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20260116 - Filament data for 10 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  753 1733 (N40E28 L= 68)   286     28        0 ( 734/1714- 777/1751)  33.7 E29-E25 N38-N41
      2 1195 1687 (N40W07 L=103)   327     47        0 (1173/1664-1223/1709)  45.0 W05-W09 N37-N41
      3  372 1486 (N21E50 L= 46)   324     98        0 ( 356/1443- 392/1536) -80.5 E51-E48 N17-N23
      4  300 1429 (N17E55 L= 41)  1855    235        5 ( 260/1311- 338/1511) -81.3 E61-E51 N09-N22
      5  490 1262 (N07E35 L= 61)   536    170        0 ( 423/1215- 565/1317)  33.7 E39-E30 N03-N10
      6  645 1181 (N02E24 L= 72)   614    105        0 ( 620/1127- 671/1237) -68.2 E25-E22 N00-N05
      7 1779 1127 (N08W50 L=146)  1090    247        1 (1666/1100-1868/1179)  16.7 W40-W60 N05-N12
      8  157 1071 (S05E64 L= 32)   530     91        1 ( 144/1026- 175/1119)  90.0 E65-E61 S07-S02
      9  369  977 (S11E42 L= 53)  1329    219        5 ( 318/ 886- 406/1082) -74.7 E46-E39 S15-S04
     10  461 1051 (S06E36 L= 60)   494     78        2 ( 429/1015- 504/1082)  21.8 E37-E32 S08-S04
     11  258  981 (S10E52 L= 43)   305     37        0 ( 242/ 957- 271/1010)  56.3 E53-E51 S11-S08
     12  268  938 (S13E52 L= 44)   949    183        1 ( 190/ 909- 315/1001)  17.1 E60-E47 S14-S09
     13  504  928 (S13E32 L= 64)   306    115        0 ( 491/ 866- 516/ 986) -74.1 E33-E31 S16-S09
     14 1919  957 (N00W67 L=163)   699     79        1 (1885/ 927-1951/ 979)  20.6 W62-W73 S02-N01
     15 1046  807 (S17W03 L= 99)   251     94        0 ( 995/ 793-1092/ 825)  11.3 W00-W05 S18-S16
     16 1883  743 (S13W69 L=165)   545     46        1 (1861/ 720-1901/ 770)  45.0 W66-W72 S14-S10
     17 1432  675 (S22W30 L=125)   261     84        0 (1397/ 650-1469/ 703)  45.0 W27-W31 S24-S20
     18  889  440 (S42E06 L= 90)   234     57        0 ( 865/ 420- 922/ 452)  26.6 E07-E02 S44-S41
  
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.