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| 20221107 - Filament data for 10 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
1 814 1855 (N66W19 L= 23) 1365 157 1 ( 764/1798- 860/1917) 15.7 W07-W39 N61-N72
2 914 1882 (N64W33 L= 37) 474 41 0 ( 900/1852- 926/1911) 28.3 W28-W41 N60-N67
3 1170 1754 (N43W37 L= 41) 732 113 0 (1140/1712-1199/1800) 26.6 W31-W41 N40-N47
4 935 1750 (N51W19 L= 23) 522 63 1 ( 892/1733- 975/1767) -26.6 W15-W22 N48-N53
5 1462 1644 (N28W49 L= 53) 640 125 0 (1407/1617-1519/1683) -50.2 W47-W53 N24-N31
6 1200 1621 (N34W29 L= 33) 262 51 1 (1179/1591-1218/1649) 53.1 W28-W31 N31-N35
7 1364 1544 (N25W36 L= 40) 429 151 0 (1283/1527-1430/1558) -16.7 W30-W40 N22-N26
8 1565 1463 (N15W46 L= 50) 378 71 1 (1539/1423-1583/1490) 63.4 W43-W48 N12-N16
9 921 1434 (N30W04 L= 8) 469 155 0 ( 846/1395- 979/1452) -49.4 W00-W07 N25-N32
10 1200 1428 (N22W21 L= 25) 391 211 1 (1090/1417-1296/1442) -22.6 W14-W26 N19-N24
11 1140 1367 (N20W15 L= 19) 288 109 0 (1088/1354-1194/1388) -33.7 W12-W18 N18-N22
12 812 1303 (N24E06 L=358) 217 67 1 ( 783/1285- 845/1325) -53.1 E07-E04 N22-N26
13 352 1128 (N25E42 L=322) 432 81 0 ( 322/1091- 392/1161) -51.3 E44-E38 N21-N26
14 314 1002 (N18E47 L=317) 485 85 1 ( 289/ 974- 346/1036) -59.0 E49-E44 N15-N20
15 846 677 (S12E19 L=345) 298 73 1 ( 823/ 643- 871/ 708) 36.9 E20-E16 S13-S10
16 1712 649 (S37W40 L= 44) 394 33 0 (1694/ 626-1730/ 672) -63.4 W38-W42 S38-S34
17 1295 444 (S38W02 L= 6) 1460 346 2 (1183/ 326-1398/ 557) 26.6 E09-W11 S44-S32
18 1460 273 (S61W14 L= 18) 660 61 1 (1424/ 251-1498/ 297) -5.2 W09-W20 S62-S58
19 1325 187 (S65E06 L=358) 521 56 0 (1297/ 168-1354/ 206) -23.2 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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