Noctilucent cloud

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Polar mesospheric cloud
Noctilucent clouds over Kuresoo bog, Viljandimaa, Estonia
Noctilucent clouds over Kuresoo bog, Viljandimaa, Estonia
Abbreviation NLC/PMC
Altitude 76,000 to 85,000 m
(250,000 to 280,000 ft)
Classification Other
Precipitation cloud? No

Night clouds or noctilucent clouds are tenuous cloud-like phenomena that are the "ragged-edge" of a much brighter and pervasive polar cloud layer called polar mesospheric clouds in the upper atmosphere, visible in a deep twilight. They are made of crystals of water ice. The name means roughly night shining in Latin. They are most commonly observed in the summer months at latitudes between 50° and 70° north and south of the equator. They can only be observed when the Sun is below the horizon.

They are the highest clouds in the Earth's atmosphere, located in the mesosphere at altitudes of around 76 to 85 kilometres (47 to 53 mi). They are normally too faint to be seen, and are visible only when illuminated by sunlight from below the horizon while the lower layers of the atmosphere are in the Earth's shadow. Noctilucent clouds are not fully understood and are a recently-discovered meteorological phenomenon; there is no record of their observation before 1885.

Noctilucent clouds can form only under very restrictive conditions; their occurrence can be used as a sensitive guide to changes in the upper atmosphere. Since they are a relatively recent classification, the occurrence of noctilucent clouds appears to be increasing in frequency, brightness and extent. It is theorized that this increase is connected to climate change.

Contents

[edit] Formation

Night clouds or noctilucent clouds are composed of tiny crystals of water ice up to 100 nm in diameter[1] and exist at a height of about 76 to 85 km (47 to 53 mi),[2] higher than any other clouds in Earth's atmosphere.[3] Clouds in the Earth's lower atmosphere form when water collects on particles, but mesospheric clouds may form directly from water vapour[4] in addition to forming on dust particles.[5]

The sources of both the dust and the water vapour in the upper atmosphere are not known with certainty. The dust is believed to come from micrometeors, although particulates from volcanoes and dust from the troposphere are also possibilities. The moisture could be lifted through gaps in the tropopause, as well as forming from the reaction of methane with hydroxyl radicals in the stratosphere.[6]

The exhaust from Space Shuttles, which is almost entirely water vapour after the detachment of the Solid Rocket Booster at a height of about 46km, has been found to generate minuscule individual clouds. About half of the vapour is released into the thermosphere, usually at altitudes of 103 to 114 km (64 to 71 mi).[7]

This exhaust can be transported to the Arctic region in little over a day, although the exact mechanism of this very high-speed transport is unknown. As the water migrates northward, it falls from the thermosphere down into the colder mesosphere, which occupies the region of the atmosphere just below.[8] Although this mechanism is the cause of individual noctilucent clouds, it is not thought to be a major contributor to the phenomenon as a whole.[6]

As the mesosphere contains very little moisture, approximately one hundred millionth that of air from the Sahara desert,[9] and is extremely thin, the ice crystals can only form at temperatures below about −120 °C (−184 °F).[6] This means that noctilucent clouds form predominantly during summer when, counterintuitively, the mesosphere is coldest.[10] Noctilucent clouds form mostly near the polar regions,[5] because the mesosphere is coldest there.[11] Clouds in the southern hemisphere are about 1 km (0.62 mi) higher than those in the northern hemisphere.[5]

Ultraviolet radiation from the Sun breaks water molecules apart, reducing the amount of water available to form noctilucent clouds. The radiation is known to vary cyclically with the solar cycle and satellites have been tracking the decrease in brightness of the clouds with the increase of ultraviolet radiation for the last two solar cycles. It has been found that changes in the clouds follow changes in the intensity of ultraviolet rays by about a year, but the reason for this long lag is not yet known.[12]

Noctilucent clouds are known to exhibit high radar reflectivity,[10] in a frequency range of 50 MHz to 1.3 GHz.[13] This behaviour is not well understood but a Caltech professor, Paul Bellan, has proposed a possible explanation: that the ice grains become coated with a thin metal film composed of sodium and iron, which makes the cloud far more reflective to radar,[10] although this explanation remains controversial.[14] Sodium and iron atoms are stripped from incoming micrometeors and settle into a layer just above the altitude of noctilucent clouds, and measurements have shown that these elements are severely depleted when the clouds are present. Other experiments have demonstrated that, at the extremely cold temperatures of a noctilucent cloud, sodium vapour can rapidly be deposited onto an ice surface.[15]

[edit] Discovery and investigation

Noctilucent clouds over Bargerveen, Drenthe, Netherlands

Noctilucent clouds are first known to have been observed in 1885, two years after the 1883 eruption of Krakatoa.[5][16] It remains unclear whether their appearance had anything to do with the volcano eruption, or whether their discovery was due to more people observing the spectacular sunsets caused by the volcanic debris in the atmosphere. Studies have shown that noctilucent clouds are not caused solely by volcanic activity, although dust and water vapour could be injected into the upper atmosphere by eruptions and contribute to their formation.[11] Scientists at the time assumed the clouds were another manifestation of volcanic ash, but after the ash had settled out of the atmosphere, the noctilucent clouds persisted.[9] Finally, the theory that the clouds were composed of volcanic dust was disproved by Malzev in 1926.[16] In the years following their discovery the clouds were studied extensively by Otto Jesse of Germany, who was the first to photograph them, in 1887, and seems to have been the one to coin the term "noctilucent cloud",[17] which means "night-shining cloud".[1] His notes provide evidence that noctilucent clouds first appeared in 1885. He had been doing detailed observations of the unusual sunsets caused by the Krakatoa eruption the previous year and firmly believed that, if the clouds had been visible then, he would undoubtedly have noticed them.[18] Systematic photographic observations of the clouds were organized in 1887 by Jesse, Foerster, and Stolze and, after that year, continuous observations were carried out at the Berlin Observatory.[19] During this research the height of the clouds was first determined, via triangulation.[20] The project was discontinued in 1896.

In the decades after Otto Jesse's death in 1901, there were few new insights into the nature of noctilucent clouds. Wegener's conjecture, that they were composed of water ice, was later shown to be correct.[21] Study was limited to ground-based observations and scientists had very little knowledge of the mesosphere until the 1960s, when direct rocket measurements began. These showed for the first time that the occurrence of the clouds coincided with very low temperatures in the mesosphere.[22]

Noctilucent clouds were first detected from space by an instrument on the OGO-6 satellite in 1972. The OGO-6 observations of a bright scattering layer over the polar caps were identified as poleward extensions of these clouds.[23] A later satellite, the Solar Mesosphere Explorer, mapped the distribution of the clouds between 1981 and 1986 with its ultraviolet spectrometer.[23] The clouds were detected with a lidar in 1995 at Utah State University, even when they were not visible with the naked eye.[24] The first physical confirmation that water ice is indeed the primary component of noctilucent clouds came from the HALOE instrument on the Upper Atmosphere Research Satellite in 2001.[25]

In 2001 the Swedish Odin satellite performed spectral analyses on the clouds, and produced daily global maps that revealed large patterns in their distribution.[26]

On April 25, 2007, the AIM satellite (Aeronomy of Ice in the Mesosphere) was launched.[27] It is the first satellite dedicated to studying noctilucent clouds,[28] and made its first observations on May 25, 2007.[29] Images taken by the satellite show shapes in the clouds that are similar to shapes in tropospheric clouds, hinting at similarities in their dynamics.[1]

On August 28, 2006, scientists with the Mars Express mission announced that they found clouds of carbon dioxide crystals over Mars that extended up to 100 km (62 mi) above the surface of the planet. They are the highest clouds discovered over the surface of a planet. Like noctilucent clouds on Earth, they can only be observed when the Sun is below the horizon.[30]

Research published in the journal Geophysical Research Letters in June 2009 suggests that noctilucent clouds observed following the Tunguska Event are evidence that the impact was caused by a comet.[31][32]

The United States Naval Research Laboratory (NRL) and the United States Department of Defense Space Test Program (STP) conducted the Charged Aerosol Release Experiment (CARE) on September 19, 2009, using exhaust particles from a Black Brant XII suborbital sounding rocket launched from NASA's Wallops Flight Facility to create an artificial noctilucent cloud. The cloud was to be observed over a period of weeks or months by ground instruments and the Spatial Heterodyne IMager for MEsospheric Radicals (SHIMMER) instrument on the NRL/STP STPSat-1 spacecraft.[33] The rocket's exhaust plume was observed and reported to news organizations in the United States from New Jersey to Massachusetts.[34]

[edit] Observation

Noctilucent clouds are generally colourless or pale blue,[35] although occasionally other colours including red and green occur.[36] The characteristic blue colour comes from absorption by ozone in the path of the sunlight illuminating the noctilucent cloud.[37] They can appear as featureless bands,[35] but frequently show distinctive patterns such as streaks, wave-like undulations, and whirls.[38] They are considered a "beautiful natural phenomenon".[39] Noctilucent clouds may be confused with cirrus clouds, but appear sharper under magnification.[35] Those caused by rocket exhausts tend to show colours other than silver or blue,[36] because of iridescence caused by the uniform size of the water droplets produced.[40]

Noctilucent clouds photographed by the crew of the ISS

Noctilucent clouds may be seen by observers at a latitude of 50° to 65°.[41] They seldom occur at lower latitudes (although there have been sightings as far south as Utah, Italy, and Paris),[35][42] and closer to the poles it does not get dark enough for the clouds to become visible.[43] They occur during summer, from mid-May to mid-August in the northern hemisphere and between mid-November and mid-February in the southern hemisphere.[35] They are very faint and tenuous, and may only be observed in twilight around sunrise and sunset when the clouds of the lower atmosphere are in shadow, but the noctilucent cloud is illuminated by the Sun.[43] They are best seen when the Sun is between 6° and 16° below the horizon.[44] Although noctilucent clouds occur in both hemispheres, they have been observed thousands of times in the northern hemisphere, but fewer than 100 times in the southern. Southern hemisphere noctilucent clouds are fainter and occur less frequently; additionally the southern hemisphere has a lower population and less land area from which to make observations.[11][45]

The clouds may show a large variety of different patterns and forms. An identification scheme was developed by Fogle in 1970 that classified five different forms. These classifications have since been modified and subdivided.[46]

They may be studied from the ground, from space, and directly by sounding rocket. Also, some noctilucent clouds are made of smaller crystals, 30 nm or less, which are invisible to observers on the ground because they do not scatter enough light.[1]

[edit] Connection to climate change

There is evidence that the relatively recent appearance of noctilucent clouds, and their gradual increase, may be linked to climate change.[47]

Atmospheric scientist Gary Thomas of the Laboratory for Atmospheric and Space Physics at the University of Colorado has pointed out[1] that the first sightings coincide with the Industrial Revolution and they have become more widespread and frequent throughout the twentieth century. The connection remains controversial however.[1] Wilfried Schröder was the first to explain noctilucent clouds as "indicators" for atmospheric processes (Gerlands Beiträge zur Geophysik, 1971, Meteorologische Rundschau 1968–1970).

Climate models predict that increased greenhouse gas emissions cause a cooling of the mesosphere, which would lead to more frequent and widespread occurrences of noctilucent clouds.[45] A competing theory is that larger methane emissions from intensive farming activities produce more water vapour in the upper atmosphere.[11] Methane concentrations have more than doubled in the past 100 years.[2]

Tromp et al. suggest that a transition to a hydrogen economy could increase the number of noctilucent clouds through increased emissions of free hydrogen.[48]

[edit] See also

Wikimedia Commons has media related to: Noctilucent clouds

[edit] Notes

  1. ^ a b c d e f Phillips, Tony (August 25, 2008). "Strange Clouds at the Edge of Space". NASA. http://science.nasa.gov/headlines/y2008/25aug_nlc.htm. 
  2. ^ a b Hsu, Jeremy (2008-09-03). "Strange clouds spotted at the edge of Earth's atmosphere". USAtoday. http://www.usatoday.com/tech/science/space/2008-09-02-strange-clouds-space_N.htm. 
  3. ^ Simons, Paul (2008-05-12). "Mysterious noctilucent clouds span the heavens". TimesOnline. http://www.timesonline.co.uk/tol/news/weather/article3912727.ece. Retrieved 2008-10-06. 
  4. ^ Murray, B.J.; Jensen, E.J. (2000). "Homogeneous nucleation of amorphous solid water particles in the upper mesosphere". J. Atm. Sol-Terr. Phys. 72 (1): 51–61. Bibcode 2010JASTP..72...51M. DOI:10.1016/j.jastp.2009.10.007. 
  5. ^ a b c d Chang, Kenneth (2007-07-24). "First Mission to Explore Those Wisps in the Night Sky". New York Times. http://www.nytimes.com/2007/04/24/science/24cloud.html?_r=2&scp=3&sq=noctilucent%20cloud&st=cse&oref=slogin&oref=slogin. Retrieved 2008-10-05. 
  6. ^ a b c About NLCs, Polar Mesospheric Clouds, from Atmospheric optics
  7. ^ "Study Finds Space Shuttle Exhaust Creates Night-Shining Clouds" (Press release). Naval Research Laboratories. 2003-03-06. http://www.nrl.navy.mil/pressRelease.php?Y=2003&R=35-03r. Retrieved 2008-10-19. 
  8. ^ "STUDY FINDS SPACE SHUTTLE EXHAUST CREATES NIGHT-SHINING CLOUDS". NASA. 2003-06-03. http://www.nasa.gov/centers/goddard/news/topstory/2003/0522shuttleshine.html. Retrieved 2008-10-05. 
  9. ^ a b Phillips, Tony (2003-02-19). "Strange Clouds". NASA. http://science.nasa.gov/headlines/y2003/19feb_nlc.htm. Retrieved 2008-10-05. 
  10. ^ a b c "Caltech Scientist Proposes Explanation for Puzzling Property of Night-Shining Clouds at the Edge of Space" (Press release). Caltech. 2008-09-25. http://mr.caltech.edu/media/Press_Releases/PR13188.html. Retrieved 2008-10-19. 
  11. ^ a b c d "Noctilucent clouds". Australian Antarctic Division. http://www.aad.gov.au/default.asp?casid=2005. 
  12. ^ Cole, Stephen (2007-03-14). "AIM at the Edge of Space". NASA. http://www.nasa.gov/mission_pages/aim/edge_of_space.html. 
  13. ^ "Project Studies Night Clouds, Radar Echoes". ECE News (Virginia Tech): 3. Fall 2003. http://www.ece.vt.edu/news/fall03/nlc.html. Retrieved 2008-10-19. 
  14. ^ Rapp, M.; Lubken, F.J. (2009). "Comment on 'Ice iron/sodium film as cause for high noctilucent cloud radar reflectivity' by P. M. Bellan". Geophys. Res, Lett. 114 (D11): D11204. Bibcode 2009JGRD..11411204R. DOI:10.1029/2008JD011323. 
  15. ^ Murray, B.J.; Plane, J.M.C. (2005). "Uptake of Fe, Na and K atoms on low-temperature ice: implications for metal atom scavenging in the vicinity of polar mesospheric clouds". Phys. Chem. Chem. Phys. 7 (23): 3970–3979. Bibcode 2005PCCP....7.3970M. DOI:10.1039/b508846a. PMID 19810327. 
  16. ^ a b Bergman, Jennifer (2004-08-17). "History of Observation of Noctilucent Clouds". http://www.windows.ucar.edu/tour/link=/earth/Atmosphere/NLC_history.html. Retrieved 2008-10-06. 
  17. ^ Schröder, Wilfried. "On the Diurnal Variation of Noctilucent Clouds". German Commission on History of Geophysics and Cosmical Physics. http://verplant.org/history-geophysics/Diurnal_V/Main.htm. Retrieved 2008-10-06. 
  18. ^ Schröder (2001), p.2457
  19. ^ Schröder (2001), p.2459
  20. ^ Schröder (2001), p.2460
  21. ^ Keesee, Bob. "Noctilucent Clouds". University of Albany. http://www.albany.edu/faculty/rgk/atm101/nlc.htm. Retrieved 2008-10-19. 
  22. ^ Schröder (2001), p.2464
  23. ^ a b Gadsden (1995), p.18.
  24. ^ http://www.agu.org/pubs/crossref/2007/2006JD007158.shtml
  25. ^ Hervig, Mark; Thompson, Robert E.; McHugh, Martin; Gordley, Larry L.; Russel, James M.; Summers, Michael E. (March 2001). "First Confirmation that Water Ice is the Primary Component of Polar Mesospheric Clouds". Geophysical Research Letters 28 (6): 971–974. Bibcode 2001GeoRL..28..971H. DOI:10.1029/2000GL012104. 
  26. ^ Karlsson, B.; Gumbel, J.; Stegman, J.; Lautier, N.; Murtagh, D.P.; The Odin Team (2004). "Studies of Noctilucent Clouds by the Odin Satellite" (PDF). 35th COSPAR Scientific Assembly: 1921. Bibcode 2004cosp...35.1921K. http://www.cosis.net/abstracts/COSPAR04/01921/COSPAR04-A-01921.pdf. Retrieved 2008-10-16. 
  27. ^ "Launch of AIM Aboard a Pegasus XL Rocket". NASA. http://www.nasa.gov/mission_pages/aim/launch/launch-index.html. Retrieved 2008-10-19. 
  28. ^ NASA/Goddard Space Flight Center Scientific Visualization Studio. "The First Season of Noctilucent Clouds from AIM". NASA. http://svs.gsfc.nasa.gov/vis/a000000/a003400/a003484/. Retrieved 2008-10-19. 
  29. ^ O'Carroll, Cynthia (2007-06-28). "NASA Satellite Captures First View of 'Night-Shining Clouds". http://www.nasa.gov/mission_pages/aim/multimedia/first_view.html. 
  30. ^ SPACE.com staff (2006-08-28). "Mars Clouds Higher Than Any On Earth". SPACE.com. http://www.space.com/scienceastronomy/060828_mars_clouds.html. Retrieved 2008-10-19. 
  31. ^ Kelly, M.C.; C.E. Seyler, M.F. Larsen (2009-06-22). "Two-dimensional turbulence, space shuttle plume transport in the thermosphere, and a possible relation to the Great Siberian Impact Event". Geophysical Research Letters 36 (14): L14103. Bibcode 2009GeoRL..3614103K. DOI:10.1029/2009GL038362. 
  32. ^ Ju, Anne (2009-06-24). "A mystery solved: Space shuttle shows 1908 Tunguska explosion was caused by comet". Cornell Chronicle. Cornell University. http://www.news.cornell.edu/stories/June09/TunguskaComet.html. Retrieved 2009-06-25. 
  33. ^ NASA (2009-09-19). "Night Time Artificial Cloud Study Using NASA Sounding Rocket". NASA. http://www.nasa.gov/centers/wallops/CARE.html. 
  34. ^ "Rocket launch prompts calls of strange lights in sky". Cable News Network (CNN). 2009-09-20. http://www.cnn.com/2009/US/09/20/strange.lights/index.html. 
  35. ^ a b c d e Cowley, Les. "Noctilucent Clouds, NLCs". Atmospheric Optics. http://www.atoptics.co.uk/highsky/nlc1.htm. Retrieved 2008-10-18. 
  36. ^ a b Gadsden (1995), p.13.
  37. ^ Gadsen, M. (October–December 1975). "Observations of the colour and polarization of noctilucent clouds". Annales de Geophysique 31: 507–516. Bibcode 1975AnG....31..507G. 
  38. ^ Gadsden (1995), pp.8–10.
  39. ^ Gadsden (1995), p.9.
  40. ^ "Rocket Trails". Atmospheric Optics. Archived from the original on August 4, 2008. http://web.archive.org/web/20080804122134/http://www.atoptics.co.uk/highsky/rktr1a.htm. Retrieved 2008-10-19. 
  41. ^ Gadsden (1995), p.8.
  42. ^ Hultgren, K.; et al. (2011). "What caused the exceptional mid-latitudinal Noctilucent Cloud event in July 2009?". Journal of Atmospheric and Solar-Terrestrial Physics 73 (14-15): 2125–2131. DOI:10.1016/j.jastp.2010.12.008. http://www.sciencedirect.com/science/article/pii/S1364682610003883. Retrieved 4 October 2011. 
  43. ^ a b Giles, Bill. "Nacreous and Noctilucent Clouds". BBC Weather. Archived from the original on 2008-10-11. http://web.archive.org/web/20081011213129/http://www.bbc.co.uk/weather/features/understanding/nacreous_noctilucent.shtml. Retrieved 2008-10-05. 
  44. ^ Gadsden (1995), p.11.
  45. ^ a b A. Klekociuk, R. Morris, J. French (2008). "First Antarctic ground-satellite view of ice aerosol clouds at the edge of space". Australian Antarctic Division. http://www.aad.gov.au/default.asp?casid=34672. Retrieved 2008-10-19. 
  46. ^ Gadsden (1995), pp.9–10.
  47. ^ Thomas, GE; Olivero, J (2001). "Noctilucent clouds as possible indicators of global change in the mesosphere". Advances in Space Research 28 (7): 939–946. Bibcode 2001AdSpR..28..937T. DOI:10.1016/S0273-1177(01)80021-1. 
  48. ^ Tracey K. Tromp, Run-Lie Shia, Mark Allen, John M. Eiler, Y.L. Yung (June 2003). "Potential Environmental Impact of a Hydrogen Economy on the Stratosphere". Science Magazine 300 (5626): 1740–1742. Bibcode 2003Sci...300.1740T. DOI:10.1126/science.1085169. PMID 12805546. http://www.sciencemag.org/cgi/content/abstract/300/5626/1740. Retrieved 2008-10-19.  A comprehensive review on the results of noctilucent clouds has been given by Wilfried Schröder, Entwicklungsphasen der Erforschung der Leuchtenden Nachtwolken (development phases of noctilucent cloud research), Berlin: Akademie-Verlag, 1975, Michael Gadsden and Wilfried Schröder, Noctilucent clouds, Heidelberg, New York Springer Verlag, 1989, Wilfried Schröder, Noctilucent clouds, Bremen, Science Edition, 1998, Wilfried Schröder, Mesospheric Circulation and Noctilucent clouds, Bremen, Science Edition, 2006.

[edit] References

[edit] External links

Cloud genera and selected species, supplementary features, and other airborne hydrometeors
Extreme-level
Polar mesospheric cirriform type: Noctilucent
Very high-level
Polar stratospheric cirriform type: Nacreous
High-level
WMO genera: Cirrostratus (Cs) · Cirrocumulus (Cc) · Cirrus (Ci) · Special cirrus variants (non-WMO terminology): Cirrus Kelvin-Helmholtz · Cirrus aviaticus (Contrail)
Medium-level
Low-level
WMO genera: Stratus (St) · Stratocumulus (Sc) · Species: Fractus · Special stratocumulus variants (non-WMO terminology): Actinoform cloud · Undulatus asperatus
Moderate vertical
WMO genera: Nimbostratus (Ns) · Cumulus (Cu) · Supplementary features: Cumulus Pileus · Cumulus Arcus (Roll)
Towering vertical
WMO genera: Cumulonimbus (Cb) · Cumulus congestus (species) (ICAO term Towering cumulus -Tcu) · WMO supplementary features: Cumulonimbus mammatus · Cumulonimbus tuba (Funnel cloud) · Cumulonimbus Pileus · Cumulonimbus Arcus (Shelf) · Special variants (non-WMO terminology): Pyrocumulus · Pyrocumulonimbus · Cumulonimbus Wall cloud  · Cumulonimbus Overshooting top
Surface based
General type: Fog
Non-height specific
General type: Accessory cloud
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