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Iberulite

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activity affecting the Iberian Peninsula, and only sporadically in spring. Based on the relation between iberulites and red rain events, as well as the morphologies and compositional attributes observed, an aqueous interphase hypothesis has been suggested as the unitary mechanism for tropospheric formation of iberulites. Interactions between water droplets and Saharan aerosols create complex hydrodynamic conditions causing the possibility of collisions (wake capture and front capture) that originate the "precursor water droplets" of the iberulites. The movement of these water droplets to lower tropospheric levels implies either simultaneous or consecutive processes such as coalescence, formation of vortex and downdraught. During this phase the iberulites acquire their spherical shape and internal structure (core and rind), although sometimes this shape can be distorted.
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formation of more or less aerosol-rich water droplets (or precursor water droplets ) (Fig. 6A). The aerosol contents, together with dissolved salts (detected in this sequence as whitish or shiny precipitates), would have gradually increased, finally producing a well-defined iberulite after desiccation (Fig. 6E). The passage of these Saharan dust outbreaks over the study site had a total mean duration of five days (Fig. 7). It was observed during this passage that the central day presented the highest air temperatures and PM
75: 195: 17: 208: 665: 440:: This is a mode of aerodynamic capture of a drop falling in the atmosphere. A large drop settling through smaller drops will sweep out a volume and their hydrodynamic flow fields interfere collecting aerosols/droplets with some efficiency by the wake, depending on size of drops and size of aerosols, being most efficient for large and giant aerosols due to high terminal velocity and cross-sectional area . 137:. The latter group of minerals could be the result of neoformations during the maturation process occurring in the atmosphere during the final stages of iberulite formation. It is striking that sulphates only appear in the periphery of the iberulites. Flight over areas with anthropogenic or natural (volcanic, as those of North Atlantic archipelagos) sulphur emissions probably adsorbs 383:: Sulfur and other gas emissions into the atmosphere from inside the Earth occur near volcanic areas. These emissions can come from both clearly visible (explosive) eruptions and from diffuse (or quiescent) emissions, and there is not a real consensus about the relative importance of the latter. At present, submarine volcanic emissions occur in the 559: 481:
tetrahedral and octahedral sheets, the layer will have no charge, or will have a net negative charge. If the layers are charged this charge is balanced by interlayer cations such as Na or K. In each case the interlayer can also contain water. The crystal structure is formed from a stack of layers interspaced with the interlayers.
452:: These refer to reactions involving components in different phases, and are a combination of simultaneous phase change and conversion of some materials into others. A general multiphase reaction generates three classes of fluxes: component mass sources, interphase mass transfer, interphase energy transfer. 190:
The general content of aerosols in the atmosphere of the southern Iberian Peninsula is clearly related to the evolution of aerosols arriving from North Africa. Monitoring of dry aerosol deposition using passive samplers determined the formation of iberulites in two periods of the year (Fig. 4). The
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Iberulites have as yet only been found in the southern Iberian Peninsula. This location is geographically close to North Africa and it is therefore influenced by the emissions of Saharan aerosols, which are the greatest contributor of particulate matter to the atmospheric global dust budget (Fig.
371:: heterogeneous mixture of reactive mineral phases. These complex associations are typically formed in nature and are characterized by high surface area, low abundance of metal oxyhydroxide phases, and organic materials that act as cementing agents or surface coatings of prominent mineral grains . 215:
Short episodes of wet deposition (more specifically red rains) were observed during Saharan dust outbreaks over the period 2004-2013. Monitoring of these episodes led to the obtaining of a sequence of droplet impacts (Fig. 6) corresponding to June 6, 2012. This sequence would have begun with the
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These microspherulites are mostly spherical in shape (roundness index=0.95), with 60-90 ÎĽm modal diameter, although some particles can be up to 200 ÎĽm in diameter. According to this roundness index, these microspherules are really elongated spheroids with two axes defined along a polar plane and
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Iberulites are linked to the evolution of high-dust air masses (plumes) which, originating in Saharan dust storms, are transported over the Iberian Peninsula and often across the eastern North Atlantic Ocean. These plumes occur in the warm season (May to September), as a result of anticyclone
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tetrahedra, and each tetrahedron shares three of its vertex oxygen atoms with other tetrahedra and in which the Al can substitute up to half the Si. The octahedral sheet is made up by the Al, Fe and Mg cations, in six-coordination with the O and OH anions. Depending on the composition of the
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main depositional period occurs throughout the summer, while the second appears as a minor peak in early spring. However, the formation of iberulites is more specifically related with Saharan dust outbreaks, or dust plumes (Fig. 5) occurring within these two defined periods.
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and a significant wave state. The marine boundary layer (MBL) over the Earth's oceans plays a critical role in regulating surface energy and moisture fluxes and in controlling the convective transfer of energy and moisture to the free atmosphere
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Composition can be determined by both X-ray diffraction (XRD) and electronic microscopy techniques (mainly SEM, EDX, HRTEM). Sections show that the body of iberulites can be divided into core and rind. The core is mainly formed by grains of
464:: This is the formation of new mineral species from previously existing ones through alteration of environmental conditions. The new minerals thus produced are therefore stable in the new conditions. 271:
attack on the minerals of the rind. This would lead to the rapid transformation of some primary minerals into products of atmospheric neoformation secondary minerals): the sulfates (mainly the
423:: This is defined as that part of the troposphere directly influenced by the presence of the ocean's surface. It reacts with little diurnal variability, is 1–2 km thick (3 km max), has a low 88:
typically presenting a depression or vortex. The presence of plant filaments in the atmosphere can distort these shapes and sizes. In any case, these are uncommon “giant” aerosol particles.
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found in the smectite rind would have a similar origin. If acid attack progresses further, the phyllosilicate grains would be completely destroyed, producing amorphous silica and releasing
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Tanaka T.Y. and Chiba M. (2006). A numerical study of the contributions of dust source regions to the global dust budget. Global Planetary Change 52, 88-104, «
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Diaz-Hernandez J.L. and Sanchez-Navas A. (2016). Saharan dust outbreaks and iberulite episodes. Journal of Geophysical Research: Atmospheres 121, 7064-7078,
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content-RH, which determined that clean atmospheres (<5 ÎĽg•m-3) with RH>65% do not present suitable conditions for iberulite formation.
232:) contents, whereas relative humidity decreased (RH). A relation was therefore established between monthly numbers of iberulite episodes and PM 643:
Pruppacher H. R. and Klett J. D. (1997). Microphysics of clouds and precipitation (2nd ed.). Dordrecht: Kluwer Academic Publishers. 954 pp.
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Low-level inversions over the tropical Pacific. Thermodynamic structure of the boundary layer and the above inversion moisture structure
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There is an additional process of atmospheric maturation of iberulites that, in detail, only happens on the smectite rind, by means of
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Fig. 5 Saharan dusty event occurring on August 15, 2005. Notice the change of direction of the plume towards the Cadiz Gulf.
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attack on the interlayer cations of the smectites, which would gradually destroy the octahedral and tetrahedral sheets of
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Characterization of complex mineral assemblages: implications for contaminant transport and environmental remediation
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and microorganisms. The iberulites eventually fall on the southern Iberian Peninsula, where they have been detected.
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geometry, consisting of well-defined mineral grains, together with non-crystalline compounds, structured around a
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Fig. 7 Time evolution of the particulate matter / Time evolution of the relative humidity (RH) and temperature.
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Aportaciones sólidas a la atmósfera originadas por un incendio forestal en el ámbito mediterráneo
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The nature and tropospheric formation of iberulites: Pinkish mineral microspherulites
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Fig. 4 Number of iberulite episodes (pl= plume, SA= Source Area, RA= Reception Area).
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Fig. 1 Group of iberulites observed under SEM. The arrows show vortex position.
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and pinkish color (Figs. 1-2), formed in the troposphere by complex
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and multiphase reactions producing sulfates as the result of
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Fig. 2 Aspect of several iberulites under optical microscope.
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Fig. 6 Traces of waterdroplets during a Saharan dust event.
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Fig. 3 Emissions and dry/wet deposition of aerosols.
677: 474:Tetrahedral, octahedral and interlayer sheets 536:Proceedings National Academy of Sciences USA 202: 144:onto the iberulite surface. Descent to the 91: 584:Kloesel, K. A. y Albrecht, B. A. (1989). « 31:(Fig. 1) that develop in the atmosphere ( 243: 206: 193: 176: 154: 73: 15: 558:DĂ­az-Hernández, J.L. y Párraga (2008) « 168: 678: 639: 637: 530:Berstch P. M. y Seaman J. C. (1999). « 624: 622: 620: 618: 616: 614: 580: 578: 576: 554: 552: 550: 548: 526: 524: 502: 500: 498: 240:Stages in the formation of iberulites 186:Saharan dust outbreaks and iberulites 630:https://doi.org/10.1002/2016JD024913 634: 13: 611: 573: 545: 521: 495: 14: 702: 657: 663: 564:Geochimica et Cosmochimica Acta 467: 455: 443: 431: 599: 414: 374: 362: 306:exoskeletons have no signs of 1: 506:DĂ­az-Hernández, J.L. (2000). 488: 42: 163: 39:where they were discovered. 7: 313: 275:) would be the product of H 10: 707: 133:, chlorides and amorphous 381:Volcanic sulfur emissions 287:creating mixed sulfates. 71:-water-gas interactions. 27:are a particular type of 355: 203:Iberulites and red rains 92:Compositional attributes 82: 590:Monthly Weather Review 249: 212: 199: 182: 160: 79: 21: 421:Marine boundary layer 247: 210: 197: 180: 158: 146:marine boundary layer 77: 19: 691:Atmospheric sciences 672:at Wikimedia Commons 450:Multiphase reactions 389:intraplate volcanism 169:Geographical setting 512:Estudios GeolĂłgicos 397:Convergent boundary 340:Red rain in Kerala 250: 213: 200: 183: 161: 80: 47:An iberulite is a 22: 668:Media related to 345:Saharan Air Layer 113:. The rind shows 37:Iberian Peninsula 698: 667: 651: 641: 632: 626: 609: 603: 597: 582: 571: 556: 543: 528: 519: 504: 482: 471: 465: 459: 453: 447: 441: 435: 429: 418: 412: 409:subduction zones 385:mid-ocean ridges 378: 372: 366: 29:microspherulites 706: 705: 701: 700: 699: 697: 696: 695: 676: 675: 660: 655: 654: 642: 635: 627: 612: 604: 600: 583: 574: 557: 546: 529: 522: 505: 496: 491: 486: 485: 479: 472: 468: 460: 456: 448: 444: 436: 432: 419: 415: 401:Plate tectonics 379: 375: 367: 363: 358: 316: 285:phyllosilicates 282: 278: 269: 265: 242: 235: 231: 227: 223: 219: 205: 188: 171: 166: 142: 123:montmorillonite 94: 85: 63:rind, only one 45: 12: 11: 5: 704: 694: 693: 688: 674: 673: 659: 658:External links 656: 653: 652: 633: 610: 598: 572: 544: 520: 493: 492: 490: 487: 484: 483: 477: 466: 454: 442: 430: 413: 387:, and also as 373: 369:Co-association 360: 359: 357: 354: 353: 352: 347: 342: 337: 332: 327: 322: 315: 312: 280: 276: 267: 263: 241: 238: 233: 229: 225: 221: 217: 204: 201: 187: 184: 170: 167: 165: 162: 140: 93: 90: 84: 81: 57:coarse-grained 49:co-association 44: 41: 9: 6: 4: 3: 2: 703: 692: 689: 687: 684: 683: 681: 671: 666: 662: 661: 650: 649:0-7923-4211-9 646: 640: 638: 631: 625: 623: 621: 619: 617: 615: 607: 602: 595: 591: 587: 581: 579: 577: 569: 565: 561: 555: 553: 551: 549: 541: 537: 533: 527: 525: 517: 513: 509: 503: 501: 499: 494: 475: 470: 463: 458: 451: 446: 439: 434: 426: 422: 417: 410: 406: 405:volcanic arcs 402: 398: 394: 390: 386: 382: 377: 370: 365: 361: 351: 348: 346: 343: 341: 338: 336: 333: 331: 328: 326: 323: 321: 318: 317: 311: 309: 305: 301: 297: 293: 288: 286: 274: 270: 259: 258:heterogeneous 254: 246: 237: 209: 196: 192: 179: 175: 157: 153: 151: 147: 143: 136: 132: 129:, as well as 128: 124: 121:(beidellite, 120: 116: 115:clay minerals 112: 108: 104: 100: 89: 76: 72: 70: 66: 62: 58: 54: 50: 40: 38: 34: 30: 26: 18: 601: 593: 589: 567: 563: 539: 535: 515: 511: 473: 469: 462:Neoformation 461: 457: 449: 445: 438:Wake capture 437: 433: 420: 416: 380: 376: 368: 364: 330:Mineral dust 289: 255: 251: 214: 189: 172: 145: 95: 86: 59:core with a 48: 46: 24: 23: 570:: 3883–3906 542:: 3350–3357 425:Bowen ratio 350:Troposphere 33:troposphere 686:Mineralogy 680:Categories 489:References 325:Dust storm 43:Definition 25:Iberulites 670:Iberulite 518:: 153–161 308:corrosion 164:Formation 119:smectites 117:, mainly 111:feldspars 596:: 87-101 393:hotspots 314:See also 304:biogenic 302:. Since 296:jarosite 150:sea salt 131:sulfates 107:dolomite 61:smectite 320:Aerosol 292:alunite 103:calcite 69:aerosol 647:  407:above 273:gypsum 228:>PM 220:and PM 135:silica 127:illite 125:) and 99:quartz 65:vortex 356:Notes 335:Plume 83:Shape 53:axial 51:with 645:ISBN 300:iron 290:The 174:3). 109:and 594:117 588:». 562:». 534:». 403:, ( 230:2.5 224:(PM 222:2.5 682:: 636:^ 613:^ 592:, 575:^ 568:72 566:, 547:^ 540:96 538:, 523:^ 516:56 514:, 510:. 497:^ 411:). 399:, 294:- 279:SO 266:SO 234:10 226:10 218:10 139:SO 105:, 101:, 608:» 478:4 428:. 391:( 281:4 277:2 268:4 264:2 262:H 141:2

Index


microspherulites
troposphere
Iberian Peninsula
axial
coarse-grained
smectite
vortex
aerosol

quartz
calcite
dolomite
feldspars
clay minerals
smectites
montmorillonite
illite
sulfates
silica
SO2
sea salt





heterogeneous
H2SO4
gypsum

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