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| 20250125 - Filament data for 10 UTC |
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Available data for 20250125: »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
1 838 1657 (N32E21 L= 94) 356 47 1 ( 817/1636- 871/1686) 0.0 E22-E18 N30-N34
2 1252 1563 (N30W09 L=124) 513 170 0 (1208/1492-1293/1637) -52.1 W05-W12 N25-N35
3 1052 1437 (N19E03 L=112) 404 135 0 (1037/1370-1080/1500) -63.4 E04-W00 N15-N23
4 1485 1464 (N27W26 L=141) 286 79 0 (1453/1442-1525/1489) -26.6 W23-W29 N25-N28
5 877 1325 (N11E12 L=103) 208 85 0 ( 848/1293- 906/1358) 59.0 E13-E10 N08-N13
6 1762 1221 (N15W48 L=163) 683 88 2 (1740/1177-1804/1261) 63.4 W45-W52 N12-N18
7 1698 1111 (N08W42 L=157) 1775 414 2 (1561/ 948-1777/1248) -34.4 W31-W50 N00-N14
8 1843 1206 (N16W56 L=171) 414 40 0 (1829/1177-1859/1237) -90.0 W54-W58 N14-N18
9 1841 1108 (N10W56 L=171) 339 61 1 (1813/1086-1866/1133) 18.4 W52-W58 N08-N11
10 306 1021 (S11E48 L= 67) 554 78 0 ( 285/ 972- 324/1067) -78.7 E49-E46 S13-S08
11 191 1023 (S11E60 L= 55) 720 71 1 ( 156/ 989- 221/1055) -23.2 E64-E56 S13-S09
12 1243 1023 (S03W13 L=128) 505 177 0 (1155/ 963-1292/1054) -12.5 W07-W16 S06-S01
13 232 854 (S21E56 L= 59) 3315 447 3 ( 121/ 762- 341/ 953) 27.6 E70-E44 S26-S15
14 517 871 (S19E31 L= 84) 937 315 2 ( 445/ 813- 583/ 952) -49.4 E36-E26 S22-S14
15 1801 717 (S13W60 L=175) 6772 0 27 (1568/ 552-1937/ 883) 25.2 W41-W76 S23-S02
16 1194 844 (S14W12 L=127) 195 53 1 (1165/ 826-1226/ 865) -14.0 W10-W14 S15-S13
17 1482 655 (S22W35 L=150) 622 152 0 (1458/ 592-1526/ 733) -41.2 W31-W39 S25-S17
18 440 549 (S40E42 L= 73) 1596 209 4 ( 342/ 516- 550/ 587) 7.1 E54-E30 S42-S37
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Download FITS filament maps as tar archive
» All Filament Data of 20250125 ...
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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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