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111:, do not inject many particles into the radiation belt, and are relatively frequent — often occurring only a few hours apart from each other. Substorms can be more intense and occur more frequently during a geomagnetic storm when one substorm may start before the previous one has completed. The source of the magnetic disturbances observed at the Earth's surface during geomagnetic storms is the
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spacecraft showing the aurora and Earth's upper atmosphere. The glowing side is the atmosphere lit up by the Sun's light energy and the oval of light is the aurora. During a substorm the auroral oval brightens in a localized area and then suddenly breaks into many different forms that expand both
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107:, and occur once or twice a month during the maximum of the solar cycle and a few times a year during solar minimum. Substorms, on the other hand, take place over a period of a few hours, are observable primarily at the
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In 2012, the THEMIS satellite mission observed the dynamics of rapidly developing substorms, confirming the existence of giant magnetic ropes and witnessed small explosions in the outskirts of Earth's magnetic field.
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satellites have registered the magnetic field dropping to half of its normal strength during a substorm. The most visible indication of a substorm is an increase in the intensity and size of
72:" of the magnetosphere and injected into the high latitude ionosphere. Visually, a substorm is seen as a sudden brightening and increased movement of
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used the term substorm about 1960 which is now the standard term. The morphology of aurora during a substorm was first described by
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in that the latter take place over a period of several days, are observable from anywhere on Earth, inject a large number of
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Short video featuring commentary by David Sibeck, project scientist for the THEMIS mission, discussing a visualization of
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toward Earth's pole and equator. This is exactly what Shun-ichi
Akasofu (1964) drew in his auroral substorm illustration.
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130:, roughly 2% of the total magnetic field strength in that region. The disturbance is much greater in space, as some
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138:. Substorms can be divided into three phases: the growth phase, the expansion phase, and the recovery phase.
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179:"Evolution of the dispersionless injection boundary associated with substorms"
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Akasofu, S.-I. (April 1964). "The development of the auroral substorm".
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http://www.nasa.gov/mission_pages/themis/auroras/northern_lights.html
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165:. New York and Christiania (now Oslo): H. Aschehoug & Co.
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Stern, David P. & Peredo, Mauricio (25 November 2001).
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A series of images made by ultraviolet light imager on the
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NASA Spacecraft Make New
Discoveries About Northern Lights
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76:. Substorms were first described in qualitative terms by
260:. Washington, D.C.: Am. Geophysical Union. p. 488.
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Substorms can cause magnetic field disturbances in the
162:The Norwegian Aurora Polaris Expedition 1902-1903
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68:that causes energy to be released from the "
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177:Sarris, T. & Li, X. (30 March 2005).
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80:which he called polar elementary storms.
88:in 1964 using data collected during the
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16:Short term magnetosphere disturbance
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309:. Southwest Research Institute
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167:out-of-print, full text online
90:International Geophysical Year
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159:Birkeland, Kristian (1913) .
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56:, sometimes referred to as a
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95:Substorms are distinct from
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223:Planetary and Space Science
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207:10.5194/angeo-23-877-2005
258:Magnetospheric Substorms
235:1964P&SS...12..273A
58:magnetospheric substorm
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66:Earth's magnetosphere
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256:Potemra, T. (1991).
105:outer radiation belt
198:2005AnGeo..23..877S
186:Annales Geophysicae
119:at high latitudes.
97:geomagnetic storms
78:Kristian Birkeland
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349:Planetary science
86:Syun-Ichi Akasofu
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82:Sydney Chapman
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311:. Retrieved
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289:. Retrieved
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113:ring current
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74:auroral arcs
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46:reconnection
286:"Substorms"
343:Categories
307:"Substorm"
146:References
117:ionosphere
103:into the
313:24 March
291:21 March
54:substorm
231:Bibcode
194:Bibcode
48:fronts.
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60:or an
359:Earth
182:(PDF)
25:Polar
315:2010
293:2010
262:ISBN
101:ions
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239:doi
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128:nT
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