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20261017 - Filament data for 09 UTC
Available data for 20261017: »08 UTC   »09 UTC   »10 UTC   »11 UTC   »13 UTC  
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  Color  xc   yc  (LatLon LCarr)  Area Length Branches (  x0/y0     x1/y1  )  Tilt Location
      1  637 1449 (N40E13 L= 65)   246     57        0 ( 613/1431- 672/1470) -31.0 E15-E10 N38-N42
      2 1227 1285 (N14W18 L= 97)   621    158        2 (1146/1243-1285/1317) -58.0 W14-W21 N10-N18
      3 1461 1226 (N05W30 L=108)   857    248        1 (1410/1099-1495/1312)  76.0 W27-W32 S02-N10
      4 1365 1267 (N10W26 L=104)   274     55        0 (1336/1247-1391/1288) -71.6 W23-W27 N08-N11
      5  380 1250 (N34E38 L= 40)   305     75        2 ( 347/1223- 412/1271) -26.6 E41-E35 N32-N36
      6 1819 1180 (S09W56 L=134)   342     95        0 (1802/1130-1831/1228)  33.7 W52-W58 S10-S06
      7 1738  951 (S18W43 L=121)   461    135        1 (1702/ 897-1780/1018)  24.0 W38-W47 S20-S15
      8  810  922 (N05E14 L= 64)   223     59        2 ( 781/ 903- 838/ 946) -14.0 E16-E12 N04-N06
      9 1796  836 (S27W47 L=125)   514    153        0 (1753/ 768-1832/ 900)  33.7 W41-W51 S30-S24
     10  211  819 (N12E61 L= 17)   452     53        1 ( 182/ 801- 246/ 833)  -7.1 E65-E57 N11-N13
  
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.