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| 20240420 - Filament data for 12 UTC |
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Available data for 20240420: »06 UTC »08 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
1 573 1759 (N27E61 L=150) 521 35 0 ( 550/1735- 596/1780) -18.4 E65-E56 N25-N28
2 431 1693 (N19E69 L=142) 818 95 0 ( 392/1659- 470/1729) 71.6 E72-E67 N16-N22
3 761 1639 (N23E36 L=175) 435 134 0 ( 710/1583- 787/1675) -18.4 E40-E31 N20-N25
4 598 1639 (N19E47 L=164) 327 59 0 ( 575/1620- 627/1666) -18.4 E50-E44 N18-N20
5 990 1442 (N17E14 L=197) 1314 542 1 ( 879/1261-1105/1664) -33.7 E29-E02 N09-N28
6 1509 1419 (N32W19 L=230) 601 192 1 (1474/1330-1529/1496) -63.4 W15-W21 N26-N36
7 406 1340 (S03E48 L=163) 1862 298 4 ( 311/1230- 467/1463) 82.9 E52-E43 S11-N05
8 688 1448 (N10E32 L=179) 226 92 0 ( 650/1425- 737/1462) 38.7 E33-E28 N07-N11
9 1340 1391 (N25W08 L=219) 542 188 1 (1293/1310-1365/1453) -45.0 W03-W11 N19-N27
10 268 1360 (S04E62 L=149) 1056 150 3 ( 236/1284- 293/1416) -32.5 E69-E57 S08-S01
11 1708 1374 (N37W38 L=249) 340 48 0 (1692/1339-1720/1399) -63.4 W35-W39 N34-N39
12 1292 1256 (N15W09 L=220) 230 80 0 (1255/1234-1327/1277) 0.0 W06-W11 N14-N15
13 1774 1111 (N22W47 L=258) 355 54 1 (1753/1076-1790/1137) -45.0 W44-W48 N20-N23
14 417 983 (S23E37 L=174) 877 212 0 ( 342/ 924- 478/1065) 56.3 E43-E34 S28-S16
15 1051 868 (S13W06 L=217) 781 268 3 ( 962/ 830-1155/ 906) 45.0 W00-W10 S17-S08
16 947 888 (S15E01 L=210) 194 24 0 ( 922/ 871- 967/ 905) 63.4 E02-W00 S15-S13
17 1192 833 (S11W15 L=226) 412 109 2 (1151/ 797-1248/ 870) 56.3 W12-W17 S13-S07
18 771 724 (S29E07 L=204) 1041 386 1 ( 630/ 685- 949/ 794) 13.4 E17-W04 S31-S23
19 658 427 (S53E07 L=204) 653 131 1 ( 595/ 401- 723/ 464) 4.4 E13-W00 S54-S51
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Download FITS filament maps as tar archive
» All Filament Data of 20240420 ...
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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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