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20251227 - Filament data for 09 UTC
Available data for 20251227: »07 UTC   »08 UTC   »09 UTC   »10 UTC   »11 UTC   »12 UTC   »13 UTC  
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  Color  xc   yc  (LatLon LCarr)  Area Length Branches (  x0/y0     x1/y1  )  Tilt Location
      1  843 1549 (N31E10 L=349)   328     48        1 ( 825/1521- 865/1582) -53.1 E11-E08 N29-N33
      2  930 1555 (N31E04 L=355)   439    106        0 ( 873/1536- 985/1571)   0.0 E08-W00 N29-N32
      3 1121 1519 (N28W08 L=  8)   509    137        1 (1060/1497-1200/1539)   0.0 W04-W13 N26-N29
      4  175 1389 (N24E69 L=290)   764     60        3 ( 155/1354- 197/1418) -45.0 E74-E65 N22-N26
      5 1675 1394 (N18W47 L= 46)   276     76        0 (1634/1382-1703/1413)   0.0 W43-W49 N17-N19
      6  198 1321 (N20E62 L=298)  1360    118        3 ( 160/1259- 239/1365)  45.0 E67-E57 N15-N22
      7 1131 1198 (N07W07 L=  7)   789    230        4 (1049/1125-1205/1263)  24.0 W01-W11 N03-N11
      8  210 1169 (N10E57 L=303)   421     50        2 ( 186/1140- 237/1198) -56.3 E60-E54 N08-N11
      9  118 1038 (N03E69 L=291)   577     83        1 (  95/1004- 148/1079)  26.6 E73-E64 N01-N05
     10  848  935 (S07E11 L=349)   184     91        0 ( 823/ 909- 884/ 961)  36.9 E12-E08 S08-S05
     11 1715  922 (S10W46 L= 45)   308     71        3 (1678/ 897-1748/ 941)   9.5 W42-W48 S11-S08
     12  210  843 (S09E59 L=301)   431     42        0 ( 184/ 820- 230/ 868)  71.6 E62-E56 S10-S07
     13  246  809 (S12E56 L=304)   466     88        1 ( 225/ 779- 282/ 860)  59.0 E58-E52 S13-S08
     14 1505  800 (S17W30 L= 30)   234     99        0 (1453/ 781-1548/ 826)  23.2 W26-W33 S18-S15
     15  200  702 (S17E65 L=294)  4182    321       13 ( 129/ 575- 263/ 815) -68.2 E73-E59 S25-S10
  
Data will be available after one hour of observations. 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.