Knowledge

Helmet streamer

Source πŸ“

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of pseudostreamers was described as "contain twin filaments at its base. Such twin filaments are topologically connected, sharing a neutral point and a separatrix dome. This was a case in which two polarity reversal boundaries contain between them fields with a polarity opposite to that of the global
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It consists of a pair of filament channels near the south pole of the Sun. On the western edge of the structure, the magnetic morphology above the filaments is that of a side-by-side double streamer, with open field between the two channels. On the eastern edge, the magnetic morphology is that of a
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Upon the eruption of a coronal mass ejection (CME), the overlying helmet streamer deforms becoming the CME's leading edge. Similarly, the helmet streamer's cavity becomes the CME's cavity and the helmet streamer's prominence becomes the CME's core.
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and called a "plasma sheets" by Hundhausen (1972). They were later renamed to "unipolar streamers" by Zhao & Webb (2003) and then termed "pseudostreamers" by Wang et al. (2007). Pseudostreamers' structure was observed in 2012 by the
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Helmet streamers during a total solar eclipse, photographed using exposure bracketing to show both the Sun's corona and the surface features of the new moon itself, illuminated by earthshine. A few
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and near the solar maximum of solar cycle 23 demonstrate the different distributions of helmet streamers around the solar disk at different points in a solar cycle.
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Single hybrid magnetic structure that consists of double-streamer/pseudostreamer was observed in the solar corona on May 5-10, 2013 by the SWAP instrument of the
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Panasenco, Olga; Martin, Sara F.; Velli, Marco; Vourlidas, Angelos (2012). "Origins of Rolling, Twisting, and Non-radial Propagation of Eruptive Solar Events".
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Small blobs of plasma, or "plasmoids" are sometimes released from the tips of helmet streamers, and this is one source of the slow component of the solar wind.
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The white-light emissions of helmet streamers is due to the high electron density of the confined plasma relative to the surrounding corona. Light from the
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Helmet streamers have cusp-like bases that taper radially outward away from the Sun forming long stalks. The base typically extends up to 1.5
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Masson, Sophie; McCauley, Patrick; Golub, Leon; Reeves, Katharine K.; DeLuca, Edward E. (13 May 2014). "Dynamics of the Transition Corona".
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off of these electrons with the intensity of scattered light depending on the number of electrons along the observer's line of sight.
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Structures in the corona, similar to a helmet streamer, but connecting holes of the same magnetic polarity, are called
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Scott, Roger B.; Pontin, David I.; Antiochos, Spiro K.; DeVore, C. Richard; Wyper, Peter F. (1 May 2021).
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Helmet streamers are structured by closed magnetic fields and lie above boundaries separating opposite
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Space Physics: An Introduction to Plasmas and Particles in the Heliosphere and Magnetospheres
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Wang, Y.-M.; Sheeley, N. R.; Socker, D. G.; Howard, R. A.; Rich, N. B. (1 November 2000).
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Rachmeler, L. A.; Platten, S. J.; Bethge, C.; Seaton, D. B.; Yeates, A. R. (1 May 2014).
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Helmet streamers appear bright in white-light relative to the surrounding coronal plasma.
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passed through the Sun's corona in early 2021, the spacecraft flew by coronal streamers.
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loops which lie above divisions between regions of opposite magnetic polarity on the
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unipolar configuration surrounding them (tripolar pseudostreamer)."
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Material was copied from this source, which is available under a
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above the surface, whereas the stalkβ€”stretched outward by the
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they are found more symmetrically distributed around the Sun.
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Wang, Y.-M.; Sheeley, Jr., N. R.; Rich, N. B. (April 2007).
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elongates these loops to pointed tips which can extend a
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satellite. Its structure was described by researchers:
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coronal pseudostreamer without the central open field.
648: 541:"Coronal mass ejections: Initiation and detection" 221: 4683: 368: 534: 532: 432:Journal of Geophysical Research: Space Physics 331: 329: 1420: 894: 265:. They were first observed using space-borne 42:, are elongated cusp-like structures in the 529: 428:"The dynamical nature of coronal streamers" 369:Koutchmy, Serge; Livshits, Moissei (1992). 326: 1427: 1413: 901: 887: 593:"The Dynamic Formation of Pseudostreamers" 538: 335: 851: 825: 776: 712: 616: 512: 502: 484: 451: 694: 692: 421: 419: 225: 96: 18: 758: 756: 466: 50:which are often visible in white-light 4684: 1408: 882: 689: 416: 207:taken near the solar minimum between 753: 586: 584: 113:β€”can extend over many solar radii. 13: 1434: 256: 14: 4708: 4604:Eclipses in mythology and culture 581: 4666: 4665: 4654: 4642: 4609:List of films featuring eclipses 3719: 2939: 1939: 1389: 1388: 638:Creative Commons Attribution 4.0 631: 191: 179: 801: 539:Gopalswamy, N. (January 2003). 473:Living Reviews in Solar Physics 642: 460: 362: 336:Kallenrode, May-Britt (2004). 222:Role in coronal mass ejections 145: 1: 1371:List of heliophysics missions 568:10.1016/S0273-1177(02)00888-8 319: 16:Structure in the Sun's corona 1450:Baily's beads (diamond ring) 1376:Category:Missions to the Sun 344:. Berlin: Springer. p.  92: 7: 908: 731:10.1088/0004-637X/787/2/145 467:Cranmer, Steven R. (2009). 297: 10: 4713: 844:10.1088/2041-8205/787/1/L3 548:Advances in Space Research 272:Solar Dynamics Observatory 245: 149: 4637: 4629:Solar eclipses in fiction 4564: 4518: 3718: 2938: 1938: 1899: 1843: 1555: 1489: 1480: 1442: 1384: 1358: 1352:G-type main-sequence star 1344: 1202: 1164: 1099: 1037: 1009: 971: 962: 929: 916: 814:The Astrophysical Journal 787:10.1007/s11207-012-0194-3 701:The Astrophysical Journal 655:The Astrophysical Journal 651:"Coronal Pseudostreamers" 597:The Astrophysical Journal 1215:In mythology and culture 618:10.3847/1538-4357/abec4f 4661:Solar System portal 27:are visible around the 1082:Supra-arcade downflows 295: 243: 102: 32: 1945:Total/hybrid eclipses 1062:Coronal mass ejection 375:Space Science Reviews 290: 248:Coronal mass ejection 246:Further information: 237: 150:Further information: 128:lower in the corona. 100: 22: 4649:Astronomy portal 4619:Magnitude of eclipse 1326:Standard solar model 1296:Solar radio emission 1114:List of solar cycles 504:10.12942/lrsp-2009-3 453:10.1029/2000JA000149 438:(A11): 25133–25142. 314:Solar radio emission 304:List of solar cycles 4587:Eclipse photography 1146:Magnetic switchback 836:2014ApJ...787L...3R 723:2014ApJ...787..145M 667:2007ApJ...658.1340W 609:2021ApJ...913...64S 560:2003AdSpR..31..869G 495:2009LRSP....6....3C 444:2000JGR...10525133W 387:1992SSRv...61..393K 371:"Coronal streamers" 1925:Muhammad's eclipse 1336:Sunlight radiation 931:Internal structure 395:10.1007/BF00222313 244: 240:Parker Solar Probe 103: 58:. They are closed 33: 4679: 4678: 4624:Planetary transit 1950:next total/hybrid 1934: 1933: 1919:Eclipse of Thales 1907:Mursili's eclipse 1482:Lists of eclipses 1402: 1401: 1366:Solar observatory 1281:Solar observation 1179:Termination shock 1095: 1094: 1047:Transition region 278:Magnetic topology 235: 137:Thomson scattered 118:magnetic polarity 74:or more into the 40:coronal streamers 25:solar prominences 4704: 4669: 4668: 4659: 4658: 4657: 4647: 4646: 4645: 4218: 3729: 3725:Partial eclipses 3723: 3433: 2949: 2945:Annular eclipses 2943: 2643: 1949: 1943: 1913:Assyrian eclipse 1487: 1486: 1460:Solar prominence 1429: 1422: 1415: 1406: 1405: 1392: 1391: 981:Supergranulation 969: 968: 903: 896: 889: 880: 879: 873: 872: 870: 868: 855: 829: 805: 799: 798: 780: 771:(1–2): 391–413. 760: 751: 750: 739:2060/20150008396 716: 696: 687: 686: 661:(2): 1340–1348. 646: 640: 635: 630: 620: 588: 579: 578: 576: 574: 545: 536: 527: 526: 516: 506: 488: 464: 458: 457: 455: 423: 414: 413: 411: 409: 366: 360: 359: 343: 333: 236: 195: 183: 38:, also known as 36:Helmet streamers 4712: 4711: 4707: 4706: 4705: 4703: 4702: 4701: 4697:Solar phenomena 4682: 4681: 4680: 4675: 4655: 4653: 4643: 4641: 4633: 4577:Eclipse chasing 4560: 4514: 4216: 3727: 3726: 3724: 3714: 3431: 2947: 2946: 2944: 2934: 2641: 1947: 1946: 1944: 1930: 1895: 1839: 1551: 1476: 1470:helmet streamer 1438: 1433: 1403: 1398: 1380: 1354: 1340: 1306:Solar telescope 1286:Solar phenomena 1261:Solar astronomy 1198: 1160: 1156:Helioseismology 1091: 1077:Helmet streamer 1033: 1005: 958: 954:Convection zone 925: 912: 907: 877: 876: 866: 864: 806: 802: 761: 754: 697: 690: 647: 643: 589: 582: 572: 570: 543: 537: 530: 469:"Coronal Holes" 465: 461: 424: 417: 407: 405: 367: 363: 356: 334: 327: 322: 300: 263:pseudostreamers 259: 257:Pseudostreamers 250: 226: 224: 219: 218: 217: 216: 209:solar cycles 22 201: 200: 199: 196: 188: 187: 184: 154: 148: 95: 17: 12: 11: 5: 4710: 4700: 4699: 4694: 4677: 4676: 4674: 4673: 4663: 4651: 4638: 4635: 4634: 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1439: 1436:Solar eclipses 1432: 1431: 1424: 1417: 1409: 1400: 1399: 1397: 1396: 1385: 1382: 1381: 1379: 1378: 1373: 1368: 1362: 1360: 1356: 1355: 1350: 1348: 1346:Spectral class 1342: 1341: 1339: 1338: 1333: 1328: 1323: 1318: 1313: 1308: 1303: 1298: 1293: 1288: 1283: 1278: 1276:Solar neutrino 1273: 1268: 1263: 1258: 1256:Solar activity 1253: 1251:Sun in fiction 1248: 1247: 1246: 1245: 1244: 1229: 1224: 1223: 1222: 1217: 1206: 1204: 1200: 1199: 1197: 1196: 1191: 1186: 1181: 1176: 1170: 1168: 1162: 1161: 1159: 1158: 1153: 1148: 1143: 1138: 1133: 1128: 1123: 1118: 1117: 1116: 1105: 1103: 1097: 1096: 1093: 1092: 1090: 1089: 1087:AlfvΓ©n surface 1084: 1079: 1074: 1069: 1064: 1059: 1054: 1049: 1043: 1041: 1035: 1034: 1032: 1031: 1026: 1021: 1015: 1013: 1007: 1006: 1004: 1003: 998: 993: 988: 983: 977: 975: 966: 960: 959: 957: 956: 951: 946: 944:Radiation zone 941: 935: 933: 927: 926: 924: 923: 917: 914: 913: 906: 905: 898: 891: 883: 875: 874: 800: 752: 688: 675:10.1086/511416 641: 580: 554:(4): 869–881. 528: 459: 415: 361: 354: 324: 323: 321: 318: 317: 316: 311: 306: 299: 296: 258: 255: 223: 220: 203: 202: 197: 190: 189: 185: 178: 177: 176: 175: 174: 147: 144: 94: 91: 56:solar eclipses 15: 9: 6: 4: 3: 2: 4709: 4698: 4695: 4693: 4690: 4689: 4687: 4672: 4664: 4662: 4652: 4650: 4640: 4639: 4636: 4630: 4627: 4625: 4622: 4620: 4617: 4615: 4614:Lunar eclipse 4612: 4610: 4607: 4605: 4602: 4600: 4597: 4595: 4594:Eclipse cycle 4592: 4588: 4585: 4583: 4580: 4579: 4578: 4575: 4573: 4572:Allais effect 4570: 4569: 4567: 4563: 4557: 4554: 4552: 4549: 4547: 4544: 4542: 4539: 4537: 4534: 4532: 4529: 4527: 4524: 4523: 4521: 4517: 4511: 4508: 4506: 4503: 4501: 4498: 4496: 4493: 4491: 4488: 4486: 4483: 4481: 4478: 4476: 4473: 4471: 4468: 4466: 4463: 4461: 4458: 4456: 4453: 4451: 4448: 4446: 4443: 4441: 4438: 4436: 4433: 4431: 4428: 4426: 4423: 4421: 4418: 4416: 4413: 4411: 4408: 4406: 4403: 4401: 4398: 4396: 4393: 4391: 4388: 4386: 4383: 4381: 4378: 4376: 4373: 4371: 4368: 4366: 4363: 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1826: 1823: 1821: 1818: 1816: 1813: 1811: 1808: 1806: 1803: 1801: 1798: 1796: 1793: 1791: 1788: 1786: 1783: 1781: 1778: 1776: 1773: 1771: 1768: 1766: 1763: 1761: 1758: 1756: 1753: 1751: 1748: 1746: 1743: 1741: 1738: 1736: 1733: 1731: 1728: 1726: 1723: 1721: 1718: 1716: 1713: 1711: 1708: 1706: 1703: 1701: 1698: 1696: 1693: 1691: 1688: 1686: 1683: 1681: 1678: 1676: 1673: 1671: 1668: 1666: 1663: 1661: 1658: 1656: 1653: 1651: 1648: 1646: 1643: 1641: 1638: 1636: 1633: 1631: 1628: 1626: 1623: 1621: 1618: 1616: 1613: 1611: 1608: 1606: 1603: 1601: 1598: 1596: 1593: 1591: 1588: 1586: 1583: 1581: 1578: 1576: 1573: 1571: 1568: 1567: 1565: 1562: 1558: 1554: 1548: 1545: 1541: 1538: 1536: 1533: 1531: 1528: 1526: 1523: 1521: 1518: 1516: 1513: 1511: 1508: 1507: 1505: 1503: 1500: 1498: 1495: 1494: 1492: 1488: 1485: 1483: 1479: 1471: 1468: 1467: 1466: 1463: 1461: 1458: 1456: 1453: 1451: 1448: 1447: 1445: 1441: 1437: 1430: 1425: 1423: 1418: 1416: 1411: 1410: 1407: 1395: 1387: 1386: 1383: 1377: 1374: 1372: 1369: 1367: 1364: 1363: 1361: 1357: 1353: 1349: 1347: 1343: 1337: 1334: 1332: 1329: 1327: 1324: 1322: 1321:Space weather 1319: 1317: 1316:Space climate 1314: 1312: 1309: 1307: 1304: 1302: 1299: 1297: 1294: 1292: 1291:Solar physics 1289: 1287: 1284: 1282: 1279: 1277: 1274: 1272: 1269: 1267: 1264: 1262: 1259: 1257: 1254: 1252: 1249: 1243: 1240: 1239: 1238: 1235: 1234: 1233: 1230: 1228: 1225: 1221: 1220:Lunar eclipse 1218: 1216: 1213: 1212: 1211: 1208: 1207: 1205: 1201: 1195: 1192: 1190: 1187: 1185: 1182: 1180: 1177: 1175: 1174:Current sheet 1172: 1171: 1169: 1167: 1163: 1157: 1154: 1152: 1149: 1147: 1144: 1142: 1139: 1137: 1134: 1132: 1131:Solar minimum 1129: 1127: 1126:Solar maximum 1124: 1122: 1121:Active region 1119: 1115: 1112: 1111: 1110: 1107: 1106: 1104: 1102: 1098: 1088: 1085: 1083: 1080: 1078: 1075: 1073: 1070: 1068: 1065: 1063: 1060: 1058: 1055: 1053: 1050: 1048: 1045: 1044: 1042: 1040: 1036: 1030: 1027: 1025: 1022: 1020: 1017: 1016: 1014: 1012: 1008: 1002: 1001:Ellerman bomb 999: 997: 994: 992: 989: 987: 984: 982: 979: 978: 976: 974: 970: 967: 965: 961: 955: 952: 950: 947: 945: 942: 940: 937: 936: 934: 932: 928: 922: 919: 918: 915: 911: 904: 899: 897: 892: 890: 885: 884: 881: 863: 859: 854: 849: 845: 841: 837: 833: 828: 823: 819: 815: 811: 804: 796: 792: 788: 784: 779: 774: 770: 766: 765:Solar Physics 759: 757: 748: 744: 740: 736: 732: 728: 724: 720: 715: 710: 706: 702: 695: 693: 684: 680: 676: 672: 668: 664: 660: 656: 652: 645: 639: 634: 628: 624: 619: 614: 610: 606: 602: 598: 594: 587: 585: 569: 565: 561: 557: 553: 549: 542: 535: 533: 524: 520: 515: 510: 505: 500: 496: 492: 487: 482: 478: 474: 470: 463: 454: 449: 445: 441: 437: 433: 429: 422: 420: 404: 400: 396: 392: 388: 384: 380: 376: 372: 365: 357: 355:3-540-20617-5 351: 347: 342: 341: 332: 330: 325: 315: 312: 310: 307: 305: 302: 301: 294: 289: 287: 282: 279: 275: 273: 268: 264: 254: 249: 241: 214: 210: 206: 198:Solar maximum 194: 186:Solar minimum 182: 173: 171: 170:solar maximum 167: 166:streamer belt 163: 159: 158:solar minimum 153: 143: 140: 138: 134: 129: 127: 126:coronal holes 123: 120:in the Sun's 119: 114: 112: 108: 99: 90: 88: 87:solar maximum 84: 83:solar minimum 79: 77: 73: 69: 65: 64:Sun's surface 61: 57: 53: 49: 45: 41: 37: 30: 26: 21: 4582:Solar viewer 4519:Other bodies 4127:31 Jul. 2000 3730:next partial 2950:next annular 1557:Saros series 1469: 1455:Shadow bands 1301:Solar System 1271:Solar energy 1266:Solar dynamo 1227:Heliophysics 1076: 1057:Coronal loop 1052:Coronal hole 1029:Moreton wave 1011:Chromosphere 865:. 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Retrieved 381:(3–4): 393. 378: 374: 364: 339: 309:Coronal loop 291: 283: 276: 267:coronagraphs 262: 260: 251: 205:Coronagraphs 165: 155: 141: 130: 115: 104: 80: 72:solar radius 52:coronagraphs 39: 35: 34: 4122:1 Jul. 2000 1871:Philippines 1506:Modern era 1502:Middle Ages 1359:Exploration 1237:Solar deity 1184:Heliosheath 1166:Heliosphere 1136:Wolf number 1109:Solar cycle 973:Photosphere 162:solar cycle 152:Solar cycle 146:Solar cycle 133:photosphere 122:photosphere 107:solar radii 54:and during 4686:Categories 1900:Historical 1844:Visibility 1311:Solar time 1232:In culture 1189:Heliopause 1141:Solar wind 1072:Prominence 964:Atmosphere 949:Tachocline 853:10023/5318 707:(2): 145. 320:References 111:solar wind 68:solar wind 29:lunar limb 4510:Oct. 2098 4505:Sep. 2098 4500:Apr. 2098 4495:Dec. 2094 4490:Jul. 2094 4485:Jun. 2094 4470:Oct. 2087 4465:Jun. 2087 4445:Aug. 2083 4440:Jul. 2083 4435:Feb. 2083 4430:Nov. 2076 4425:Jul. 2076 4420:Jun. 2076 4405:Oct. 2069 4395:Apr. 2069 4385:Dec. 2065 4380:Aug. 2065 4375:Jul. 2065 4370:Feb. 2065 4365:Sep. 2062 4360:Mar. 2062 4355:Nov. 2058 4350:Jun. 2058 4335:Sep. 2054 4330:Aug. 2054 4325:Mar. 2054 4320:Oct. 2051 4315:Apr. 2051 4305:Dec. 2047 4300:Jul. 2047 4295:Jun. 2047 4290:Jan. 2047 4285:Nov. 2040 4270:Aug. 2036 4265:Jul. 2036 4260:Feb. 2036 4245:Dec. 2029 4240:Jul. 2029 4235:Jun. 2029 4230:Jan. 2029 4225:Sep. 2025 4220:Mar. 2025 4212:Oct. 2022 4207:Apr. 2022 4202:Jan. 2019 4197:Aug. 2018 4192:Jul. 2018 4187:Feb. 2018 4182:Sep. 2015 4177:Oct. 2014 4172:Nov. 2011 4167:Jul. 2011 4162:Jun. 2011 4157:Jan. 2011 4152:Sep. 2007 4147:Mar. 2007 4142:Oct. 2004 4137:Apr. 2004 4132:Dec. 2000 4117:Feb. 2000 4112:Sep. 1997 4107:Oct. 1996 4102:Apr. 1996 4097:Nov. 1993 4087:Dec. 1992 4082:Aug. 1989 4077:Mar. 1989 4072:Apr. 1986 4062:Dec. 1982 4057:Jul. 1982 4052:Jun. 1982 4047:Jan. 1982 4042:Oct. 1978 4037:Apr. 1978 4032:Nov. 1975 4022:Dec. 1974 4017:Aug. 1971 4012:Jul. 1971 4007:Feb. 1971 4002:Mar. 1968 3992:Dec. 1964 3987:Jul. 1964 3982:Jun. 1964 3977:Jan. 1964 3972:Sep. 1960 3967:Mar. 1960 3962:Dec. 1956 3957:Aug. 1953 3952:Jul. 1953 3947:Feb. 1953 3942:Oct. 1949 3937:Apr. 1949 3932:Nov. 1946 3927:Jun. 1946 3917:Jan. 1946 3912:Sep. 1942 3907:Aug. 1942 3902:Mar. 1942 3897:Nov. 1938 3892:Jul. 1935 3887:Jun. 1935 3882:Feb. 1935 3877:Jan. 1935 3872:Oct. 1931 3867:Sep. 1931 3862:Apr. 1931 3857:Nov. 1928 3852:Jun. 1928 3847:Dec. 1927 3842:Aug. 1924 3837:Jul. 1924 3832:Mar. 1924 3827:Nov. 1920 3817:Jul. 1917 3812:Jun. 1917 3807:Jan. 1917 3802:Dec. 1916 3797:Sep. 1913 3792:Aug. 1913 3787:Apr. 1913 3782:Nov. 1910 3777:Dec. 1909 3772:Aug. 1906 3767:Jul. 1906 3762:Feb. 1906 3757:Oct. 1902 3747:Apr. 1902 3742:Nov. 1873 3737:Jan. 1639 3680:Aug. 2092 3675:Feb. 2092 3660:Dec. 2085 3655:Jun. 2085 3615:Jul. 2074 3610:Jan. 2074 3555:Jul. 2056 3550:Jan. 2056 3490:Jul. 2038 3485:Jan. 2038 3262:Dec. 1973 3257:Jan. 1973 3242:Sep. 1969 3237:Mar. 1969 3187:Dec. 1954 3182:Jan. 1954 3172:Sep. 1951 3167:Mar. 1951 3142:Jul. 1944 3097:Aug. 1933 3092:Feb. 1933 3027:Aug. 1915 3022:Feb. 1915 2765:Dec. 2057 2760:Jan. 2057 2342:Jan. 1944 2292:Oct. 1930 2287:Apr. 1930 2222:Oct. 1912 2217:Apr. 1912 2197:Dec. 1908 2192:Jan. 1908 2142:Dec. 1889 2137:Jan. 1889 1909:(1312 BC) 1851:Australia 1497:Antiquity 1194:Bow shock 1101:Variation 1067:Nanoflare 862:0004-637X 827:1312.3153 820:(1): L3. 795:118374791 778:1211.1376 747:119182452 714:1301.0740 683:250768165 627:235281960 603:(1): 64. 573:27 August 486:0909.2847 403:189775835 93:Structure 4671:Category 4460:May 2087 4400:May 2069 4345:May 2058 4280:May 2040 4092:May 1993 4067:May 1985 4027:May 1975 3997:May 1967 3922:May 1946 3822:May 1920 3752:May 1902 1927:(632 AD) 1921:(585 BC) 1915:(763 BC) 1443:Features 1394:Category 867:10 March 523:27194961 479:(1): 3. 298:See also 60:magnetic 4565:Related 4541:Neptune 4536:Jupiter 1886:Ukraine 1210:Eclipse 1203:Related 1024:Spicule 996:Sunspot 991:Faculae 986:Granule 910:The Sun 832:Bibcode 719:Bibcode 663:Bibcode 605:Bibcode 556:Bibcode 514:4841186 491:Bibcode 440:Bibcode 408:30 July 383:Bibcode 156:Around 81:During 4556:Uranus 4551:Saturn 1881:Turkey 1876:Russia 1866:Israel 1547:Future 1490:By era 1039:Corona 860:  793:  745:  681:  625:  521:  511:  401:  352:  286:PROBA2 76:corona 66:. 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Index


solar prominences
lunar limb
Sun
corona
coronagraphs
solar eclipses
magnetic
Sun's surface
solar wind
solar radius
corona
solar minimum
solar maximum

solar radii
solar wind
magnetic polarity
photosphere
coronal holes
photosphere
Thomson scattered
Solar cycle
solar minimum
solar cycle
solar maximum


Coronagraphs
solar cycles 22

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