logo kso logo uni graz

20251128 - Filament data for 08 UTC
Available data for 20251128: »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  986 1909 (N64W29 L= 52)   727     60        2 ( 951/1878-1022/1926)  -5.2 W24-W36 N60-N66
      2 1469 1774 (N39W57 L= 80)   611     64        0 (1435/1747-1500/1800)   9.5 W51-W63 N37-N40
      3  558 1424 (N33E25 L=358)  2041    412        4 ( 387/1366- 758/1496) -24.3 E41-E10 N26-N41
      4 1885 1029 (S13W62 L= 84)   717     80        4 (1851/ 999-1913/1071)  23.2 W57-W65 S14-S11
      5  778  994 (N03E15 L=  8)   615    136        0 ( 762/ 925- 795/1063)  60.3 E16-E12 N00-N07
      6 1677  855 (S20W40 L= 62)  1811    351        2 (1597/ 742-1719/ 986)  74.1 W32-W43 S25-S11
      7  676  624 (S16E29 L=354)   218     43        0 ( 660/ 594- 695/ 649)  45.0 E30-E26 S17-S14
      8  290  546 (S15E64 L=319)   480     40        0 ( 279/ 515- 307/ 573)  31.0 E67-E61 S16-S13
      9 1603  487 (S43W35 L= 58)   354     78        0 (1566/ 470-1637/ 506)   8.1 W31-W38 S44-S42
     10  542  452 (S25E45 L=337)   500     89        0 ( 513/ 414- 577/ 496)  24.0 E49-E40 S26-S22
     11  442  344 (S30E63 L=319)  1917    154        5 ( 415/ 278- 480/ 429)  23.5 E78-E54 S34-S24
     12 1087  288 (S47E13 L= 10)  1663    230        5 ( 980/ 257-1198/ 326) -12.5 E21-E03 S50-S42
     13 1194  178 (S62E09 L= 14)   493     61        1 (1158/ 165-1229/ 194)  -7.1 E12-E04 S63-S59
     14 1087  142 (S62E24 L=358)   424     43        1 (1069/ 122-1109/ 169)  29.1 E29-E20 S64-S59
     15 1010  139 (S60E32 L=350)   735     78        1 ( 966/ 123-1046/ 157)   0.0 E37-E26 S62-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.