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| 20250622 - Filament data for 11 UTC |
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Available data for 20250622: »04 UTC »05 UTC »06 UTC »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
1 727 1660 (N41E31 L=290) 4058 545 8 ( 487/1528- 931/1770) -11.0 E73-E11 N32-N47
2 1142 1540 (N36W04 L=325) 1350 293 3 (1010/1496-1283/1564) 8.5 E05-W15 N32-N38
3 426 1462 (N24E49 L=272) 373 63 0 ( 410/1441- 455/1496) -26.6 E51-E45 N22-N26
4 238 1414 (N19E68 L=252) 1683 122 2 ( 198/1366- 268/1469) -50.2 E74-E64 N16-N22
5 1428 1383 (N27W25 L=346) 600 203 1 (1365/1303-1490/1457) -48.4 W21-W29 N22-N31
6 1221 1348 (N23W10 L=331) 482 142 0 (1194/1279-1237/1418) 83.7 W08-W11 N18-N27
7 1121 1334 (N22W04 L=325) 323 132 2 (1095/1285-1154/1407) -63.4 W02-W06 N18-N26
8 342 1139 (N03E47 L=273) 2053 336 2 ( 309/ 987- 375/1296) -86.8 E49-E44 S05-N13
9 1833 1237 (N20W62 L= 22) 1139 145 3 (1776/1204-1878/1276) 0.0 W54-W68 N17-N22
10 1623 1245 (N19W40 L= 1) 312 98 0 (1574/1235-1669/1255) 7.1 W35-W43 N18-N20
11 1898 1158 (N15W70 L= 30) 1292 61 1 (1859/1125-1930/1194) 29.7 W63-W77 N13-N17
12 182 971 (S08E63 L=258) 477 112 1 ( 149/ 929- 211/1018) 33.7 E68-E59 S11-S05
13 1907 959 (N03W70 L= 31) 610 70 1 (1882/ 927-1936/ 981) 21.8 W66-W76 N00-N04
14 564 769 (S17E28 L=292) 250 95 0 ( 518/ 752- 601/ 793) -9.5 E31-E25 S18-S16
15 1333 656 (S19W23 L=344) 1173 238 1 (1229/ 618-1454/ 704) 19.7 W16-W30 S21-S14
16 364 679 (S25E46 L=274) 306 75 1 ( 340/ 654- 396/ 699) 26.6 E49-E42 S27-S23
17 1029 520 (S30W04 L=325) 722 140 1 ( 963/ 498-1102/ 543) 12.5 W00-W09 S32-S28
18 666 375 (S45E25 L=296) 302 29 1 ( 645/ 360- 687/ 396) 0.0 E27-E22 S46-S43
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Download FITS filament maps as tar archive
» All Filament Data of 20250622 ...
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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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