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20140610 - Filament data for 10 UTC
Available data for 20140610: »05 UTC   »06 UTC   »07 UTC   »08 UTC   »09 UTC   »10 UTC   »11 UTC   »12 UTC   »13 UTC  
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  Color  xc   yc  (LatLon LCarr)  Area Length Branches (  x0/y0     x1/y1  )  Tilt Location
      1  307 1475 (N18E62 L=171)   612    138        0 ( 292/1418- 319/1524) -60.3 E64-E58 N14-N21
      2  430 1475 (N20E49 L=183)   760    169        2 ( 400/1433- 474/1524) -24.0 E53-E44 N17-N23
      3  956 1414 (N24E10 L=223)   429    168        1 ( 933/1350- 985/1497) -78.7 E11-E08 N19-N29
      4  582 1335 (N13E33 L=200)   288    113        0 ( 546/1298- 615/1363) -23.2 E36-E29 N11-N15
      5  932 1230 (N12E08 L=224)   368     80        0 ( 901/1194- 960/1268) -36.9 E10-E06 N09-N13
      6  315 1187 (N01E51 L=182)   384     67        2 ( 295/1159- 335/1221) -26.6 E53-E48 N00-N02
      7 1677 1137 (N16W43 L=276)   728    178        1 (1643/1085-1705/1205) -49.4 W39-W45 N12-N19
      8 1448 1141 (N13W25 L=258)   405    194        1 (1359/1121-1524/1164)   5.2 W19-W30 N11-N15
      9 1562  922 (N01W36 L=269)  1617    357        3 (1509/ 792-1632/1064) -68.2 W32-W43 S05-N10
     10  122  916 (S18E71 L=162)  1114    139        0 ( 106/ 884- 136/ 946) -63.4 E73-E68 S20-S16
     11 1347  818 (S08W23 L=256)   251     81        0 (1315/ 794-1384/ 836) -11.3 W20-W25 S09-S06
     12 1274  707 (S16W20 L=253)   951    316        3 (1161/ 665-1402/ 755)  18.4 W13-W28 S19-S12
     13 1647  732 (S09W46 L=279)   451     80        2 (1613/ 707-1678/ 754)  36.9 W43-W49 S10-S07
     14 1606  628 (S16W46 L=279)  1264    236        3 (1502/ 530-1671/ 709)  58.4 W40-W49 S23-S10
     15 1216  572 (S25W19 L=252)   451    168        0 (1164/ 552-1288/ 613)  20.6 W15-W23 S26-S22
     16 1356  450 (S31W33 L=266)   718    216        2 (1279/ 430-1413/ 479)  18.4 W27-W38 S33-S29
  
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.