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| 20251024 - Filament data for 10 UTC |
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Available data for 20251024: »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
1 925 1738 (N51W20 L=142) 599 111 1 ( 892/1685- 960/1782) 28.6 W13-W24 N47-N54
2 1296 1713 (N36W43 L=166) 577 131 1 (1237/1676-1363/1738) -15.3 W37-W49 N34-N37
3 1248 1596 (N31W32 L=155) 303 44 1 (1218/1575-1279/1613) -26.6 W30-W34 N29-N32
4 242 1349 (N43E55 L= 67) 433 84 1 ( 214/1313- 272/1389) 33.7 E59-E51 N41-N45
5 800 1354 (N29E05 L=118) 272 58 0 ( 761/1335- 833/1370) -36.9 E06-E02 N27-N30
6 1728 1274 (S01W51 L=173) 960 155 2 (1681/1228-1792/1318) -54.5 W46-W55 S05-N02
7 342 1075 (N24E43 L= 80) 2376 423 3 ( 186/ 986- 518/1210) -32.3 E60-E30 N14-N34
8 1806 942 (S21W49 L=172) 632 135 0 (1779/ 880-1825/1007) 54.5 W45-W51 S24-S17
9 1915 939 (S26W64 L=186) 673 43 1 (1886/ 921-1948/ 956) -5.2 W58-W70 S26-S23
10 1566 881 (S17W28 L=151) 227 63 1 (1529/ 868-1596/ 899) -11.3 W25-W30 S18-S16
11 243 811 (N11E58 L= 65) 1127 124 4 ( 197/ 751- 292/ 849) -29.1 E62-E52 N07-N13
12 1264 730 (S17W06 L=129) 727 316 0 (1162/ 642-1388/ 830) 14.0 E01-W15 S20-S14
13 903 766 (S06E13 L=110) 1205 308 1 ( 834/ 662-1026/ 810) 4.4 E19-E06 S10-S03
14 1602 662 (S32W27 L=150) 1581 381 0 (1500/ 556-1737/ 810) 21.4 W17-W40 S36-S26
15 289 731 (N05E56 L= 67) 1230 132 4 ( 238/ 684- 350/ 782) 0.0 E62-E50 N02-N08
16 471 589 (S06E46 L= 77) 423 51 2 ( 443/ 562- 502/ 610) 9.5 E48-E42 S07-S05
17 589 507 (S14E41 L= 82) 846 179 1 ( 532/ 441- 638/ 591) 32.5 E48-E35 S16-S09
18 943 234 (S41E34 L= 89) 304 52 1 ( 923/ 210- 959/ 271) 26.6 E37-E29 S43-S38
19 833 163 (S44E50 L= 72) 666 78 0 ( 799/ 143- 866/ 191) 10.3 E55-E44 S45-S42
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Download FITS filament maps as tar archive
» All Filament Data of 20251024 ...
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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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