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| 20250918 - Filament data for 09 UTC |
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Available data for 20250918: »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 1466 1792 (N36W69 L=307) 470 21 0 (1447/1773-1487/1808) 0.0 W63-W73 N35-N37
2 1402 1783 (N39W61 L=299) 449 63 0 (1386/1751-1430/1802) 6.3 W56-W65 N37-N39
3 1717 1486 (N12W62 L=300) 1594 210 3 (1610/1447-1805/1534) -36.3 W53-W70 N07-N18
4 1023 1355 (N26W09 L=247) 658 186 3 ( 931/1304-1092/1412) -52.1 W04-W11 N21-N31
5 1063 1261 (N19W08 L=247) 419 180 0 ( 977/1232-1141/1281) -11.3 W02-W12 N17-N20
6 1613 1147 (S02W38 L=276) 716 153 0 (1588/1066-1638/1207) 50.2 W35-W41 S05-N01
7 1076 1072 (N08W04 L=242) 227 137 0 (1045/1015-1108/1136) 45.0 W01-W07 N05-N11
8 323 1069 (N25E46 L=192) 365 46 1 ( 293/1042- 347/1096) -31.0 E49-E44 N22-N26
9 264 909 (N16E54 L=184) 560 104 1 ( 226/ 862- 293/ 945) -59.0 E58-E52 N13-N18
10 1861 871 (S26W56 L=294) 734 111 0 (1815/ 848-1895/ 907) -20.0 W49-W61 S28-S23
11 467 847 (N09E38 L=200) 341 66 0 ( 442/ 810- 496/ 881) -68.2 E39-E36 N06-N11
12 235 788 (N10E61 L=178) 409 36 0 ( 214/ 772- 264/ 806) -21.8 E63-E57 N08-N10
13 438 537 (S08E51 L=187) 715 165 0 ( 384/ 473- 465/ 600) -90.0 E54-E49 S12-S03
14 1383 391 (S42W06 L=244) 3577 731 4 (1085/ 221-1652/ 574) 7.4 E23-W31 S47-S36
15 1190 520 (S27E03 L=235) 367 80 0 (1171/ 482-1210/ 566) 80.5 E04-E02 S29-S23
16 638 472 (S16E39 L=199) 1164 236 3 ( 582/ 403- 707/ 545) -71.6 E43-E35 S21-S11
17 782 428 (S22E32 L=207) 557 115 0 ( 731/ 397- 814/ 471) 7.1 E35-E27 S24-S19
18 564 396 (S20E49 L=190) 464 150 1 ( 534/ 314- 591/ 446) 55.0 E54-E46 S25-S15
19 762 237 (S36E46 L=192) 470 81 1 ( 749/ 194- 777/ 284) 38.7 E51-E41 S39-S31
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Download FITS filament maps as tar archive
» All Filament Data of 20250918 ...
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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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