Knowledge

Solar physics

Source 📝

370: 251: 1513: 209: 356: 94:
knowledge, especially those written in Greek. This, plus de-urbanisation and diseases such as the Black Death led to a decline in scientific knowledge in Medieval Europe, especially in the early Middle Ages. During this period, observations of the Sun were taken either in relation to the zodiac, or to assist in building places of worship such as churches and cathedrals.
89:
Solar observations were taken with the purpose of navigation, but mostly for timekeeping. Islam requires its followers to pray five times a day, at specific position of the Sun in the sky. As such, accurate observations of the Sun and its trajectory on the sky were needed. In the late 10th century, Iranian astronomer
325:
The Big Bear Solar Observatory in California houses several telescopes including the New Solar Telescope(NTS) which is a 1.6 meter, clear-aperture, off-axis Gregorian telescope. The NTS saw first light in December 2008. Until the ATST comes on line, the NTS remains the largest solar telescope in the
62:
Because the Sun is uniquely situated for close-range observing (other stars cannot be resolved with anything like the spatial or temporal resolution that the Sun can), there is a split between the related discipline of observational astrophysics (of distant stars) and observational solar physics.
93:
built a massive observatory near Tehran. There, he took accurate measurements of a series of meridian transits of the Sun, which he later used to calculate the obliquity of the ecliptic. Following the fall of the Western Roman Empire, Western Europe was cut from all sources of ancient scientific
88:
Astronomical knowledge flourished in the Islamic world during medieval times. Many observatories were built in cities from Damascus to Baghdad, where detailed astronomical observations were taken. Particularly, a few solar parameters were measured and detailed observations of the Sun were taken.
79:
Babylonians were keeping a record of solar eclipses, with the oldest record originating from the ancient city of Ugarit, in modern-day Syria. This record dates to about 1300 BC. Ancient Chinese astronomers were also observing solar phenomena (such as solar eclipses and visible sunspots) with the
343:
The Extreme Ultraviolet Normal Incidence Spectrograph (EUNIS) is a two channel imaging spectrograph that first flew in 2006. It observes the solar corona with high spectral resolution. So far, it has provided information on the nature of coronal bright points, cool transients and coronal loop
258:
The Solar Dynamics Observatory (SDO) was launched by NASA in February 2010 from Cape Canaveral. The main goals of the mission are understanding how solar activity arises and how it affects life on Earth by determining how the Sun's magnetic field is generated and structured and how the stored
235:
A publicly funded mission led by the Japanese Aerospace Exploration Agency, the HINODE satellite, launched in 2006, consists of a coordinated set of optical, extreme ultraviolet and X-ray instruments. These investigate the interaction between the solar corona and the Sun's magnetic field.
80:
purpose of keeping track of calendars, which were based on lunar and solar cycles. Unfortunately, records kept before 720 BC are very vague and offer no useful information. However, after 720 BC, 37 solar eclipses were noted over the course of 240 years.
292:
The Advanced Technology Solar Telescope (ATST) is a solar telescope facility that is under construction in Maui. Twenty-two institutions are collaborating on the ATST project, with the main funding agency being the National Science Foundation.
130:
Modern day solar physics is focused towards understanding the many phenomena observed with the help of modern telescopes and satellites. Of particular interest are the structure of the solar photosphere, the coronal heat problem and sunspots.
193:
and NASA. Their orbits approach the Sun closer than Mercury. They included instruments to measure the solar wind, magnetic fields, cosmic rays, and interplanetary dust. Helios-A continued to transmit data until 1986.
220:
and ESA that was launched in December 1995. It was launched to probe the interior of the Sun, make observations of the solar wind and phenomena associated with it and investigate the outer layers of the Sun.
273:
The Parker Solar Probe (PSP) was launched in 2018 with the mission of making detailed observations of the outer solar corona. It has made the closest approaches to the Sun of any artificial object.
106:. He proposed that planets revolve around the Sun and not around the Earth, as it was believed at the time. This model is known as the heliocentric model. His work was later expanded by 763: 955: 788: 166:. Studies of phenomena that affect multiple systems in the heliosphere, or that are considered to fit within a heliospheric context, are called 1779: 189:
Helios-A and Helios-B are a pair of spacecraft launched in December 1974 and January 1976 from Cape Canaveral, as a joint venture between the
1549: 114:. Particularly, Galilei used his new telescope to look at the Sun. In 1610, he discovered sunspots on its surface. In the autumn of 1611, 1868: 858: 1747: 425: 1043: 930: 287: 828: 687: 327: 203: 326:
world. The Big Bear Observatory is one of several facilities operated by the Center for Solar-Terrestrial Research at
1542: 1337: 1023: 455: 66:
The study of solar physics is also important as it provides a "physical laboratory" for the study of plasma physics.
652: 971: 369: 308: 150:
A major thrust of current (2009) effort in the field of solar physics is integrated understanding of the entire
1695: 1493: 144: 17: 1535: 1498: 1832: 710: 682: 398: 1663: 1636: 1296: 575: 447: 320: 245: 1474: 302: 1769: 1169: 509: 190: 38: 1899: 1853: 1715: 1468: 1311: 1204: 140: 524: 147:
boasts 555 members (as of May 2007), compared to several thousand in the parent organization.
1889: 1858: 1827: 1690: 1611: 1364: 1184: 1016: 1817: 1641: 1601: 1448: 1418: 1301: 1236: 1053: 8: 1792: 1651: 1646: 1631: 1606: 1583: 1559: 1268: 626: 417: 184: 103: 1848: 1725: 1720: 1673: 1354: 1086: 440: 268: 230: 115: 601: 1863: 1812: 1757: 1737: 1623: 1488: 1403: 1306: 949: 782: 451: 421: 388: 1209: 981: 1802: 1742: 1668: 1194: 1103: 1009: 991: 479: 361: 737: 170:, a new coinage that entered usage in the early years of the current millennium. 1822: 1732: 1678: 1578: 1428: 1408: 1383: 1278: 1223: 1199: 1076: 111: 107: 31: 1752: 1707: 1685: 1573: 1398: 1378: 1373: 1161: 1066: 375: 344:
arcades. Data from it also helped calibrating SOHO and a few other telescopes.
250: 549: 1883: 1762: 1443: 1438: 1342: 1332: 1253: 1248: 1243: 1146: 1123: 1108: 836: 154:
including the Sun and its effects throughout interplanetary space within the
1527: 1894: 1787: 1516: 1423: 1393: 1388: 1349: 1179: 1174: 1151: 1133: 1113: 435: 393: 167: 151: 56: 996: 904: 1359: 1288: 1273: 1258: 1231: 1141: 1095: 660: 216:
The Solar and Heliospheric Observatory, SOHO, is a joint project between
155: 90: 1807: 1797: 1433: 1263: 1071: 1061: 208: 163: 986: 976: 1658: 1316: 1189: 1458: 383: 47:
is the branch of astrophysics that specializes in the study of the
1118: 52: 928: 802: 573: 159: 102:
In astronomy, the renaissance period started with the work of
503: 1453: 982:
NASA's Goddard Space Flight Center Solar Physics Laboratory
908: 217: 1001: 1032: 48: 602:"Nicolaus Copernicus biography: facts & discoveries" 879: 977:
NASA's Marshall Space Flight Center Solar Physics Page
259:
magnetic energy is converted and released into space.
761: 351: 931:"Extreme Ultraviolet Normal Incidence Spectrograph" 650: 439: 1881: 929:Sciences and Exploration Directorate, Code 600. 905:"Center for Solar-Terrestrial Research Welcome!" 51:. It intersects with many disciplines of pure 1557: 1543: 1017: 504:Littman, M.; Willcox, F; Espenak, F. (2000). 478:Solar Physics, Marshall Space Flight Center. 307:Sunspot Solar Observatory (SSO) operates the 516: 954:: CS1 maint: numeric names: authors list ( 787:: CS1 maint: numeric names: authors list ( 1550: 1536: 1024: 1010: 736:SOHO, Solar and Heliospheric Observatory. 477: 249: 207: 30:For broader coverage of this topic, see 599: 14: 1882: 1748:Atomic, molecular, and optical physics 411: 122:("On the spots observed in the Sun"). 1531: 1005: 997:Center for Solar-Terrestrial Research 576:"Theme: medieval astronomy in Europe" 574:Portal to the heritage of astronomy. 434: 97: 859:"NASA Press Kit: Parker Solar Probe" 762:Solar Physics Laboratory, Code 671. 401:(in La Palma in the Canary Islands) 288:Advanced Technology Solar Telescope 24: 715:National Space Science Data Center 688:National Space Science Data Center 414:Physics of the Sun: A First Course 405: 328:New Jersey Institute of Technology 204:Solar and Heliospheric Observatory 118:wrote the first book on sunspots, 25: 1911: 965: 827:SDO, Solar Dynamics Observatory. 807:NASA Marshall Space Flight Centre 83: 1512: 1511: 935:NASA Goddard Space Flight Centre 833:NASA Goddard Space Flight Centre 768:NASA Goddard Space Flight Centre 735: 529:NASA Goddard Space Flight Center 522: 368: 354: 74: 1869:Timeline of physics discoveries 972:Living Reviews in Solar Physics 922: 897: 872: 851: 826: 820: 795: 755: 729: 711:"Helios-B – Trajectory Details" 703: 683:"Helios-A – Trajectory Details" 309:Richard B. Dunn Solar Telescope 276: 125: 675: 644: 619: 593: 567: 542: 497: 471: 173: 13: 1: 1494:List of heliophysics missions 657:American Astronomical Society 554:StarTeach Astronomy Education 506:Totality: Eclipses of the Sun 465: 145:American Astronomical Society 120:De Maculis in Sole Observatis 1499:Category:Missions to the Sun 550:"Arab and Islamic astronomy" 311:(DST) on behalf of the NSF. 7: 1833:Quantum information science 1031: 525:"Ancient eclipses in China" 412:Mullan, Dermott J. (2009). 399:Institute for Solar Physics 347: 314: 134: 10: 1916: 1664:Classical electromagnetism 992:SUPARCO Solar physics Page 448:Cambridge University Press 321:Big Bear Solar Observatory 318: 300: 285: 266: 246:Solar Dynamics Observatory 243: 228: 201: 182: 69: 36: 29: 1841: 1778: 1706: 1622: 1594: 1566: 1507: 1481: 1475:G-type main-sequence star 1467: 1325: 1287: 1222: 1160: 1132: 1094: 1085: 1052: 1039: 303:Sunspot Solar Observatory 224: 178: 1770:Condensed matter physics 1338:In mythology and culture 738:"About the SOHO mission" 651:Solar Physics Division. 338: 333: 212:Image of SOHO spacecraft 37:Not to be confused with 987:MPS Solar Physics Group 829:"About the SDO mission" 510:Oxford University Press 442:Astrophysics of the Sun 281: 197: 191:German Aerospace Center 39:Solar Physics (journal) 1854:Nobel Prize in Physics 1716:Relativistic mechanics 1205:Supra-arcade downflows 480:"Why we study the Sun" 296: 262: 255: 239: 213: 141:Solar Physics Division 27:Branch of astrophysics 1859:Philosophy of physics 1185:Coronal mass ejection 880:"Welcome to the ATST" 253: 211: 1818:Mathematical physics 1449:Standard solar model 1419:Solar radio emission 1237:List of solar cycles 868:. NASA. August 2018. 418:Taylor & Francis 1793:Atmospheric physics 1632:Classical mechanics 1560:branches of physics 1269:Magnetic switchback 631:The Galileo Project 600:Taylor Redd, Nola. 185:Helios (spacecraft) 104:Nicolaus Copernicus 91:Abu-Mahmud Khojandi 1849:History of physics 1459:Sunlight radiation 1054:Internal structure 269:Parker Solar Probe 256: 231:Hinode (satellite) 214: 116:Johannes Fabricius 98:Renaissance period 1877: 1876: 1864:Physics education 1813:Materials science 1780:Interdisciplinary 1738:Quantum mechanics 1525: 1524: 1489:Solar observatory 1404:Solar observation 1302:Termination shock 1218: 1217: 1170:Transition region 427:978-1-4200-8307-1 389:Helioseismography 254:The SDO satellite 16:(Redirected from 1907: 1803:Chemical physics 1743:Particle physics 1669:Classical optics 1552: 1545: 1538: 1529: 1528: 1515: 1514: 1104:Supergranulation 1092: 1091: 1026: 1019: 1012: 1003: 1002: 960: 959: 953: 945: 943: 941: 926: 920: 919: 917: 915: 901: 895: 894: 892: 890: 876: 870: 869: 863: 855: 849: 848: 846: 844: 835:. Archived from 824: 818: 817: 815: 813: 799: 793: 792: 786: 778: 776: 774: 759: 753: 752: 750: 748: 733: 727: 726: 724: 722: 707: 701: 700: 698: 696: 679: 673: 672: 670: 668: 663:on 22 March 2014 659:. Archived from 648: 642: 641: 639: 637: 623: 617: 616: 614: 612: 597: 591: 590: 588: 586: 571: 565: 564: 562: 560: 546: 540: 539: 537: 535: 523:Sten, Odenwald. 520: 514: 513: 508:(2nd ed.). 501: 495: 494: 492: 490: 475: 461: 445: 431: 378: 373: 372: 364: 362:Astronomy portal 359: 358: 357: 21: 1915: 1914: 1910: 1909: 1908: 1906: 1905: 1904: 1880: 1879: 1878: 1873: 1837: 1823:Medical physics 1774: 1733:Nuclear physics 1702: 1696:Non-equilibrium 1618: 1590: 1562: 1556: 1526: 1521: 1503: 1477: 1463: 1429:Solar telescope 1409:Solar phenomena 1384:Solar astronomy 1321: 1283: 1279:Helioseismology 1214: 1200:Helmet streamer 1156: 1128: 1081: 1077:Convection zone 1048: 1035: 1030: 968: 963: 947: 946: 939: 937: 927: 923: 913: 911: 903: 902: 898: 888: 886: 878: 877: 873: 861: 857: 856: 852: 842: 840: 839:on 30 June 2007 825: 821: 811: 809: 801: 800: 796: 780: 779: 772: 770: 760: 756: 746: 744: 734: 730: 720: 718: 709: 708: 704: 694: 692: 681: 680: 676: 666: 664: 649: 645: 635: 633: 625: 624: 620: 610: 608: 598: 594: 584: 582: 572: 568: 558: 556: 548: 547: 543: 533: 531: 521: 517: 502: 498: 488: 486: 476: 472: 468: 458: 428: 408: 406:Further reading 374: 367: 360: 355: 353: 350: 341: 336: 323: 317: 305: 299: 290: 284: 279: 271: 265: 248: 242: 233: 227: 206: 200: 187: 181: 176: 137: 128: 112:Galileo Galilei 108:Johannes Kepler 100: 86: 77: 72: 42: 35: 32:Stellar physics 28: 23: 22: 15: 12: 11: 5: 1913: 1903: 1902: 1897: 1892: 1875: 1874: 1872: 1871: 1866: 1861: 1856: 1851: 1845: 1843: 1839: 1838: 1836: 1835: 1830: 1825: 1820: 1815: 1810: 1805: 1800: 1795: 1790: 1784: 1782: 1776: 1775: 1773: 1772: 1767: 1766: 1765: 1760: 1755: 1745: 1740: 1735: 1730: 1729: 1728: 1723: 1712: 1710: 1704: 1703: 1701: 1700: 1699: 1698: 1693: 1686:Thermodynamics 1683: 1682: 1681: 1676: 1666: 1661: 1656: 1655: 1654: 1649: 1644: 1639: 1628: 1626: 1620: 1619: 1617: 1616: 1615: 1614: 1604: 1598: 1596: 1592: 1591: 1589: 1588: 1587: 1586: 1576: 1570: 1568: 1564: 1563: 1555: 1554: 1547: 1540: 1532: 1523: 1522: 1520: 1519: 1508: 1505: 1504: 1502: 1501: 1496: 1491: 1485: 1483: 1479: 1478: 1473: 1471: 1469:Spectral class 1465: 1464: 1462: 1461: 1456: 1451: 1446: 1441: 1436: 1431: 1426: 1421: 1416: 1411: 1406: 1401: 1399:Solar neutrino 1396: 1391: 1386: 1381: 1379:Solar activity 1376: 1374:Sun in fiction 1371: 1370: 1369: 1368: 1367: 1352: 1347: 1346: 1345: 1340: 1329: 1327: 1323: 1322: 1320: 1319: 1314: 1309: 1304: 1299: 1293: 1291: 1285: 1284: 1282: 1281: 1276: 1271: 1266: 1261: 1256: 1251: 1246: 1241: 1240: 1239: 1228: 1226: 1220: 1219: 1216: 1215: 1213: 1212: 1210:Alfvén surface 1207: 1202: 1197: 1192: 1187: 1182: 1177: 1172: 1166: 1164: 1158: 1157: 1155: 1154: 1149: 1144: 1138: 1136: 1130: 1129: 1127: 1126: 1121: 1116: 1111: 1106: 1100: 1098: 1089: 1083: 1082: 1080: 1079: 1074: 1069: 1067:Radiation zone 1064: 1058: 1056: 1050: 1049: 1047: 1046: 1040: 1037: 1036: 1029: 1028: 1021: 1014: 1006: 1000: 999: 994: 989: 984: 979: 974: 967: 966:External links 964: 962: 961: 921: 896: 871: 850: 819: 794: 754: 728: 702: 674: 643: 618: 592: 566: 541: 515: 496: 469: 467: 464: 463: 462: 456: 432: 426: 407: 404: 403: 402: 396: 391: 386: 380: 379: 376:Physics portal 365: 349: 346: 340: 337: 335: 332: 319:Main article: 316: 313: 301:Main article: 298: 295: 286:Main article: 283: 280: 278: 275: 267:Main article: 264: 261: 244:Main article: 241: 238: 229:Main article: 226: 223: 202:Main article: 199: 196: 183:Main article: 180: 177: 175: 172: 162:and planetary 136: 133: 127: 124: 99: 96: 85: 84:Medieval times 82: 76: 73: 71: 68: 26: 9: 6: 4: 3: 2: 1912: 1901: 1900:Space science 1898: 1896: 1893: 1891: 1888: 1887: 1885: 1870: 1867: 1865: 1862: 1860: 1857: 1855: 1852: 1850: 1847: 1846: 1844: 1840: 1834: 1831: 1829: 1828:Ocean physics 1826: 1824: 1821: 1819: 1816: 1814: 1811: 1809: 1806: 1804: 1801: 1799: 1796: 1794: 1791: 1789: 1786: 1785: 1783: 1781: 1777: 1771: 1768: 1764: 1763:Modern optics 1761: 1759: 1756: 1754: 1751: 1750: 1749: 1746: 1744: 1741: 1739: 1736: 1734: 1731: 1727: 1724: 1722: 1719: 1718: 1717: 1714: 1713: 1711: 1709: 1705: 1697: 1694: 1692: 1689: 1688: 1687: 1684: 1680: 1677: 1675: 1672: 1671: 1670: 1667: 1665: 1662: 1660: 1657: 1653: 1650: 1648: 1645: 1643: 1640: 1638: 1635: 1634: 1633: 1630: 1629: 1627: 1625: 1621: 1613: 1612:Computational 1610: 1609: 1608: 1605: 1603: 1600: 1599: 1597: 1593: 1585: 1582: 1581: 1580: 1577: 1575: 1572: 1571: 1569: 1565: 1561: 1553: 1548: 1546: 1541: 1539: 1534: 1533: 1530: 1518: 1510: 1509: 1506: 1500: 1497: 1495: 1492: 1490: 1487: 1486: 1484: 1480: 1476: 1472: 1470: 1466: 1460: 1457: 1455: 1452: 1450: 1447: 1445: 1444:Space weather 1442: 1440: 1439:Space climate 1437: 1435: 1432: 1430: 1427: 1425: 1422: 1420: 1417: 1415: 1414:Solar physics 1412: 1410: 1407: 1405: 1402: 1400: 1397: 1395: 1392: 1390: 1387: 1385: 1382: 1380: 1377: 1375: 1372: 1366: 1363: 1362: 1361: 1358: 1357: 1356: 1353: 1351: 1348: 1344: 1343:Lunar eclipse 1341: 1339: 1336: 1335: 1334: 1331: 1330: 1328: 1324: 1318: 1315: 1313: 1310: 1308: 1305: 1303: 1300: 1298: 1297:Current sheet 1295: 1294: 1292: 1290: 1286: 1280: 1277: 1275: 1272: 1270: 1267: 1265: 1262: 1260: 1257: 1255: 1254:Solar minimum 1252: 1250: 1249:Solar maximum 1247: 1245: 1244:Active region 1242: 1238: 1235: 1234: 1233: 1230: 1229: 1227: 1225: 1221: 1211: 1208: 1206: 1203: 1201: 1198: 1196: 1193: 1191: 1188: 1186: 1183: 1181: 1178: 1176: 1173: 1171: 1168: 1167: 1165: 1163: 1159: 1153: 1150: 1148: 1145: 1143: 1140: 1139: 1137: 1135: 1131: 1125: 1124:Ellerman bomb 1122: 1120: 1117: 1115: 1112: 1110: 1107: 1105: 1102: 1101: 1099: 1097: 1093: 1090: 1088: 1084: 1078: 1075: 1073: 1070: 1068: 1065: 1063: 1060: 1059: 1057: 1055: 1051: 1045: 1042: 1041: 1038: 1034: 1027: 1022: 1020: 1015: 1013: 1008: 1007: 1004: 998: 995: 993: 990: 988: 985: 983: 980: 978: 975: 973: 970: 969: 957: 951: 936: 932: 925: 910: 906: 900: 885: 881: 875: 867: 860: 854: 838: 834: 830: 823: 808: 804: 798: 790: 784: 769: 765: 758: 743: 739: 732: 716: 712: 706: 690: 689: 684: 678: 662: 658: 654: 647: 632: 628: 622: 607: 603: 596: 581: 577: 570: 555: 551: 545: 530: 526: 519: 511: 507: 500: 485: 481: 474: 470: 459: 457:0-521-30268-4 453: 449: 444: 443: 437: 436:Zirin, Harold 433: 429: 423: 419: 415: 410: 409: 400: 397: 395: 392: 390: 387: 385: 382: 381: 377: 371: 366: 363: 352: 345: 331: 329: 322: 312: 310: 304: 294: 289: 274: 270: 260: 252: 247: 237: 232: 222: 219: 210: 205: 195: 192: 186: 171: 169: 165: 161: 157: 153: 148: 146: 142: 132: 123: 121: 117: 113: 109: 105: 95: 92: 81: 75:Ancient times 67: 64: 60: 58: 54: 50: 46: 45:Solar physics 40: 33: 19: 18:Solar Physics 1890:Astrophysics 1788:Astrophysics 1602:Experimental 1424:Solar System 1413: 1394:Solar energy 1389:Solar dynamo 1350:Heliophysics 1180:Coronal loop 1175:Coronal hole 1152:Moreton wave 1134:Chromosphere 938:. Retrieved 934: 924: 912:. Retrieved 899: 887:. Retrieved 883: 874: 865: 853: 841:. Retrieved 837:the original 832: 822: 810:. Retrieved 806: 797: 771:. Retrieved 767: 757: 745:. Retrieved 741: 731: 719:. Retrieved 714: 705: 693:. Retrieved 686: 677: 665:. Retrieved 661:the original 656: 653:"Membership" 646: 634:. Retrieved 630: 621: 609:. Retrieved 605: 595: 583:. Retrieved 579: 569: 557:. Retrieved 553: 544: 532:. Retrieved 528: 518: 505: 499: 487:. Retrieved 483: 473: 441: 413: 394:Heliophysics 342: 324: 306: 291: 277:Ground based 272: 257: 234: 215: 188: 168:heliophysics 152:Solar System 149: 138: 129: 126:Modern times 119: 101: 87: 78: 65: 61: 57:astrophysics 44: 43: 1691:Statistical 1607:Theoretical 1584:Engineering 1482:Exploration 1360:Solar deity 1307:Heliosheath 1289:Heliosphere 1259:Wolf number 1232:Solar cycle 1096:Photosphere 174:Space based 164:atmospheres 156:heliosphere 1884:Categories 1808:Geophysics 1798:Biophysics 1642:Analytical 1595:Approaches 1434:Solar time 1355:In culture 1312:Heliopause 1264:Solar wind 1195:Prominence 1087:Atmosphere 1072:Tachocline 940:17 January 889:17 January 843:17 January 812:17 January 773:17 January 747:17 January 667:28 January 636:18 January 627:"Sunspots" 611:18 January 585:18 January 559:18 January 534:17 January 489:28 January 466:References 1758:Molecular 1659:Acoustics 1652:Continuum 1647:Celestial 1637:Newtonian 1624:Classical 1567:Divisions 1317:Bow shock 1224:Variation 1190:Nanoflare 742:ESA; NASA 606:Space.com 1517:Category 950:cite web 866:nasa.gov 803:"Hinode" 783:cite web 764:"HINODE" 438:(1988). 384:Aeronomy 348:See also 330:(NJIT). 315:Big Bear 135:Research 1842:Related 1726:General 1721:Special 1579:Applied 1333:Eclipse 1326:Related 1147:Spicule 1119:Sunspot 1114:Faculae 1109:Granule 1033:The Sun 721:May 26, 695:May 26, 160:planets 158:and on 143:of the 70:History 53:physics 1753:Atomic 1708:Modern 1558:Major 1162:Corona 914:29 May 717:. NASA 691:. NASA 580:UNESCO 454:  424:  225:HINODE 179:Helios 1274:Flare 1142:Plage 862:(PDF) 339:EUNIS 334:Other 1679:Wave 1574:Pure 1454:Star 1365:List 1062:Core 1044:List 956:link 942:2014 916:2016 909:NJIT 891:2014 845:2014 814:2014 789:link 775:2014 749:2014 723:2021 697:2021 669:2014 638:2014 613:2014 587:2014 561:2014 536:2014 491:2014 484:NASA 452:ISBN 422:ISBN 282:ATST 218:NASA 198:SOHO 139:The 110:and 55:and 1895:Sun 1674:Ray 884:NSO 297:SSO 263:PSP 240:SDO 49:Sun 1886:: 952:}} 948:{{ 933:. 907:. 882:. 864:. 831:. 805:. 785:}} 781:{{ 766:. 740:. 713:. 685:. 655:. 629:. 604:. 578:. 552:. 527:. 482:. 450:. 446:. 420:. 416:. 59:. 1551:e 1544:t 1537:v 1025:e 1018:t 1011:v 958:) 944:. 918:. 893:. 847:. 816:. 791:) 777:. 751:. 725:. 699:. 671:. 640:. 615:. 589:. 563:. 538:. 512:. 493:. 460:. 430:. 41:. 34:. 20:)

Index

Solar Physics
Stellar physics
Solar Physics (journal)
Sun
physics
astrophysics
Abu-Mahmud Khojandi
Nicolaus Copernicus
Johannes Kepler
Galileo Galilei
Johannes Fabricius
Solar Physics Division
American Astronomical Society
Solar System
heliosphere
planets
atmospheres
heliophysics
Helios (spacecraft)
German Aerospace Center
Solar and Heliospheric Observatory

NASA
Hinode (satellite)
Solar Dynamics Observatory

Parker Solar Probe
Advanced Technology Solar Telescope
Sunspot Solar Observatory
Richard B. Dunn Solar Telescope

Text is available under the Creative Commons Attribution-ShareAlike License. Additional terms may apply.