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| 20251106 - Filament data for 13 UTC |
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Available data for 20251106: »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 1023 1938 (N64W54 L= 4) 861 76 0 (1010/1896-1039/1978) 10.7 W42-W79 N59-N66
2 958 1897 (N63W38 L=348) 613 55 1 ( 930/1869- 980/1924) 0.0 W32-W46 N59-N65
3 1309 1810 (N42W52 L= 2) 2025 351 2 (1160/1765-1465/1853) -15.9 W36-W64 N35-N46
4 966 1663 (N43W16 L=325) 473 68 0 ( 941/1623- 996/1699) 33.7 W12-W19 N40-N45
5 776 1596 (N44E01 L=309) 418 81 0 ( 728/1569- 821/1619) 7.1 E05-W03 N42-N45
6 1742 1203 (S04W49 L=359) 2975 524 4 (1677/ 956-1785/1420) 58.0 W39-W56 S16-N08
7 679 1255 (N25E15 L=294) 295 79 0 ( 640/1225- 710/1279) -36.9 E17-E13 N22-N26
8 364 1183 (N27E40 L=270) 350 108 1 ( 350/1139- 383/1238) 63.4 E41-E37 N24-N30
9 991 1175 (N13W02 L=311) 753 220 1 ( 902/1139-1083/1238) -59.0 E02-W06 N08-N18
10 529 1180 (N24E27 L=283) 250 68 1 ( 500/1162- 565/1205) -36.9 E28-E24 N22-N25
11 280 1106 (N24E48 L=261) 1626 343 2 ( 149/ 982- 382/1193) -33.7 E65-E40 N15-N32
12 486 1034 (N16E32 L=278) 330 150 0 ( 418/1002- 551/1054) 0.0 E37-E27 N15-N17
13 237 839 (N10E57 L=253) 780 94 2 ( 202/ 805- 276/ 885) 12.5 E61-E52 N07-N11
14 392 798 (N05E44 L=266) 541 127 0 ( 331/ 775- 440/ 819) -26.6 E48-E40 N02-N06
15 891 737 (S09E14 L=296) 346 80 0 ( 870/ 691- 915/ 779) 80.5 E14-E12 S12-S06
16 1432 660 (S27W16 L=326) 332 33 0 (1410/ 632-1451/ 687) 45.0 W14-W17 S28-S25
17 359 430 (S16E66 L=244) 5637 423 7 ( 259/ 247- 509/ 570) 87.5 E79-E60 S31-S06
18 1494 410 (S47W18 L=327) 422 69 0 (1452/ 395-1524/ 430) -15.9 W13-W20 S49-S45
19 901 331 (S35E28 L=281) 886 181 0 ( 832/ 271- 959/ 387) 14.9 E36-E21 S37-S31
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Download FITS filament maps as tar archive
» All Filament Data of 20251106 ...
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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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