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| 20251001 - Filament data for 07 UTC |
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Available data for 20251001: »06 UTC »07 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
1 687 1714 (N60E02 L= 66) 938 183 0 ( 625/1652- 759/1782) 20.2 E10-W10 N56-N64
2 502 1629 (N60E27 L= 41) 704 119 1 ( 444/1598- 554/1657) 0.0 E35-E19 N57-N62
3 1169 1330 (N19W17 L= 85) 535 154 2 (1089/1304-1246/1348) -24.0 W12-W21 N17-N22
4 1866 1102 (S14W59 L=127) 3492 367 8 (1797/1010-1933/1281) -75.3 W51-W68 S21-S02
5 1873 1202 (S09W64 L=132) 1404 122 3 (1845/1142-1898/1256) -90.0 W59-W69 S12-S05
6 416 1207 (N32E36 L= 32) 236 30 0 ( 394/1191- 440/1223) 0.0 E37-E33 N30-N32
7 1460 1174 (N03W29 L= 97) 292 86 0 (1445/1128-1476/1218) 59.0 W26-W30 N00-N05
8 226 1122 (N30E56 L= 12) 543 105 2 ( 182/1101- 277/1151) -13.0 E62-E49 N28-N32
9 813 1048 (N13E11 L= 57) 450 170 2 ( 757/ 983- 878/1081) 7.1 E15-E07 N10-N14
10 1716 967 (S16W41 L=109) 886 256 3 (1689/ 855-1740/1066) 81.3 W38-W43 S23-S10
11 656 1015 (N15E22 L= 47) 334 133 1 ( 595/ 994- 705/1044) -23.2 E25-E17 N14-N17
12 1837 986 (S19W53 L=121) 409 36 1 (1823/ 957-1857/1013) 45.0 W51-W55 S20-S17
13 499 977 (N16E33 L= 35) 337 118 0 ( 440/ 952- 559/1001) -35.5 E36-E29 N13-N19
14 1785 904 (S22W46 L=114) 413 36 2 (1767/ 875-1805/ 930) 56.3 W44-W48 S24-S20
15 227 836 (N13E60 L= 8) 722 106 1 ( 202/ 787- 262/ 868) 29.7 E63-E55 N10-N15
16 552 636 (S04E38 L= 30) 329 73 2 ( 527/ 611- 584/ 662) -11.3 E40-E35 S05-S02
17 1702 575 (S41W36 L=104) 2046 202 3 (1630/ 519-1762/ 659) 19.7 W28-W42 S45-S35
18 435 399 (S16E61 L= 7) 2058 171 6 ( 374/ 344- 499/ 455) -73.3 E66-E55 S21-S11
19 1268 354 (S41E05 L= 63) 1607 292 5 (1158/ 290-1407/ 432) 2.6 E15-W07 S44-S38
20 963 185 (S45E38 L= 30) 1170 119 1 ( 913/ 153-1025/ 225) 11.3 E44-E29 S48-S42
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Download FITS filament maps as tar archive
» All Filament Data of 20251001 ...
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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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