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| 20240219 - Filament data for 12 UTC |
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Available data for 20240219: »09 UTC »10 UTC »11 UTC »12 UTC »13 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 977 1632 (N29E17 L=278) 801 277 0 ( 935/1545-1057/1729) 86.4 E19-E14 N22-N38
2 463 1697 (N25E60 L=235) 544 63 2 ( 438/1674- 490/1725) 26.6 E63-E56 N23-N26
3 1128 1630 (N32E07 L=288) 711 182 0 (1074/1551-1172/1699) -39.3 E13-E02 N27-N36
4 315 1577 (N15E68 L=228) 2347 186 3 ( 260/1515- 367/1647) 84.3 E74-E61 N10-N20
5 534 1562 (N16E44 L=251) 1040 171 3 ( 497/1510- 585/1646) -33.7 E50-E38 N13-N21
6 1549 1586 (N41W25 L=321) 1012 153 0 (1465/1549-1617/1609) 4.1 W17-W32 N38-N43
7 1781 1467 (N40W51 L=347) 537 61 1 (1748/1446-1813/1485) 5.7 W46-W56 N39-N41
8 1179 1286 (N11W04 L=299) 750 203 1 (1144/1199-1226/1377) 85.2 W02-W05 N05-N17
9 1342 1258 (N13W14 L=309) 409 122 1 (1321/1209-1364/1315) -63.4 W12-W15 N10-N16
10 1536 1111 (N09W29 L=324) 682 189 0 (1480/1045-1577/1189) 73.3 W26-W30 N04-N14
11 1250 1070 (N00W12 L=308) 379 96 0 (1202/1042-1302/1090) 0.0 W08-W15 N00-N01
12 1926 1052 (N17W68 L= 3) 600 63 1 (1900/1025-1961/1067) 21.0 W63-W76 N14-N19
13 1868 999 (N12W60 L=355) 503 95 0 (1849/ 955-1885/1041) 90.0 W57-W61 N09-N14
14 1123 919 (S11W08 L=303) 568 280 0 (1001/ 882-1247/ 944) 26.6 W01-W15 S15-S08
15 1919 904 (N09W70 L= 5) 638 97 0 (1889/ 863-1940/ 940) 45.0 W65-W73 N05-N11
16 677 887 (S21E18 L=277) 441 127 0 ( 620/ 854- 725/ 934) 54.5 E21-E15 S24-S17
17 1244 728 (S19W20 L=315) 522 143 1 (1187/ 677-1294/ 786) 77.5 W17-W21 S23-S14
18 1444 633 (S20W36 L=331) 552 192 0 (1367/ 572-1512/ 675) 58.0 W32-W39 S24-S15
19 1248 405 (S38W34 L=329) 398 83 1 (1212/ 386-1292/ 436) 8.1 W30-W37 S39-S36
20 1570 380 (S30W62 L=357) 659 134 0 (1505/ 353-1621/ 419) 40.6 W56-W64 S32-S26
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Download FITS filament maps as tar archive
» All Filament Data of 20240219 ...
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The tar archive contains filament maps for all processed Hα images
with at least quality=1.
The maps contain the values 0 and 1, where 1 is the position of a detected filament.
The header in the FITS files is mostly taken from the corresponding Hα file,
so it should be compatible with standard solar software routines.
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