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| 20241112 - Filament data for 10 UTC |
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Available data for 20241112: »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 1536 1728 (N30W62 L= 72) 983 115 1 (1496/1682-1582/1762) 0.0 W55-W71 N27-N31
2 1792 1247 (S03W56 L= 65) 491 57 1 (1764/1222-1821/1275) 21.8 W52-W58 S04-S01
3 1905 1186 (S09W67 L= 77) 537 47 4 (1890/1161-1924/1210) 18.4 W64-W70 S10-S07
4 206 1146 (N27E57 L=313) 399 53 0 ( 178/1126- 238/1166) 8.1 E60-E52 N26-N28
5 1313 1018 (S04W16 L= 26) 1972 572 5 (1124/ 837-1448/1151) -53.6 W06-W20 S16-N05
6 1810 1124 (S10W54 L= 64) 379 50 0 (1788/1099-1841/1142) -9.5 W51-W57 S11-S08
7 1587 1083 (S07W35 L= 44) 609 143 1 (1545/1015-1620/1135) -82.9 W32-W36 S10-S02
8 413 1114 (N21E36 L=333) 257 62 0 ( 380/1093- 444/1132) -36.9 E38-E33 N19-N22
9 1669 1011 (S13W39 L= 49) 930 290 3 (1593/ 935-1726/1094) 21.0 W32-W45 S15-S09
10 752 1036 (N10E15 L=355) 629 166 1 ( 662/1008- 824/1062) -29.1 E20-E11 N07-N12
11 1680 821 (S24W37 L= 47) 524 105 0 (1660/ 778-1706/ 881) -90.0 W35-W39 S26-S20
12 1772 791 (S29W46 L= 56) 905 148 0 (1706/ 769-1841/ 824) -4.1 W39-W53 S30-S27
13 1549 735 (S26W26 L= 36) 451 111 1 (1534/ 681-1565/ 800) -90.0 W24-W26 S29-S21
14 905 716 (S11E14 L=356) 646 150 3 ( 857/ 685- 968/ 754) -45.0 E16-E10 S13-S08
15 764 475 (S23E30 L=340) 3410 815 6 ( 513/ 247-1006/ 689) 16.9 E65-E09 S33-S14
16 1556 555 (S38W25 L= 35) 2735 272 7 (1475/ 447-1638/ 662) 52.4 W18-W32 S46-S32
17 477 582 (S10E45 L=325) 421 150 0 ( 409/ 563- 535/ 619) -5.2 E51-E39 S10-S08
18 1415 478 (S39W12 L= 22) 294 54 1 (1387/ 456-1439/ 501) 26.6 W10-W14 S40-S37
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Download FITS filament maps as tar archive
» All Filament Data of 20241112 ...
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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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