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| 20250403 - Filament data for 12 UTC |
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Available data for 20250403: »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 1147 1709 (N38E15 L=283) 985 213 0 (1057/1663-1243/1763) 0.0 E23-E07 N36-N39
2 598 1527 (N11E40 L=258) 982 223 2 ( 546/1442- 650/1630) -31.0 E48-E33 N07-N16
3 1528 1376 (N28W20 L=318) 263 82 0 (1500/1340-1556/1411) -26.6 W17-W23 N26-N29
4 1469 1328 (N23W17 L=315) 303 101 0 (1421/1299-1508/1361) 0.0 W13-W20 N22-N24
5 1889 1087 (N24W59 L=357) 768 105 0 (1851/1044-1917/1130) -11.3 W53-W64 N22-N25
6 688 1044 (S14E19 L=279) 334 72 3 ( 660/1019- 713/1089) 90.0 E20-E17 S15-S11
7 1770 944 (N12W49 L=347) 669 100 2 (1749/ 899-1789/1001) -81.9 W46-W51 N08-N15
8 1835 885 (N11W57 L=355) 1886 210 3 (1788/ 810-1887/ 977) 76.0 W52-W62 N05-N17
9 1045 906 (S12W04 L=302) 392 146 0 ( 994/ 853-1087/ 969) -20.6 W00-W08 S14-S09
10 952 816 (S20W02 L=300) 442 133 1 ( 894/ 788-1013/ 840) 15.9 E02-W05 S21-S17
11 1782 776 (N03W56 L=354) 384 31 1 (1756/ 756-1803/ 797) 26.6 W53-W58 N02-N04
12 806 717 (S29E04 L=294) 298 118 0 ( 777/ 669- 858/ 740) 63.4 E05-E01 S32-S26
13 217 688 (S47E62 L=236) 608 75 1 ( 175/ 670- 253/ 708) 11.9 E73-E54 S48-S44
14 1445 609 (S16W38 L=336) 280 58 1 (1412/ 594-1479/ 630) 21.8 W35-W40 S17-S15
15 546 542 (S48E20 L=278) 711 184 2 ( 462/ 503- 624/ 580) 6.7 E28-E11 S50-S46
16 868 452 (S44W10 L=308) 321 71 0 ( 843/ 428- 907/ 484) -8.1 W06-W13 S44-S41
17 1445 343 (S30W55 L=353) 496 83 0 (1410/ 314-1480/ 377) 0.0 W49-W60 S31-S29
18 1584 326 (S26W70 L= 8) 576 47 0 (1562/ 301-1605/ 348) 0.0 W65-W76 S26-S24
19 1027 168 (S58W49 L=347) 532 58 0 (1007/ 135-1049/ 197) -11.3 W42-W57 S59-S55
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Download FITS filament maps as tar archive
» All Filament Data of 20250403 ...
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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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