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| 20251106 - Filament data for 10 UTC |
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Available data for 20251106: »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 1295 1806 (N42W50 L= 2) 2108 353 2 (1145/1759-1457/1849) -17.8 W34-W62 N35-N46
2 949 1655 (N43W14 L=325) 451 77 1 ( 916/1615- 985/1691) 29.7 W11-W18 N40-N44
3 776 1596 (N44E01 L=310) 401 135 1 ( 724/1566- 851/1618) -5.7 E05-W05 N42-N45
4 1710 1360 (N05W52 L= 4) 932 136 2 (1664/1294-1745/1411) -90.0 W49-W54 N00-N08
5 654 1243 (N25E17 L=294) 289 79 1 ( 610/1214- 682/1263) -31.0 E20-E15 N22-N25
6 1731 1112 (S09W46 L=357) 1805 311 1 (1674/ 952-1763/1250) 49.1 W38-W51 S16-S01
7 908 1205 (N16E02 L=309) 208 60 0 ( 877/1184- 937/1228) -56.3 E03-W00 N14-N18
8 236 1131 (N27E53 L=258) 1472 273 1 ( 127/1055- 341/1204) -24.0 E70-E43 N20-N33
9 382 1149 (N25E39 L=273) 370 68 2 ( 360/1107- 403/1182) -90.0 E40-E36 N22-N27
10 995 1144 (N11W01 L=313) 405 108 0 ( 943/1128-1054/1162) -21.8 E01-W04 N09-N12
11 503 1061 (N17E31 L=281) 630 263 0 ( 400/ 992- 562/1138) 15.9 E39-E25 N14-N20
12 216 833 (N10E60 L=252) 886 128 2 ( 178/ 783- 261/ 880) 20.0 E65-E53 N07-N11
13 374 792 (N05E46 L=266) 589 119 1 ( 317/ 767- 424/ 813) -20.6 E50-E41 N02-N06
14 867 729 (S09E16 L=296) 335 75 0 ( 850/ 684- 886/ 769) 78.7 E16-E14 S11-S06
15 1407 646 (S27W14 L=326) 320 48 0 (1385/ 614-1428/ 676) 33.7 W12-W15 S28-S25
16 724 570 (S15E29 L=282) 263 67 0 ( 705/ 531- 744/ 605) 78.7 E29-E27 S17-S12
17 350 428 (S16E67 L=244) 5200 426 9 ( 245/ 256- 480/ 560) 73.7 E79-E61 S30-S06
18 1497 410 (S47W18 L=329) 489 92 0 (1440/ 392-1532/ 437) -6.3 W12-W21 S49-S45
19 878 321 (S35E31 L=281) 932 175 1 ( 799/ 265- 938/ 379) 14.0 E39-E23 S37-S32
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Download FITS filament maps as tar archive
» All Filament Data of 20251106 ...
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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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