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| 20230926 - Latest Filament data |
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Available data for 20230926: »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
1 976 1629 (N44W18 L= 77) 441 52 1 ( 937/1602-1004/1652) -36.9 W15-W20 N41-N46
2 1600 1492 (N15W52 L=111) 519 138 3 (1585/1439-1621/1553) 29.1 W48-W57 N12-N18
3 1492 1390 (N14W39 L= 98) 601 96 3 (1438/1362-1541/1414) -23.2 W35-W43 N11-N15
4 811 1211 (N23E08 L= 51) 364 72 1 ( 774/1179- 843/1237) -68.2 E09-E05 N20-N25
5 1788 1133 (S09W53 L=111) 396 67 1 (1762/1102-1814/1163) 9.5 W49-W55 S10-S07
6 1685 1077 (S09W42 L=101) 254 37 0 (1667/1055-1703/1100) 18.4 W40-W43 S10-S07
7 506 998 (N18E32 L= 26) 556 154 2 ( 454/ 952- 567/1060) 15.3 E37-E26 N15-N20
8 200 1015 (N24E61 L=357) 459 66 0 ( 165/ 991- 231/1034) 6.3 E66-E57 N23-N25
9 268 948 (N19E54 L= 5) 625 128 1 ( 234/ 900- 315/1010) -40.6 E56-E49 N16-N23
10 828 953 (N08E13 L= 46) 215 63 0 ( 812/ 918- 845/ 984) 45.0 E14-E11 N06-N09
11 181 859 (N15E67 L=352) 856 133 0 ( 158/ 797- 210/ 922) -63.4 E69-E63 N11-N19
12 1363 848 (S12W15 L= 73) 299 63 0 (1339/ 815-1386/ 871) 56.3 W12-W16 S13-S10
13 1643 803 (S24W33 L= 92) 721 170 0 (1590/ 728-1693/ 862) 26.6 W27-W37 S26-S21
14 1722 762 (S29W39 L= 98) 404 85 0 (1692/ 730-1748/ 805) 26.6 W36-W42 S30-S27
15 1225 680 (S18W02 L= 61) 1052 392 0 (1054/ 662-1401/ 709) -21.8 E07-W13 S22-S13
16 1734 605 (S41W41 L=100) 552 60 2 (1702/ 576-1762/ 635) 36.9 W37-W45 S42-S39
17 1096 555 (S22E09 L= 50) 238 79 0 (1081/ 522-1115/ 590) 53.1 E09-E06 S24-S20
18 431 437 (S14E59 L=360) 2050 325 3 ( 381/ 346- 471/ 579) 51.3 E73-E47 S20-S05
19 719 430 (S20E37 L= 22) 356 76 1 ( 703/ 391- 739/ 468) 63.4 E38-E35 S23-S17
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Download FITS filament maps as tar archive
» All Filament Data of 20230926 ...
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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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