logo kso logo uni graz

20260103 - Filament data for 08 UTC
Available data for 20260103: »08 UTC   »09 UTC   »10 UTC   »11 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 1546 1712 (N43W47 L=315)   731     75        0 (1511/1690-1590/1728)  14.0 W42-W54 N41-N44
      2 1660 1688 (N42W61 L=329)   628     51        0 (1633/1667-1689/1709)  14.0 W55-W71 N39-N44
      3  936 1613 (N34E06 L=262)   699    141        1 ( 878/1561- 979/1669) -41.2 E11-E03 N30-N38
      4 1453 1133 (N04W26 L=294)   301     92        1 (1419/1102-1497/1173)  33.7 W23-W29 N01-N06
      5  688  919 (S09E20 L=248)   655    152        2 ( 662/ 851- 716/1002)  71.6 E22-E18 S13-S04
      6  944  744 (S20E05 L=263)  1058    402        0 ( 914/ 565- 978/ 910)  79.2 E06-E02 S31-S10
      7 1409  843 (S14W24 L=292)   653    119        5 (1374/ 792-1443/ 891) -56.3 W21-W26 S16-S10
      8 1352  854 (S13W20 L=288)   229     19        0 (1331/ 837-1377/ 873) -18.4 W18-W21 S14-S11
      9 1137  793 (S17W07 L=275)   420    225        1 (1051/ 723-1214/ 868)  35.0 W01-W11 S21-S12
     10  181  776 (S16E65 L=203)  2012    164        7 ( 133/ 699- 218/ 857)  56.3 E72-E59 S21-S11
     11  652  766 (S18E24 L=244)   252     86        0 ( 615/ 731- 686/ 795)  38.7 E26-E21 S20-S16
     12  910  540 (S33E08 L=260)   276     48        2 ( 891/ 516- 936/ 567) -71.6 E09-E06 S34-S31
     13  874  430 (S41E12 L=256)   288     43        0 ( 848/ 407- 899/ 453)  31.0 E14-E09 S42-S39
     14 1210  207 (S61W23 L=291)   349     42        1 (1185/ 185-1228/ 228)  45.0 W20-W26 S62-S58
     15 1022  185 (S63E00 L=268)   704    100        1 ( 969/ 165-1066/ 207) -10.3 E06-W05 S65-S60
  
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.