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20141122 - Filament data for 10 UTC
Available data for 20141122: »10 UTC   »11 UTC   »12 UTC  
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  Color  xc   yc  (LatLon LCarr)  Area Length Branches (  x0/y0     x1/y1  )  Tilt Location
      1 1496 1545 (N22W43 L=256)  1187    288        0 (1375/1508-1622/1596) -26.6 W36-W53 N18-N27
      2 1572 1380 (N11W42 L=255)   383    100        1 (1518/1342-1606/1416) -51.3 W39-W44 N08-N14
      3  934 1348 (N23W01 L=214)  1732    465        4 ( 731/1311-1145/1375) -13.5 E11-W14 N18-N26
      4 1391 1262 (N08W27 L=240)   217     50        1 (1362/1241-1418/1282) -33.7 W24-W27 N06-N09
      5 1390 1202 (N05W25 L=238)   240     24        1 (1373/1177-1410/1230)  56.3 W23-W26 N03-N06
      6 1695 1113 (S07W44 L=257)   817    251        2 (1595/1059-1780/1166) -37.6 W37-W51 S11-S01
      7  504 1106 (N17E30 L=183)   427    127        1 ( 455/1057- 547/1152) -58.0 E33-E27 N12-N20
      8 1702 1021 (S12W43 L=256)   579    117        2 (1666/ 977-1738/1064) -56.3 W40-W45 S14-S08
      9 1690  919 (S18W40 L=253)   552    126        1 (1630/ 879-1727/ 960)  14.0 W35-W43 S19-S15
     10 1334  897 (S11W16 L=229)   302    141        1 (1266/ 858-1376/ 923) -15.9 W11-W18 S14-S10
     11 1690  830 (S23W40 L=253)   518    160        0 (1625/ 768-1724/ 895)  33.7 W33-W42 S25-S19
     12 1563  815 (S21W29 L=243)   324     65        1 (1529/ 795-1597/ 841) -18.4 W26-W32 S22-S19
     13  478  452 (S21E51 L=163)  1127    313        2 ( 420/ 381- 517/ 548)  26.6 E59-E43 S25-S16
     14 1731  500 (S48W47 L=260)  1338    278        2 (1692/ 471-1791/ 540) -23.6 W42-W58 S52-S44
     15 1035  443 (S33E13 L=200)   852    176        0 ( 952/ 386-1089/ 516)  24.8 E20-E07 S36-S29
     16  606  347 (S31E46 L=167)  1139    306        0 ( 560/ 272- 652/ 437)  30.5 E55-E38 S35-S25
  
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.