logo kso logo uni graz

20150611 - Filament data for 08 UTC
Available data for 20150611: »06 UTC   »07 UTC   »08 UTC   »09 UTC   »10 UTC   »11 UTC   »12 UTC   »13 UTC   »14 UTC   »15 UTC  
Click on image to open sensitive map!
 
  Color  xc   yc  (LatLon LCarr)  Area Length Branches (  x0/y0     x1/y1  )  Tilt Location
      1 1053 1567 (N36E06 L= 77)  1107    275        2 ( 995/1457-1085/1655) -52.4 E12-E02 N28-N41
      2  694 1544 (N29E31 L= 52)   761    239        2 ( 644/1470- 767/1620) -31.0 E38-E23 N24-N33
      3  395 1435 (N17E51 L= 32)  2637    511        6 ( 354/1267- 445/1572) -43.5 E60-E41 N07-N25
      4 1661 1470 (N38W44 L=127)   355     35        1 (1643/1451-1680/1492) -56.3 W41-W45 N36-N39
      5  877 1381 (N20E14 L= 69)   216     74        0 ( 829/1366- 913/1396)  21.8 E17-E12 N19-N21
      6 1694 1256 (N23W44 L=127)  1050    251        1 (1625/1133-1760/1359) -49.8 W38-W50 N16-N29
      7 1100 1246 (N15W02 L= 85)   361    168        0 (1029/1221-1158/1303)  33.7 E02-W05 N12-N19
      8 1346 1244 (N18W18 L=101)   226     69        0 (1331/1211-1370/1283) -53.1 W16-W19 N16-N20
      9  893 1223 (N11E11 L= 73)   211     56        0 ( 864/1197- 922/1254) -36.9 E12-E08 N09-N12
     10  676 1166 (N05E23 L= 60)   258    102        0 ( 626/1152- 733/1178)  15.9 E26-E19 N03-N05
     11 1624 1094 (N12W39 L=122)   253     59        1 (1607/1066-1643/1126)  76.0 W37-W40 N10-N14
     12  190 1009 (S11E62 L= 21)  1243    478        2 (  99/ 982- 277/1032)   4.4 E77-E51 S13-S08
     13  736  945 (S08E17 L= 66)   229    106        2 ( 709/ 893- 778/ 998)  66.8 E18-E14 S11-S04
     14 1690  658 (S13W53 L=136)   434     82        1 (1652/ 635-1715/ 674)   0.0 W48-W55 S14-S12
     15 1076  431 (S37W13 L= 96)   363     54        2 (1043/ 413-1108/ 452)  36.9 W11-W15 S38-S35
  
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.