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20141224 - Filament data for 10 UTC
Available data for 20141224: »09 UTC   »10 UTC   »12 UTC   »13 UTC  
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  Color  xc   yc  (LatLon LCarr)  Area Length Branches (  x0/y0     x1/y1  )  Tilt Location
      1 1538 1591 (N31W42 L=193)  1407    240        6 (1430/1549-1617/1618) -12.1 W33-W49 N27-N33
      2  500 1567 (N36E36 L=115)   722    190        4 ( 426/1542- 582/1592)   4.4 E42-E29 N34-N37
      3 1429 1488 (N24W30 L=182)   243     45        1 (1406/1466-1453/1508) -45.0 W28-W32 N22-N25
      4 1708 1395 (N17W50 L=202)   623    113        3 (1680/1354-1738/1446) -71.6 W47-W52 N14-N20
      5 1850 1263 (N09W62 L=213)   719    182        4 (1817/1220-1877/1307)  39.8 W57-W66 N06-N11
      6  468 1233 (N14E35 L=117)   332     85        2 ( 431/1203- 500/1255) -21.8 E37-E32 N12-N15
      7  779 1134 (N06E14 L=137)   322     97        1 ( 753/1108- 816/1184)  63.4 E15-E11 N04-N08
      8  183 1033 (N04E61 L= 91)   621    153        1 ( 150/ 973- 224/1077) -41.2 E64-E56 N00-N07
      9 1322  915 (S10W18 L=169)   483    200        0 (1257/ 821-1362/ 996) -59.0 W13-W19 S15-S05
     10 1881  949 (S10W62 L=214)  1098    198        3 (1843/ 914-1929/ 982)  20.0 W58-W69 S12-S08
     11 1838  839 (S17W58 L=209)   572    112        0 (1814/ 797-1865/ 883) -51.3 W55-W61 S19-S14
     12 1917  831 (S17W68 L=219)   892    176        3 (1885/ 783-1944/ 881)  63.4 W63-W72 S20-S14
     13  232  811 (S09E58 L= 93)   333     94        1 ( 205/ 797- 259/ 830)   9.5 E61-E54 S10-S08
     14 1626  721 (S24W39 L=191)  1085    182        3 (1569/ 640-1679/ 819)  84.8 W35-W43 S28-S17
     15  238  600 (S22E63 L= 88)  2968    374        4 ( 203/ 537- 282/ 674)  71.6 E69-E57 S26-S17
     16  312  574 (S24E56 L= 95)   741    157        6 ( 291/ 512- 336/ 632)  76.0 E58-E53 S28-S20
  
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.