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| 20250124 - Filament data for 10 UTC |
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Available data for 20250124: »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
1 923 1741 (N40E17 L=111) 418 63 2 ( 891/1722- 966/1769) 21.8 E19-E13 N38-N42
2 672 1678 (N33E34 L= 94) 360 55 2 ( 645/1656- 705/1706) 11.3 E35-E30 N31-N35
3 1155 1543 (N28W03 L=131) 1095 384 1 (1056/1478-1328/1639) -24.0 E04-W14 N25-N33
4 1609 1261 (N15W35 L=163) 464 81 3 (1582/1223-1632/1299) 59.0 W33-W37 N12-N17
5 1721 1223 (N15W44 L=172) 332 104 1 (1699/1176-1751/1273) -71.6 W42-W46 N11-N17
6 1542 1127 (N06W31 L=159) 1311 391 1 (1401/ 977-1612/1267) -40.9 W20-W36 S01-N13
7 1939 1168 (N16W70 L=198) 685 46 3 (1923/1142-1961/1194) 33.7 W67-W75 N13-N17
8 1015 1071 (S03E01 L=127) 461 172 0 ( 937/1015-1078/1097) -20.6 E05-W03 S05-S01
9 164 895 (S18E64 L= 64) 4482 378 7 ( 102/ 760- 211/1083) 55.6 E82-E57 S26-S07
10 102 1004 (S12E73 L= 55) 932 70 3 ( 66/ 981- 131/1031) -8.1 E82-E67 S13-S09
11 353 894 (S18E44 L= 84) 1065 306 2 ( 287/ 825- 416/ 966) -48.8 E49-E38 S22-S13
12 1370 761 (S17W24 L=153) 1913 758 6 (1206/ 645-1614/ 930) -3.8 W12-W42 S24-S07
13 1795 867 (S05W54 L=182) 777 87 2 (1757/ 826-1836/ 903) -12.5 W50-W59 S07-S03
14 1739 713 (S15W53 L=182) 1357 224 4 (1644/ 663-1816/ 769) 21.8 W46-W61 S18-S11
15 1644 728 (S15W45 L=173) 288 32 0 (1624/ 702-1664/ 757) 90.0 W43-W45 S16-S13
16 1216 692 (S23W16 L=144) 187 51 1 (1201/ 657-1237/ 722) 90.0 W14-W16 S25-S21
17 967 645 (S29W00 L=128) 283 80 1 ( 944/ 605- 994/ 688) 90.0 W00-W01 S31-S25
18 323 551 (S40E56 L= 72) 1874 179 2 ( 241/ 502- 399/ 590) 9.5 E75-E45 S43-S37
19 1638 395 (S35W63 L=191) 1472 107 3 (1598/ 358-1685/ 432) 0.0 W56-W71 S37-S32
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Download FITS filament maps as tar archive
» All Filament Data of 20250124 ...
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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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