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| 20250720 - Latest Filament data |
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Available data for 20250720: »06 UTC »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC »13 UTC »14 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 684 1749 (N57E33 L=276) 435 69 0 ( 643/1731- 728/1765) 5.7 E37-E26 N55-N58
2 887 1531 (N38E07 L=302) 501 154 0 ( 816/1493- 961/1559) 10.3 E12-E01 N35-N39
3 561 1527 (N39E35 L=274) 351 94 1 ( 519/1503- 608/1553) -18.4 E39-E30 N37-N41
4 1779 1426 (N23W65 L= 14) 2583 213 9 (1732/1341-1839/1521) 71.6 W60-W71 N17-N29
5 1670 1427 (N24W52 L= 1) 478 84 0 (1650/1380-1688/1470) 71.6 W50-W54 N21-N27
6 1474 1391 (N24W34 L=343) 250 99 0 (1429/1376-1528/1408) -26.6 W30-W38 N22-N25
7 257 1214 (N19E57 L=252) 1198 158 5 ( 228/1140- 288/1296) 90.0 E59-E53 N14-N23
8 1819 1264 (N12W62 L= 11) 487 47 1 (1796/1244-1840/1286) 9.5 W59-W65 N11-N13
9 994 1141 (N12E01 L=308) 374 174 0 ( 931/1096-1064/1168) -29.7 E05-W02 N08-N13
10 122 1106 (N11E75 L=234) 870 81 1 ( 108/1062- 139/1148) -45.0 E79-E71 N08-N13
11 385 1057 (N09E43 L=266) 385 120 1 ( 358/1014- 435/1090) 23.2 E45-E38 N06-N11
12 677 892 (S02E22 L=286) 1541 443 1 ( 603/ 766- 808/1072) -58.6 E26-E14 S09-N09
13 1528 939 (S04W32 L=340) 664 216 0 (1442/ 890-1600/1014) 18.4 W25-W37 S06-N00
14 313 749 (S10E52 L=257) 436 99 0 ( 296/ 701- 325/ 798) 81.9 E54-E50 S13-S06
15 314 622 (S18E56 L=252) 2304 375 4 ( 248/ 501- 400/ 730) -75.1 E63-E49 S26-S11
16 948 565 (S24E08 L=301) 396 168 0 ( 874/ 544-1019/ 592) -24.0 E12-E03 S25-S21
17 1138 432 (S35W04 L=313) 360 66 1 (1115/ 394-1162/ 467) 71.6 W02-W06 S37-S31
18 1057 306 (S45E03 L=306) 1274 149 3 ( 996/ 249-1118/ 363) 31.0 E08-W02 S50-S39
19 626 258 (S47E47 L=262) 1885 189 2 ( 538/ 233- 713/ 289) 7.4 E68-E35 S50-S44
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Download FITS filament maps as tar archive
» All Filament Data of 20250720 ...
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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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