245:
253:
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.
156:
178:
216:
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
173:
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
87:
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
252:
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
480:
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
191:
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.
427:
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
96:
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.
298:
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
244:
605:
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, «
628:
Diaz-Hernandez J.L. and
Sanchez-Navas A. (2016). Saharan dust outbreaks and iberulite episodes. Journal of Geophysical Research: Atmospheres 121, 7064-7078,
236:
content-RH, which determined that clean atmospheres (<5 μg•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.
586:
Low-level inversions over the tropical Pacific. Thermodynamic structure of the boundary layer and the above inversion moisture structure
256:
There is an additional process of atmospheric maturation of iberulites that, in detail, only happens on the smectite rind, by means of
310:, they must have been incorporated after the acid attack described above, probably simultaneously with the incorporation of sea salt.
476:: The basic structural feature of the phyllosilicates is the stack of three types of layers: the tetrahedral sheet is formed by SiO
198:
Fig. 5 Saharan dusty event occurring on August 15, 2005. Notice the change of direction of the plume towards the Cadiz Gulf.
283:
attack on the interlayer cations of the smectites, which would gradually destroy the octahedral and tetrahedral sheets of
507:
648:
532:
Characterization of complex mineral assemblages: implications for contaminant transport and environmental remediation
152:
and microorganisms. The iberulites eventually fall on the southern Iberian Peninsula, where they have been detected.
55:
geometry, consisting of well-defined mineral grains, together with non-crystalline compounds, structured around a
585:
248:
Fig. 7 Time evolution of the particulate matter / Time evolution of the relative humidity (RH) and temperature.
690:
669:
284:
155:
508:
Aportaciones sólidas a la atmósfera originadas por un incendio forestal en el ámbito mediterráneo
334:
8:
685:
396:
339:
106:
531:
644:
560:
The nature and tropospheric formation of iberulites: Pinkish mineral microspherulites
392:
344:
181:
Fig. 4 Number of iberulite episodes (pl= plume, SA= Source Area, RA= Reception Area).
36:
606:
400:
384:
134:
122:
28:
177:
138:
74:
20:
Fig. 1 Group of iberulites observed under SEM. The arrows show vortex position.
679:
395:); subaerial terrestrial volcanism is related with destructive plate margins
261:
257:
148:(MBL) of the Iberian-Moroccan Atlantic coast leads to the incorporation of
118:
114:
60:
329:
424:
349:
56:
32:
629:
408:
404:
324:
207:
194:
52:
16:
307:
67:
and pinkish color (Figs. 1-2), formed in the troposphere by complex
303:
295:
149:
110:
35:), finally falling to the Earth's surface. The name comes from the
388:
319:
291:
130:
102:
68:
664:
272:
126:
98:
64:
260:
and multiphase reactions producing sulfates as the result of
78:
Fig. 2 Aspect of several iberulites under optical microscope.
299:
211:
Fig. 6 Traces of waterdroplets during a Saharan dust event.
239:
185:
159:
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
Text is available under the Creative Commons Attribution-ShareAlike License. Additional terms may apply.