUC → DUP).</p><p>Striking trace elements concentrations were analyzed in pelite (Ba, Co, Ni, Sr, Y, Zn, Zr, B, Sc, V) in paleosol (Ba, Co, Cu, Ni, Sr, Zr, B, Sc, V) and in Fe-glaebules (Co, Cu, Ni, Be, Zn, Sc, V, Cr, Li) (<xref ref-type="table" rid="table2">Table 2</xref>).</p><p>Of special interest are mm/cm-thick white-grey shaly/silty tuff-suspicious beds, always overlying the paleosols and overlain itself by the next FUC ( [<xref ref-type="bibr" rid="scirp.118251-ref17">17</xref>], <xref ref-type="fig" rid="fig1">Figure 1</xref>0), unfortunately not analyzed.</p><table-wrap id="table2" ><label><xref ref-type="table" rid="table2">Table 2</xref></label><caption><title> Major elements and trace elements of pelite and paleosol [<xref ref-type="bibr" rid="scirp.118251-ref28">28</xref>] and glaebules of the Um Irna F. [<xref ref-type="bibr" rid="scirp.118251-ref17">17</xref>]</title></caption><table><tbody><thead><tr><th align="center" valign="middle" >Major elements %</th><th align="center" valign="middle" >Pelite [<xref ref-type="bibr" rid="scirp.118251-ref28">28</xref>]</th><th align="center" valign="middle" >Paleosol [<xref ref-type="bibr" rid="scirp.118251-ref28">28</xref>]</th><th align="center" valign="middle" >Fe-Glaebules [<xref ref-type="bibr" rid="scirp.118251-ref17">17</xref>]</th></tr></thead><tr><td align="center" valign="middle" >SiO<sub>2</sub></td><td align="center" valign="middle" >50.48</td><td align="center" valign="middle" >50.00</td><td align="center" valign="middle" >18.9 - 29.0</td></tr><tr><td align="center" valign="middle" >Al<sub>2</sub>O<sub>3</sub></td><td align="center" valign="middle" >26.72</td><td align="center" valign="middle" >26.07</td><td align="center" valign="middle" >6.1 - 11.2</td></tr><tr><td align="center" valign="middle" >CaO</td><td align="center" valign="middle" >0.22</td><td align="center" valign="middle" >0.06</td><td align="center" valign="middle" >0.14 - 0.18</td></tr><tr><td align="center" valign="middle" >TiO<sub>2</sub></td><td align="center" valign="middle" >1.25</td><td align="center" valign="middle" >0.39</td><td align="center" valign="middle" >0.60 - 0.89</td></tr><tr><td align="center" valign="middle" >Na<sub>2</sub>O</td><td align="center" valign="middle" >0.21</td><td align="center" valign="middle" >0.18</td><td align="center" valign="middle" >0.05 - 0.07</td></tr><tr><td align="center" valign="middle" >K<sub>2</sub>O</td><td align="center" valign="middle" >3.22</td><td align="center" valign="middle" >0.09</td><td align="center" valign="middle" >0.19 - 0.29</td></tr><tr><td align="center" valign="middle" >MgO</td><td align="center" valign="middle" >1.11</td><td align="center" valign="middle" >0.04</td><td align="center" valign="middle" >0.16 - 0.31</td></tr><tr><td align="center" valign="middle" >Fe<sub>2</sub>O<sub>3</sub></td><td align="center" valign="middle" >7.07</td><td align="center" valign="middle" >14.75</td><td align="center" valign="middle" >54.9 - 67.8</td></tr><tr><td align="center" valign="middle" >MnO</td><td align="center" valign="middle" >0.01</td><td align="center" valign="middle" >0.01</td><td align="center" valign="middle" >0.01 - 0.14</td></tr><tr><td align="center" valign="middle" >P<sub>2</sub>O<sub>5</sub></td><td align="center" valign="middle" >0.04</td><td align="center" valign="middle" >0.16</td><td align="center" valign="middle" >0.03 - 0.04</td></tr><tr><td align="center" valign="middle" >L. O. I.</td><td align="center" valign="middle" >12.88</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >4.40 - 7.50</td></tr><tr><td align="center" valign="middle" >Total</td><td align="center" valign="middle" >100</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >99.33 - 100.77</td></tr><tr><td align="center" valign="middle" >Trace elements (ppm)</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" >Ba</td><td align="center" valign="middle" >77</td><td align="center" valign="middle" >798</td><td align="center" valign="middle" >-</td></tr><tr><td align="center" valign="middle" >Co</td><td align="center" valign="middle" >30</td><td align="center" valign="middle" >18</td><td align="center" valign="middle" >14 - 68</td></tr><tr><td align="center" valign="middle" >Cu</td><td align="center" valign="middle" >3</td><td align="center" valign="middle" >12</td><td align="center" valign="middle" >5 - 16</td></tr><tr><td align="center" valign="middle" >Ni</td><td align="center" valign="middle" >74</td><td align="center" valign="middle" >30</td><td align="center" valign="middle" >65 - 134</td></tr><tr><td align="center" valign="middle" >Sr</td><td align="center" valign="middle" >60</td><td align="center" valign="middle" >97</td><td align="center" valign="middle" >-</td></tr><tr><td align="center" valign="middle" >Y</td><td align="center" valign="middle" >78</td><td align="center" valign="middle" >7</td><td align="center" valign="middle" >-</td></tr><tr><td align="center" valign="middle" >Be</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >6 - 16</td></tr><tr><td align="center" valign="middle" >Zn</td><td align="center" valign="middle" >74</td><td align="center" valign="middle" >23</td><td align="center" valign="middle" >41 - 131</td></tr><tr><td align="center" valign="middle" >Zr</td><td align="center" valign="middle" >604</td><td align="center" valign="middle" >230</td><td align="center" valign="middle" >-</td></tr><tr><td align="center" valign="middle" >B</td><td align="center" valign="middle" >1388</td><td align="center" valign="middle" >506</td><td align="center" valign="middle" >-</td></tr><tr><td align="center" valign="middle" >Sc</td><td align="center" valign="middle" >22</td><td align="center" valign="middle" >15</td><td align="center" valign="middle" >25 - 30</td></tr><tr><td align="center" valign="middle" >V</td><td align="center" valign="middle" >198</td><td align="center" valign="middle" >222</td><td align="center" valign="middle" >678 - 1020</td></tr><tr><td align="center" valign="middle" >Cr</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >109 - 300</td></tr><tr><td align="center" valign="middle" >Li</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >24 - 74</td></tr><tr><td align="center" valign="middle" >Rb</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >3 - 9</td></tr></tbody></table></table-wrap><p>P-T Transitional Zone at Wadi Bassat En Nimra ( [<xref ref-type="bibr" rid="scirp.118251-ref28">28</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref30">30</xref>], <xref ref-type="fig" rid="fig3">Figure 3</xref>)</p><p>The upper most 20 m of the carbonate-free Um Irna F. comprise five paleosol-bearing cycles; however, in total some 15 - 20 minor hazardous FUCs of varying transport energy and completion without paleosolsunits. The last paleosol bed is overlain with the next flash flood deposit comprising reworked paleosol pebbles (Sm → Fm).</p><p>The overlying 10 - 12 m thick more or less laminated shaly/marly red-colored clastics (subarkosic sandstone) of the Himara M. increasingly becomes calcite-indurated indicating a rising pH (&gt;7) and the transition from continental swamp via supra- to intertidal environments during the transgressive System Tract (TST) providing diachronous lithofacies boundaries (<xref ref-type="fig" rid="fig1">Figure 1</xref>1).</p><p>The following sequence (~10 m) is characterized by a burrowing ichnofacies, the first appearance of glauconite (K, Mg, (Fe<sup>2+</sup>, Fe<sup>3+</sup>, Al). (SiO<sub>3</sub>)<sub>6</sub>∙3H<sub>2</sub>O), increasing carbonate cement and preserved unstable heavy minerals: hornblende, epidote, garnet [<xref ref-type="bibr" rid="scirp.118251-ref30">30</xref>], (<xref ref-type="table" rid="table1">Table 1</xref>). Glauconite represents a typical intertidal transformation from detrital biotite under defined Eh/pH conditions (<xref ref-type="fig" rid="fig1">Figure 1</xref>2).</p><p>Obviously, there doesn’t appear any hint on a hiatus or an abrupt change of sediment architecture across this transition zone.</p><p>The next overlying 10 m built up with grey shaly/sandy clastics, ichnofacies-free, interbedded with shell lags, culminate in two limestone beds (wackestone) 0.2 resp. 0.5 m thick. They contain conodonts and euryhaline foraminifera of early Induan age in a shallow environment of the Nimra M. ( [<xref ref-type="bibr" rid="scirp.118251-ref12">12</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref16">16</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref23">23</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref24">24</xref>], <xref ref-type="fig" rid="fig3">Figure 3</xref>, <xref ref-type="fig" rid="fig1">Figure 1</xref>1).</p><p>A rich ichnofacies assemblage (Phycodes, Diplocraterion, Rusophycos, Rhizocorallium) characterizes the overlying sequenceof intertidal/supratidal dolomite (dolo-arenite) of the Dardur M. Algal lamination and pseudomorphs after sulfate neomorphism indicate coastal sabkha conditions [<xref ref-type="bibr" rid="scirp.118251-ref12">12</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref28">28</xref>]. Siliciclastic intercalations mostly consolidated by carbonate cement, may be interpreted as tailing or continued continental input.</p><p>With regard to the thin tuff-suspicious beds intercalated in the Um Irna F. [<xref ref-type="bibr" rid="scirp.118251-ref31">31</xref>], similar deposits in the Dardur M. cause high interest for interpretation [<xref ref-type="bibr" rid="scirp.118251-ref28">28</xref>].</p><p>Finally stated, the P-T transitional zone exposes a hiatus-free diachronous lithofacies transition at Wadi Bassat en Nimra throughout a tropical/arid flash flood/paleosol scenery to a shallow marine environment during a TST.</p><p>The P-T transition covers both Khuff B and Khuff A of the Saudi-Arabian Shelf, at least between the MFSs P40 (254 Ma) and Tr 30 (249.75 Ma) to be discussed below [<xref ref-type="bibr" rid="scirp.118251-ref14">14</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref15">15</xref>] <xref ref-type="fig" rid="fig1">Figure 1</xref>3). Comprising in connection with the Siberian LIP degassing a total time-span of 4.25 Ma, the P-T main pulse, however, concerns the interval 252.3 - 251.3 Ma [<xref ref-type="bibr" rid="scirp.118251-ref26">26</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref32">32</xref>].</p><p>It has become obvious that the humid/tropical Um Irna flash flood events correlate on the Arabian Shelf (Khuff B) with a MFS; accordingly long term paleosol formation (up to several 10<sup>4</sup> a) coincides with a SB.</p><p>For a broader understanding of global effects by Siberian LIP degassing, additional data from Central Europe are useful [<xref ref-type="bibr" rid="scirp.118251-ref33">33</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref34">34</xref>].</p></sec><sec id="s3"><title>3. Comparison of the P-T Transitional Data with Those of the Germanic Basin/Central Europe ( [<xref ref-type="bibr" rid="scirp.118251-ref32">32</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref33">33</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref34">34</xref>], Figures 14-16)</title><p>The Upper Permian Zechstein F. of Central Europe comprises seven main evaporate/siliciclastic cycles [<xref ref-type="bibr" rid="scirp.118251-ref33">33</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref34">34</xref>]. Most relevant for correlation with the Jordanian Um Irna/Himara M. transitional zone is the upper most cycle (Fulda F.: z 7, <xref ref-type="fig" rid="fig1">Figure 1</xref>5). The latter owns an intraformational unconformity (~251.5 Ma) and is overlain with the Calv&#246;rde F. built up with ten minor FUCs and the Bernburg F. both Lower Buntsandstein. Thereby, the commonly assigned “PTB” (~251 Ma) is to be placed ~0.2 Ma above the isochronous lithostratigraphicZechstein/Buntsandstein boundary [<xref ref-type="bibr" rid="scirp.118251-ref33">33</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref34">34</xref>].</p><p>With regard to the outrunning volcanic activity, we correlate the Lower Fulda/ Upper Fulda F. unconformity of the Hessian Depression ( [<xref ref-type="bibr" rid="scirp.118251-ref34">34</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref35">35</xref>], <xref ref-type="fig" rid="fig1">Figure 1</xref>5) with the Lower/Upper M. unconformity of the Um Irna F. (<xref ref-type="fig" rid="fig4">Figure 4</xref>). In both cases re-organization of the near-located source areas and change of sediment transport direction took place.</p><p>Around the “PTB” a general trend from evaporiticsabkha to playa facies developed in the Germanic Basin while on the Jordanian Platform hazardous atmospheric events caused cyclic flash flooding (super cyclones) under tropical climatic conditions with subsequent drying upward paleosol formation by increasing aridity (5 major cycles, 20 minor cycles). On the Arabian Shelf the Khuff Cycles B, A dominates this time-span (<xref ref-type="fig" rid="fig1">Figure 1</xref>3).</p><p>Based on tectonic quiescence, the Zechstein/Buntsandsteinlithofacies boundary appears as isochronous which is well documented across the Helgoland Basin, North Sea ( [<xref ref-type="bibr" rid="scirp.118251-ref36">36</xref>], <xref ref-type="fig" rid="fig1">Figure 1</xref>6), while the Um Irna/Ma’in F. boundary at Wadi Bassat en Nimra, Jordan exposes a hiatus-free continental/marine transitional sequence during transgression, however, of diachronous character.</p><p>The Calv&#246;rde F. (10 minor FUCs: <xref ref-type="fig" rid="fig1">Figure 1</xref>5: each 100 kyr) that can be reliably traced across Central Europe (Netherlands–Poland), was very probably directed by perturbation cycles of Milankovitch origin [<xref ref-type="bibr" rid="scirp.118251-ref3">3</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref4">4</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref37">37</xref>]. Thereby, a few calcoolite interrelations in the siliciclastic cycles indicate short-term playa conditions.</p><p>High resolution geochemical analysis of the siliciclastic minor cycles from the cored Wulften-1 borehole, NE Hessian Depression [<xref ref-type="bibr" rid="scirp.118251-ref34">34</xref>] provides significantly high concentrations of toxic metals (As, Co, Cu, Pb, Zn, et al.) hosted in grey colored pelite beds of the Fulda F. (z 6, z 7, z 7 low/z 7 up, z 7 top) as well as through the Calv&#246;rde F. (c 2, c 7, c 8; <xref ref-type="fig" rid="fig1">Figure 1</xref>7). These thin white-grey-greenish pelite beds challenge an interpretation of tuff layers, as also encountered overlying paleosols in Wadi Himara, Jordan [<xref ref-type="bibr" rid="scirp.118251-ref17">17</xref>]. Are they really tuffs sourced in Siberian LIP degassing?</p><p>Astronomical tuning by spectral gamma ray logs of the P-T transitional zone through marine hiatus-free sections in S China [<xref ref-type="bibr" rid="scirp.118251-ref37">37</xref>] and integrated magnetostratigraphic scaling of climate cycles [<xref ref-type="bibr" rid="scirp.118251-ref38">38</xref>] in the Germanic Basin [<xref ref-type="bibr" rid="scirp.118251-ref33">33</xref>] provide substage boundary ages of the Lower Triassic relative to an assigned 251.902 &#177; 0.024 Ma age of the PTB [<xref ref-type="bibr" rid="scirp.118251-ref39">39</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref40">40</xref>] and for recurrent carbon isotope excursions through the Early Triassic.</p><p><xref ref-type="fig" rid="fig1">Figure 1</xref>8 shows high resolution ∂<sup>13</sup>C fluctuations based on conodont biostratigraphy from Early Triassic shallow marine carbonate to rocks of the Musandam Peninsula/United Arab Emirate [<xref ref-type="bibr" rid="scirp.118251-ref40">40</xref>] for finding approach to the Jordanian Platform, Arabian Plate, NGondwana.</p><p>Here we apply the substage boundary data of Li et al. [<xref ref-type="bibr" rid="scirp.118251-ref37">37</xref>] and the sequence analytical data (MFSs, SBs: [<xref ref-type="bibr" rid="scirp.118251-ref14">14</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref15">15</xref>]) for further evaluation in connection with the Siberian LIP magmatism [<xref ref-type="bibr" rid="scirp.118251-ref26">26</xref>].</p></sec><sec id="s4"><title>4. The Siberian LIP: Implications to Climate and Sedimentary Geology across the P-T Transition Zone (Jordanian Platform, Intercontinental Germanic Basin)<sup> </sup></title><p>For tracing the influence of the Siberian LIP on the target areas in Jordan and Central Europe, the following compiled age and petrologic data are highly appreciated [<xref ref-type="bibr" rid="scirp.118251-ref26">26</xref>].</p><p>&#173; The track of Siberian for the period 260 - 240 Ma is anchored at the head of the TazovskaGuba (TG in <xref ref-type="fig" rid="fig1">Figure 1</xref>9) and changes through an angle of 70˚ at 250 Ma by a six fold increase in rate of plate movement [<xref ref-type="bibr" rid="scirp.118251-ref8">8</xref>].</p><p>&#173; The Tungaska basin itself hosts the main Siberian Trap Basalt sequence (Central Basalt Flow) owning a volume of ~2.5 M∙km<sup>3</sup>. However, most recent investigations document an additional spread of magmatic rock volume (~20%) across the Taimyr Belt, the Yenisei/Khatanga Trough, and the Maymecha/Kotny area, so covering in total ~5 Mm<sup>3</sup> recovered by outcropping, sedimentary imaged and by drilling ( [<xref ref-type="bibr" rid="scirp.118251-ref26">26</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref41">41</xref>], <xref ref-type="fig" rid="fig2">Figure 2</xref>0).</p><p>&#173; The main pulse of volcanic/subvolcanic activity covers the time span 252.3 - 251.3 &#177; 0.11 Ma based on the first high precision U-Pb zircon geochronology [<xref ref-type="bibr" rid="scirp.118251-ref39">39</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref42">42</xref>]. The basalt flows of both Taimyr Peninsula and Tunguska Basin show a synchronicity of ~100.000 a error bar.</p><p>&#173; During increasing exploration it has become obvious that the magmatic spectrum comprises–apart from tholeiitic flood basalts-a broad variety of alkaline (ultra)-mafic to felsic intrusive complexes, layered intrusive bodies, plutons, sill, and dykes [<xref ref-type="bibr" rid="scirp.118251-ref26">26</xref>]. So the magmatites of the Yenisei/Khataga Trench reveal syenite, granite, quartz-syenite, carbonatite, and monzo-syenite, partly displaying crustal assimilation while alkaline lavas ascended rapidly without crustal interaction. Accordingly, trace elements assemblage dissolved in magmatic gas is expected to be exceptionally high.</p><p>&#173; In the Siberian LIP commonly tholeiites build up the lower portion of the lava pile intruded and penetrated by the scarcely younger alkaline rocks in the Maymecha/Kotny area. The latter exposes a broad petrochemical composition (12 distinct geochemical lava units in the Norilsk region). Alkaline series include trachy-dacite with evolved composition (&gt;60% SiO<sub>2</sub>).</p><p>&#173; A final emplacement of monzo-diorite (250.8 - 250.4 Ma) associates with the main Siberian main rock suite.</p><p>&#173; Trachyte tuff (251.904 &#177; 0.061 Ma) and trachy-rhyodacite tuff (251.483 &#177; 0.088 Ma) are known from the Delkansky F. [<xref ref-type="bibr" rid="scirp.118251-ref39">39</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref41">41</xref>]. Other ash beds yield an U-Pb zircon age of 251.22 &#177; 0.02 Ma) [<xref ref-type="bibr" rid="scirp.118251-ref42">42</xref>] resp. 250.55 &#177; 0.51 Ma [<xref ref-type="bibr" rid="scirp.118251-ref43">43</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref44">44</xref>].</p><p>&#173; Apart from primary magmatic gas, there are additional drivers for atmospheric implications like a) (CO<sub>2</sub> and CH<sub>4</sub> (100.000 Gt) via contact metamorphism with organic-rich and petroleum-bearing Paleozoic sedimentary rocks around sill intrusions (1.6 M∙km<sup>2</sup>) in the Tunguska Basin plus 20% of subvolcanic intrusions in both Taimyr and Yenisei/Khatanga area [<xref ref-type="bibr" rid="scirp.118251-ref45">45</xref>], and b) primary CH<sub>4</sub> sourced in the Lower Mantle [<xref ref-type="bibr" rid="scirp.118251-ref46">46</xref>].</p><p>&#173; Alkaline rocks of the Taimyr Fold Belt were previously dated by <sup>40</sup>Ar-<sup>39</sup>Ar, U-Pb secondary ion mass spectrometry on between 249 - 230 Ma and interpreted as tailings of the main Siberian LIP [<xref ref-type="bibr" rid="scirp.118251-ref47">47</xref>]. However, none of these rocks were dated by high precision U-Pb zircon geochronology; so uncertainties are large and data questionable.</p><p>&#173; Since depending on the petrochemical magma variety, its origin and ascent through mantle and crust rocks suits, a broad spectrum of volatiles including toxic metals dissolved, are expected to have massive influence on atmosphere, hydrosphere, rock mineralogy, and biosphere [<xref ref-type="bibr" rid="scirp.118251-ref48">48</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref49">49</xref>].</p><p>The most important magmatic gases are H<sub>2</sub>O, (35 - 90 Mol-%), CO<sub>2</sub> (5% - 50%), SO<sub>2</sub> (2% - 30%), HCl and HF [<xref ref-type="bibr" rid="scirp.118251-ref50">50</xref>]. Gas compound in magma and time of gasemanation during ascend depend on the silicate melt composition. Accordingly, because of low viscosity basaltic melts have a fast ascent through mantle and crust while SiO<sub>2</sub> richer melts may differentiate and react with the rock column [<xref ref-type="bibr" rid="scirp.118251-ref26">26</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref45">45</xref>].</p><p>Many elements dissolved in magmatic gas are precipitated as chloride (Na, K, NH<sub>4</sub>, Ca, Pb, Mn, Fe), fluoride (Na, Mg) nitride (Fe), sulfate (S, Se, As, Pb, Cu, Co, Hg, Zn, Fi, Ni), oxide (Mg. Cu, Pb, B) and arsenide (Fe, Co, Ni) during cooling down and reaction with the atmosphere [<xref ref-type="bibr" rid="scirp.118251-ref51">51</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref52">52</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref53">53</xref>].</p><p>Most relevant for correlation attempts to both target areas (Jordan, Germanic Basin) are the geochemical data available from borehole W&#252;lften-1, Hessian Depression ( [<xref ref-type="bibr" rid="scirp.118251-ref33">33</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref34">34</xref>], <xref ref-type="fig" rid="fig7">Figure 7</xref>) with a main focus on As, Co and Cu-minerals (AsS, As<sub>2</sub>S<sub>3</sub>, Cu<sub>3</sub>AsS<sub>4</sub>, (Cu, Fe, Zn), As<sub>2</sub>S<sub>3</sub>, FeAsS, CoAsS, CoAs<sub>2-3</sub>, Co<sub>3</sub>S<sub>4</sub>, CuS, CuO [<xref ref-type="bibr" rid="scirp.118251-ref51">51</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref53">53</xref>]. During weathering primary As, Cu-minerals react with O<sub>2</sub>to arsenolite/claudetite (As<sub>2</sub>O<sub>3</sub>), i.e. 2FeAsS + 5O<sub>2 </sub>→ Fe<sub>2</sub>O<sub>3</sub> + 2SO<sub>2</sub>+ As<sub>2</sub>O<sub>3</sub> [<xref ref-type="bibr" rid="scirp.118251-ref53">53</xref>].</p><p>Arsenolite represents itself as a white/grey powder that may influence the color of tuff deposits which already carried the primary As, Co-minerals to the depositional site.</p><p>Indeed the thin grey pelite beds intercalated between paleosol and the next FUC of the Um Irna F. ( [<xref ref-type="bibr" rid="scirp.118251-ref17">17</xref>] <xref ref-type="fig" rid="fig1">Figure 1</xref>0) and the color change (red-grey) at the Himara/Nimra M. boundary as well as the so-called “grey beds” intercalated through the P-T transition zone in the W&#252;lften-1 borehole ( [<xref ref-type="bibr" rid="scirp.118251-ref34">34</xref>], <xref ref-type="fig" rid="fig1">Figure 1</xref>7) would verify a correlation with explosive Siberian LIP-events. They would represent synchronous markers in contrast to the diachronounslithofacies/ichnofacies that migrated southward during Tethys transgression as an intermittent event between arid paleosol formation and the next flash flood (humid tropical climate).</p><p>The grey beds (tuff, ash?) generally relate to pelite and frequently to base resp. top of cycles (z 4 - 7, c 1 - 10) while the minor sandstone cycles in the W&#252;lften-1 drill core appear asymmetrically within one cycle showing a steep ascent and a flat descent from base to top.</p><p><xref ref-type="table" rid="table3">Table 3</xref> exposes more or less striking concentrations of elements relevant in the exhalative phase of magmatism [<xref ref-type="bibr" rid="scirp.118251-ref51">51</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref52">52</xref>] through the P-T transitional zone [<xref ref-type="bibr" rid="scirp.118251-ref17">17</xref>]. A few analytical data from the Um Irna F. are added (comp. <xref ref-type="table" rid="table2">Table 2</xref>). With regard to volatiles, i.e. As concentrations vary by 50 - 100 ppm in pelite of the Wulften-1 drill core, B varies between 506 - 1388 ppm in pelite and paleosol of the Um Irna F.</p><p>Furthermore, there is evidence for crustal assimilation by Ba, Rb, Th, K, Rb, Ta, Nb, Ce and Sn [<xref ref-type="bibr" rid="scirp.118251-ref54">54</xref>] while subalkaline rocks show a petrogenetic origin from a rather primitive mantle source and a plausible crustal overprint with intrusion temperatures of 915˚C - 1080˚C [<xref ref-type="bibr" rid="scirp.118251-ref52">52</xref>].</p><p>Primary crystals enclosed in ascending magma and originated in the deeper mantle, comprise droplets of the gas intrusions (“frozen Glass”). The latter show</p><table-wrap id="table3" ><label><xref ref-type="table" rid="table3">Table 3</xref></label><caption><title> As, co minerals of the exhalative, hydrothermal and oxidation phase [<xref ref-type="bibr" rid="scirp.118251-ref51">51</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref53">53</xref>]</title></caption><table><tbody><thead><tr><th align="center" valign="middle" >Metal arsenides</th><th align="center" valign="middle" >Arsenic sulfides</th><th align="center" valign="middle" >Elemental arsenic</th><th align="center" valign="middle" >Arsenic oxide</th></tr></thead><tr><td align="center" valign="middle" >Arsenopyrite (FeAsS)</td><td align="center" valign="middle" >Realgar (As<sub>4</sub>S<sub>4</sub>) Auripiment (As<sub>2</sub>S<sub>3</sub>)</td><td align="center" valign="middle" >Arsenic (As), (with strong acids → Arsenic acid)</td><td align="center" valign="middle" >Arsenolite (As<sub>2</sub>O<sub>3</sub>), → (weathering product)</td></tr><tr><td align="center" valign="middle" >Glanzcobalt (CoAsS)</td><td align="center" valign="middle" >Proustite (Ag<sub>3</sub>AsS<sub>3</sub>)</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" >Arsennickl (NiAsS)</td><td align="center" valign="middle" >Enargite (Cu<sub>3</sub>AsS<sub>4</sub>)</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" >L&#246;llingite (FeAs<sub>2</sub>)</td><td align="center" valign="middle" >Tennantite (Cu, Fe, Zn As<sub>2</sub>S<sub>3</sub>)</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" >Chloantite (NiAs<sub>2-3</sub>)</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" >Rammelsbergite (NiAs<sub>1-2</sub>)</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" >Safflorite (CoAs<sub>2-3</sub>)</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" >Linnaeite Co<sub>3</sub>S<sub>4</sub></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr></tbody></table></table-wrap><p>high levels of sulfur, chlorine and fluorine such as: 0.51 wt-% S, 0.94 wt-% Cl, 1.95 wt-% F [<xref ref-type="bibr" rid="scirp.118251-ref48">48</xref>] passing Paleozoic sedimentary source rocks, coal and hydrocarbons [<xref ref-type="bibr" rid="scirp.118251-ref45">45</xref>].</p><p>Degassing from the Siberian LIP is estimated on ~6300 - 7800 Gt S, ~3400 - 8700 GtCl and ~7100 - 13,600 Gt F, injected into the atmosphere and resulting in atmospheric hazard, acid rain (“lemon juice”), ocean acidification and more or less unknown chemical impact on continental surface rocks for an unique deterioration in global scale [<xref ref-type="bibr" rid="scirp.118251-ref48">48</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref49">49</xref>].</p><p>The transfer of the eruptive gas/particle mixture took place from the magmatic source (including high amount of pre-eruptive origin from the magma chamber via troposphere (1/3 S) and stratosphere (1/2 S) to the depositional site [<xref ref-type="bibr" rid="scirp.118251-ref50">50</xref>].</p><p>Because of the lower located base of the atmosphere (7 - 10 km) in high latitude (as the Siberian LIP), the eruptive gas/particle column (up to 20 - 30 km) may faster reach the dry stratosphere [<xref ref-type="bibr" rid="scirp.118251-ref50">50</xref>]. Especially higher evolved magma may release eruptive column into the atmosphere to be carried away, within a few weeks, as a veil of some km in thickness. Thereby photochemical oxidation and reduction of SO<sub>2</sub> and H<sub>2</sub>S react with H<sub>2</sub>O to H<sub>2</sub>SO<sub>4</sub> droplets (diameter &lt; 1 mm) to remain up to ~3 a in the atmosphere prior to be settled on Earth [<xref ref-type="bibr" rid="scirp.118251-ref50">50</xref>].</p><p>As negative climate forcing, the effects of aerosol veils (H<sub>2</sub>SO<sub>4</sub>) and ash cause temperature decrease worldwide and ozone reduction (up to 70%) (<xref ref-type="fig" rid="fig2">Figure 2</xref>1); H<sub>2</sub>SO<sub>4</sub> reacts with NO<sub>x</sub> to HNO<sub>3</sub> and with inactive Cl-reservoirs of the Stratosphere (ClONO<sub>2</sub>, HCl) to reactive Cl and ClO that attacks the ozone layer (i.e. Pinatubo, 1991/92: 15% - 20% loss) [<xref ref-type="bibr" rid="scirp.118251-ref50">50</xref>].</p><p>Contrasting the negative climate forcing (−3.0 Wm<sup>2</sup>), greenhouse gases (CO<sub>2</sub>, CH<sub>4</sub>, FCKW, NO<sub>x</sub>) cause a temperature rise as positive climate forcing (+2.2 Wm<sup>2</sup> <xref ref-type="fig" rid="fig2">Figure 2</xref>1). Thus, there occurredan interplay of both through the time-span of the Siberian LIP (at least from 252.33 to 251.3 Ma without possible</p><p>precursor’s tailings!) which mainly directs the P-T transitional zone via climate change.</p></sec><sec id="s5"><title>5. Discussion and Conclusions: P-T Transitional Sedimentological/Mineralogical Patterns Meet Siberian LIP Degassing Effects</title><p>The main pulse (252.3 - 251.3 Ma) followed by recurrent magmatism (250.8 - 250.4 Ma) provides the framework for correlation relating to “indirect effects” of this LIP degassing via climate change. The total time-span covers the Zechstein F. Z7 (~2 Ma) and the Buntsandstein Calv&#246;rde F. (su C1-C7 (~0.7 Ma)) in the Germanic Basin [<xref ref-type="bibr" rid="scirp.118251-ref33">33</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref34">34</xref>] as well as part of the Khuff-Cycles B, A (~2.5 Ma) on the Arabian Plate [<xref ref-type="bibr" rid="scirp.118251-ref14">14</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref15">15</xref>]. Most of this period is characterized by normal magnetization [<xref ref-type="bibr" rid="scirp.118251-ref38">38</xref>].</p><p>In a broader sense the P-T transitional zone on the Arabian Plate is embedded between both MFSs P 40 (~254 Ma) and Tr10 (~250.5 Ma) covering in total more or less a SB time-span of ~3.5 Ma [<xref ref-type="bibr" rid="scirp.118251-ref14">14</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref15">15</xref>].</p><p>The onset of mass extinction was determined on 251.9 Ma [<xref ref-type="bibr" rid="scirp.118251-ref26">26</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref42">42</xref>] during magmatism in the Tunguska Basin. The foraminifera Cornuspiramabajeri encountered in the Nimra M. wackestone was interpreted as an opportunistic “disaster species” in a survival phase after mass extinction and prior tothe recovery phase [<xref ref-type="bibr" rid="scirp.118251-ref12">12</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref22">22</xref>]. This subject is in detail discussed on a micropaleontologic basis [<xref ref-type="bibr" rid="scirp.118251-ref20">20</xref>]. So the focus of faunal recovery is directed to the MFS Tr 10 (250.5 Ma), [<xref ref-type="bibr" rid="scirp.118251-ref14">14</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref15">15</xref>]. Thus, the following correlation attempts may be rich in meaning.</p><p>&#173; The lower/upper M. unconformity of the Um Irna F. may coincide with the unconformity of the Lower/Upper Fulda F., Germanic Basin, however questionable because of missing radiometric age data (~251 Ma).</p><p>&#173; A significant change of the mineral assemblage and Eh/pH conditions passing the Um Irna F./Himara M. transitional zone by changing sedimentary environment during transgression.</p><p>&#173; Similar lithofacies cycles in the Um Irna F. and in the Fulda F. Germanic Basin (humid tropical FUC → arid DUP).</p><p>&#173; Continuation of minor FUCs in the Lower Triassic Ma’in F. in the Buntsandstein Calv&#246;rde F. (Hessian Basin). The cycles of the latter F. can be precisely traced between Netherlands and Poland!</p><p>&#173; Parts of the Khuff Cycles B, A, Arabian Plate relate to the P-T transitional zone in Jordan.</p><p>&#173; The ?tuff/ash beds intercalated in the Siberian LIP suite, may partially correlate with the grey pelite beds in the Um Irna F. as well as in the drill core W&#252;lften-1, Germanic Basin. The colored column of the latter does promise a higher number of tuff-layers (<xref ref-type="fig" rid="fig1">Figure 1</xref>7).</p><p>&#173; Toxic metals (As, Co, Cu, Zn, Pb) analyzed in W&#252;lften-1 may be correlated to the exhalative phase of the Siberian LIP-Complex (<xref ref-type="fig" rid="fig1">Figure 1</xref>7 and <xref ref-type="fig" rid="fig1">Figure 1</xref>8).</p><p>&#173; Sequence-Analytical patterns (MFSs, SBs) and the Khuff Cycles B, A on the Arabian Platform may be correlated to the Substage Boundaries within the P-T transitional zone recovered via ∂<sup>13</sup>O excursions by astronomical tuning ( [<xref ref-type="bibr" rid="scirp.118251-ref37">37</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref40">40</xref>], <xref ref-type="fig" rid="fig1">Figure 1</xref>8).</p><p>&#173; Accepting the tuff-character of the thin grey pelite beds intercalated in the Um Irna F. sequence, Jordan between paleosol and overlying FUC (<xref ref-type="fig" rid="fig1">Figure 1</xref>0), one may assume initial tuff eruption from the Siberians LIP, followed by magmatic intrusion/effusion that brought atmospheric hazard and climate change by degassing , after a long period (10<sup>4</sup> a) of arid climate in low latitudes, Arabian Plate, to initiate the interplay of greenhouse gas effect, aerosols, ozon layer reduction and toxic metal’s impact onmarine (90%) and continental fauna extinction (70%) [<xref ref-type="bibr" rid="scirp.118251-ref40">40</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref49">49</xref>].</p><p>As astronomical tuning throughout the P-T transitional zone exhibits, Milankovitch-Croll cycles may play an important role in the Feed Back System on the Earth [<xref ref-type="bibr" rid="scirp.118251-ref37">37</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref54">54</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref55">55</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref56">56</xref>]. That concerns the following three perturbations:</p><p>&#173; The change of Sun-Earth distance by the ellipticity of the Earth’s orbit in 100.000 a cycles during which the solar input to the atmosphere may change by 30% of the current global average. This is shown in the case of the Lower Buntsandstein, Germanic Basin [<xref ref-type="bibr" rid="scirp.118251-ref33">33</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref34">34</xref>].</p><p>&#173; The obliquity of the Earth’s axis (21.8˚ - 24.4˚) cause cycles of 40.000 a.</p><p>&#173; The precession of the equinoxes affects the variation of the Sun-Earth distance causing solar irradiation (21.000 a cycles).</p><p>Both the latters are relevant for the time-span of drying upward paleosol formation throughout the Um Irna F., Jordan [<xref ref-type="bibr" rid="scirp.118251-ref17">17</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref28">28</xref>].</p><p>Furthermore, the Moon becomes relevant as an acting force in the Earth’s Feedback System [<xref ref-type="bibr" rid="scirp.118251-ref55">55</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref56">56</xref>]: from 290 to 220 Ma its recession rate exhibits a slowdown from 110.31 km/Ma to 50.76 km/Ma according to Kepler’s 3<sup>rd</sup> Planetary Law, accompanied by a sea level rise from −30 m (~250 Ma) to +75 m (~220 Ma) and a steep fall of the Earth’s magnetic field that meets a maximum sea level rise (<xref ref-type="fig" rid="fig2">Figure 2</xref>2), compare <xref ref-type="fig" rid="fig1">Figure 1</xref>8.</p><p><xref ref-type="table" rid="table4">Table 4</xref> evidences a temporal coincidence of the Moon’s recession rate and the spin angular velocity of the Earth with the Siberian LIP activity as well as with Upper Triassic impacting followed by the volcanism too [<xref ref-type="bibr" rid="scirp.118251-ref55">55</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref56">56</xref>].</p><p>Compiling the most important processes in the Earth’s feedback system applied to our subject [<xref ref-type="bibr" rid="scirp.118251-ref55">55</xref>].</p><table-wrap id="table4" ><label><xref ref-type="table" rid="table4">Table 4</xref></label><caption><title> Siberian LIP activity (252 - 250 Ma) and Upper Triassic impacting (219 - 214 Ma) followed by volcanism (202 - 201 Ma) temporarily relate to the Moon’s recession rate (km/Ma) and the spin angular velocity of Earth (days/month) [<xref ref-type="bibr" rid="scirp.118251-ref55">55</xref>]</title></caption><table><tbody><thead><tr><th align="center" valign="middle" >Ma</th><th align="center" valign="middle" >Moon’s recession rate (km/Ma)</th><th align="center" valign="middle" >Spin angular velocity of the Earth (days/month)</th></tr></thead><tr><td align="center" valign="middle" >153</td><td align="center" valign="middle" >18.66 volcanism impacting</td><td align="center" valign="middle" >30.15 deceleration</td></tr><tr><td align="center" valign="middle" >220</td><td align="center" valign="middle" >59.76 Siberian LIP</td><td align="center" valign="middle" >29.66 acceleration</td></tr><tr><td align="center" valign="middle" >290</td><td align="center" valign="middle" >110.31</td><td align="center" valign="middle" >30.16</td></tr></tbody></table></table-wrap><p>&#173; Earth’s rotation slowing down and Moon recession cause variations of the Earth Mantle rotation and relating motion of the Earth’s Core.</p><p>&#173; Earth’s magnetic field borne at the core/mantle boundary, provides in case of normal magnetization increased magmatic transport within convection cells in the mantle , developing plumes, high spreading rates of MORBs and relevant plate motion.</p><p>Consequences: Rising sea level, growing shelf areas, maximal magmatic emplacement up to ~10 Ma delaying after shelf development, long-lasting magmatic degassing.</p><p>Thus, rising sea level (TST), shelf development (tidal dissipation), normal magnetization during complete activity of the Siberian LIP (at least 2 Ma) are coupled with the opening of the Neo-Tethys, MORB activity, and the Siberian Plume event.</p><p>Further aspects of feedback systems with special regard to formation boundaries can be efficiently discussed by the creative compilations as by (i.e. [<xref ref-type="bibr" rid="scirp.118251-ref57">57</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref58">58</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref59">59</xref>] [<xref ref-type="bibr" rid="scirp.118251-ref60">60</xref>]).</p><p>Thus, it becomes evident: the more methods applied to the same subject the more we remove from “well-defined results” to “transitional zone data (“Unsch&#228;rfe” sensu AUTOPOIESIS [<xref ref-type="bibr" rid="scirp.118251-ref61">61</xref>]). It seems that abiotic processes in the fields of Geosciences may underlay similar principles as of Biology, characterized as follows:</p></sec><sec id="s6"><title>6. Closing Statement</title><p>“We do regard evolution as a structural drifting during continuous phylogenetic selection: there is no progress senso improvement of environmental use (exploitation) but merely the maintenance of adaption and autopoiesis (self-regulation) in a process where organism and environment remain in a lasting structural interplay”.</p><p>H. E. Maturana and F. J. Varela, Biologists [<xref ref-type="bibr" rid="scirp.118251-ref61">61</xref>], transl. Sch.</p><p>Applied to Geoscience:</p><p>We, the authors, regard Earth History and accordingly Formation Boundaries as a structural drifting during a more or less continuous unstable equipoise. There is no restrained process concerning the improvement of the state of matter, but merely the maintenance of physical/chemical adaption and self-regulation (autopoiesis) under continuously changing conditions.</p><p>Parameters like P, T, pH, and Eh play a dominant role in the dissolution, transformation, and neoformation of minerals and sedimentary rocks during cosmic influence, climate forcing by LIP degassing, metamorphism, and diagenesis. Substitution, polymorphy, isomorphy, disorder, paragenesis, and replacement represent an entertaining interplay in the crystal lattice scale.</p></sec><sec id="s7"><title>Acknowledgements</title><p>As the most important basics for the interpretation of the Siberian LIP effects on Sedimentary Geology/Mineralogy we especially appreciate the publications of B. S. Amireh, D. E. Augland et al., M. O. Clarkson et al., M. Hiete et al., and I. M. Makhlouf et al. We are grateful to Kjell Paris for digital support.</p></sec><sec id="s8"><title>Conflicts of Interest</title><p>The authors declare no conflicts of interest regarding the publication of this paper.</p></sec><sec id="s9"><title>Cite this paper</title><p>Schneider, W. and Salameh, E. (2022) The Permian-Triassic Transitional Zone: Jordan, Arabian Plate; Linked to Siberian Large Igneous Province and Neo-Tethys Breakup Degassing via Climate Forcing, Atmospheric Hazard and Metal Toxicity. Open Journal of Geology, 12, 472-503. https://doi.org/10.4236/ojg.2022.126023</p></sec></body><back><ref-list><title>References</title><ref id="scirp.118251-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">Walter Jens, W. (1987) Das A und das O. Die Offenbarung des Johannes. Radius Verlag, Stuttgart, 93 p.</mixed-citation></ref><ref id="scirp.118251-ref2"><label>2</label><mixed-citation publication-type="other" xlink:type="simple">Tollmann, A. and Tollmann, E. 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