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| 20251024 - Latest Filament data |
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Available data for 20251024: »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
1 925 1724 (N50W19 L=140) 374 65 1 ( 903/1690- 944/1760) 26.6 W14-W22 N47-N52
2 1308 1721 (N36W45 L=166) 606 122 1 (1250/1687-1371/1745) -9.5 W39-W51 N34-N37
3 1268 1606 (N31W34 L=155) 305 50 0 (1235/1590-1299/1621) -21.8 W31-W36 N29-N31
4 252 1348 (N43E54 L= 67) 432 72 1 ( 225/1312- 281/1380) 38.7 E57-E49 N40-N44
5 824 1364 (N29E03 L=118) 282 58 1 ( 787/1343- 856/1380) -45.0 E04-W00 N27-N30
6 1750 1280 (S01W53 L=174) 1094 171 2 (1697/1245-1838/1320) -13.0 W47-W62 S04-N02
7 340 1098 (N25E43 L= 78) 2410 505 3 ( 197/1002- 541/1269) -36.6 E59-E28 N15-N38
8 1824 960 (S21W51 L=172) 609 138 0 (1797/ 899-1839/1035) 54.5 W47-W53 S23-S16
9 1924 947 (S25W65 L=186) 757 81 1 (1896/ 927-1955/ 973) -4.8 W60-W72 S26-S23
10 1594 894 (S17W30 L=151) 222 51 2 (1562/ 877-1620/ 914) -11.3 W27-W32 S18-S16
11 261 813 (N10E56 L= 65) 1028 121 3 ( 217/ 753- 309/ 849) -32.0 E60-E50 N07-N13
12 1296 750 (S17W08 L=129) 708 307 0 (1194/ 655-1409/ 842) 16.4 W00-W17 S20-S14
13 915 793 (S05E12 L=109) 1285 269 3 ( 808/ 745-1048/ 823) -33.7 E17-E05 S10-S01
14 1606 654 (S32W28 L=149) 1398 336 0 (1518/ 565-1724/ 795) 21.8 W19-W39 S36-S27
15 304 734 (N05E54 L= 67) 1160 151 3 ( 249/ 690- 363/ 785) 0.0 E61-E49 N02-N07
16 258 654 (N01E62 L= 59) 411 43 0 ( 243/ 630- 273/ 684) 33.7 E64-E59 N00-N02
17 488 595 (S06E44 L= 77) 375 57 0 ( 459/ 577- 522/ 613) 0.0 E46-E40 S07-S05
18 1285 486 (S33W01 L=122) 247 55 0 (1268/ 456-1300/ 518) 56.3 W00-W02 S35-S31
19 853 176 (S44E47 L= 74) 988 144 1 ( 803/ 143- 921/ 222) 3.6 E54-E36 S46-S41
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Download FITS filament maps as tar archive
» All Filament Data of 20251024 ...
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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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