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| 20250122 - Filament data for 10 UTC |
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Available data for 20250122: »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
1 733 1600 (N28E26 L=129) 845 276 0 ( 676/1555- 843/1674) 4.8 E30-E17 N25-N33
2 1740 1379 (N25W48 L=202) 835 89 2 (1701/1336-1778/1426) -51.3 W44-W51 N22-N27
3 317 1366 (N11E52 L=103) 446 84 1 ( 289/1325- 351/1404) 68.2 E53-E49 N08-N13
4 1234 1352 (N16W10 L=164) 242 49 1 (1203/1330-1256/1375) 0.0 W07-W11 N15-N17
5 1330 1318 (N15W16 L=170) 297 59 1 (1303/1285-1356/1341) 71.6 W14-W17 N13-N16
6 1670 1312 (N19W40 L=195) 269 53 0 (1652/1288-1691/1341) -56.3 W39-W42 N17-N20
7 1126 1209 (N06W04 L=159) 1221 394 2 ( 979/1058-1199/1337) -45.0 E05-W09 S01-N12
8 1676 1215 (N13W41 L=195) 265 91 0 (1663/1176-1695/1248) 59.0 W39-W42 N10-N15
9 563 1131 (S02E29 L=125) 525 159 1 ( 503/1086- 630/1165) -12.5 E33-E24 S04-N00
10 1027 1044 (S04W00 L=154) 220 72 0 ( 992/1026-1074/1060) -14.0 E02-W02 S04-S03
11 870 973 (S09E09 L=146) 272 118 0 ( 827/ 935- 924/1004) 38.7 E11-E05 S12-S07
12 198 931 (S15E59 L= 95) 404 90 0 ( 180/ 888- 221/ 967) 38.7 E61-E56 S17-S13
13 277 892 (S18E51 L=103) 652 143 1 ( 250/ 825- 298/ 956) -82.9 E53-E49 S21-S13
14 139 873 (S19E68 L= 86) 1277 168 4 ( 108/ 819- 169/ 947) -74.1 E74-E64 S21-S14
15 1419 894 (S09W25 L=180) 214 13 0 (1398/ 876-1439/ 912) -18.4 W23-W26 S09-S07
16 1113 785 (S18W08 L=162) 1480 709 1 ( 855/ 719-1415/ 861) 8.4 E08-W26 S23-S13
17 380 652 (S32E45 L=109) 864 170 3 ( 308/ 619- 460/ 698) 14.0 E53-E37 S34-S28
18 1413 462 (S35W36 L=190) 803 133 1 (1349/ 441-1490/ 498) 0.0 W30-W43 S36-S33
19 1415 360 (S42W42 L=197) 747 131 1 (1378/ 327-1480/ 408) -4.4 W37-W50 S44-S38
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Download FITS filament maps as tar archive
» All Filament Data of 20250122 ...
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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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