logo kso logo uni graz

20140430 - Filament data for 12 UTC
Available data for 20140430: »06 UTC   »07 UTC   »08 UTC   »09 UTC   »10 UTC   »11 UTC   »12 UTC   »13 UTC   »14 UTC  
Click on image to open sensitive map!
 
  Color  xc   yc  (LatLon LCarr)  Area Length Branches (  x0/y0     x1/y1  )  Tilt Location
      1  936 1632 (N29E24 L= 30)  1087    229        3 ( 898/1554- 988/1717) -48.0 E29-E18 N24-N34
      2  994 1474 (N21E14 L= 40)   363     76        1 ( 948/1448-1033/1498)   0.0 E17-E11 N19-N22
      3  815 1360 (N09E21 L= 33)   821    182        1 ( 763/1284- 854/1455) -84.8 E22-E19 N04-N15
      4 1125 1399 (N20E04 L= 50)   225     38        1 (1099/1375-1149/1424) -26.6 E06-E02 N18-N21
      5  751 1187 (S02E20 L= 34)   365    131        0 ( 707/1154- 811/1235)  -7.1 E23-E15 S03-N00
      6  385 1139 (S13E43 L= 11)   303     95        0 ( 358/1118- 423/1166)   0.0 E45-E39 S14-S11
      7 1734 1028 (N16W45 L= 99)  2099    313        4 (1665/ 870-1767/1163) -45.0 W36-W51 N07-N22
      8  240 1020 (S23E53 L=  1)  1259    235        1 ( 171/ 950- 280/1114)  57.5 E59-E50 S28-S16
      9  554 1040 (S15E28 L= 26)   725    249        0 ( 462/1001- 675/1076)  29.7 E34-E20 S19-S11
     10  774 1010 (S11E14 L= 40)   231     76        1 ( 729/ 996- 807/1030)  21.8 E16-E11 S13-S09
     11  584  866 (S24E23 L= 31)   221     75        0 ( 549/ 849- 629/ 887)   9.5 E25-E19 S24-S23
     12 1156  789 (S14W14 L= 68)   573    162        2 (1117/ 715-1214/ 848)  83.7 W11-W16 S18-S09
     13  372  723 (S39E38 L= 16)  2221    383        4 ( 234/ 661- 519/ 823)  -4.1 E52-E24 S42-S34
     14  982  702 (S23W06 L= 60)   590    205        1 ( 877/ 677-1086/ 721)  17.1 W00-W13 S26-S21
     15 1454  463 (S24W45 L= 99)  1594    431        0 (1251/ 386-1620/ 583)  55.7 W35-W53 S34-S12
  
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.