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20260309 - Latest Filament data
Available data for 20260309: »08 UTC   »09 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 1092 1647 (N31E14 L=116)   454     77        3 (1045/1616-1132/1675)  31.0 E16-E11 N29-N33
      2  342 1623 (N13E68 L= 61)   588     60        1 ( 316/1601- 368/1651)  76.0 E70-E64 N11-N15
      3  405 1502 (N06E53 L= 77)   346     64        2 ( 378/1473- 433/1533)  33.7 E54-E50 N04-N08
      4  177 1204 (S14E65 L= 64)  2628    221        3 (  94/1152- 262/1293)  20.9 E80-E56 S17-S08
      5 1056 1178 (N02E02 L=128)   448    107        1 (1021/1122-1089/1237)  90.0 E03-W00 S01-N05
      6 1852 1138 (N23W53 L=183)   380     52        0 (1821/1121-1878/1153)  23.2 W49-W56 N21-N24
      7 1726  987 (N10W44 L=173)   816    219        3 (1695/ 895-1778/1080)  85.2 W40-W46 N04-N16
      8  855  979 (S14E08 L=121)   435    106        0 ( 818/ 940- 887/1022) -18.4 E11-E05 S15-S12
      9 1861  883 (N09W60 L=189)   640     98        0 (1824/ 849-1887/ 927)  63.4 W56-W62 N06-N12
     10 1745  850 (N04W49 L=179)   357    100        0 (1708/ 833-1780/ 877)  18.4 W45-W51 N02-N05
     11 1581  812 (S04W38 L=168)   379    105        0 (1555/ 764-1606/ 866) -80.5 W37-W39 S06-N00
     12  476  793 (S33E30 L= 99)  1389    292        3 ( 336/ 745- 623/ 833)  24.6 E43-E19 S39-S28
     13  182  728 (S43E67 L= 63)   795     85        1 ( 148/ 695- 223/ 760)  14.0 E77-E57 S45-S40
     14  904  426 (S45W12 L=141)   483    101        2 ( 852/ 404- 950/ 449)  29.7 W08-W15 S48-S43
     15  696  400 (S54E04 L=125)   417    103        0 ( 665/ 365- 743/ 442) -20.6 E07-W01 S56-S51
     16  818  390 (S51W07 L=136)   252     19        0 ( 799/ 373- 839/ 410) -33.7 W05-W08 S51-S49
  
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.