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| 20250104 - Filament data for 09 UTC |
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Available data for 20250104: »07 UTC »08 UTC »09 UTC »10 UTC »11 UTC »12 UTC |
Click on image to open sensitive map! |
Color xc yc (LatLon LCarr) Area Length Branches ( x0/y0 x1/y1 ) Tilt Location
1 1552 1667 (N39W45 L= 77) 391 42 0 (1528/1646-1573/1690) 23.2 W40-W47 N37-N40
2 1331 1598 (N33W22 L= 54) 273 84 0 (1287/1581-1370/1613) -18.4 W18-W24 N31-N34
3 1820 1460 (N25W65 L= 97) 900 75 1 (1780/1420-1858/1502) -35.5 W61-W70 N22-N27
4 502 1268 (N12E33 L=359) 723 135 2 ( 478/1211- 547/1338) -63.4 E35-E29 N08-N16
5 328 1233 (N10E47 L=345) 637 143 1 ( 298/1166- 372/1289) 54.5 E48-E43 N06-N13
6 390 1220 (N09E41 L=351) 293 32 1 ( 371/1199- 409/1242) 71.6 E42-E39 N07-N10
7 720 1082 (N00E18 L= 14) 825 252 2 ( 609/1038- 828/1118) 4.1 E25-E11 S02-N02
8 1043 888 (S12W01 L= 33) 1560 501 3 ( 989/ 665-1085/1099) -87.8 E02-W03 S25-N01
9 1789 922 (S08W53 L= 85) 885 180 3 (1758/ 859-1818/1008) 82.9 W49-W55 S11-S03
10 637 893 (S11E24 L= 8) 740 140 5 ( 575/ 855- 698/ 943) 12.5 E28-E19 S13-S07
11 1724 903 (S10W47 L= 79) 428 35 1 (1702/ 869-1747/ 932) -76.0 W44-W49 S11-S07
12 1767 794 (S16W53 L= 85) 1559 321 2 (1676/ 723-1872/ 867) 26.6 W45-W63 S20-S11
13 1576 763 (S18W37 L= 69) 795 243 0 (1518/ 666-1606/ 866) 76.0 W33-W39 S24-S12
14 603 740 (S20E28 L= 5) 371 142 1 ( 565/ 702- 667/ 787) -26.6 E29-E23 S22-S17
15 415 654 (S25E44 L=348) 979 179 4 ( 334/ 595- 480/ 714) 21.8 E52-E37 S28-S21
16 1417 668 (S25W26 L= 59) 233 39 1 (1396/ 651-1446/ 689) -14.0 W24-W28 S25-S23
17 927 592 (S30E07 L= 25) 557 145 0 ( 858/ 554- 989/ 634) 24.0 E11-E02 S32-S27
18 503 417 (S41E46 L=347) 3550 361 7 ( 328/ 367- 673/ 477) 5.4 E80-E27 S43-S37
19 1554 364 (S45W51 L= 83) 3317 405 8 (1381/ 260-1707/ 447) 30.0 W39-W65 S54-S38
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Download FITS filament maps as tar archive
» All Filament Data of 20250104 ...
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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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