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20251129 - Filament data for 12 UTC
Available data for 20251129: »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 1014 1926 (N65W34 L= 42)   750     86        0 ( 993/1881-1045/1960)  21.4 W26-W49 N59-N69
      2  900 1877 (N63W14 L= 21)   475     72        1 ( 870/1849- 936/1901)  15.3 W09-W20 N60-N65
      3 1333 1725 (N38W40 L= 47)   524     94        0 (1280/1708-1386/1739)  -6.3 W35-W44 N36-N40
      4  799 1480 (N32E07 L=  0)  2432    564        4 ( 538/1426-1053/1554) -24.6 E26-W09 N24-N41
      5 1044 1070 (N03W02 L=  9)   650    153        0 (1020/ 998-1065/1145)  66.8 W00-W03 N00-N07
      6 1826  889 (S20W54 L= 61)  3027    378        3 (1739/ 791-1889/1043)  71.6 W45-W61 S25-S10
      7 1404  943 (S10W21 L= 28)   217     47        2 (1384/ 914-1421/ 970) -76.0 W19-W22 S11-S07
      8 1389  854 (S15W19 L= 26)   211     88        0 (1350/ 829-1416/ 890)  21.8 W16-W21 S15-S12
      9  912  702 (S16E12 L=355)   298    129        0 ( 875/ 644- 952/ 755)  35.5 E15-E08 S18-S13
     10 1152  650 (S23W01 L=  9)   367     97        0 (1099/ 622-1189/ 674)  11.3 E02-W04 S24-S21
     11  257  555 (S14E67 L=300)  3617    210        5 ( 182/ 478- 306/ 641)  63.4 E80-E56 S19-S09
     12  625  437 (S27E39 L=328)  1886    330        4 ( 548/ 310- 750/ 550)  24.0 E53-E26 S34-S22
     13 1229  333 (S47W01 L=  8)  1488    251        5 (1119/ 298-1338/ 374) -22.4 E07-W10 S50-S41
     14  971  289 (S45E21 L=346)   318     61        0 ( 945/ 269-1005/ 303)   8.1 E24-E17 S45-S43
     15 1122  163 (S61E17 L=350)  1482    155        4 (1045/ 145-1207/ 184) -19.4 E25-E07 S65-S56
  
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.