logo kso logo uni graz

20260104 - Filament data for 10 UTC
Available data for 20260104: »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 1338 1753 (N46W27 L=281)   609    102        0 (1289/1737-1398/1770)  -5.7 W22-W32 N44-N47
      2 1139 1632 (N35W08 L=262)  1099    210        1 (1051/1557-1211/1688) -39.3 W01-W12 N30-N39
      3 1439 1487 (N26W28 L=282)   267     88        0 (1402/1458-1479/1505) -31.0 W25-W30 N23-N26
      4  307 1218 (N09E48 L=206)   922    131        0 ( 265/1182- 366/1269) -29.1 E52-E43 N06-N12
      5 1679 1143 (N05W42 L=296)   287     81        0 (1649/1117-1706/1179)  45.0 W40-W44 N03-N07
      6 1569  984 (S05W34 L=288)   228     68        0 (1533/ 960-1601/1003)  31.0 W31-W36 S06-S03
      7 1583  920 (S09W36 L=290)   257     48        0 (1558/ 901-1611/ 937)  14.0 W33-W37 S09-S07
      8 1616  843 (S13W39 L=293)  1426    249        5 (1547/ 725-1675/ 933)  69.0 W35-W43 S20-S07
      9 1162  745 (S20W09 L=263)   999    349        0 (1134/ 597-1190/ 900)  87.0 W07-W10 S29-S10
     10  884  787 (S18E09 L=245)   362    116        1 ( 835/ 747- 926/ 830)  33.7 E11-E05 S19-S14
     11  302  746 (S19E52 L=202)   480     56        1 ( 280/ 713- 325/ 775)  45.0 E54-E48 S21-S17
     12  227  736 (S19E60 L=194)   534     56        0 ( 202/ 708- 251/ 771) -90.0 E62-E57 S21-S17
     13  269  585 (S29E62 L=192)  1534     98        2 ( 239/ 532- 304/ 632)  31.0 E67-E56 S32-S26
     14 1306  314 (S50W27 L=281)   472     92        0 (1267/ 288-1349/ 343) -20.0 W22-W33 S51-S47
     15 1299  198 (S61W37 L=291)   413     25        1 (1280/ 176-1315/ 225) -21.8 W32-W42 S63-S57
  
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.