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20150606 - Filament data for 09 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  792 1771 (N46E37 L=112)   355     69        0 ( 774/1745- 817/1795)  90.0 E38-E35 N43-N48
      2 1297 1616 (N43W10 L=159)   438     44        1 (1269/1598-1334/1638)   0.0 W07-W13 N41-N44
      3 1252 1565 (N38W07 L=156)   239     23        0 (1228/1548-1275/1584)  45.0 W05-W08 N36-N40
      4  421 1449 (N17E49 L= 99)   514     99        2 ( 382/1423- 459/1487)  45.0 E52-E46 N14-N19
      5  561 1388 (N15E36 L=113)   303    107        0 ( 512/1373- 613/1400)  15.9 E39-E32 N13-N16
      6  791 1310 (N14E19 L=130)   333     44        1 ( 757/1289- 817/1332)  45.0 E20-E17 N12-N15
      7  781 1216 (N08E18 L=131)   954    312        4 ( 695/1107- 879/1298) -28.1 E24-E09 N02-N11
      8  160 1069 (S10E67 L= 82)  1111    168        4 ( 132/1000- 187/1160)  73.3 E69-E63 S14-S04
      9 1777 1108 (N16W51 L=200)   472    114        0 (1753/1052-1796/1152) -71.6 W48-W53 N12-N18
     10  459 1008 (S09E36 L=113)   285    100        0 ( 417/ 984- 498/1034)  26.6 E39-E33 S11-S07
     11  771  915 (S10E14 L=135)  1005    213        2 ( 730/ 814- 812/1023) -69.0 E16-E10 S16-S03
     12 1260  985 (N01W15 L=164)   237     43        0 (1231/ 969-1287/1005)  18.4 W13-W16 N00-N02
     13 1458  907 (S01W29 L=178)   476    115        0 (1413/ 881-1518/ 949)  33.7 W25-W32 S02-N02
     14  299  589 (S40E52 L= 97)   623    156        1 ( 268/ 567- 338/ 616)  21.8 E56-E46 S41-S36
     15 1315  414 (S34W33 L=182)   314     71        0 (1277/ 394-1352/ 433)  53.1 W30-W35 S36-S32
     16 1429  370 (S35W44 L=193)   525    108        1 (1390/ 350-1474/ 396)   7.1 W40-W48 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.