logo kso logo uni graz

20251218 - Filament data for 09 UTC
Available data for 20251218: »07 UTC   »08 UTC   »09 UTC   »10 UTC   »11 UTC   »12 UTC   »13 UTC  
Click on image to open sensitive map!
 
  Color  xc   yc  (LatLon LCarr)  Area Length Branches (  x0/y0     x1/y1  )  Tilt Location
      1 1014 1613 (N36W05 L=123)   223     74        0 ( 987/1597-1053/1637) -14.0 W03-W07 N34-N37
      2 1779 1435 (N18W60 L=179)  1473    186        1 (1706/1373-1840/1509) -52.1 W55-W65 N13-N22
      3  137 1244 (N20E69 L= 50)  1207    185        5 (  98/1172- 163/1332)  90.0 E74-E65 N15-N25
      4 1135 1212 (N09W08 L=126)  1093    296        0 (1101/1080-1177/1329)  74.1 W06-W11 N01-N15
      5  205 1198 (N16E58 L= 61)  1072    236        1 ( 165/1088- 258/1290)  63.4 E62-E52 N09-N21
      6 1831 1266 (N07W60 L=178)   460     47        0 (1802/1249-1858/1284)   8.1 W56-W63 N06-N08
      7  213 1090 (N09E56 L= 62)   370     92        2 ( 202/1045- 230/1141)  71.6 E57-E54 N06-N12
      8 1160  855 (S12W07 L=125)   228     59        1 (1140/ 817-1175/ 894)  76.0 W05-W07 S14-S10
      9 1817  762 (S23W57 L=175)   704    137        0 (1793/ 698-1846/ 832)  76.0 W55-W59 S26-S18
     10 1594  744 (S22W36 L=154)   499    169        0 (1536/ 718-1652/ 785) -12.5 W31-W40 S24-S19
     11  167  674 (S14E73 L= 46)   705     83        0 ( 150/ 636- 182/ 718)  68.2 E75-E70 S16-S11
     12 1082  531 (S32E01 L=118)  1412    489        3 ( 920/ 374-1272/ 676)  30.7 E14-W13 S42-S24
     13  277  617 (S19E60 L= 58)   575     53        2 ( 257/ 585- 302/ 645) -76.0 E62-E57 S21-S17
     14  679  335 (S42E37 L= 81)   336     66        2 ( 647/ 316- 717/ 354)  -8.1 E40-E33 S43-S40
     15  635  282 (S46E46 L= 73)   393     62        1 ( 603/ 265- 665/ 304)  11.3 E50-E40 S46-S44
  
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.