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| 20221107 - Filament data for 12 UTC |
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Available data for 20221107: »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
1 920 1882 (N64W34 L= 37) 463 49 0 ( 904/1854- 931/1910) 24.8 W28-W41 N60-N66
2 811 1838 (N65W16 L= 19) 917 96 1 ( 769/1798- 844/1879) 13.2 W08-W25 N61-N68
3 1180 1762 (N44W38 L= 41) 774 116 1 (1149/1714-1213/1812) 28.6 W32-W43 N40-N47
4 945 1753 (N51W20 L= 23) 550 86 2 ( 901/1737- 995/1778) -20.6 W15-W23 N48-N54
5 1474 1649 (N27W51 L= 54) 690 136 1 (1417/1621-1528/1688) -56.3 W48-W54 N24-N31
6 1210 1626 (N34W30 L= 33) 241 57 0 (1189/1597-1230/1654) 76.0 W29-W32 N31-N35
7 1376 1550 (N25W37 L= 40) 471 131 0 (1310/1533-1443/1564) -26.6 W33-W41 N22-N26
8 1581 1474 (N15W48 L= 51) 432 53 1 (1553/1449-1603/1504) 9.5 W45-W51 N13-N15
9 937 1441 (N30W05 L= 8) 403 120 0 ( 876/1411- 991/1458) -45.0 W01-W08 N26-N32
10 1275 1437 (N21W26 L= 29) 219 102 0 (1219/1424-1319/1450) -26.6 W22-W28 N19-N22
11 1155 1375 (N20W17 L= 20) 302 101 0 (1105/1362-1204/1394) -38.7 W14-W19 N18-N22
12 362 1134 (N25E41 L=322) 486 59 0 ( 334/1105- 397/1167) -45.0 E43-E38 N22-N26
13 328 1011 (N18E46 L=317) 463 71 1 ( 298/ 980- 356/1041) -53.1 E48-E43 N16-N20
14 256 915 (N14E54 L=309) 305 50 0 ( 245/ 881- 272/ 939) 33.7 E55-E52 N12-N15
15 862 686 (S12E17 L=346) 282 66 0 ( 841/ 652- 886/ 712) 45.0 E18-E15 S13-S10
16 1713 646 (S37W40 L= 43) 315 37 0 (1696/ 628-1733/ 672) -45.0 W38-W42 S38-S35
17 1297 439 (S39W02 L= 5) 1356 301 2 (1190/ 332-1399/ 529) 22.8 E08-W11 S44-S34
18 1466 275 (S61W15 L= 18) 648 55 0 (1429/ 254-1504/ 298) -5.7 W10-W21 S63-S58
19 1327 187 (S65E06 L=357) 488 59 0 (1302/ 169-1356/ 204) 0.0 E09-E01 S67-S61
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Download FITS filament maps as tar archive
» All Filament Data of 20221107 ...
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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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