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| 20250815 - Filament data for 12 UTC |
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Available data for 20250815: »06 UTC »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC »13 UTC »14 UTC »15 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 1229 1898 (N60W65 L= 31) 837 105 1 (1174/1878-1272/1921) -2.0 W52-W82 N58-N61
2 637 1701 (N59E24 L=302) 367 51 0 ( 614/1683- 662/1726) -9.5 E27-E20 N57-N61
3 1158 1674 (N45W27 L=352) 945 182 3 (1079/1634-1250/1700) -3.6 W18-W34 N43-N46
4 541 1673 (N58E37 L=289) 527 56 2 ( 515/1645- 566/1698) 63.4 E41-E33 N55-N60
5 1301 1644 (N39W36 L= 2) 327 52 0 (1266/1623-1329/1663) -53.1 W33-W38 N37-N41
6 1556 1617 (N31W56 L= 22) 712 64 2 (1532/1581-1591/1649) 45.0 W51-W60 N29-N33
7 1373 1508 (N29W34 L=360) 290 93 0 (1329/1483-1410/1529) -51.3 W31-W36 N26-N31
8 865 1388 (N31E04 L=322) 1988 536 6 ( 628/1310-1093/1480) -31.0 E21-W09 N22-N40
9 1720 1444 (N17W60 L= 26) 443 96 1 (1671/1428-1761/1459) -20.6 W55-W64 N15-N18
10 1784 1319 (N09W60 L= 26) 373 83 1 (1754/1299-1816/1347) -26.6 W57-W63 N06-N10
11 1474 1269 (N13W33 L=358) 282 81 0 (1442/1232-1495/1308) -78.7 W31-W33 N10-N15
12 1116 1089 (N09W06 L=332) 234 77 0 (1102/1044-1132/1127) 68.2 W04-W07 N06-N11
13 441 995 (N13E38 L=288) 1092 300 1 ( 335/ 873- 534/1067) -42.9 E46-E32 N04-N18
14 1427 871 (S09W22 L=348) 548 130 0 (1405/ 808-1448/ 938) 63.4 W20-W24 S13-S05
15 919 619 (S16E13 L=312) 311 111 0 ( 878/ 587- 953/ 662) 33.7 E16-E10 S17-S13
16 588 576 (S14E36 L=290) 263 72 0 ( 566/ 547- 619/ 611) -68.2 E36-E34 S16-S11
17 1089 446 (S31E06 L=319) 1260 326 2 ( 996/ 378-1198/ 577) 30.5 E14-W03 S34-S23
18 676 220 (S43E52 L=274) 916 99 0 ( 628/ 187- 718/ 249) 10.8 E65-E44 S45-S40
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Download FITS filament maps as tar archive
» All Filament Data of 20250815 ...
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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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