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| 20250206 - Filament data for 10 UTC |
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Available data for 20250206: »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
1 692 1635 (N26E33 L=284) 311 45 1 ( 672/1614- 724/1660) 14.0 E34-E30 N24-N28
2 406 1482 (N13E49 L=268) 481 87 1 ( 364/1444- 448/1507) 38.7 E51-E46 N10-N15
3 222 1384 (N06E64 L=253) 948 128 4 ( 191/1320- 247/1437) 76.0 E66-E61 N01-N09
4 1332 1349 (N18W13 L=330) 342 165 0 (1265/1333-1422/1369) 11.3 W09-W19 N16-N19
5 1661 1242 (N17W37 L=354) 2336 360 11 (1542/1130-1746/1366) -25.2 W27-W45 N10-N23
6 350 1340 (N04E49 L=268) 313 77 0 ( 310/1325- 387/1359) 18.4 E52-E46 N02-N05
7 497 1293 (N02E37 L=280) 767 142 2 ( 464/1221- 529/1346) -56.3 E40-E34 S01-N05
8 386 1274 (N00E45 L=272) 495 102 3 ( 332/1246- 436/1300) -6.3 E49-E40 S01-N01
9 1607 1164 (N12W34 L=351) 720 130 6 (1571/1105-1638/1224) 90.0 W31-W36 N07-N15
10 1440 1162 (N08W22 L=339) 461 107 3 (1393/1112-1478/1204) -38.7 W19-W25 N05-N10
11 452 877 (S22E35 L=282) 245 78 0 ( 433/ 845- 474/ 921) 59.0 E36-E33 S24-S19
12 1842 837 (S02W60 L= 17) 516 65 0 (1808/ 812-1874/ 859) 26.6 W56-W63 S03-N00
13 597 790 (S26E24 L=293) 1113 285 4 ( 479/ 725- 727/ 838) 21.3 E33-E15 S31-S22
14 1410 600 (S24W33 L=350) 3497 853 5 (1148/ 516-1737/ 738) 18.9 W13-W56 S29-S13
15 1781 671 (S12W60 L= 17) 341 38 1 (1762/ 648-1797/ 698) -71.6 W58-W61 S13-S10
16 614 628 (S36E22 L=295) 292 94 0 ( 574/ 616- 663/ 645) 15.9 E25-E18 S37-S34
17 482 524 (S45E36 L=281) 644 148 1 ( 427/ 502- 552/ 551) 0.0 E41-E28 S46-S43
18 750 490 (S44E11 L=306) 878 281 1 ( 632/ 449- 893/ 524) 2.6 E21-W01 S45-S41
19 1072 416 (S43W16 L=333) 346 120 0 (1031/ 394-1136/ 445) -6.3 W12-W21 S43-S41
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Download FITS filament maps as tar archive
» All Filament Data of 20250206 ...
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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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