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| 20250421 - Filament data for 06 UTC |
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Available data for 20250421: »06 UTC »07 UTC »08 UTC »09 UTC »10 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 448 1651 (N17E60 L= 3) 2908 333 6 ( 392/1549- 519/1797) -46.6 E72-E53 N10-N28
2 1506 1483 (N36W18 L= 81) 2351 504 5 (1397/1262-1623/1668) -41.2 W05-W30 N25-N47
3 510 1593 (N14E50 L= 13) 311 47 1 ( 484/1577- 538/1608) 33.7 E52-E48 N13-N15
4 310 1509 (N05E65 L=359) 2493 255 5 ( 197/1461- 410/1574) 17.7 E82-E54 N01-N10
5 893 1444 (N15E19 L= 44) 351 126 0 ( 841/1403- 925/1475) 0.0 E22-E16 N13-N16
6 617 1380 (N04E33 L= 30) 715 162 3 ( 545/1345- 679/1428) 53.1 E37-E30 N00-N08
7 1346 1394 (N25W09 L= 72) 380 159 0 (1287/1337-1409/1428) -6.3 W04-W13 N23-N26
8 1859 1323 (N39W57 L=121) 595 69 1 (1815/1308-1894/1340) 17.4 W50-W66 N36-N41
9 1777 1174 (N25W46 L=109) 1402 287 3 (1721/1095-1855/1289) -42.0 W39-W55 N21-N30
10 240 1238 (S12E59 L= 4) 372 75 0 ( 219/1199- 254/1267) -36.9 E62-E57 S13-S09
11 1457 1231 (N18W19 L= 83) 230 41 0 (1436/1203-1473/1256) -18.4 W17-W20 N16-N19
12 544 1190 (S08E32 L= 31) 321 138 0 ( 511/1133- 566/1241) -63.4 E35-E30 S11-S05
13 1329 1167 (N11W13 L= 77) 218 94 1 (1297/1128-1363/1199) -18.4 W10-W16 N09-N12
14 401 1136 (S14E41 L= 22) 279 84 0 ( 365/1098- 425/1156) -11.3 E44-E39 S15-S12
15 147 1032 (S25E67 L=356) 2165 188 6 ( 103/ 983- 203/1113) 58.0 E76-E58 S28-S20
16 1140 868 (S10W11 L= 74) 222 41 1 (1112/ 849-1168/ 886) 33.7 W08-W11 S11-S08
17 1862 787 (N07W65 L=129) 1109 137 4 (1822/ 737-1903/ 841) 56.3 W61-W71 N02-N11
18 1722 712 (S02W53 L=117) 1841 167 7 (1676/ 640-1774/ 795) -33.7 W47-W59 S05-N01
19 1885 742 (N06W72 L=135) 813 81 3 (1866/ 705-1902/ 780) 78.7 W68-W76 N03-N08
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Download FITS filament maps as tar archive
» All Filament Data of 20250421 ...
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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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