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| 20250905 - Filament data for 09 UTC |
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Available data for 20250905: »06 UTC »07 UTC »08 UTC »09 UTC »10 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 1074 1853 (N58W44 L= 94) 449 69 0 (1041/1826-1107/1875) -14.0 W38-W50 N56-N59
2 1585 1581 (N24W56 L=106) 699 111 0 (1539/1536-1631/1613) -63.4 W53-W58 N19-N26
3 1256 1549 (N32W30 L= 80) 423 83 2 (1232/1513-1294/1582) -90.0 W28-W31 N28-N34
4 1702 1385 (N10W55 L=105) 2720 462 5 (1593/1324-1841/1485) -39.8 W45-W69 N02-N17
5 1401 1445 (N22W35 L= 85) 250 17 0 (1380/1424-1423/1463) -71.6 W33-W36 N20-N23
6 532 1345 (N37E27 L= 23) 405 91 1 ( 493/1312- 567/1374) -39.8 E30-E24 N33-N39
7 1649 1179 (N00W42 L= 92) 773 214 0 (1624/1073-1668/1280) 74.7 W39-W44 S05-N06
8 1127 1192 (N14W10 L= 60) 664 296 2 (1061/1108-1186/1259) 26.6 W04-W14 N09-N17
9 469 1078 (N21E34 L= 16) 519 149 1 ( 403/1041- 524/1117) -29.1 E39-E30 N19-N24
10 752 1047 (N14E15 L= 35) 475 124 0 ( 699/1024- 815/1076) -39.8 E18-E11 N11-N16
11 1873 983 (S18W59 L=109) 1261 155 1 (1834/ 909-1911/1048) -59.0 W55-W65 S23-S13
12 1828 936 (S19W53 L=103) 909 174 1 (1791/ 866-1866/1020) -61.4 W49-W57 S24-S13
13 677 932 (N09E22 L= 28) 302 41 1 ( 658/ 901- 697/ 962) 56.3 E23-E20 N07-N10
14 1408 764 (S17W17 L= 67) 1376 432 3 (1256/ 685-1535/ 903) 14.0 W06-W27 S19-S11
15 354 793 (N06E49 L= 1) 690 172 0 ( 328/ 722- 374/ 877) 83.7 E51-E46 N02-N11
16 1592 519 (S39W28 L= 78) 4830 628 5 (1345/ 359-1831/ 675) 7.0 W05-W57 S45-S33
17 696 589 (S11E30 L= 20) 320 67 1 ( 663/ 573- 736/ 613) -26.6 E31-E27 S12-S09
18 318 505 (S11E65 L=345) 1425 207 1 ( 294/ 414- 356/ 604) 52.4 E72-E59 S17-S04
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Download FITS filament maps as tar archive
» All Filament Data of 20250905 ...
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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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