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| 20250403 - Filament data for 07 UTC |
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Available data for 20250403: »06 UTC »07 UTC »08 UTC »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 1085 1735 (N38E20 L=281) 511 126 0 (1033/1697-1145/1763) -5.7 E24-E14 N36-N39
2 1305 1630 (N38E01 L=299) 332 89 0 (1266/1606-1348/1648) 11.3 E03-W02 N35-N39
3 575 1509 (N09E41 L=260) 460 76 0 ( 546/1476- 610/1544) -15.9 E44-E37 N07-N11
4 1438 1340 (N23W15 L=316) 250 79 1 (1399/1313-1474/1369) -11.3 W12-W17 N21-N23
5 1712 1211 (N25W38 L=339) 426 158 0 (1653/1157-1740/1246) -7.1 W32-W40 N21-N26
6 1874 1095 (N24W57 L=358) 703 114 0 (1839/1050-1909/1146) -10.3 W51-W62 N22-N26
7 651 1069 (S14E22 L=278) 360 96 2 ( 624/1031- 674/1125) -80.5 E23-E20 S16-S10
8 1737 955 (N11W45 L=346) 658 132 1 (1712/ 889-1759/1014) 90.0 W43-W47 N06-N14
9 1008 925 (S12W02 L=303) 389 147 0 ( 960/ 871-1056/ 987) -23.2 E02-W05 S14-S09
10 1797 864 (N08W54 L=355) 1869 274 6 (1730/ 772-1885/ 925) 42.5 W50-W62 N02-N13
11 927 834 (S19E00 L=301) 326 115 1 ( 880/ 810- 983/ 855) 9.5 E03-W03 S20-S18
12 773 734 (S29E07 L=294) 289 128 0 ( 738/ 688- 828/ 760) 56.3 E08-E03 S32-S26
13 205 695 (S47E64 L=237) 551 50 1 ( 173/ 675- 235/ 722) 7.6 E73-E58 S48-S44
14 1402 626 (S17W34 L=335) 323 91 1 (1357/ 603-1445/ 646) 38.7 W31-W37 S19-S15
15 526 554 (S48E22 L=279) 733 184 2 ( 441/ 515- 595/ 594) 0.0 E31-E14 S50-S45
16 839 471 (S44W07 L=307) 299 75 0 ( 809/ 445- 878/ 498) 0.0 W03-W10 S44-S41
17 1427 359 (S30W52 L=353) 396 70 1 (1393/ 332-1457/ 392) -6.3 W47-W56 S31-S28
18 1575 337 (S25W68 L= 9) 628 52 0 (1547/ 311-1596/ 359) 0.0 W62-W74 S26-S24
19 1013 195 (S56W43 L=344) 426 52 1 ( 995/ 165-1029/ 228) -22.6 W37-W49 S58-S53
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Download FITS filament maps as tar archive
» All Filament Data of 20250403 ...
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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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