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20260102 - Filament data for 08 UTC
Available data for 20260102: »08 UTC   »09 UTC   »11 UTC   »12 UTC  
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  Color  xc   yc  (LatLon LCarr)  Area Length Branches (  x0/y0     x1/y1  )  Tilt Location
      1  852 1783 (N49E15 L=266)   473     54        2 ( 818/1759- 879/1806)  21.8 E17-E12 N46-N50
      2 1529 1710 (N42W45 L=327)  2405    331        8 (1370/1678-1673/1744)  -3.3 W28-W65 N40-N45
      3  739 1648 (N37E21 L=260)   949    179        1 ( 696/1564- 787/1713) -50.2 E26-E16 N30-N42
      4 1056 1432 (N22W02 L=283)   641    295        2 ( 997/1306-1144/1538) -65.0 E01-W07 N13-N28
      5 1103  961 (S07W05 L=286)   385    147        0 (1066/ 900-1155/1001)  56.3 W02-W07 S10-S04
      6 1163  894 (S11W08 L=289)   626    185        3 (1119/ 829-1219/ 949)  54.5 W05-W11 S14-S07
      7  486  885 (S11E34 L=247)   439     58        2 ( 465/ 848- 513/ 917)  53.1 E35-E32 S12-S08
      8  729  789 (S17E19 L=262)   788    233        1 ( 706/ 689- 756/ 892)  85.6 E20-E16 S23-S10
      9  885  829 (S15E09 L=273)   284    101        2 ( 846/ 802- 926/ 859) -26.6 E10-E06 S16-S12
     10  842  767 (S18E12 L=270)   412    201        0 ( 798/ 721- 912/ 830) -33.7 E14-E07 S21-S14
     11 1373  801 (S16W22 L=303)   254     71        0 (1348/ 781-1393/ 827)  56.3 W20-W23 S17-S14
     12 1859  727 (S20W66 L=347)   421     60        1 (1835/ 703-1879/ 751)  71.6 W63-W69 S21-S18
     13  273  626 (S26E59 L=222)  1623    223        7 ( 233/ 559- 327/ 717)  63.4 E65-E53 S29-S19
     14 1857  650 (S24W70 L=351)   770     85        0 (1820/ 639-1903/ 664)   3.6 W63-W81 S24-S23
     15  647  496 (S36E29 L=252)   838    231        2 ( 583/ 428- 722/ 591) -61.4 E32-E24 S40-S28
     16  921  189 (S62E14 L=267)   550     52        1 ( 892/ 168- 950/ 216) -51.3 E18-E10 S64-S59
  
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.