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Noctilucent cloud
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<h2 id="general">General</h2> <p>No confirmed record of their observation exists before 1885, although they may have been observed a few decades earlier by <a href="/facts/Thomas_Romney_Robinson/fsTxkPJ5">Thomas Romney Robinson</a> in <a href="/facts/Armagh/ouTQWndq">Armagh</a>.<a class="footnote-ref" id="fnref:3" href="#fn:3"><sup>3</sup></a> </p> <h2 id="formation">Formation</h2> <p>Noctilucent clouds are composed of tiny crystals of <a href="/facts/Ice/BGvkKFjD">water ice</a> up to 100 <a href="/facts/Nanometer/a98sjHyu">nm</a> in diameter<a class="footnote-ref" id="fnref:4" href="#fn:4"><sup>4</sup></a> and exist at a height of about 76 to 85 km (249,000 to 279,000 ft),<a class="footnote-ref" id="fnref:5" href="#fn:5"><sup>5</sup></a> higher than any other clouds in Earth's atmosphere.<a class="footnote-ref" id="fnref:6" href="#fn:6"><sup>6</sup></a> Clouds in the Earth's lower atmosphere form when water collects on particles, but <a href="/facts/Mesosphere/JBPKmMuk">mesospheric</a> clouds may form directly from water vapour in addition to forming on dust particles.<a class="footnote-ref" id="fnref:7" href="#fn:7"><sup>7</sup></a><a class="footnote-ref" id="fnref:8" href="#fn:8"><sup>8</sup></a> </p> <p>Data from the <a href="/facts/Aeronomy_of_Ice_in_the_Mesosphere/4cyr0M0a">Aeronomy of Ice in the Mesosphere</a> satellite suggests that noctilucent clouds require water vapour, dust, and very cold temperatures to form.<a class="footnote-ref" id="fnref:9" href="#fn:9"><sup>9</sup></a> The sources of both the dust and the water vapour in the <a href="/facts/Upper_atmosphere/5yH29VP8">upper atmosphere</a> are not known with certainty. The dust is believed to come from <a href="/facts/Meteor/gcoGYw6o">micrometeors</a>, although particulates from <a href="/facts/Volcano/c2M5upml">volcanoes</a> and dust from the <a href="/facts/Troposphere/JPDQq8cL">troposphere</a> are also possibilities. The moisture could be lifted through gaps in the <a href="/facts/Tropopause/26rub4PU">tropopause</a>, as well as forming from the reaction of <a href="/facts/Methane/kBHneYnh">methane</a> with <a href="/facts/Hydroxyl_radical/XafpvqK5">hydroxyl radicals</a> in the <a href="/facts/Stratosphere/taBra67V">stratosphere</a>.<a class="footnote-ref" id="fnref:10" href="#fn:10"><sup>10</sup></a> </p><p>The exhaust from <a href="/facts/Space_Shuttle/7BoyetEv">Space Shuttles</a>, in use between 1981 and 2011, which was almost entirely water vapour after the detachment of the <a href="/facts/Space_Shuttle_Solid_Rocket_Booster/ETayF0Xh">Solid Rocket Booster</a> at a height of about 46 km (151,000 ft), was found to generate minuscule individual clouds. About half of the vapour was released into the <a href="/facts/Thermosphere/uhG50e2V">thermosphere</a>, usually at altitudes of 103 to 114 km (338,000 to 374,000 ft).<a class="footnote-ref" id="fnref:11" href="#fn:11"><sup>11</sup></a> In August 2014, a <a href="/facts/SpaceX/2tKHsVdJ">SpaceX</a> <a href="/facts/Falcon_9/mNck6vby">Falcon 9</a> also caused noctilucent clouds over <a href="/facts/Orlando,_Florida/QeW5fkCp">Orlando, Florida</a> after a launch.<a class="footnote-ref" id="fnref:12" href="#fn:12"><sup>12</sup></a> </p> <p>The exhaust can be transported to the <a href="/facts/Arctic/bxbuUz7Q">Arctic</a> region in little over a day, although the exact mechanism of this very high-speed transfer is unknown. As the water migrates northward, it falls from the thermosphere into the colder mesosphere, which occupies the region of the atmosphere just below.<a class="footnote-ref" id="fnref:13" href="#fn:13"><sup>13</sup></a> 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.<a class="footnote-ref" id="fnref:14" href="#fn:14"><sup>14</sup></a> </p><p>As the <a href="/facts/Mesosphere/JBPKmMuk">mesosphere</a> contains very little moisture, approximately one hundred millionth that of air from the <a href="/facts/Sahara/JVlJd2VC">Sahara</a>,<a class="footnote-ref" id="fnref:15" href="#fn:15"><sup>15</sup></a> and is extremely thin, the ice crystals can form only at temperatures below about −120 °C (−184 °F).<a class="footnote-ref" id="fnref:16" href="#fn:16"><sup>16</sup></a> This means that noctilucent clouds form predominantly during summer when, counterintuitively, the mesosphere is coldest as a result of seasonally varying vertical winds, leading to cold summertime conditions in the upper mesosphere (<a href="/facts/Upwelling/UuJovSjH">upwelling</a>, resulting in <a href="/facts/Adiabatic_cooling/rJj42U5h">adiabatic cooling</a>) and wintertime heating (<a href="/facts/Downwelling/y4ep6Gyy">downwelling</a>, resulting in <a href="/facts/Adiabatic_heating/rJj42U5h">adiabatic heating</a>). Therefore, they cannot be observed (even if they are present) inside the <a href="/facts/Polar_circle/kYAguHqs">Polar circles</a> because the Sun is never low enough under the horizon at this season at these latitudes.<a class="footnote-ref" id="fnref:17" href="#fn:17"><sup>17</sup></a> Noctilucent clouds form mostly near the polar regions,<a class="footnote-ref" id="fnref:18" href="#fn:18"><sup>18</sup></a> because the mesosphere is coldest there.<a class="footnote-ref" id="fnref:19" href="#fn:19"><sup>19</sup></a> Clouds in the southern hemisphere are about 1 km (3,300 ft) higher than those in the northern hemisphere.<a class="footnote-ref" id="fnref:20" href="#fn:20"><sup>20</sup></a> </p><p><a href="/facts/Ultraviolet_radiation/kncBUqn5">Ultraviolet radiation</a> 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 <a href="/facts/Solar_cycle/QrP4Egea">solar cycle</a> 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.<a class="footnote-ref" id="fnref:21" href="#fn:21"><sup>21</sup></a> </p><p>Noctilucent clouds are known to exhibit high <a href="/facts/Radar/jk9BTbFA">radar</a> reflectivity,<a class="footnote-ref" id="fnref:22" href="#fn:22"><sup>22</sup></a> in a frequency range of 50 <a href="/facts/Hertz/6Wshj5qm">MHz</a> to 1.3 GHz.<a class="footnote-ref" id="fnref:23" href="#fn:23"><sup>23</sup></a> This behaviour is not well understood but a possible explanation is that the ice grains become coated with a thin metal film composed of <a href="/facts/Sodium/eYuSPu2V">sodium</a> and <a href="/facts/Iron/QK1JYy8E">iron</a>, which makes the cloud far more reflective to radar,<a class="footnote-ref" id="fnref:24" href="#fn:24"><sup>24</sup></a> although this explanation remains controversial.<a class="footnote-ref" id="fnref:25" href="#fn:25"><sup>25</sup></a> Sodium and iron atoms are stripped from incoming <a href="/facts/Meteorite/NsmHlBlX">micrometeors</a> 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 low temperatures of a noctilucent cloud, sodium vapour can rapidly be deposited onto an ice surface.<a class="footnote-ref" id="fnref:26" href="#fn:26"><sup>26</sup></a> </p> <h2 id="discovery-and-investigation">Discovery and investigation</h2> <p>Noctilucent clouds are first known to have been observed in 1885, two years after the <a href="/facts/1883_eruption_of_Krakatoa/C8fvLt2Q">1883 eruption of Krakatoa</a>.<a class="footnote-ref" id="fnref:27" href="#fn:27"><sup>27</sup></a><a class="footnote-ref" id="fnref:28" href="#fn:28"><sup>28</sup></a> It remains unclear whether their appearance had anything to do with the volcanic 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.<a class="footnote-ref" id="fnref:29" href="#fn:29"><sup>29</sup></a> 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.<a class="footnote-ref" id="fnref:30" href="#fn:30"><sup>30</sup></a> Finally, the theory that the clouds were composed of volcanic dust was disproved by Malzev in 1926.<a class="footnote-ref" id="fnref:31" href="#fn:31"><sup>31</sup></a> In the years following their discovery, the clouds were studied extensively by Otto Jesse of <a href="/facts/Germany/paluuWBX">Germany</a>, who was the first to photograph them, in 1887, and seems to have been the one to coin the term "noctilucent cloud".<a class="footnote-ref" id="fnref:32" href="#fn:32"><sup>32</sup></a><a class="footnote-ref" id="fnref:33" href="#fn:33"><sup>33</sup></a> 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.<a class="footnote-ref" id="fnref:34" href="#fn:34"><sup>34</sup></a> Systematic photographic observations of the clouds were organized in 1887 by Jesse, <a href="/facts/Wilhelm_Julius_Foerster/hyL6et6k">Foerster</a>, and Stolze and, after that year, continuous observations were carried out at the <a href="/facts/Berlin_Observatory/RjKmxSpP">Berlin Observatory</a>.<a class="footnote-ref" id="fnref:35" href="#fn:35"><sup>35</sup></a> </p><p>In the decades after Otto Jesse's death in 1901, there were few new insights into the nature of noctilucent clouds. <a href="/facts/Alfred_Wegener/sXu37sav">Wegener</a>'s conjecture, that they were composed of water ice, was later shown to be correct.<a class="footnote-ref" id="fnref:36" href="#fn:36"><sup>36</sup></a> 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 clouds' occurrence coincided with very low temperatures in the mesosphere.<a class="footnote-ref" id="fnref:37" href="#fn:37"><sup>37</sup></a> </p><p>Noctilucent clouds were first detected from space by an instrument on the <a href="/facts/Orbiting_Geophysical_Observatory/oXlxwWyd">OGO</a>-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.<a class="footnote-ref" id="fnref:38" href="#fn:38"><sup>38</sup></a> A later satellite, the <a href="/facts/Solar_Mesosphere_Explorer/GQ39TavX">Solar Mesosphere Explorer</a>, mapped the distribution of the clouds between 1981 and 1986 with its ultraviolet spectrometer.<a class="footnote-ref" id="fnref:39" href="#fn:39"><sup>39</sup></a> The clouds were detected with a <a href="/facts/Lidar/b9SPUmLM">lidar</a> in 1995 at <a href="/facts/Utah_State_University/qamWhgaC">Utah State University</a>, even when they were not visible to the naked eye.<a class="footnote-ref" id="fnref:40" href="#fn:40"><sup>40</sup></a> The first physical confirmation that water ice is indeed the primary component of noctilucent clouds came from the HALOE instrument on the <a href="/facts/Upper_Atmosphere_Research_Satellite/jUI52Hqx">Upper Atmosphere Research Satellite</a> in 2001.<a class="footnote-ref" id="fnref:41" href="#fn:41"><sup>41</sup></a> </p><p>In 2001, the <a href="/facts/Sweden/u3qC7lyj">Swedish</a> <a href="/facts/Odin_satellite/FzjhN7Q0">Odin satellite</a> performed spectral analyses on the clouds, and produced daily global maps that revealed large patterns in their distribution.<a class="footnote-ref" id="fnref:42" href="#fn:42"><sup>42</sup></a> </p><p>The AIM (<a href="/facts/Aeronomy_of_Ice_in_the_Mesosphere/4cyr0M0a">Aeronomy of Ice in the Mesosphere</a>) satellite was launched on 25 April 2007.<a class="footnote-ref" id="fnref:43" href="#fn:43"><sup>43</sup></a> It was the first satellite dedicated to studying noctilucent clouds,<a class="footnote-ref" id="fnref:44" href="#fn:44"><sup>44</sup></a> and made its first observations a month later (25 May).<a class="footnote-ref" id="fnref:45" href="#fn:45"><sup>45</sup></a> Images taken by the satellite show shapes in the clouds that are similar to shapes in tropospheric clouds, hinting at similarities in their dynamics.<a class="footnote-ref" id="fnref:46" href="#fn:46"><sup>46</sup></a> </p><p>In the previous year, scientists with the <a href="/facts/Mars_Express/wM1scUfh">Mars Express</a> mission had announced their discovery of <a href="/facts/Carbon_dioxide/xGzpppEp">carbon dioxide</a>–crystal clouds on Mars that extended to 100 km (330,000 ft) above the planet's surface. These are the highest clouds discovered over the surface of a rocky planet. Like noctilucent clouds on Earth, they can be observed only when the Sun is below the horizon.<a class="footnote-ref" id="fnref:47" href="#fn:47"><sup>47</sup></a> </p><p>Research published in the journal <i>Geophysical Research Letters</i> in June 2009 suggests that noctilucent clouds observed following the <a href="/facts/Tunguska_Event/x3cCog2j">Tunguska Event</a> of 1908 are evidence that the impact was caused by a comet.<a class="footnote-ref" id="fnref:48" href="#fn:48"><sup>48</sup></a><a class="footnote-ref" id="fnref:49" href="#fn:49"><sup>49</sup></a> </p><p>The <a href="/facts/United_States_Naval_Research_Laboratory/brXxYx34">United States Naval Research Laboratory</a> (NRL) and the <a href="/facts/United_States_Department_of_Defense/dWAvf7e3">United States Department of Defense</a> <a href="/facts/Space_Test_Program/2El3p9sv">Space Test Program</a> (STP) conducted the <a href="/facts/Charged_Aerosol_Release_Experiment/9vSwhQsj">Charged Aerosol Release Experiment</a> (CARE) on September 19, 2009, using exhaust particles from a <a href="/facts/Black_Brant_(rocket)/mxjN9D4v">Black Brant</a> <a href="/facts/Black_Brant_(rocket)/mxjN9D4v">XII</a> suborbital sounding rocket launched from NASA's <a href="/facts/Wallops_Flight_Facility/F6QvD712">Wallops Flight Facility</a> 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.<a class="footnote-ref" id="fnref:50" href="#fn:50"><sup>50</sup></a> The rocket's exhaust plume was observed and reported to news organizations in the United States from <a href="/facts/New_Jersey/pI5k19S7">New Jersey</a> to <a href="/facts/Massachusetts/9uumCbFI">Massachusetts</a>.<a class="footnote-ref" id="fnref:51" href="#fn:51"><sup>51</sup></a> </p><p>A 2018 experiment briefly created noctilucent clouds over Alaska, allowing ground-based measurements and experiments aimed at verifying computer simulations of the phenomenon. A suborbital NASA rocket was launched on 26 January 2018 by University of Alaska professor Richard Collins. It carried water-filled canisters, which were released at about 53 mi (85 km) above the Earth. Since the naturally-occurring clouds only appear in summer, this experiment was conducted in mid-winter to assure that its results would not be mixed with a natural event.<a class="footnote-ref" id="fnref:52" href="#fn:52"><sup>52</sup></a> </p> <h2 id="description-from-satellites">Description from satellites</h2> <p>PMC's have four major types based on physical structure and appearance. Type I veils are very tenuous and lack well-defined structure, somewhat like cirrostratus or poorly defined cirrus.<a class="footnote-ref" id="fnref:53" href="#fn:53"><sup>53</sup></a> Type II bands are long streaks that often occur in groups arranged roughly parallel to each other. They are usually more widely spaced than the bands or elements seen with cirrocumulus clouds.<a class="footnote-ref" id="fnref:54" href="#fn:54"><sup>54</sup></a> Type III billows are arrangements of closely spaced, roughly parallel short streaks that mostly resemble cirrus.<a class="footnote-ref" id="fnref:55" href="#fn:55"><sup>55</sup></a> Type IV whirls are partial or, more rarely, complete rings of cloud with dark centres.<a class="footnote-ref" id="fnref:56" href="#fn:56"><sup>56</sup></a> </p><p>Satellite observations allow the very coldest parts of the polar mesosphere to be observed, all the way to the geographic pole. In the early 1970s, visible airglow photometers first scanned the atmospheric horizon throughout the summer polar mesospause region.<a class="footnote-ref" id="fnref:57" href="#fn:57"><sup>57</sup></a> This experiment, which flew on the OGO-6 satellite, was the first to trace noctilucent-like cloud layers across the polar cap. The very bright scattering layer was seen in full daylight conditions, and was identified as the poleward extension of noctilucent clouds. In the early 1980s, the layer was observed again from a satellite, the Solar Mesospheric Explorer (SME). On board this satellite was an ultraviolet spectrometer, which mapped the distributions of clouds over the time period 1981 to 1986. The experiment measured the altitude profile of scattering from clouds at two spectral channels (primarily) 265 nm and 296 nm.<a class="footnote-ref" id="fnref:58" href="#fn:58"><sup>58</sup></a> </p><p>Polar mesospheric clouds generally increase in brightness and occurrence frequency with increasing latitude, from about 60° to the highest latitudes observed (85°). So far, no apparent dependence on longitude has been found, nor is there any evidence of a dependence on auroral activity.<a class="footnote-ref" id="fnref:59" href="#fn:59"><sup>59</sup></a> </p><p>On 8 July 2018, <a href="/facts/NASA/TIMCV0yV">NASA</a> launched a giant balloon from <a href="/facts/Esrange/SHd6XSeQ">Esrange</a>, <a href="/facts/Sweden/u3qC7lyj">Sweden</a> which traveled through the <a href="/facts/Stratosphere/taBra67V">stratosphere</a> across the <a href="/facts/Arctic/bxbuUz7Q">Arctic</a> to Western <a href="/facts/Nunavut/aFaAad0W">Nunavut</a>, <a href="/facts/Canada/cWWFM8oc">Canada</a> in five days. The giant balloon was loaded with cameras, which captured six million high-resolution images filling up 120 terabytes of data storage, aiming to study the PMCs which are affected by the atmospheric <a href="/facts/Gravity_waves/HHazND81">gravity waves</a>, resulted from air being pushed up by mountain ranges all the way up to the mesosphere. These images would aid in studying turbulence in the atmosphere, and consequently better <a href="/facts/Weather_forecasting/nzqyMFCa">weather forecasting</a>.<a class="footnote-ref" id="fnref:60" href="#fn:60"><sup>60</sup></a><a class="footnote-ref" id="fnref:61" href="#fn:61"><sup>61</sup></a> </p><p>NASA uses <a href="/facts/Aeronomy_of_Ice_in_the_Mesosphere/4cyr0M0a">AIM</a> satellite to study these noctilucent clouds, which always occur during the summer season near the poles. However, <a href="/facts/Tomography/HGqzMl2s">tomographic</a> analyses of AIM satellite indicate that there is a spatial negative correlation between <a href="/facts/Albedo/TJDRdKEB">albedo</a> and wave‐induced altitude.<a class="footnote-ref" id="fnref:62" href="#fn:62"><sup>62</sup></a> </p> <h2 id="observation">Observation</h2> <p>Noctilucent clouds are generally colourless or pale blue,<a class="footnote-ref" id="fnref:63" href="#fn:63"><sup>63</sup></a> although occasionally other colours including red and green have been observed.<a class="footnote-ref" id="fnref:64" href="#fn:64"><sup>64</sup></a> The characteristic blue colour comes from absorption by <a href="/facts/Ozone/o0E5gn2p">ozone</a> in the path of the sunlight illuminating the noctilucent cloud.<a class="footnote-ref" id="fnref:65" href="#fn:65"><sup>65</sup></a> They can appear as featureless bands,<a class="footnote-ref" id="fnref:66" href="#fn:66"><sup>66</sup></a> but frequently show distinctive patterns such as streaks, wave-like undulations, and whirls.<a class="footnote-ref" id="fnref:67" href="#fn:67"><sup>67</sup></a> They are considered a "beautiful natural phenomenon".<a class="footnote-ref" id="fnref:68" href="#fn:68"><sup>68</sup></a> Noctilucent clouds may be confused with <a href="/facts/Cirrus_cloud/AznU9a7L">cirrus clouds</a>, but appear sharper under magnification.<a class="footnote-ref" id="fnref:69" href="#fn:69"><sup>69</sup></a> Those caused by rocket exhausts tend to show colours other than silver or blue,<a class="footnote-ref" id="fnref:70" href="#fn:70"><sup>70</sup></a> because of iridescence caused by the uniform size of the water droplets produced.<a class="footnote-ref" id="fnref:71" href="#fn:71"><sup>71</sup></a> </p><p>Noctilucent clouds may be seen at <a href="/facts/Latitude/IBYqkjhU">latitudes</a> of 50° to 65°.<a class="footnote-ref" id="fnref:72" href="#fn:72"><sup>72</sup></a> They seldom occur at lower latitudes (although there have been sightings as far south as <a href="/facts/Paris/DrNHpwnA">Paris</a>, <a href="/facts/Utah/te7zUyBX">Utah</a>, <a href="/facts/Italy/tUf0PDYF">Italy</a>, <a href="/facts/Turkey/KIYAWAs0">Turkey</a> and <a href="/facts/Spain/bIyrB8EY">Spain</a>),<a class="footnote-ref" id="fnref:73" href="#fn:73"><sup>73</sup></a><a class="footnote-ref" id="fnref:74" href="#fn:74"><sup>74</sup></a><a class="footnote-ref" id="fnref:75" href="#fn:75"><sup>75</sup></a><a class="footnote-ref" id="fnref:76" href="#fn:76"><sup>76</sup></a> and closer to the poles it does not get dark enough for the clouds to become visible.<a class="footnote-ref" id="fnref:77" href="#fn:77"><sup>77</sup></a> 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.<a class="footnote-ref" id="fnref:78" href="#fn:78"><sup>78</sup></a> They are very faint and tenuous, and may be observed only in <a href="/facts/Twilight/hNUKeCT8">twilight</a> around sunrise and sunset when the clouds of the lower atmosphere are in shadow, but the noctilucent cloud is illuminated by the <a href="/facts/Sun/CadPCVHh">Sun</a>.<a class="footnote-ref" id="fnref:79" href="#fn:79"><sup>79</sup></a> They are best seen when the Sun is between 6° and 16° below the horizon.<a class="footnote-ref" id="fnref:80" href="#fn:80"><sup>80</sup></a> 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.<a class="footnote-ref" id="fnref:81" href="#fn:81"><sup>81</sup></a><a class="footnote-ref" id="fnref:82" href="#fn:82"><sup>82</sup></a> </p><p>These clouds may be studied from the ground, from space, and directly by <a href="/facts/Sounding_rocket/em1GgGND">sounding rocket</a>. 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.<a class="footnote-ref" id="fnref:83" href="#fn:83"><sup>83</sup></a> </p> <h2 id="forms">Forms</h2> <p>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.<a class="footnote-ref" id="fnref:84" href="#fn:84"><sup>84</sup></a> </p> <ol><li>Type I veils are very tenuous and lack well-defined structure, somewhat like cirrostratus or poorly defined cirrus.<a class="footnote-ref" id="fnref:85" href="#fn:85"><sup>85</sup></a></li> <li>Type II bands are long streaks that often occur in roughly parallel groups, usually more widely spaced than the bands or elements seen with cirrocumulus clouds.<a class="footnote-ref" id="fnref:86" href="#fn:86"><sup>86</sup></a></li> <li>Type III billows are arrangements of closely spaced, roughly parallel short streaks that mostly resemble cirrus.<a class="footnote-ref" id="fnref:87" href="#fn:87"><sup>87</sup></a></li> <li>Type IV whirls are partial or, more rarely, complete rings of cloud with dark centres.<a class="footnote-ref" id="fnref:88" href="#fn:88"><sup>88</sup></a></li></ol> <h2 id="see-also">See also</h2> <ul> <li>Weather portal</li></ul> <ul><li><a href="/facts/Aeronomy/1WTPMBm6">Aeronomy</a> <ul><li><a href="/facts/Aeronomy_of_Ice_in_the_Mesosphere/4cyr0M0a">Aeronomy of Ice in the Mesosphere</a></li></ul></li> <li><a href="/facts/Cloud_iridescence/CmMGxPh9">Cloud iridescence</a></li> <li><a href="/facts/Iridescent_cloud/CmMGxPh9">Iridescent cloud</a></li> <li><a href="/facts/Polar_stratospheric_cloud/wpQfDlBI">Polar stratospheric cloud</a></li> <li><a href="/facts/Space_jellyfish/KlTdjLGu">Space jellyfish</a></li> <li><a href="/facts/Twilight_phenomenon/UaLRcokj">Twilight phenomenon</a></li></ul> <h2 id="citations">Citations</h2> <h2 id="general-and-cited-references">General and cited references</h2> <ul><li>Gadsden, Michael; Parviainen, Pekka (1995). <a href="https://web.archive.org/web/20081031003710/http://www.iugg.org/IAGA/iaga_pages/pdf/ONC_Sep06.pdf"><i>Observing Noctilucent Clouds</i></a> (PDF). International Association of Geomagnetism & Aeronomy. <a href="/facts/ISBN_(identifier)/15AdSPa9">ISBN</a> 978-0-9650686-0-4. Archived from <a href="http://www.iugg.org/IAGA/iaga_pages/pdf/ONC_Sep06.pdf">the original</a> (PDF) on 31 October 2008. Retrieved 16 October 2008.</li> <li>Schröder, Wilfried (November 2001). <a href="http://ams.allenpress.com/archive/1520-0477/82/11/pdf/i1520-0477-82-11-2457.pdf">"Otto Jesse and the Investigation of Noctilucent Clouds 115 Years Ago"</a> (PDF). <i>Bulletin of the American Meteorological Society</i>. 82 (11): 2457–2468. <a href="/facts/Bibcode_(identifier)/9HtdQSGB">Bibcode</a>:<a href="https://ui.adsabs.harvard.edu/abs/2001BAMS...82.2457S">2001BAMS...82.2457S</a>. <a href="/facts/Doi_(identifier)/muM9Etpq">doi</a>:<a href="https://doi.org/10.1175%2F1520-0477%282001%29082%3C2457%3AOJATIO%3E2.3.CO%3B2">10.1175/1520-0477(2001)082<2457:OJATIO>2.3.CO;2</a>. Retrieved 18 October 2008. [<i>dead link</i>]</li></ul> <h2 id="external-links">External links</h2> Wikimedia Commons has media related to Noctilucent cloud. <ul><li><a href="http://www.misu.su.se/~jacek/nlcmovies.html">NLC time-lapse movies</a></li> <li><a href="http://aim.hamptonu.edu/">AIM satellite mission</a></li> <li><a href="http://news.bbc.co.uk/1/hi/sci/tech/5021778.stm">BBC News Article – Mission to Target Highest Clouds</a></li> <li><a href="http://www.nlcnet.co.uk/">Noctilucent Cloud Observers' Homepage</a></li> <li><a href="https://web.archive.org/web/20051130234721/http://sofiedata.org/">Solar Occultation for Ice Experiment (SOFIE)</a></li> <li><a href="https://sites.google.com/site/fisicaespacialumag/investigacion/proyectos/nlc">Southern Noctilucent Clouds observed at Punta Arenas, Chile</a> <a href="https://web.archive.org/web/20200805031004/https://sites.google.com/site/fisicaespacialumag/investigacion/proyectos/nlc">Archived</a> 2020-08-05 at the <a href="/facts/Wayback_Machine/nmQ3a6JC">Wayback Machine</a></li> <li><a href="https://apod.nasa.gov/apod/ap060718.html">NASA Astronomy Picture of the Day: Noctilucent Clouds Over Sweden (18 July 2006)</a></li> <li><a href="http://news.bbc.co.uk/1/hi/sci/tech/7137905.stm">BBC Article – Spacecraft Chases Highest Clouds</a></li> <li><a href="http://edition.cnn.com/2009/US/09/20/strange.lights/index.html">CNN Article – Rocket launch prompts calls of strange lights in sky</a></li> <li><a href="https://www.bbc.co.uk/news/science-environment-10635796">BBC News – Audio slideshow: Noctilucent clouds</a></li> <li><a href="https://zen.yandex.ru/suite/4b93adf0-738f-4c24-b1e2-a8acfa5f7395">Time-lapse videos playlist of noctilucent clouds observed in Samara, Russia</a></li></ul> <h2 id="references">References</h2> <ol> <li id="fn:1"><p>"Noctilucent clouds: What are they and when can you see them? | Royal Observatory". <a href="https://www.rmg.co.uk/stories/topics/space-astronomy/noctilucent-clouds" target="_blank">https://www.rmg.co.uk/stories/topics/space-astronomy/noctilucent-clouds</a> <a href="#fnref:1" class="footnote-back-ref">↩</a></p></li> <li id="fn:2"><p>"Climate Change Is Responsible for These Rare High-Latitude Clouds". Smithsonian. 2018. <a href="https://www.smithsonianmag.com/smart-news/climate-change-responsible-these-rare-high-latitude-clouds-180969712" target="_blank">https://www.smithsonianmag.com/smart-news/climate-change-responsible-these-rare-high-latitude-clouds-180969712</a> <a href="#fnref:2" class="footnote-back-ref">↩</a></p></li> <li id="fn:3"><p>Robinson made a series of interesting observations between 1849 and 1852, and two of his entries in May 1850 may describe noctilucent clouds. On 1 May 1850, he notes 'strange luminous clouds in NW, not auroral'. This does seem like NLCs even though early May is outside the typical NLC 'window'; however it is still possible as NLCs can form at Armagh's latitude within this period. <a href="#fnref:3" class="footnote-back-ref">↩</a></p></li> <li id="fn:4"><p>Phillips, Tony (August 25, 2008). "Strange Clouds at the Edge of Space". NASA. Archived from the original on February 1, 2010. <a href="https://web.archive.org/web/20100201052153/http://science.nasa.gov/headlines/y2008/25aug_nlc.htm" target="_blank">https://web.archive.org/web/20100201052153/http://science.nasa.gov/headlines/y2008/25aug_nlc.htm</a> <a href="#fnref:4" class="footnote-back-ref">↩</a></p></li> <li id="fn:5"><p>Hsu, Jeremy (3 September 2008). "Strange clouds spotted at the edge of Earth's atmosphere". USA Today. <a href="https://www.usatoday.com/tech/science/space/2008-09-02-strange-clouds-space_N.htm" target="_blank">https://www.usatoday.com/tech/science/space/2008-09-02-strange-clouds-space_N.htm</a> <a href="#fnref:5" class="footnote-back-ref">↩</a></p></li> <li id="fn:6"><p>Simons, Paul (12 May 2008). "Mysterious noctilucent clouds span the heavens". Times Online. Archived from the original on July 24, 2008. Retrieved 6 October 2008. <a href="https://web.archive.org/web/20080724141500/http://www.timesonline.co.uk/tol/news/weather/article3912727.ece" target="_blank">https://web.archive.org/web/20080724141500/http://www.timesonline.co.uk/tol/news/weather/article3912727.ece</a> <a href="#fnref:6" class="footnote-back-ref">↩</a></p></li> <li id="fn:7"><p>Chang, Kenneth (24 July 2007). "First Mission to Explore Those Wisps in the Night Sky". New York Times. Retrieved 5 October 2008. <a href="https://www.nytimes.com/2007/04/24/science/24cloud.html?_r=2&scp=3&sq=noctilucent%20cloud&st=cse&oref=slogin&oref=slogin" target="_blank">https://www.nytimes.com/2007/04/24/science/24cloud.html?_r=2&scp=3&sq=noctilucent%20cloud&st=cse&oref=slogin&oref=slogin</a> <a href="#fnref:7" class="footnote-back-ref">↩</a></p></li> <li id="fn:8"><p>Murray, B.J.; Jensen, E.J. (2000). "Homogeneous nucleation of amorphous solid water particles in the upper mesosphere". Journal of Atmospheric and Solar-Terrestrial Physics. 72 (1): 51–61. Bibcode:2010JASTP..72...51M. doi:10.1016/j.jastp.2009.10.007. <a href="/wiki/Journal_of_Atmospheric_and_Solar-Terrestrial_Physics" target="_blank">/wiki/Journal_of_Atmospheric_and_Solar-Terrestrial_Physics</a> <a href="#fnref:8" class="footnote-back-ref">↩</a></p></li> <li id="fn:9"><p>"Appearance of night-shining clouds has increased". Science Daily. 11 April 2014. 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