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| 20251105 - Filament data for 13 UTC |
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Available data for 20251105: »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
1 985 1931 (N65W50 L= 13) 709 79 1 ( 963/1899-1012/1963) 8.4 W39-W66 N61-N67
2 898 1862 (N62W27 L=350) 816 112 2 ( 854/1818- 944/1891) -16.7 W21-W33 N57-N65
3 1208 1749 (N41W38 L= 1) 2413 464 2 (1015/1704-1417/1792) -20.1 W21-W52 N33-N46
4 815 1605 (N44W02 L=325) 368 98 0 ( 792/1555- 842/1638) 45.0 W00-W05 N40-N45
5 1764 1499 (N11W66 L= 29) 686 103 0 (1733/1452-1790/1540) 80.5 W64-W68 N07-N13
6 1592 1118 (S05W36 L=358) 2155 482 2 (1536/ 889-1624/1323) 58.2 W26-W42 S16-N06
7 307 1141 (N26E46 L=277) 947 196 2 ( 234/1071- 360/1193) -56.3 E53-E40 N21-N30
8 1894 1167 (S10W65 L= 28) 440 68 0 (1868/1140-1919/1187) -33.7 W61-W68 S12-S08
9 142 1112 (N28E66 L=257) 1820 165 1 ( 88/1054- 198/1169) -20.0 E80-E57 N23-N31
10 779 1088 (N13E12 L=311) 647 198 2 ( 703/1047- 868/1150) -55.0 E15-E07 N08-N18
11 270 1104 (N25E49 L=273) 700 79 2 ( 241/1057- 300/1146) -63.4 E52-E46 N21-N27
12 375 1028 (N18E41 L=282) 1013 230 1 ( 276/ 958- 416/1109) 23.2 E50-E36 N14-N22
13 356 867 (N09E45 L=277) 271 56 0 ( 336/ 833- 373/ 890) -76.0 E46-E43 N07-N11
14 260 739 (N04E58 L=265) 758 152 0 ( 210/ 680- 302/ 773) -50.2 E62-E54 N00-N06
15 1289 619 (S26W06 L=329) 492 177 0 (1232/ 558-1360/ 680) 21.8 W01-W11 S28-S23
16 1761 575 (S44W47 L= 10) 1121 171 1 (1688/ 529-1827/ 628) 6.3 W37-W55 S45-S40
17 367 536 (S10E57 L=266) 344 41 0 ( 345/ 521- 394/ 558) -14.0 E58-E54 S10-S08
18 1397 382 (S46W08 L=331) 345 45 1 (1371/ 361-1421/ 405) 0.0 W05-W10 S47-S43
19 748 262 (S36E44 L=278) 934 123 1 ( 694/ 219- 795/ 319) 14.0 E52-E36 S37-S32
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Download FITS filament maps as tar archive
» All Filament Data of 20251105 ...
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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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