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| 20250101 - Filament data for 11 UTC |
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Available data for 20250101: »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC »13 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 1067 1756 (N46W05 L= 76) 369 30 1 (1039/1740-1096/1775) 11.3 W02-W07 N44-N47
2 1099 1683 (N39W07 L= 77) 358 58 1 (1076/1651-1127/1721) 80.5 W05-W09 N36-N42
3 1704 1545 (N29W55 L=125) 2152 257 6 (1587/1476-1799/1617) -22.8 W44-W65 N24-N34
4 810 1571 (N32E14 L= 56) 789 169 0 ( 730/1512- 870/1604) -28.6 E20-E09 N27-N34
5 1452 1479 (N24W30 L=100) 719 170 2 (1369/1439-1533/1508) -4.4 W23-W36 N21-N26
6 1658 1340 (N16W43 L=114) 1310 390 1 (1582/1150-1733/1468) -69.8 W39-W47 N04-N23
7 1852 1294 (N13W62 L=132) 1847 196 7 (1810/1215-1903/1382) -78.7 W58-W68 N08-N18
8 213 1061 (N02E57 L= 14) 346 69 1 ( 181/1046- 243/1074) 8.1 E60-E53 N00-N02
9 450 860 (S11E37 L= 33) 1855 533 4 ( 366/ 623- 487/1068) -85.6 E42-E34 S25-N01
10 196 856 (S10E61 L= 10) 5156 327 12 ( 128/ 710- 293/1007) 62.1 E72-E50 S18-S01
11 1176 929 (S09W09 L= 79) 229 101 0 (1130/ 918-1226/ 946) -11.3 W06-W11 S09-S07
12 636 891 (S10E24 L= 46) 300 61 1 ( 598/ 862- 663/ 922) 26.6 E26-E22 S11-S08
13 990 845 (S14E02 L= 68) 440 178 1 ( 923/ 779-1033/ 920) -58.0 E06-W00 S17-S09
14 1260 841 (S14W14 L= 85) 228 96 0 (1210/ 808-1286/ 862) -26.6 W11-W15 S16-S12
15 280 756 (S17E54 L= 16) 1038 160 5 ( 212/ 705- 336/ 794) -20.0 E60-E49 S19-S14
16 870 692 (S23E10 L= 60) 1356 458 2 ( 720/ 649-1043/ 774) -6.0 E19-W00 S25-S17
17 1533 542 (S33W38 L=108) 961 179 2 (1466/ 515-1621/ 570) 4.4 W31-W45 S34-S31
18 368 466 (S35E58 L= 12) 1907 246 2 ( 305/ 373- 444/ 558) 12.8 E89-E45 S40-S29
19 1351 498 (S36W23 L= 94) 370 61 0 (1324/ 477-1390/ 520) 36.9 W21-W26 S37-S34
20 1172 406 (S43W11 L= 81) 895 167 3 (1102/ 371-1258/ 442) 22.6 W05-W17 S45-S40
21 1191 255 (S56W16 L= 86) 336 62 0 (1165/ 235-1213/ 280) 45.0 W13-W17 S57-S53
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Download FITS filament maps as tar archive
» All Filament Data of 20250101 ...
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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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