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20260108 - Filament data for 09 UTC
Available data for 20260108: »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  929 1442 (N21E07 L=194)   593    202        1 ( 844/1405-1021/1481) -20.0 E12-E01 N19-N23
      2  639 1387 (N17E26 L=176)   346     93        0 ( 612/1343- 666/1435) -56.3 E28-E23 N14-N20
      3 1831 1267 (N15W58 L=259)   438     40        0 (1805/1248-1853/1289)   0.0 W54-W60 N13-N16
      4 1744 1200 (N10W48 L=250)   293     49        1 (1728/1167-1758/1232) -76.0 W46-W49 N07-N11
      5  191 1182 (N05E60 L=141)   381     80        0 ( 154/1160- 225/1209)  14.0 E64-E56 N04-N06
      6  567  996 (S06E28 L=174)   292     65        0 ( 550/ 969- 586/1040)  76.0 E29-E26 S07-S03
      7  454  989 (S07E36 L=166)   589    171        1 ( 390/ 918- 502/1037) -45.0 E40-E32 S10-S03
      8  911  869 (S13E06 L=195)   438    145        1 ( 886/ 803- 951/ 919)  74.1 E07-E04 S17-S10
      9  719  567 (S33E20 L=181)  3708    851        6 ( 562/ 442- 960/ 805) -43.5 E31-E03 S41-S17
     10 1615  723 (S19W41 L=243)   765    254        0 (1508/ 637-1711/ 798)  37.6 W34-W47 S25-S14
     11 1827  728 (S17W62 L=263)   515    122        0 (1799/ 672-1853/ 786)  81.9 W59-W63 S20-S13
     12 1300  611 (S28W20 L=222)   208    102        0 (1251/ 581-1331/ 647)  51.3 W16-W21 S30-S25
     13 1702  494 (S33W59 L=261)   741     75        2 (1674/ 469-1740/ 525)  26.6 W54-W63 S34-S31
     14 1102  414 (S42W08 L=210)   584    132        1 (1031/ 398-1164/ 441)   5.2 W02-W13 S43-S40
     15  572  350 (S49E41 L=161)   710     84        1 ( 530/ 324- 628/ 377)   0.0 E46-E34 S50-S46
     16  821  154 (S68E27 L=174)   793     93        0 ( 780/ 130- 858/ 181)  16.9 E41-E18 S71-S64
  
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.