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| 20240409 - Filament data for 09 UTC |
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Available data for 20240409: »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 1202 1712 (N41E13 L=345) 726 122 0 (1162/1662-1234/1757) -29.1 E17-E08 N38-N44
2 741 1542 (N16E32 L=325) 682 228 1 ( 714/1427- 762/1637) -58.4 E36-E27 N09-N22
3 857 1550 (N19E26 L=332) 696 189 2 ( 822/1458- 880/1635) -47.7 E31-E21 N13-N24
4 300 1458 (N01E63 L=294) 705 101 2 ( 252/1432- 346/1481) 18.4 E68-E59 S01-N02
5 1653 1388 (N35W31 L= 29) 1143 162 3 (1624/1311-1679/1461) -79.7 W27-W33 N29-N40
6 967 1307 (N08E11 L=347) 1277 302 0 ( 869/1206-1079/1399) 69.4 E13-E07 N00-N16
7 1441 1163 (N14W20 L= 17) 378 200 0 (1382/1093-1507/1231) -20.0 W14-W25 N11-N15
8 315 1201 (S14E51 L=307) 749 175 1 ( 249/1161- 389/1230) 4.1 E57-E43 S16-S12
9 1189 1074 (N01W08 L= 5) 1172 272 2 (1104/1028-1272/1149) -5.2 W01-W12 N00-N05
10 780 1006 (S14E13 L=345) 486 145 1 ( 719/ 965- 840/1050) 49.4 E16-E10 S17-S09
11 1656 942 (N08W40 L= 38) 485 106 2 (1636/ 880-1669/ 996) -50.2 W37-W42 N05-N11
12 650 963 (S19E20 L=338) 310 65 0 ( 609/ 942- 685/ 983) 0.0 E23-E17 S20-S18
13 294 820 (S37E48 L=310) 1374 246 2 ( 188/ 766- 416/ 874) 20.1 E65-E35 S42-S31
14 1115 638 (S24W17 L= 15) 2491 606 6 ( 869/ 540-1381/ 759) 51.8 W04-W28 S37-S09
15 1626 551 (S13W55 L= 53) 940 189 2 (1553/ 505-1704/ 586) 14.9 W47-W62 S14-S09
16 404 535 (S54E37 L=321) 987 113 2 ( 350/ 507- 455/ 573) 0.0 E45-E30 S56-S51
17 1486 426 (S24W52 L= 50) 464 119 1 (1431/ 414-1542/ 442) 26.6 W48-W56 S25-S21
18 1381 284 (S35W58 L= 56) 1874 182 2 (1312/ 224-1459/ 346) 90.0 W54-W64 S40-S29
19 1150 252 (S46W45 L= 43) 547 81 1 (1122/ 222-1174/ 294) -36.9 W40-W49 S49-S43
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Download FITS filament maps as tar archive
» All Filament Data of 20240409 ...
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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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