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| 20241125 - Filament data for 11 UTC |
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Available data for 20241125: »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 1089 1485 (N27W14 L=211) 486 143 1 (1023/1438-1147/1518) -49.4 W09-W16 N23-N30
2 1560 1373 (N11W40 L=238) 762 157 0 (1495/1323-1631/1404) -41.2 W36-W44 N07-N14
3 779 1360 (N26E09 L=189) 344 117 0 ( 721/1330- 822/1402) 15.9 E12-E05 N24-N27
4 838 1219 (N16E07 L=191) 513 268 0 ( 726/1177- 934/1278) -4.4 E13-W00 N14-N18
5 193 1070 (N19E58 L=140) 2748 271 12 ( 109/ 995- 284/1154) -23.5 E71-E48 N14-N24
6 1876 1092 (S11W61 L=259) 1741 131 5 (1834/1041-1919/1151) 50.2 W55-W67 S13-S07
7 1282 1029 (S03W15 L=213) 295 99 0 (1225/1005-1325/1044) -26.6 W11-W17 S04-S01
8 1330 874 (S13W15 L=213) 369 186 0 (1246/ 843-1390/ 931) 5.7 W09-W19 S13-S10
9 1197 888 (S09W07 L=205) 349 81 0 (1169/ 853-1232/ 922) -68.2 W05-W08 S11-S06
10 390 590 (S12E51 L=147) 2635 455 7 ( 331/ 447- 433/ 838) 47.7 E65-E44 S20-N02
11 1549 762 (S24W28 L=226) 339 94 0 (1523/ 721-1574/ 813) 45.0 W25-W30 S25-S20
12 1758 651 (S36W48 L=246) 2196 439 1 (1588/ 529-1917/ 785) 13.7 W31-W69 S40-S30
13 647 658 (S13E30 L=168) 896 247 1 ( 567/ 601- 734/ 752) 17.1 E35-E22 S15-S08
14 188 640 (S06E72 L=126) 1277 131 0 ( 158/ 577- 217/ 691) -82.9 E75-E69 S10-S02
15 813 641 (S17E20 L=178) 210 66 0 ( 801/ 599- 827/ 673) 59.0 E21-E18 S19-S14
16 612 530 (S20E37 L=161) 597 140 3 ( 577/ 479- 643/ 592) 36.9 E40-E32 S22-S16
17 1490 460 (S43W23 L=220) 551 108 1 (1434/ 438-1535/ 500) 0.0 W17-W26 S44-S40
18 543 411 (S26E48 L=150) 952 174 0 ( 465/ 384- 639/ 448) -7.6 E55-E38 S27-S24
19 936 365 (S37E22 L=176) 245 26 0 ( 919/ 345- 955/ 390) -90.0 E23-E20 S38-S34
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Download FITS filament maps as tar archive
» All Filament Data of 20241125 ...
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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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