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20260116 - Filament data for 09 UTC
Available data for 20260116: »08 UTC   »09 UTC   »10 UTC   »11 UTC   »12 UTC   »13 UTC   »14 UTC  
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  Color  xc   yc  (LatLon LCarr)  Area Length Branches (  x0/y0     x1/y1  )  Tilt Location
      1  746 1733 (N40E28 L= 68)   288     14        0 ( 728/1714- 767/1752)  71.6 E30-E26 N38-N41
      2 1189 1686 (N39W07 L=103)   337     44        1 (1170/1659-1219/1707)  36.9 W05-W09 N37-N41
      3  367 1486 (N21E51 L= 46)   307     90        0 ( 353/1441- 385/1535) -71.6 E52-E49 N17-N23
      4  297 1431 (N17E56 L= 41)  2046    241        7 ( 256/1309- 333/1521) -74.1 E62-E51 N09-N23
      5  467 1250 (N06E37 L= 60)   432    135        1 ( 417/1213- 527/1294)  26.6 E40-E32 N03-N08
      6  638 1188 (N03E24 L= 72)   645    117        2 ( 613/1132- 673/1240) -51.3 E26-E21 N00-N05
      7 1779 1127 (N08W50 L=147)  1057    216        0 (1680/1100-1862/1178)  18.4 W41-W59 N05-N12
      8  152 1069 (S05E65 L= 32)   528    106        3 ( 139/1010- 170/1115) -80.5 E66-E62 S08-S02
      9  451 1050 (S06E36 L= 60)   521     87        1 ( 413/1014- 494/1083)  26.6 E39-E33 S08-S03
     10  328  958 (S12E46 L= 50)  2572    411        6 ( 194/ 872- 408/1082) -17.5 E59-E39 S16-S04
     11  497  925 (S13E33 L= 64)   355    121        0 ( 483/ 860- 509/ 987) -82.9 E33-E31 S17-S09
     12 1913  957 (S00W67 L=163)   801     76        1 (1878/ 930-1947/ 980)  18.4 W62-W72 S02-N01
     13 1032  805 (S18W02 L= 98)   248     99        0 ( 988/ 789-1079/ 824)  14.0 W00-W04 S18-S16
     14 1882  743 (S13W69 L=165)   702     65        2 (1856/ 709-1901/ 772) -63.4 W65-W73 S14-S10
     15 1417  670 (S23W29 L=125)   279     75        1 (1385/ 639-1454/ 697)  45.0 W26-W30 S24-S20
  
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.