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| 20241123 - Filament data for 07 UTC |
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Available data for 20241123: »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 1766 1461 (N12W63 L=289) 1462 119 2 (1702/1417-1813/1495) -26.6 W57-W68 N08-N14
2 690 1358 (N28E14 L=212) 405 116 0 ( 638/1314- 738/1396) -49.4 E17-E11 N24-N31
3 1630 1292 (N05W43 L=270) 709 163 1 (1555/1248-1694/1328) 4.4 W36-W49 N03-N06
4 397 1234 (N26E37 L=189) 418 102 0 ( 343/1211- 439/1269) 0.0 E42-E33 N24-N27
5 1133 1233 (N11W10 L=237) 332 84 0 (1094/1209-1181/1261) -45.0 W08-W12 N09-N13
6 1329 1168 (N04W20 L=247) 349 88 0 (1288/1133-1364/1204) -59.0 W18-W21 N01-N06
7 402 1114 (N18E38 L=189) 1505 481 1 ( 240/1059- 612/1168) -20.8 E52-E23 N12-N24
8 798 872 (S03E16 L=211) 366 177 0 ( 724/ 844- 874/ 889) -12.5 E20-E11 S04-S01
9 767 740 (S10E21 L=206) 567 189 0 ( 721/ 684- 841/ 817) -71.6 E22-E17 S13-S04
10 893 735 (S12E13 L=213) 237 103 0 ( 842/ 717- 931/ 768) 0.0 E16-E10 S12-S10
11 313 553 (S12E61 L=165) 6911 378 10 ( 229/ 433- 408/ 713) -86.8 E73-E51 S21-S03
12 482 658 (S09E41 L=185) 507 82 2 ( 444/ 629- 517/ 698) -21.8 E44-E39 S11-S06
13 1148 650 (S22E00 L=226) 258 95 0 (1125/ 607-1171/ 696) 51.3 E02-W02 S24-S19
14 1459 548 (S36W19 L=246) 1825 540 3 (1246/ 401-1662/ 695) 17.0 W01-W37 S41-S30
15 632 529 (S19E36 L=191) 380 62 1 ( 603/ 493- 672/ 561) -45.0 E36-E32 S21-S17
16 1714 521 (S45W46 L=273) 522 82 0 (1675/ 490-1755/ 555) 18.4 W41-W51 S46-S43
17 466 505 (S18E49 L=177) 334 71 2 ( 450/ 474- 484/ 543) 38.7 E51-E46 S19-S15
18 857 322 (S38E30 L=196) 999 165 0 ( 787/ 266- 911/ 396) 23.6 E38-E22 S41-S33
19 1021 255 (S47E22 L=204) 469 66 1 ( 988/ 234-1060/ 274) 0.0 E25-E18 S48-S45
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Download FITS filament maps as tar archive
» All Filament Data of 20241123 ...
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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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