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| 20250403 - Filament data for 08 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 1115 1721 (N38E18 L=283) 843 199 1 (1037/1673-1207/1769) 0.0 E25-E10 N36-N39
2 1312 1628 (N38E01 L=299) 326 80 1 (1276/1603-1354/1650) 0.0 E03-W02 N36-N39
3 567 1543 (N11E43 L=257) 839 195 2 ( 520/1469- 616/1640) -29.7 E50-E36 N07-N16
4 1445 1338 (N23W16 L=316) 250 71 1 (1409/1309-1480/1369) 0.0 W12-W18 N21-N24
5 1721 1209 (N25W39 L=339) 410 132 0 (1680/1151-1744/1246) -33.7 W34-W40 N21-N26
6 1867 1106 (N24W56 L=356) 696 131 2 (1814/1053-1905/1148) -8.7 W48-W61 N22-N25
7 657 1058 (S14E22 L=279) 316 68 2 ( 631/1027- 681/1097) 90.0 E23-E20 S16-S11
8 1018 920 (S12W02 L=303) 424 160 0 ( 966/ 866-1075/ 982) -20.6 E01-W07 S13-S09
9 1738 927 (N10W46 L=346) 372 78 0 (1716/ 889-1757/ 964) 90.0 W45-W47 N07-N11
10 1796 857 (N08W54 L=354) 1536 206 5 (1740/ 770-1858/ 918) 59.0 W50-W59 N02-N12
11 926 831 (S19E00 L=300) 371 121 1 ( 866/ 806- 979/ 853) 9.5 E03-W03 S20-S18
12 777 724 (S30E06 L=294) 384 153 0 ( 744/ 665- 833/ 758) 74.1 E07-E03 S33-S26
13 207 692 (S47E64 L=237) 577 55 1 ( 174/ 672- 239/ 722) 7.1 E73-E57 S48-S44
14 1408 624 (S17W35 L=335) 345 77 0 (1363/ 610-1448/ 642) 18.4 W31-W37 S18-S15
15 523 551 (S49E22 L=278) 808 177 4 ( 441/ 514- 601/ 591) 3.6 E31-E14 S51-S46
16 843 466 (S44W07 L=307) 285 64 0 ( 818/ 444- 879/ 493) -9.5 W04-W10 S44-S42
17 1423 362 (S30W52 L=352) 462 96 1 (1371/ 329-1459/ 401) -4.8 W45-W57 S30-S28
18 1577 334 (S25W68 L= 8) 587 51 0 (1552/ 310-1598/ 355) 0.0 W63-W74 S26-S24
19 1016 184 (S57W45 L=345) 461 65 1 ( 999/ 150-1029/ 217) -21.0 W39-W52 S59-S54
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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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