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| 20240509 - Filament data for 13 UTC |
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Available data for 20240509: »06 UTC »13 UTC »14 UTC »15 UTC »16 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 674 1750 (N33E50 L=269) 711 93 2 ( 644/1704- 706/1790) -24.8 E57-E44 N29-N35
2 460 1662 (N22E62 L=257) 1149 149 1 ( 439/1590- 481/1715) -34.7 E72-E57 N16-N25
3 514 1626 (N20E54 L=266) 864 186 0 ( 469/1557- 559/1711) -65.6 E57-E51 N15-N26
4 1255 1684 (N45E04 L=315) 483 75 1 (1219/1664-1295/1703) 8.1 E07-W00 N42-N46
5 343 1579 (N14E69 L=251) 1343 96 2 ( 306/1533- 378/1619) -56.3 E72-E64 N10-N16
6 621 1558 (N18E41 L=279) 483 75 2 ( 581/1529- 649/1583) -8.1 E44-E37 N16-N20
7 309 1422 (N04E61 L=259) 451 65 1 ( 275/1404- 338/1443) 36.9 E64-E57 N02-N05
8 1122 1271 (N13E00 L=319) 392 161 2 (1093/1207-1148/1349) -49.4 E04-W02 N09-N17
9 1624 1279 (N27W33 L=352) 476 88 1 (1602/1232-1649/1319) 90.0 W31-W35 N24-N30
10 1899 1124 (N26W66 L= 26) 3251 252 3 (1854/1015-1939/1252) -40.9 W59-W76 N20-N33
11 1807 1135 (N24W52 L= 12) 364 49 1 (1787/1112-1828/1158) -11.3 W49-W55 N22-N25
12 420 1133 (S11E41 L=279) 256 27 0 ( 396/1117- 443/1148) 26.6 E42-E38 S11-S09
13 1864 1060 (N21W61 L= 20) 436 35 2 (1843/1040-1886/1078) 8.1 W57-W64 N19-N22
14 1860 981 (N16W61 L= 21) 887 152 1 (1813/ 942-1897/1031) -8.7 W54-W67 N14-N18
15 303 772 (S36E48 L=271) 665 113 1 ( 270/ 724- 351/ 800) 33.7 E52-E42 S39-S32
16 1123 682 (S20W15 L=334) 313 140 0 (1101/ 628-1157/ 744) -76.0 W13-W17 S23-S15
17 452 621 (S42E32 L=287) 1391 252 3 ( 344/ 594- 573/ 659) 7.1 E44-E20 S44-S38
18 1430 605 (S17W37 L=356) 407 80 2 (1394/ 581-1465/ 624) 0.0 W33-W40 S18-S15
19 1530 418 (S25W56 L= 15) 343 35 0 (1506/ 401-1555/ 433) 26.6 W53-W57 S25-S23
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Download FITS filament maps as tar archive
» All Filament Data of 20240509 ...
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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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