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| 20250205 - Latest Filament data |
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Available data for 20250205: »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
1 606 1720 (N32E44 L=284) 386 49 0 ( 579/1705- 635/1739) 0.0 E46-E41 N30-N33
2 307 1469 (N12E58 L=270) 836 111 2 ( 278/1417- 330/1514) -56.3 E62-E54 N08-N14
3 1166 1399 (N18W03 L=331) 495 191 2 (1075/1382-1267/1420) 5.2 E02-W09 N16-N19
4 479 1372 (N07E40 L=288) 363 81 1 ( 439/1350- 521/1390) 18.4 E42-E36 N05-N08
5 1547 1280 (N17W29 L=357) 1771 268 5 (1439/1189-1628/1363) -24.8 W20-W34 N12-N22
6 349 1299 (N02E48 L=280) 555 89 2 ( 326/1253- 376/1338) 90.0 E50-E46 S01-N04
7 224 1302 (N01E61 L=267) 512 58 2 ( 193/1276- 264/1322) 0.0 E64-E56 N00-N02
8 1174 1294 (N12W05 L=333) 200 98 0 (1146/1253-1218/1319) 51.3 W03-W07 N08-N13
9 1454 1251 (N14W23 L=351) 283 38 0 (1427/1225-1476/1276) -71.6 W20-W24 N12-N15
10 1445 1200 (N11W22 L=350) 250 66 0 (1411/1180-1475/1219) 26.6 W20-W24 N09-N12
11 1529 1079 (N05W29 L=358) 242 89 0 (1480/1067-1574/1092) 18.4 W26-W32 N03-N06
12 1749 890 (S01W49 L= 17) 439 89 0 (1705/ 873-1798/ 910) 14.0 W45-W53 S02-N00
13 459 817 (S26E35 L=293) 928 239 0 ( 366/ 758- 574/ 855) 21.3 E43-E25 S30-S22
14 1267 642 (S25W22 L=350) 3671 898 4 ( 981/ 563-1668/ 804) 8.1 W02-W51 S29-S17
15 499 655 (S36E32 L=296) 347 76 1 ( 464/ 638- 531/ 680) 31.0 E35-E29 S36-S33
16 1825 595 (S15W71 L= 39) 634 87 1 (1790/ 578-1869/ 619) 24.0 W66-W77 S16-S12
17 446 536 (S45E40 L=288) 1312 331 5 ( 290/ 507- 584/ 561) 1.7 E60-E25 S46-S42
18 719 507 (S43E14 L=314) 466 112 1 ( 662/ 478- 779/ 533) -5.7 E18-E08 S43-S41
19 955 451 (S42W06 L=334) 218 56 1 ( 925/ 439- 989/ 469) -11.3 W03-W08 S43-S41
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Download FITS filament maps as tar archive
» All Filament Data of 20250205 ...
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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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