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| 20251106 - Filament data for 12 UTC |
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Available data for 20251106: »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 1023 1944 (N64W57 L= 7) 710 63 1 (1011/1910-1039/1979) 10.0 W46-W80 N60-N66
2 956 1898 (N63W38 L=348) 547 48 2 ( 927/1870- 980/1924) 0.0 W33-W46 N59-N65
3 1305 1808 (N42W52 L= 2) 2028 348 1 (1154/1763-1462/1851) -16.5 W35-W63 N35-N47
4 960 1659 (N43W15 L=325) 445 76 0 ( 936/1617- 988/1694) 33.7 W11-W18 N40-N44
5 771 1595 (N44E01 L=309) 365 93 0 ( 725/1568- 818/1619) 0.0 E05-W02 N42-N45
6 1737 1205 (S04W49 L=359) 2983 519 3 (1675/ 959-1776/1428) 56.3 W39-W56 S16-N08
7 672 1250 (N24E16 L=294) 278 80 0 ( 633/1224- 701/1271) -36.9 E18-E13 N22-N25
8 976 1177 (N13W01 L=311) 723 271 0 ( 875/1134-1074/1257) -54.0 E03-W05 N09-N20
9 374 1174 (N27E39 L=271) 686 161 2 ( 345/1114- 415/1240) -90.0 E41-E35 N22-N30
10 252 1131 (N26E51 L=259) 1270 261 0 ( 145/1058- 352/1193) -26.6 E66-E42 N20-N32
11 477 1030 (N16E33 L=277) 358 156 0 ( 408/ 996- 544/1051) 0.0 E38-E27 N14-N17
12 231 836 (N10E58 L=252) 828 122 1 ( 186/ 795- 272/ 882) 14.0 E64-E52 N07-N11
13 389 794 (N04E45 L=266) 551 138 0 ( 328/ 761- 436/ 817) -35.5 E49-E40 N01-N06
14 1480 709 (S25W20 L=330) 673 235 2 (1402/ 628-1583/ 801) 21.8 W13-W28 S28-S21
15 884 734 (S09E15 L=296) 326 82 0 ( 863/ 690- 905/ 775) 80.5 E15-E13 S12-S06
16 324 565 (S08E59 L=251) 387 61 0 ( 311/ 531- 342/ 601) 63.4 E61-E57 S09-S05
17 351 436 (S16E66 L=244) 4920 424 7 ( 266/ 252- 477/ 567) 61.6 E78-E61 S30-S06
18 1504 417 (S47W19 L=329) 669 106 2 (1445/ 394-1548/ 453) -5.7 W13-W23 S49-S44
19 893 326 (S35E29 L=281) 939 173 0 ( 824/ 266- 956/ 384) 14.9 E37-E22 S37-S31
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Download FITS filament maps as tar archive
» All Filament Data of 20251106 ...
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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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