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Substorm

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33: 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 20: 36: 40: 38: 34: 39: 27:
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
37: 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 141:
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 84:
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.
265: 130:, roughly 2% of the total magnetic field strength in that region. The disturbance is much greater in space, as some 115:, whereas the sources of magnetic disturbances observed on the ground during substorms are electric currents in the 89: 81: 138:. Substorms can be divided into three phases: the growth phase, the expansion phase, and the recovery phase. 330: 348: 65: 353: 45: 234: 178: 306: 230: 193: 104: 8: 160: 197: 135: 123: 77: 73: 261: 242: 96: 85: 24: 238: 201: 358: 131: 285: 206: 179:"Evolution of the dispersionless injection boundary associated with substorms" 342: 108: 127: 112: 69: 221:
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
19: 283: 165:. New York and Christiania (now Oslo): H. Aschehoug & Co. 284:
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
100: 76:. Substorms were first described in qualitative terms by 260:. Washington, D.C.: Am. Geophysical Union. p. 488. 122:
Substorms can cause magnetic field disturbances in the
162:The Norwegian Aurora Polaris Expedition 1902-1903 340: 176: 220: 68:that causes energy to be released from the " 205: 177:Sarris, T. & Li, X. (30 March 2005). 158: 80:which he called polar elementary storms. 88:in 1964 using data collected during the 31: 18: 279: 277: 255: 341: 299: 274: 16:Short term magnetosphere disturbance 152: 13: 14: 370: 64:, is a brief disturbance in the 126:up to a magnitude of 1000  321: 309:. Southwest Research Institute 249: 214: 170: 167:out-of-print, full text online 90:International Geophysical Year 1: 159:Birkeland, Kristian (1913) . 145: 56:, sometimes referred to as a 243:10.1016/0032-0633(64)90151-5 95:Substorms are distinct from 7: 223:Planetary and Space Science 10: 375: 207:10.5194/angeo-23-877-2005 258:Magnetospheric Substorms 235:1964P&SS...12..273A 58:magnetospheric substorm 49: 29: 66:Earth's magnetosphere 43: 22: 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 50: 30: 349:Planetary science 86:Syun-Ichi Akasofu 41: 366: 333: 325: 319: 318: 316: 314: 303: 297: 296: 294: 292: 281: 272: 271: 253: 247: 246: 218: 212: 211: 209: 183: 174: 168: 166: 156: 62:auroral substorm 42: 374: 373: 369: 368: 367: 365: 364: 363: 339: 338: 337: 336: 326: 322: 312: 310: 305: 304: 300: 290: 288: 282: 275: 268: 254: 250: 219: 215: 181: 175: 171: 157: 153: 148: 32: 17: 12: 11: 5: 372: 362: 361: 356: 351: 335: 334: 320: 298: 273: 266: 248: 229:(4): 273–282. 213: 192:(3): 877–884. 169: 150: 149: 147: 144: 132:geosynchronous 82:Sydney Chapman 15: 9: 6: 4: 3: 2: 371: 360: 357: 355: 352: 350: 347: 346: 344: 332: 329: 324: 308: 302: 287: 280: 278: 269: 267:0-87590-030-5 263: 259: 252: 244: 240: 236: 232: 228: 224: 217: 208: 203: 199: 195: 191: 187: 180: 173: 164: 163: 155: 151: 143: 139: 137: 136:polar auroras 133: 129: 125: 124:auroral zones 120: 118: 114: 110: 109:polar regions 106: 102: 98: 93: 91: 87: 83: 79: 75: 71: 67: 63: 59: 55: 47: 26: 21: 354:Geomagnetism 327: 323: 311:. Retrieved 301: 289:. Retrieved 257: 251: 226: 222: 216: 189: 185: 172: 161: 154: 140: 121: 113:ring current 94: 74:auroral arcs 61: 57: 53: 51: 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. 264:  60:or an 359:Earth 182:(PDF) 25:Polar 315:2010 293:2010 262:ISBN 101:ions 70:tail 239:doi 202:doi 345:: 276:^ 237:. 227:12 225:. 200:. 190:23 188:. 184:. 128:nT 92:. 52:A 317:. 295:. 270:. 245:. 241:: 233:: 210:. 204:: 196::

Index


Polar
reconnection
Earth's magnetosphere
tail
auroral arcs
Kristian Birkeland
Sydney Chapman
Syun-Ichi Akasofu
International Geophysical Year
geomagnetic storms
ions
outer radiation belt
polar regions
ring current
ionosphere
auroral zones
nT
geosynchronous
polar auroras
The Norwegian Aurora Polaris Expedition 1902-1903
"Evolution of the dispersionless injection boundary associated with substorms"
Bibcode
2005AnGeo..23..877S
doi
10.5194/angeo-23-877-2005
Bibcode
1964P&SS...12..273A
doi
10.1016/0032-0633(64)90151-5

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