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20150606 - Filament data for 10 UTC
Available data for 20150606: »05 UTC   »06 UTC   »07 UTC   »08 UTC   »09 UTC   »10 UTC   »11 UTC   »12 UTC   »13 UTC   »14 UTC  
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  Color  xc   yc  (LatLon LCarr)  Area Length Branches (  x0/y0     x1/y1  )  Tilt Location
      1  804 1760 (N45E35 L=113)   457    106        1 ( 775/1725- 825/1798) -50.2 E37-E31 N42-N48
      2 1304 1615 (N43W11 L=159)   443    160       -1 (1277/1587-1339/1637)   0.0 W08-W14 N40-N44
      3 1249 1554 (N37W07 L=155)   306     60       -1 (1205/1528-1280/1586)  39.8 W03-W09 N34-N40
      4  449 1474 (N19E48 L=100)   681    156        2 ( 407/1429- 478/1550)  82.9 E50-E45 N15-N23
      5  566 1387 (N15E36 L=112)   275    101        0 ( 522/1370- 618/1397)  26.6 E38-E32 N13-N16
      6  760 1274 (N11E20 L=128)   900    181        3 ( 698/1211- 827/1332)  45.0 E23-E16 N06-N15
      7  854 1164 (N06E12 L=136)   312     95        1 ( 812/1130- 885/1213) -33.7 E15-E09 N03-N08
      8 1782 1090 (N15W52 L=200)   598    128        1 (1758/1029-1802/1147) -66.8 W49-W54 N11-N18
      9  160 1040 (S12E66 L= 82)   576     92        2 ( 141/1009- 173/1080)  63.4 E68-E63 S13-S09
     10  459 1002 (S10E36 L=112)   294    112        0 ( 413/ 981- 499/1032)  26.6 E39-E33 S11-S07
     11  779  912 (S10E13 L=135)  1118    254        3 ( 734/ 807- 825/1013) -71.6 E16-E09 S16-S04
     12 1271  981 (N01W15 L=164)   235     48        1 (1245/ 965-1297/1001)   0.0 W14-W17 N00-N02
     13 1471  903 (S01W30 L=178)   438    103        0 (1427/ 875-1527/ 935)  26.6 W27-W33 S02-N01
     14  305  590 (S40E51 L= 97)   636    165        3 ( 274/ 565- 340/ 613)  26.6 E55-E46 S41-S37
     15 1333  418 (S33W34 L=182)   279     56        0 (1305/ 401-1368/ 434)  45.0 W32-W36 S35-S31
     16 1437  369 (S35W45 L=193)   577    127        0 (1397/ 347-1487/ 395)   7.1 W41-W49 S36-S33
  
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.