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| 20250402 - Latest Filament data |
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Available data for 20250402: »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 959 1792 (N38E32 L=279) 397 88 2 ( 913/1765-1002/1815) 0.0 E36-E27 N36-N39
2 1160 1694 (N37E13 L=298) 488 123 1 (1104/1672-1214/1723) 0.0 E18-E08 N35-N39
3 457 1540 (N09E51 L=260) 600 136 1 ( 427/1487- 506/1590) -24.4 E56-E44 N06-N11
4 1633 1544 (N45W27 L=339) 384 53 0 (1601/1528-1660/1564) 26.6 W24-W30 N42-N46
5 1653 1451 (N38W30 L=341) 558 109 0 (1622/1395-1671/1498) -56.3 W26-W31 N34-N41
6 1594 1282 (N25W27 L=338) 412 166 1 (1529/1238-1629/1314) -7.1 W22-W30 N22-N26
7 1146 1235 (N08W01 L=312) 186 60 2 (1131/1198-1162/1265) -78.7 W00-W01 N05-N10
8 1799 1121 (N22W47 L=359) 927 260 1 (1745/1063-1846/1200) -21.0 W40-W53 N18-N25
9 869 982 (S13E07 L=304) 357 160 0 ( 819/ 924- 908/1056) -24.0 E12-E03 S15-S10
10 1723 969 (N11W44 L=355) 635 123 2 (1676/ 946-1772/ 994) 12.5 W39-W48 N08-N13
11 795 905 (S19E10 L=302) 308 118 0 ( 736/ 880- 844/ 926) 8.1 E13-E06 S19-S17
12 1665 877 (N04W42 L=353) 278 82 1 (1626/ 864-1704/ 899) 38.7 W39-W44 N02-N06
13 165 711 (S46E72 L=239) 740 79 1 ( 137/ 683- 200/ 736) 2.4 E88-E64 S47-S44
14 1286 707 (S16W24 L=335) 272 73 1 (1250/ 691-1326/ 723) 21.8 W21-W26 S17-S14
15 479 578 (S48E27 L=284) 332 67 0 ( 458/ 551- 506/ 607) -26.6 E29-E23 S49-S45
16 1695 499 (S13W64 L= 15) 682 94 2 (1672/ 453-1714/ 548) -39.8 W59-W68 S15-S10
17 1301 437 (S30W38 L=349) 537 172 2 (1235/ 384-1372/ 492) 0.0 W30-W45 S31-S28
18 1519 380 (S26W58 L= 9) 556 86 1 (1477/ 351-1560/ 404) 0.0 W52-W64 S26-S24
19 946 246 (S56W31 L=342) 476 68 0 ( 930/ 204- 962/ 289) -26.6 W25-W37 S58-S52
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Download FITS filament maps as tar archive
» All Filament Data of 20250402 ...
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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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