Rain dust

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The leaves of this Schefflera show the dust marks left by rain dust (near Paris, France) Pluie saharienne sur Schlefflera 2.jpg
The leaves of this Schefflera show the dust marks left by rain dust (near Paris, France)
Air pollution often causes rain to leave stains of dust after it evaporates, in Monterrey, Mexico. Rain Dust in Plant.jpg
Air pollution often causes rain to leave stains of dust after it evaporates, in Monterrey, Mexico.

Rain dust or snow dust, traditionally known as muddy rain, red rain, or coloured rain, is a variety of rain (or any other form of precipitation) which contains enough mineral dust, from soils (particularly from deserts), for the dust to be visible without using a microscope.

Contents

History

The rain dust phenomenon was studied by Italian scientist Giuseppe Maria Giovene (1753–1837), who managed to correctly explain the phenomenon as early as 1803. On 7 March 1803, rain dust fell over Southern Italy's region Apulia. At that time, people believed that the rain was caused by the explosions of Italy's volcanoes Mount Vesuvius or Etna, or that it was due to the transport of matter coming from the sea floor and raised by vapor. Giuseppe Maria Giovene related the phenomenon to the wind which occurred prior to the rain event, and he came to the conclusion that the sand had come from Africa and that it had been pushed by the wind coming from south-east. [1] [2]

Geography

Rain dust is common in the Western and Southern Mediterranean, where the dust supply comes from the atmospheric depressions going through the northern part of North Africa. The main sources of desert dust reach the Iberian Peninsula and the Balearic Islands in the form of dust transported by wind or rain from the Sahara, Atlas Mountains in Morocco and Central Algeria. [3]

Mud rains are relatively frequent and had been increasing in early 1990s in the Mediterranean Basin. [4]

It also occurs in arid desert regions of North America such as west Texas or Arizona. It occasionally happens in the grasslands as it did in Bexar County, Texas on March 18, 2008.

Dust composition

The rain dust is very alkaline. [3] Some of the large particles contain mixtures of chemicals such as sulfate and sea salt (chiefly with sodium, chlorine and magnesium). Major minerals in order of decreasing abundance are: illite, quartz, smectite, palygorskite, kaolinite, calcite, dolomite and feldspars. [3] In Majorca a study finds that the size, by volume, 89% of the particles from rain dust fraction corresponded to silt (between 0.002 mm and 0.063 mm) and that there was virtually no clay sized particles (less than 0.29%). [5]

Importance

Blood/red rain

Rain dust is the most common cause of blood rain.

Red rain is however not always rain dust, see for example the Red rain in Kerala.

See also

Related Research Articles

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Desertification is a type of land degradation in drylands in which biological productivity is lost due to natural processes or induced by human activities whereby fertile areas become arid. It is the spread of arid areas caused by a variety of factors, such as overexploitation of soil as a result of human activity and the effects of climate change. Geographic areas most affected include the Sahel region in Africa, the Gobi Desert and Mongolia in Asia as well as parts of South America. Drylands occupy approximately 40–41% of Earth's land area and are home to more than 2 billion people.

<span class="mw-page-title-main">Sahara desert (ecoregion)</span> The ecology of the Sahara desert

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<span class="mw-page-title-main">Geography of Mauritania</span>

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<span class="mw-page-title-main">Dust storm</span> Meteorological phenomenon common in arid and semi-arid regions

A dust storm, also called a sandstorm, is a meteorological phenomenon common in arid and semi-arid regions. Dust storms arise when a gust front or other strong wind blows loose sand and dirt from a dry surface. Fine particles are transported by saltation and suspension, a process that moves soil from one place and deposits it in another.

<span class="mw-page-title-main">Sahara</span> Desert on the African continent

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<span class="mw-page-title-main">Sirocco</span> Mediterranean wind

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<span class="mw-page-title-main">Niter</span> Mineral form of potassium nitrate

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<span class="mw-page-title-main">Aeolian processes</span> Processes due to wind activity

Aeolian processes, also spelled eolian, pertain to wind activity in the study of geology and weather and specifically to the wind's ability to shape the surface of the Earth. Winds may erode, transport, and deposit materials and are effective agents in regions with sparse vegetation, a lack of soil moisture and a large supply of unconsolidated sediments. Although water is a much more powerful eroding force than wind, aeolian processes are important in arid environments such as deserts.

<span class="mw-page-title-main">Desert pavement</span> Type of desert earth surface

A desert pavement, also called reg, serir, gibber, or saï is a desert surface covered with closely packed, interlocking angular or rounded rock fragments of pebble and cobble size. They typically top alluvial fans. Desert varnish collects on the exposed surface rocks over time.

<span class="mw-page-title-main">Brown earth</span> Soil type

Brown earth is a type of soil. Brown earths are mostly located between 35° and 55° north of the Equator. The largest expanses cover western and central Europe, large areas of western and trans-Uralian Russia, the east coast of America and eastern Asia. Here, areas of brown earth soil types are found particularly in Japan, Korea, China, eastern Australia and New Zealand. Brown earths cover 45% of the land in England and Wales. They are common in lowland areas on permeable parent material. The most common vegetation types are deciduous woodland and grassland. Due to the reasonable natural fertility of brown earths, large tracts of deciduous woodland have been cut down and the land is now used for farming. They are normally located in regions with a humid temperate climate. Rainfall totals are moderate, usually below 76 cm per year, and temperatures range from 4 °C in the winter to 18 °C in the summer. They are well-drained fertile soils with a pH of between 5.0 and 6.5.

<span class="mw-page-title-main">Red rain in Kerala</span> Episodes of rain containing vast amounts of red algal spores in India

The Kerala red rain phenomenon was a blood rain event that occurred in Wayanad district region of Malabar on Monday, 15 July 1957 and the colour subsequently turned yellow and also 25 July to 23 September 2001, when heavy downpours of red-coloured rain fell sporadically on the southern Indian state of Kerala, staining clothes pink. Yellow, green and black rain was also reported. Coloured rain was also reported in Kerala in 1896 and several times since, most recently in June 2012, and from 15 November 2012 to 27 December 2012 in eastern and north-central provinces of Sri Lanka.

<span class="mw-page-title-main">Mineral dust</span> Dust made from soil minerals

Mineral dust is atmospheric aerosol originated from the suspension of minerals constituting the soil, composed of various oxides and carbonates. Human activities lead to 30% of the airborne dust (particulates) load in the atmosphere. The Sahara Desert is the major source of mineral dust, which subsequently spreads across the Mediterranean and Caribbean seas into northern South America, Central America, and eastern North America, and Europe. Additionally, it plays a significant role in the nutrient inflow to the Amazon rainforest. The Gobi Desert is another source of dust in the atmosphere, which affects eastern Asia and western North America.

<span class="mw-page-title-main">Alkaline precipitation</span>

Alkaline precipitation occurs due to natural and anthropogenic causes. It happens when minerals, such as calcium, aluminum, or magnesium combine with other minerals to form alkaline residues that are emitted into the atmosphere, absorbed by water droplets in clouds, and eventually fall as rain. Aquatic environments are especially impacted by alkaline precipitation. Because alkaline precipitation can be harmful to the environment, it is important to utilize various methods such as air pollution control, solidification and stabilization, and remediation to manage it.

<span class="mw-page-title-main">Desert</span> Area of land where little precipitation occurs

A desert is a landscape where little precipitation occurs and, consequently, living conditions create unique biomes and ecosystems. The lack of vegetation exposes the unprotected surface of the ground to denudation. About one-third of the land surface of the Earth is arid or semi-arid. This includes much of the polar regions, where little precipitation occurs, and which are sometimes called polar deserts or "cold deserts". Deserts can be classified by the amount of precipitation that falls, by the temperature that prevails, by the causes of desertification or by their geographical location.

<span class="mw-page-title-main">Martian soil</span> Fine regolith found on the surface of Mars

Martian soil is the fine regolith found on the surface of Mars. Its properties can differ significantly from those of terrestrial soil, including its toxicity due to the presence of perchlorates. The term Martian soil typically refers to the finer fraction of regolith. So far, no samples have been returned to Earth, the goal of a Mars sample-return mission, but the soil has been studied remotely with the use of Mars rovers and Mars orbiters.

Blood rain or red rain is a phenomenon in which blood is perceived to fall from the sky in the form of rain. Cases have been recorded since Homer's Iliad, composed approximately 8th century BC, and are widespread. Before the 17th century it was generally believed that the rain was actually blood. Literature mirrors cult practice, in which the appearance of blood rain was considered a bad omen. It was used as a tool foreshadowing events, but while some of these may be literary devices, some occurrences are historic. There is now a scientific consensus that the blood rain phenomenon is caused by aerial spores of green microalgae Trentepohlia annulata.

<span class="mw-page-title-main">Martian regolith simulant</span>

Martian regolith simulant is a terrestrial material that is used to simulate the chemical and mechanical properties of Martian regolith for research, experiments and prototype testing of activities related to Martian regolith such as dust mitigation of transportation equipment, advanced life support systems and in-situ resource utilization.

Giuseppe Maria Giovene was an Italian archpriest, naturalist, agronomist, geologist, meteorologist, entomologist and ichthyologist. He is best known for his studies on the "nitrosity" of Pulo di Molfetta, which made him famous abroad, so as to be cited and appreciated by many Italian and foreign scholars, including Eberhard August Wilhelm von Zimmermann in a French publication.

<span class="mw-page-title-main">Saharan dust</span> Wind-borne mineral dust from the Sahara

Saharan dust is an aeolian mineral dust from the Sahara desert, the largest hot desert in the world. The desert spans just over 9 million square kilometers, from the Atlantic Ocean to the Red Sea, from the Mediterranean sea to the Niger River valley and the Sudan region in the south.

<span class="mw-page-title-main">Calima (Saharan sand)</span> Calima or Kalima (Saharan sand)

Calima or Kalima is a term used to describe a meteorological phenomenon that occurs when fine sand and dust particles from the Sahara Desert are lifted into the atmosphere and transported by prevailing winds.

References

  1. elogio-storico, pag. 20
  2. pioggia-rossa
  3. 1 2 3 Avila, Anna; Queralt-Mitjans, Ignasi; Alarcón, Marta (1997). "Mineralogical composition of African dust delivered by red rains over northeastern Spain". Journal of Geophysical Research. 102 (D18): 21977–21996. Bibcode:1997JGR...10221977A. doi: 10.1029/97JD00485 .
  4. Sala, José Quereda; Cantos, Jorge Olcina; Chiva, Enrique Montón (1996). "Red dust rain within the Spanish Mediterranean area". Climatic Change. 32 (2): 215. Bibcode:1996ClCh...32..215S. doi:10.1007/BF00143711. S2CID   154475201.
  5. Fornós, Joan J., Crespí, Damià; Fiol, Lluís (1997). "Aspectes mineralogics i texturals de la pols procedent de les pluges de 1ang a les IIles Balears: la seva importancia en alguns processos geologics recents". Boll. Soc. Hist. Nat. Balears. 40: 114–122.{{cite journal}}: CS1 maint: multiple names: authors list (link)
  6. Papastefanou, C; Manolopoulou, M; Stoulos, S; Ioannidou, A; Gerasopoulos, E (2001). "Coloured rain dust from Sahara Desert is still radioactive". Journal of Environmental Radioactivity. 55 (1): 109–112. doi:10.1016/S0265-931X(00)00182-X. PMID   11381550.

Bibliography