Knowledge

Solar prominence

Source πŸ“

3405: 4185: 2405: 301: 145: 5131: 1854: 33: 5181: 5205: 5120: 1332: 259:(PIL). The presence of a filament channel is a necessary condition for the formation of a prominence, but a filament channel can exist without containing a prominence. Multiple prominences may form and erupt from within one filament channel over the channel's lifetime. The magnetic field making up the filament channel is predominantly horizontal, pointing in the same direction on both sides of the PIL (see 5157: 5108: 5193: 5169: 237:. The spectra of active region prominences is identical to that of the upper chromosphere having strong He II lines but very weak ionized metal lines. On the other hand, the spectra of quiescent prominences is identical to the spectra measured at 1,500 km (930 mi) in the chromosphere with strong H, He I, and ionized metal lines, but weak He II lines. 367:
PIL with positive magnetic polarity, dextral channels have fibrils which stream to the right and barbs which bear to the right, whereas sinistral channels have fibrils which stream to the left and barbs which bear to the left. Additionally, the overlying magnetic arcades of dextral channels are left-skewed, and those of sinistral channels are right-skewed.
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The horizontally oriented magnetic field causes chromospheric fibrils along the filament channel to lie nearly parallel to the PIL and anti-parallel to one another on opposite sides of the PIL. The directions that these fibrils are oriented depend on the chirality of the channel. On the side of the
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Typical prominences have a narrow structure oriented along the filament channel known as a spine. The spine defines the upper main body of a prominence and is generally in the form of a vertical sheet that diverges towards the photosphere at both ends. Many prominences also have smaller structures
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where they are thermally shielded from the surrounding corona and supported against gravity. These channels are found in the chromosphere and lower corona above divisions between regions of opposite photospheric magnetic polarity known as
136:. The following day, Janssen confirmed his measurements by recording the emission lines from the now unobstructed Sun, a task that had never been done before. Using his new techniques, astronomers were able to study prominences daily. 171:
There are a number of different prominence classification schemes in use today. One of the most widely used and basic schemes classifies prominences based on the magnetic environment in which they had formed. There are three classes:
300: 398: 219:, form in the weak background magnetic field far from any active regions. Unlike active region prominences, quiescent prominences are relatively stable and can have lifetimes ranging from weeks to months, hence the name 330:
which can extend from 50,000 to 70,000 km (31,000 to 43,000 mi) into the corona. Above these arcades, the closed coronal magnetic field may extend radially outward, forming what is known as a
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Prominences form over timescales of about a day and may persist in the corona for several weeks or months, looping hundreds of thousands of kilometers into space. Some prominences may give rise to
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referred to as barbs that similarly diverge from the spine towards the chromosphere and photosphere. Spines and barbs are both composed of thin threads that trace the magnetic field similar to
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The exact mechanism which leads to the formation of solar prominences is not currently known. Models must be able to explain the formation of the filament channel and its hemisphere-dependent
413:. These eruptions can have speeds ranging from 600 km/s to more than 1000 km/s. At least 70% of prominence eruptions are associated with an ejection of coronal material into the 363:
if it is oriented leftward. Dextral channels have been found more frequently in the Sun's northern hemisphere and sinistral channels more frequently in the southern hemisphere.
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When viewed against the background of space (off-limb), they are referred to as prominences; when viewed against the Sun's surface (on-disk), they are referred to as filaments.
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were for the first time able to detect the presence of emission lines from prominences. The detection of a hydrogen line confirmed that prominences were gaseous in nature.
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more often than prominences belonging to the other classes. As a consequence of being located within active regions, active region prominences are usually found in low
164:, was considered a solar prominence. Today, due to a better understanding of the diversity of these phenomena, most of these are classified separately, and the word 307: 86:
A typical prominence extends over many thousands of kilometers; the largest on record was estimated at over 800,000 km (500,000 mi) long, roughly of
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Grayscale H-alpha image of the Solar disk showing quiescent filaments (QF), intermediate filaments (IF), and active region filaments (ARF).
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Prominence material does not occupy the entire width of the filament channel; a tunnel-like region less dense than the corona, known as a
2349: 2344: 2339: 2329: 2003: 1998: 1993: 1988: 1983: 1978: 1973: 2324: 1965: 725:; Ballester, J. L.; Schmieder, B.; Aulanier, G. (April 2010). "Physics of Solar Prominences: II – Magnetic Structure and Dynamics". 631: 72:. While the corona consists of extremely hot plasma, prominences contain much cooler plasma, similar in composition to that of the 1890: 2024: 117:. From these photographs, altitude, emissivity, and many other important parameters were able to be derived for the first time. 702: 667: 310:
H-alpha image of an active region filament showing a spine, two barbs, and chromospheric fibrils oriented parallel to the PIL
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was also able to detect an emission line corresponding to an at the time unknown element now known as
64:'s surface, often in a loop shape. Prominences are anchored to the Sun's surface in the much brighter 5092: 5004: 4999: 1815: 5225: 5019: 5014: 286:
The cool prominence material that makes up spines and barbsβ€”the prominence coreβ€”is surrounded by a
234: 1158:"Prominence Eruptions and Coronal Mass Ejection: A Statistical Study Using Microwave Observations" 468:
Divisions between regions of opposite photospheric magnetic polarity are variously referred to as
225:. Quiescent prominences are typically located at high latitudes around what is referred to as the 5134: 5009: 1945: 1876: 1510: 1156:
Gopalswamy, N.; Shimojo, M.; Lu, W.; Yashiro, S.; Shibasaki, K.; Howard, R. A. (March 20, 2003).
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Historically, any feature that was visible extending above the surface of the sun, including
144: 80: 5082: 2370: 1789: 1759: 1642: 1577: 1394: 1280: 1222: 1169: 1120: 1007: 945: 898: 794: 744: 684: 280: 125: 821:"Time-Latitude Prominence and the Green Corona Distribution over the Solar Activity Cycle" 8: 5209: 5124: 5087: 5050: 1609: 1284: 1226: 1173: 1124: 1011: 949: 902: 798: 748: 83:. Exact mechanism of prominence generation is an ongoing target of scientific research. 5197: 5185: 1695: 1427: 1187: 1138: 1089: 1028: 963: 760: 734: 359: 221: 2382: 2020: 1829: 1744: 1647: 1310: 1253: 1191: 1142: 1093: 1081: 1033: 967: 764: 698: 663: 1550: 886: 233:
Active region and quiescent prominences can also be differentiated by their emitted
5161: 5112: 2376: 1913: 1444: 1350: 1288: 1230: 1177: 1128: 1109:"A Magnetohydrodynamic Description of Coronal Helmet Streamers Containing a Cavity" 1071: 1023: 1015: 953: 906: 865: 832: 752: 690: 606: 99: 53: 353: 5040: 2298: 2293: 2288: 2283: 2278: 2273: 2268: 2263: 2258: 2253: 2248: 2243: 2238: 2233: 2228: 2223: 2218: 2213: 2208: 2203: 2198: 2193: 2188: 2183: 2178: 2173: 2168: 2163: 2158: 2153: 2148: 2143: 2138: 2133: 2128: 2123: 2118: 2113: 2108: 2103: 2098: 2093: 2088: 2083: 2078: 2073: 2068: 2063: 2058: 2053: 2048: 2043: 2038: 2033: 1933: 1769: 1749: 1724: 1619: 1564: 1540: 1417: 332: 321: 782: 270:, occupies the volume between the prominence and the overlying magnetic arcade. 5062: 1928: 1739: 1719: 1714: 1502: 1407: 532: 379:, as well as the origin of the dense plasma that makes up the prominence core. 153: 129: 57: 1076: 1059: 1019: 870: 853: 837: 820: 756: 694: 5219: 5077: 5057: 5035: 1899: 1784: 1779: 1754: 1683: 1673: 1594: 1589: 1584: 1487: 1464: 1449: 1085: 430: 184: 157: 114: 41: 5173: 5045: 1918: 1857: 1764: 1734: 1729: 1690: 1520: 1515: 1492: 1474: 1454: 1037: 336: 87: 73: 69: 993:"Solar prominences: theory and models: Fleshing out the magnetic skeleton" 187:. Active region prominences have lifetimes ranging from hours to days and 1700: 1629: 1614: 1599: 1572: 1482: 1436: 958: 722: 440: 435: 206: 98:
The first detailed description of a solar prominence was in 14th-century
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Solar prominence seen in true color during totality of a Solar eclipse.
32: 689:. Cham Heielberg New York Dordrecht London: Springer. pp. 33–37. 183:, form within the relatively strong magnetic fields at the centers of 1657: 1530: 376: 348: 1799: 1293: 1268: 1235: 1210: 1182: 1157: 1133: 1108: 911: 739: 1868: 1459: 1060:"Filament Channels: Essential Ingredients for Filament Formation" 409:
Some prominences are ejected from the Sun in what is known as a
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Filament channels and their prominence, if present, exhibit
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A solar prominence erupting. False color ultraviolet image.
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if the horizontal magnetic field is oriented rightward and
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is primarily used to refer to larger and cooler features.
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Menzel, Donald H.; Jones, F. Shirley (December 1962).
5145: 884: 1211:"Formation of solar prominences by flux convergence" 1243: 787:
Journal of the Royal Astronomical Society of Canada
1266: 573:"1185: The first description of solar prominences" 555:"1185: The first description of solar prominences" 854:"Observations of Filament Structure and Dynamics" 819:Minarovjech, M.; RybanskΓ½, M.; RuΕ‘in, V. (1998). 326:Above filament channels lie overarching magnetic 250:Prominences form in magnetic structures known as 5217: 1301: 814: 812: 885:Zirin, Harold; Tandberg-Hanssen, Einar (1960). 604: 109:Prominences were first photographed during the 582:. UniversitΓ© de MontrΓ©al. 2008. Archived from 528:"Huge Solar Filament Stretches Across the Sun" 1884: 1358: 809: 683:Vial, Jean-Claude; Engvold, OddbjΓΈrn (2015). 658:Vial, Jean-Claude; Engvold, OddbjΓΈrn (2015). 580:Great Moments in the History of Solar Physics 924: 922: 845: 27:Structure extending off of the Sun's surface 1107:Guo, W. P.; Wu, S. T. (February 10, 1998). 1064:International Astronomical Union Colloquium 986: 984: 858:International Astronomical Union Colloquium 825:International Astronomical Union Colloquium 780: 776: 774: 716: 714: 682: 657: 605:Poitevin, Patrick; Edmonds, Joanne (2003). 1891: 1877: 1365: 1351: 1269:"The mass of a solar quiescent prominence" 1057: 559:Solar Physics Historical Timeline (0–1599) 1292: 1234: 1181: 1132: 1075: 1027: 957: 919: 910: 869: 836: 738: 598: 499: 497: 1209:Galsgaard, K.; Longbottom, A.W. (1999). 981: 771: 711: 653: 651: 649: 647: 645: 643: 525: 519: 392: 143: 31: 928: 851: 676: 636:. Paris: Gauthier-Villars. p. 378. 565: 315: 14: 5218: 990: 783:"Solar Prominence Activity, 1944–1954" 629: 494: 1872: 1346: 1267:Low, B.C.; Fong, B.; Fan, Y. (2003). 1106: 640: 60:structure extending outward from the 446: 245: 288:prominence-corona transition region 273: 24: 1898: 1244:Golub, L.; Pasachoff J.M. (1997). 1202: 991:Gibson, Sarah E. (December 2018). 805:from the original on June 2, 2021. 561:. High Altitude Observatory. 2008. 526:Atkinson, Nancy (August 6, 2012). 25: 5237: 5068:Eclipses in mythology and culture 1324: 931:"Solar Prominences: Observations" 505:"About Filaments and Prominences" 339:or more above the Sun's surface. 139: 5203: 5191: 5179: 5167: 5155: 5130: 5129: 5118: 5106: 5073:List of films featuring eclipses 4183: 3403: 2403: 1853: 1852: 1330: 299: 122:solar eclipse of August 18, 1868 1307:The Nature of Solar Prominences 1149: 1100: 1051: 1000:Living Reviews in Solar Physics 938:Living Reviews in Solar Physics 878: 462: 205:, form between a weak unipolar 68:, and extend outwards into the 623: 547: 453: 335:. These streamers may reach a 260: 111:solar eclipse of July 18, 1860 13: 1: 1835:List of heliophysics missions 487: 240: 188: 48:, sometimes referred to as a 1914:Baily's beads (diamond ring) 1840:Category:Missions to the Sun 474:polarity reversal boundaries 370: 342: 104:solar eclipse of May 1, 1185 7: 1372: 507:. solar.physics.montana.edu 424: 382: 209:regions and active regions. 10: 5242: 1309:. Dordrecht: Kluwer Acad. 1250:Cambridge University Press 852:Engvold, OddbjΓΈrn (1998). 607:"Solar Eclipse Newsletter" 386: 319: 93: 5101: 5093:Solar eclipses in fiction 5028: 4982: 4182: 3402: 2402: 2363: 2307: 2019: 1953: 1944: 1906: 1848: 1822: 1816:G-type main-sequence star 1808: 1666: 1628: 1563: 1501: 1473: 1435: 1426: 1393: 1380: 1162:The Astrophysical Journal 1113:The Astrophysical Journal 1077:10.1017/S0252921100047709 1020:10.1007/s41116-018-0016-2 929:Parenti, Susanna (2014). 891:The Astrophysical Journal 871:10.1017/S0252921100047229 838:10.1017/S0252921100048132 757:10.1007/s11214-010-9628-0 695:10.1007/978-3-319-10416-4 177:Active region prominences 1679:In mythology and culture 470:polarity inversion lines 257:polarity inversion lines 199:Intermediate prominences 5125:Solar System portal 1303:Tandberg-Hanssen, Einar 1058:Gaizauskas, V. (1998). 630:Secchi, Angelo (1870). 181:active region filaments 1546:Supra-arcade downflows 406: 358: 352: 220: 203:intermediate filaments 193:heliographic latitudes 162:coronal mass ejections 149: 81:coronal mass ejections 37: 2409:Total/hybrid eclipses 1526:Coronal mass ejection 1273:Astrophysical Journal 1215:Astrophysical Journal 727:Space Science Reviews 419:coronal mass ejection 404: 389:Coronal mass ejection 281:chromospheric fibrils 213:Quiescent prominences 147: 35: 5113:Astronomy portal 5083:Magnitude of eclipse 1790:Standard solar model 1760:Solar radio emission 1578:List of solar cycles 1339:at Wikimedia Commons 959:10.12942/lrsp-2014-1 316:Overlying structures 5051:Eclipse photography 1610:Magnetic switchback 1285:2003ApJ...594.1060L 1227:1999ApJ...510..444G 1174:2003ApJ...586..562G 1125:1998ApJ...494..419G 1012:2018LRSP...15....7G 950:2014LRSP...11....1P 903:1960ApJ...131..717Z 799:1962JRASC..56..193M 749:2010SSRv..151..333M 411:prominence eruption 217:quiescent filaments 2389:Muhammad's eclipse 1800:Sunlight radiation 1395:Internal structure 407: 150: 38: 5143: 5142: 5088:Planetary transit 2414:next total/hybrid 2398: 2397: 2383:Eclipse of Thales 2371:Mursili's eclipse 1946:Lists of eclipses 1866: 1865: 1830:Solar observatory 1745:Solar observation 1643:Termination shock 1559: 1558: 1511:Transition region 1335:Media related to 704:978-3-319-10416-4 686:Solar prominences 669:978-3-319-10415-7 660:Solar Prominences 633:Le Soleil, Part 1 447:Explanatory notes 402: 252:filament channels 246:Filament channels 102:, describing the 18:Solar prominences 16:(Redirected from 5233: 5208: 5207: 5206: 5196: 5195: 5194: 5184: 5183: 5182: 5172: 5171: 5160: 5159: 5158: 5151: 5133: 5132: 5123: 5122: 5121: 5111: 5110: 5109: 4682: 4193: 4189:Partial eclipses 4187: 3897: 3413: 3409:Annular eclipses 3407: 3107: 2413: 2407: 2377:Assyrian eclipse 1951: 1950: 1924:Solar prominence 1893: 1886: 1879: 1870: 1869: 1856: 1855: 1445:Supergranulation 1433: 1432: 1367: 1360: 1353: 1344: 1343: 1334: 1320: 1298: 1296: 1263: 1246:The Solar Corona 1240: 1238: 1196: 1195: 1185: 1153: 1147: 1146: 1136: 1104: 1098: 1097: 1079: 1055: 1049: 1048: 1046: 1044: 1031: 997: 988: 979: 978: 976: 974: 961: 935: 926: 917: 916: 914: 882: 876: 875: 873: 849: 843: 842: 840: 816: 807: 806: 778: 769: 768: 742: 718: 709: 708: 680: 674: 673: 655: 638: 637: 627: 621: 620: 618: 616: 611: 602: 596: 595: 593: 591: 586:on April 2, 2015 577: 569: 563: 562: 551: 545: 544: 542: 540: 523: 517: 516: 514: 512: 501: 481: 466: 460: 457: 403: 303: 274:Spines and barbs 261:Β§ Chirality 100:Laurentian Codex 21: 5241: 5240: 5236: 5235: 5234: 5232: 5231: 5230: 5226:Solar phenomena 5216: 5215: 5214: 5204: 5202: 5192: 5190: 5180: 5178: 5166: 5156: 5154: 5146: 5144: 5139: 5119: 5117: 5107: 5105: 5097: 5041:Eclipse chasing 5024: 4978: 4680: 4191: 4190: 4188: 4178: 3895: 3411: 3410: 3408: 3398: 3105: 2411: 2410: 2408: 2394: 2359: 2303: 2015: 1940: 1934:helmet streamer 1902: 1897: 1867: 1862: 1844: 1818: 1804: 1770:Solar telescope 1750:Solar phenomena 1725:Solar astronomy 1662: 1624: 1620:Helioseismology 1555: 1541:Helmet streamer 1497: 1469: 1422: 1418:Convection zone 1389: 1376: 1371: 1327: 1317: 1260: 1205: 1203:Further reading 1200: 1199: 1154: 1150: 1105: 1101: 1056: 1052: 1042: 1040: 995: 989: 982: 972: 970: 933: 927: 920: 883: 879: 850: 846: 817: 810: 779: 772: 721:Mackay, D. H.; 719: 712: 705: 681: 677: 670: 656: 641: 628: 624: 614: 612: 609: 603: 599: 589: 587: 575: 571: 570: 566: 553: 552: 548: 538: 536: 524: 520: 510: 508: 503: 502: 495: 490: 485: 484: 467: 463: 458: 454: 449: 427: 393: 391: 385: 373: 345: 333:helmet streamer 324: 322:Helmet streamer 318: 313: 312: 311: 309: 304: 276: 248: 243: 142: 96: 28: 23: 22: 15: 12: 11: 5: 5239: 5229: 5228: 5213: 5212: 5200: 5188: 5176: 5164: 5141: 5140: 5138: 5137: 5127: 5115: 5102: 5099: 5098: 5096: 5095: 5090: 5085: 5080: 5075: 5070: 5065: 5063:Eclipse season 5060: 5055: 5054: 5053: 5048: 5038: 5032: 5030: 5026: 5025: 5023: 5022: 5017: 5012: 5007: 5002: 4997: 4992: 4986: 4984: 4980: 4979: 4977: 4976: 4971: 4966: 4961: 4956: 4951: 4946: 4941: 4936: 4931: 4926: 4921: 4916: 4911: 4906: 4901: 4896: 4891: 4886: 4881: 4876: 4871: 4866: 4861: 4856: 4851: 4846: 4841: 4836: 4831: 4826: 4821: 4816: 4811: 4806: 4801: 4796: 4791: 4786: 4781: 4776: 4771: 4766: 4761: 4756: 4751: 4746: 4741: 4736: 4731: 4726: 4721: 4716: 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3048: 3043: 3038: 3033: 3028: 3023: 3018: 3013: 3008: 3003: 2998: 2993: 2988: 2983: 2978: 2973: 2968: 2963: 2958: 2953: 2948: 2943: 2938: 2933: 2928: 2923: 2918: 2913: 2908: 2903: 2898: 2893: 2888: 2883: 2878: 2873: 2868: 2863: 2858: 2853: 2848: 2843: 2838: 2833: 2828: 2823: 2818: 2813: 2808: 2803: 2798: 2793: 2788: 2783: 2778: 2773: 2768: 2763: 2758: 2753: 2748: 2743: 2738: 2733: 2728: 2723: 2718: 2713: 2708: 2703: 2698: 2693: 2688: 2683: 2678: 2673: 2668: 2663: 2658: 2653: 2648: 2643: 2638: 2633: 2628: 2623: 2618: 2613: 2608: 2603: 2598: 2593: 2588: 2583: 2578: 2573: 2568: 2563: 2558: 2553: 2548: 2543: 2538: 2533: 2528: 2523: 2518: 2513: 2508: 2503: 2498: 2493: 2488: 2483: 2478: 2473: 2468: 2463: 2458: 2453: 2448: 2443: 2438: 2433: 2428: 2423: 2417: 2415: 2400: 2399: 2396: 2395: 2393: 2392: 2386: 2380: 2374: 2367: 2365: 2361: 2360: 2358: 2357: 2352: 2347: 2342: 2337: 2332: 2327: 2322: 2317: 2311: 2309: 2305: 2304: 2302: 2301: 2296: 2291: 2286: 2281: 2276: 2271: 2266: 2261: 2256: 2251: 2246: 2241: 2236: 2231: 2226: 2221: 2216: 2211: 2206: 2201: 2196: 2191: 2186: 2181: 2176: 2171: 2166: 2161: 2156: 2151: 2146: 2141: 2136: 2131: 2126: 2121: 2116: 2111: 2106: 2101: 2096: 2091: 2086: 2081: 2076: 2071: 2066: 2061: 2056: 2051: 2046: 2041: 2036: 2030: 2028: 2017: 2016: 2014: 2013: 2008: 2007: 2006: 2001: 1996: 1991: 1986: 1981: 1976: 1968: 1963: 1957: 1955: 1948: 1942: 1941: 1939: 1938: 1937: 1936: 1929:Stellar corona 1926: 1921: 1916: 1910: 1908: 1904: 1903: 1900:Solar eclipses 1896: 1895: 1888: 1881: 1873: 1864: 1863: 1861: 1860: 1849: 1846: 1845: 1843: 1842: 1837: 1832: 1826: 1824: 1820: 1819: 1814: 1812: 1810:Spectral class 1806: 1805: 1803: 1802: 1797: 1792: 1787: 1782: 1777: 1772: 1767: 1762: 1757: 1752: 1747: 1742: 1740:Solar neutrino 1737: 1732: 1727: 1722: 1720:Solar activity 1717: 1715:Sun in fiction 1712: 1711: 1710: 1709: 1708: 1693: 1688: 1687: 1686: 1681: 1670: 1668: 1664: 1663: 1661: 1660: 1655: 1650: 1645: 1640: 1634: 1632: 1626: 1625: 1623: 1622: 1617: 1612: 1607: 1602: 1597: 1592: 1587: 1582: 1581: 1580: 1569: 1567: 1561: 1560: 1557: 1556: 1554: 1553: 1551:AlfvΓ©n surface 1548: 1543: 1538: 1533: 1528: 1523: 1518: 1513: 1507: 1505: 1499: 1498: 1496: 1495: 1490: 1485: 1479: 1477: 1471: 1470: 1468: 1467: 1462: 1457: 1452: 1447: 1441: 1439: 1430: 1424: 1423: 1421: 1420: 1415: 1410: 1408:Radiation zone 1405: 1399: 1397: 1391: 1390: 1388: 1387: 1381: 1378: 1377: 1370: 1369: 1362: 1355: 1347: 1341: 1340: 1326: 1325:External links 1323: 1322: 1321: 1316:978-0792333746 1315: 1299: 1294:10.1086/377042 1264: 1258: 1241: 1236:10.1086/306559 1221:(1): 444–459. 1204: 1201: 1198: 1197: 1183:10.1086/367614 1168:(1): 562–578. 1148: 1134:10.1086/305196 1119:(1): 419–429. 1099: 1050: 980: 918: 912:10.1086/146884 877: 844: 808: 770: 733:(4): 333–399. 710: 703: 675: 668: 639: 622: 597: 564: 546: 533:Universe Today 518: 492: 491: 489: 486: 483: 482: 461: 451: 450: 448: 445: 444: 443: 438: 433: 426: 423: 384: 381: 372: 369: 344: 341: 320:Main article: 317: 314: 306: 305: 298: 297: 296: 275: 272: 268:coronal cavity 247: 244: 242: 239: 231: 230: 210: 196: 185:active regions 154:solar spicules 141: 140:Classification 138: 130:Pierre Janssen 95: 92: 58:magnetic field 26: 9: 6: 4: 3: 2: 5238: 5227: 5224: 5223: 5221: 5211: 5201: 5199: 5189: 5187: 5177: 5175: 5170: 5165: 5163: 5153: 5152: 5149: 5136: 5128: 5126: 5116: 5114: 5104: 5103: 5100: 5094: 5091: 5089: 5086: 5084: 5081: 5079: 5078:Lunar eclipse 5076: 5074: 5071: 5069: 5066: 5064: 5061: 5059: 5058:Eclipse cycle 5056: 5052: 5049: 5047: 5044: 5043: 5042: 5039: 5037: 5036:Allais effect 5034: 5033: 5031: 5027: 5021: 5018: 5016: 5013: 5011: 5008: 5006: 5003: 5001: 4998: 4996: 4993: 4991: 4988: 4987: 4985: 4981: 4975: 4972: 4970: 4967: 4965: 4962: 4960: 4957: 4955: 4952: 4950: 4947: 4945: 4942: 4940: 4937: 4935: 4932: 4930: 4927: 4925: 4922: 4920: 4917: 4915: 4912: 4910: 4907: 4905: 4902: 4900: 4897: 4895: 4892: 4890: 4887: 4885: 4882: 4880: 4877: 4875: 4872: 4870: 4867: 4865: 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2323: 2321: 2320:British Isles 2318: 2316: 2313: 2312: 2310: 2306: 2300: 2297: 2295: 2292: 2290: 2287: 2285: 2282: 2280: 2277: 2275: 2272: 2270: 2267: 2265: 2262: 2260: 2257: 2255: 2252: 2250: 2247: 2245: 2242: 2240: 2237: 2235: 2232: 2230: 2227: 2225: 2222: 2220: 2217: 2215: 2212: 2210: 2207: 2205: 2202: 2200: 2197: 2195: 2192: 2190: 2187: 2185: 2182: 2180: 2177: 2175: 2172: 2170: 2167: 2165: 2162: 2160: 2157: 2155: 2152: 2150: 2147: 2145: 2142: 2140: 2137: 2135: 2132: 2130: 2127: 2125: 2122: 2120: 2117: 2115: 2112: 2110: 2107: 2105: 2102: 2100: 2097: 2095: 2092: 2090: 2087: 2085: 2082: 2080: 2077: 2075: 2072: 2070: 2067: 2065: 2062: 2060: 2057: 2055: 2052: 2050: 2047: 2045: 2042: 2040: 2037: 2035: 2032: 2031: 2029: 2026: 2022: 2018: 2012: 2009: 2005: 2002: 2000: 1997: 1995: 1992: 1990: 1987: 1985: 1982: 1980: 1977: 1975: 1972: 1971: 1969: 1967: 1964: 1962: 1959: 1958: 1956: 1952: 1949: 1947: 1943: 1935: 1932: 1931: 1930: 1927: 1925: 1922: 1920: 1917: 1915: 1912: 1911: 1909: 1905: 1901: 1894: 1889: 1887: 1882: 1880: 1875: 1874: 1871: 1859: 1851: 1850: 1847: 1841: 1838: 1836: 1833: 1831: 1828: 1827: 1825: 1821: 1817: 1813: 1811: 1807: 1801: 1798: 1796: 1793: 1791: 1788: 1786: 1785:Space weather 1783: 1781: 1780:Space climate 1778: 1776: 1773: 1771: 1768: 1766: 1763: 1761: 1758: 1756: 1755:Solar physics 1753: 1751: 1748: 1746: 1743: 1741: 1738: 1736: 1733: 1731: 1728: 1726: 1723: 1721: 1718: 1716: 1713: 1707: 1704: 1703: 1702: 1699: 1698: 1697: 1694: 1692: 1689: 1685: 1684:Lunar eclipse 1682: 1680: 1677: 1676: 1675: 1672: 1671: 1669: 1665: 1659: 1656: 1654: 1651: 1649: 1646: 1644: 1641: 1639: 1638:Current sheet 1636: 1635: 1633: 1631: 1627: 1621: 1618: 1616: 1613: 1611: 1608: 1606: 1603: 1601: 1598: 1596: 1595:Solar minimum 1593: 1591: 1590:Solar maximum 1588: 1586: 1585:Active region 1583: 1579: 1576: 1575: 1574: 1571: 1570: 1568: 1566: 1562: 1552: 1549: 1547: 1544: 1542: 1539: 1537: 1534: 1532: 1529: 1527: 1524: 1522: 1519: 1517: 1514: 1512: 1509: 1508: 1506: 1504: 1500: 1494: 1491: 1489: 1486: 1484: 1481: 1480: 1478: 1476: 1472: 1466: 1465:Ellerman bomb 1463: 1461: 1458: 1456: 1453: 1451: 1448: 1446: 1443: 1442: 1440: 1438: 1434: 1431: 1429: 1425: 1419: 1416: 1414: 1411: 1409: 1406: 1404: 1401: 1400: 1398: 1396: 1392: 1386: 1383: 1382: 1379: 1375: 1368: 1363: 1361: 1356: 1354: 1349: 1348: 1345: 1338: 1333: 1329: 1328: 1318: 1312: 1308: 1304: 1300: 1295: 1290: 1286: 1282: 1278: 1274: 1270: 1265: 1261: 1259:0-521-48535-5 1255: 1251: 1247: 1242: 1237: 1232: 1228: 1224: 1220: 1216: 1212: 1207: 1206: 1193: 1189: 1184: 1179: 1175: 1171: 1167: 1163: 1159: 1152: 1144: 1140: 1135: 1130: 1126: 1122: 1118: 1114: 1110: 1103: 1095: 1091: 1087: 1083: 1078: 1073: 1069: 1065: 1061: 1054: 1039: 1035: 1030: 1025: 1021: 1017: 1013: 1009: 1005: 1001: 994: 987: 985: 969: 965: 960: 955: 951: 947: 943: 939: 932: 925: 923: 913: 908: 904: 900: 896: 892: 888: 881: 872: 867: 863: 859: 855: 848: 839: 834: 830: 826: 822: 815: 813: 804: 800: 796: 792: 788: 784: 777: 775: 766: 762: 758: 754: 750: 746: 741: 736: 732: 728: 724: 723:Karpen, J. T. 717: 715: 706: 700: 696: 692: 688: 687: 679: 671: 665: 661: 654: 652: 650: 648: 646: 644: 635: 634: 626: 608: 601: 585: 581: 574: 568: 560: 556: 550: 535: 534: 529: 522: 506: 500: 498: 493: 479: 478:neutral lines 475: 471: 465: 456: 452: 442: 439: 437: 434: 432: 431:Active region 429: 428: 422: 420: 416: 412: 390: 380: 378: 368: 364: 362: 361: 356: 355: 350: 340: 338: 334: 329: 323: 308: 302: 295: 293: 289: 284: 282: 271: 269: 264: 262: 258: 253: 238: 236: 228: 224: 223: 218: 214: 211: 208: 204: 200: 197: 194: 190: 186: 182: 178: 175: 174: 173: 169: 167: 163: 159: 158:coronal loops 155: 146: 137: 135: 131: 127: 126:spectroscopes 123: 118: 116: 115:Angelo Secchi 112: 107: 105: 101: 91: 89: 84: 82: 77: 75: 71: 67: 63: 59: 55: 52:, is a large 51: 47: 43: 42:solar physics 34: 30: 19: 5210:Solar System 5046:Solar viewer 4983:Other bodies 4591:31 Jul. 2000 4194:next partial 3414:next annular 2021:Saros series 1923: 1919:Shadow bands 1765:Solar System 1735:Solar energy 1730:Solar dynamo 1691:Heliophysics 1535: 1521:Coronal loop 1516:Coronal hole 1493:Moreton wave 1475:Chromosphere 1306: 1276: 1272: 1245: 1218: 1214: 1165: 1161: 1151: 1116: 1112: 1102: 1067: 1063: 1053: 1041:. Retrieved 1003: 999: 971:. Retrieved 941: 937: 894: 890: 880: 861: 857: 847: 828: 824: 790: 786: 730: 726: 685: 678: 662:. Springer. 659: 632: 625: 613:. Retrieved 600: 588:. Retrieved 584:the original 579: 567: 558: 549: 537:. Retrieved 531: 521: 509:. 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4974:Oct. 2098 4969:Sep. 2098 4964:Apr. 2098 4959:Dec. 2094 4954:Jul. 2094 4949:Jun. 2094 4934:Oct. 2087 4929:Jun. 2087 4909:Aug. 2083 4904:Jul. 2083 4899:Feb. 2083 4894:Nov. 2076 4889:Jul. 2076 4884:Jun. 2076 4869:Oct. 2069 4859:Apr. 2069 4849:Dec. 2065 4844:Aug. 2065 4839:Jul. 2065 4834:Feb. 2065 4829:Sep. 2062 4824:Mar. 2062 4819:Nov. 2058 4814:Jun. 2058 4799:Sep. 2054 4794:Aug. 2054 4789:Mar. 2054 4784:Oct. 2051 4779:Apr. 2051 4769:Dec. 2047 4764:Jul. 2047 4759:Jun. 2047 4754:Jan. 2047 4749:Nov. 2040 4734:Aug. 2036 4729:Jul. 2036 4724:Feb. 2036 4709:Dec. 2029 4704:Jul. 2029 4699:Jun. 2029 4694:Jan. 2029 4689:Sep. 2025 4684:Mar. 2025 4676:Oct. 2022 4671:Apr. 2022 4666:Jan. 2019 4661:Aug. 2018 4656:Jul. 2018 4651:Feb. 2018 4646:Sep. 2015 4641:Oct. 2014 4636:Nov. 2011 4631:Jul. 2011 4626:Jun. 2011 4621:Jan. 2011 4616:Sep. 2007 4611:Mar. 2007 4606:Oct. 2004 4601:Apr. 2004 4596:Dec. 2000 4581:Feb. 2000 4576:Sep. 1997 4571:Oct. 1996 4566:Apr. 1996 4561:Nov. 1993 4551:Dec. 1992 4546:Aug. 1989 4541:Mar. 1989 4536:Apr. 1986 4526:Dec. 1982 4521:Jul. 1982 4516:Jun. 1982 4511:Jan. 1982 4506:Oct. 1978 4501:Apr. 1978 4496:Nov. 1975 4486:Dec. 1974 4481:Aug. 1971 4476:Jul. 1971 4471:Feb. 1971 4466:Mar. 1968 4456:Dec. 1964 4451:Jul. 1964 4446:Jun. 1964 4441:Jan. 1964 4436:Sep. 1960 4431:Mar. 1960 4426:Dec. 1956 4421:Aug. 1953 4416:Jul. 1953 4411:Feb. 1953 4406:Oct. 1949 4401:Apr. 1949 4396:Nov. 1946 4391:Jun. 1946 4381:Jan. 1946 4376:Sep. 1942 4371:Aug. 1942 4366:Mar. 1942 4361:Nov. 1938 4356:Jul. 1935 4351:Jun. 1935 4346:Feb. 1935 4341:Jan. 1935 4336:Oct. 1931 4331:Sep. 1931 4326:Apr. 1931 4321:Nov. 1928 4316:Jun. 1928 4311:Dec. 1927 4306:Aug. 1924 4301:Jul. 1924 4296:Mar. 1924 4291:Nov. 1920 4281:Jul. 1917 4276:Jun. 1917 4271:Jan. 1917 4266:Dec. 1916 4261:Sep. 1913 4256:Aug. 1913 4251:Apr. 1913 4246:Nov. 1910 4241:Dec. 1909 4236:Aug. 1906 4231:Jul. 1906 4226:Feb. 1906 4221:Oct. 1902 4211:Apr. 1902 4206:Nov. 1873 4201:Jan. 1639 4144:Aug. 2092 4139:Feb. 2092 4124:Dec. 2085 4119:Jun. 2085 4079:Jul. 2074 4074:Jan. 2074 4019:Jul. 2056 4014:Jan. 2056 3954:Jul. 2038 3949:Jan. 2038 3726:Dec. 1973 3721:Jan. 1973 3706:Sep. 1969 3701:Mar. 1969 3651:Dec. 1954 3646:Jan. 1954 3636:Sep. 1951 3631:Mar. 1951 3606:Jul. 1944 3561:Aug. 1933 3556:Feb. 1933 3491:Aug. 1915 3486:Feb. 1915 3229:Dec. 2057 3224:Jan. 2057 2806:Jan. 1944 2756:Oct. 1930 2751:Apr. 1930 2686:Oct. 1912 2681:Apr. 1912 2661:Dec. 1908 2656:Jan. 1908 2606:Dec. 1889 2601:Jan. 1889 2373:(1312 BC) 2315:Australia 1961:Antiquity 1658:Bow shock 1565:Variation 1531:Nanoflare 1192:119654267 1143:120452722 1094:124424544 1086:0252-9211 968:122831380 864:: 22–31. 765:118391089 740:1001.1635 615:March 30, 590:March 30, 377:chirality 371:Formation 360:sinistral 349:chirality 343:Chirality 222:quiescent 5220:Category 5135:Category 4924:May 2087 4864:May 2069 4809:May 2058 4744:May 2040 4556:May 1993 4531:May 1985 4491:May 1975 4461:May 1967 4386:May 1946 4286:May 1920 4216:May 1902 2391:(632 AD) 2385:(585 BC) 2379:(763 BC) 1907:Features 1858:Category 1305:(1995). 1038:30872983 1006:(1): 7. 944:(1): 1. 803:Archived 425:See also 383:Eruption 50:filament 5148:Portals 5029:Related 5005:Neptune 5000:Jupiter 2350:Ukraine 1674:Eclipse 1667:Related 1488:Spicule 1460:Sunspot 1455:Faculae 1450:Granule 1374:The Sun 1281:Bibcode 1223:Bibcode 1170:Bibcode 1121:Bibcode 1029:6390890 1008:Bibcode 946:Bibcode 899:Bibcode 795:Bibcode 793:: 193. 745:Bibcode 472:(PIL), 354:dextral 328:arcades 235:spectra 94:History 5020:Uranus 5015:Saturn 2345:Turkey 2340:Russia 2330:Israel 2011:Future 1954:By era 1503:Corona 1313:  1256:  1190:  1141:  1092:  1084:  1036:  1026:  966:  763:  701:  666:  134:helium 54:plasma 5174:Stars 5010:Pluto 2325:China 1615:Flare 1483:Plage 1188:S2CID 1139:S2CID 1090:S2CID 996:(PDF) 964:S2CID 934:(PDF) 761:S2CID 735:arXiv 610:(PDF) 576:(PDF) 215:, or 207:plage 201:, or 189:erupt 179:, or 113:, by 4995:Moon 4990:Mars 4944:2091 4939:2090 4919:2086 4914:2084 4879:2073 4874:2072 4854:2068 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Index

Solar prominences

solar physics
plasma
magnetic field
Sun
photosphere
solar corona
chromosphere
coronal mass ejections
solar radius
Laurentian Codex
solar eclipse of May 1, 1185
solar eclipse of July 18, 1860
Angelo Secchi
solar eclipse of August 18, 1868
spectroscopes
Pierre Janssen
helium

solar spicules
coronal loops
coronal mass ejections
active regions
erupt
heliographic latitudes
plage
quiescent
spectra
Β§ Chirality

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