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| 20230927 - Filament data for 07 UTC |
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Available data for 20230927: »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 1035 1686 (N45W26 L= 75) 944 151 2 ( 968/1650-1113/1711) -20.0 W19-W31 N42-N48
2 1384 1552 (N26W40 L= 89) 488 108 2 (1344/1527-1427/1569) -31.0 W37-W43 N23-N27
3 1671 1517 (N14W60 L=109) 419 65 1 (1656/1488-1685/1552) 53.1 W57-W63 N12-N16
4 1576 1449 (N14W48 L= 97) 778 151 0 (1511/1431-1647/1482) -13.0 W42-W55 N12-N15
5 929 1274 (N23W01 L= 50) 283 61 1 ( 906/1248- 951/1302) -76.0 W00-W02 N21-N25
6 1642 1227 (N00W43 L= 92) 302 57 0 (1618/1194-1661/1253) -71.6 W41-W44 S01-N02
7 1839 1146 (S11W59 L=108) 1438 199 3 (1784/1067-1907/1207) 8.5 W50-W71 S13-S07
8 635 1060 (N18E22 L= 27) 624 201 0 ( 563/1001- 707/1124) 18.4 E28-E16 N16-N20
9 173 984 (N23E66 L=343) 1979 167 5 ( 144/ 906- 219/1063) 71.6 E70-E59 N18-N27
10 340 984 (N20E46 L= 3) 995 257 3 ( 240/ 896- 390/1049) -45.0 E56-E42 N14-N25
11 971 1010 (N07E03 L= 46) 268 70 1 ( 940/ 967- 996/1036) 45.0 E04-E01 N05-N08
12 263 870 (N15E56 L=353) 873 166 3 ( 235/ 807- 309/ 956) -84.3 E59-E51 N10-N20
13 1502 912 (S12W25 L= 74) 320 102 3 (1475/ 874-1537/ 950) 53.1 W23-W26 S14-S10
14 1747 862 (S24W43 L= 92) 932 208 2 (1684/ 774-1796/ 937) 26.6 W35-W48 S27-S20
15 1803 811 (S29W49 L= 98) 456 71 0 (1776/ 785-1830/ 842) 9.5 W45-W52 S30-S27
16 1380 752 (S18W13 L= 62) 988 373 2 (1213/ 727-1545/ 787) -20.0 W03-W25 S22-S13
17 508 449 (S15E51 L=358) 1605 353 2 ( 439/ 356- 558/ 598) 33.1 E65-E40 S20-S05
18 855 459 (S22E27 L= 22) 444 78 2 ( 832/ 412- 879/ 494) 51.3 E28-E24 S24-S19
19 637 287 (S29E53 L=356) 442 73 0 ( 615/ 255- 658/ 317) 39.8 E57-E50 S30-S25
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Download FITS filament maps as tar archive
» All Filament Data of 20230927 ...
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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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