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| 20251109 - Filament data for 06 UTC |
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Available data for 20251109: »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 1278 1823 (N45W51 L=325) 1392 154 2 (1223/1766-1333/1884) 11.8 W41-W66 N41-N47
2 1148 1773 (N45W36 L=309) 545 62 1 (1123/1737-1180/1797) 18.4 W30-W39 N43-N47
3 1499 1409 (N14W39 L=312) 1162 281 1 (1393/1346-1620/1483) -52.4 W34-W44 N07-N20
4 300 1464 (N47E51 L=222) 540 64 0 ( 269/1442- 343/1478) 0.0 E56-E44 N45-N48
5 603 1306 (N29E20 L=254) 1604 384 5 ( 422/1256- 773/1338) -27.5 E34-E09 N22-N35
6 998 1239 (N16W03 L=277) 577 273 1 ( 910/1181-1122/1299) 8.1 E02-W12 N14-N17
7 735 989 (N08E17 L=257) 1518 597 2 ( 504/ 878- 968/1053) -5.7 E33-E03 N03-N11
8 1451 963 (S10W23 L=297) 476 136 0 (1417/ 906-1487/1028) -82.9 W21-W24 S13-S05
9 426 1000 (N15E37 L=236) 285 61 1 ( 396/ 980- 459/1020) -21.8 E39-E34 N13-N16
10 1658 953 (S16W37 L=311) 303 53 0 (1639/ 926-1679/ 983) 56.3 W35-W39 S17-S14
11 261 714 (N02E59 L=215) 714 73 3 ( 232/ 678- 293/ 750) 26.6 E62-E54 N00-N03
12 651 648 (S10E31 L=243) 443 108 3 ( 610/ 595- 683/ 695) -90.0 E32-E28 S12-S06
13 595 640 (S09E35 L=239) 241 61 0 ( 568/ 613- 615/ 665) -90.0 E36-E33 S10-S07
14 1802 556 (S47W57 L=331) 616 41 1 (1774/ 539-1827/ 581) -17.1 W51-W64 S49-S44
15 571 521 (S15E41 L=233) 326 87 1 ( 552/ 484- 594/ 556) 45.0 E42-E38 S17-S13
16 1343 526 (S34W08 L=282) 412 62 1 (1314/ 501-1381/ 548) 11.3 W05-W10 S35-S31
17 364 438 (S17E65 L=209) 988 70 7 ( 327/ 411- 396/ 470) -45.0 E70-E60 S18-S14
18 780 358 (S30E35 L=239) 1125 213 3 ( 689/ 304- 839/ 433) 13.2 E44-E27 S34-S26
19 776 173 (S45E53 L=220) 1506 136 0 ( 724/ 133- 812/ 225) 14.0 E64-E44 S48-S40
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Download FITS filament maps as tar archive
» All Filament Data of 20251109 ...
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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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