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20140415 - Filament data for 06 UTC
Available data for 20140415: »06 UTC   »07 UTC   »08 UTC   »09 UTC   »10 UTC   »11 UTC   »12 UTC   »14 UTC   »15 UTC   »16 UTC  
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  Color  xc   yc  (LatLon LCarr)  Area Length Branches (  x0/y0     x1/y1  )  Tilt Location
      1 1535 1659 (N52W21 L=277)   416     53        0 (1506/1637-1562/1678)   7.1 W18-W25 N51-N53
      2  391 1627 (N14E67 L=189)   657    137        2 ( 369/1599- 417/1658) -24.0 E74-E61 N13-N16
      3  790 1486 (N14E27 L=228)   363    114        1 ( 736/1440- 842/1537)  76.0 E33-E22 N13-N16
      4 1124 1480 (N23E08 L=248)   400     61        1 (1104/1442-1153/1513) -78.7 E10-E05 N22-N25
      5  673 1333 (N03E29 L=227)   373     90        0 ( 645/1281- 698/1383) -39.8 E32-E25 N00-N05
      6  191 1257 (S12E67 L=189)  1577    240        6 ( 141/1157- 219/1341)  76.0 E85-E60 S17-S07
      7  557 1313 (S01E35 L=220)   420    129        2 ( 492/1294- 611/1335)  14.0 E41-E31 S01-S01
      8 1028 1254 (N07E06 L=250)   308     96        0 ( 981/1219-1071/1280)  -8.1 E09-E03 N06-N07
      9  350 1152 (S15E47 L=209)   560    198        1 ( 295/1095- 431/1205)  37.9 E53-E39 S16-S13
     10  909 1152 (S02E10 L=246)   459    153        0 ( 847/1128- 991/1203)   0.0 E15-E05 S01-S00
     11  192 1149 (S18E63 L=192)   452     75        0 ( 176/1115- 214/1177)  90.0 E66-E60 S20-S17
     12  495  999 (S20E32 L=224)   708    220        1 ( 462/ 902- 524/1087) -68.2 E36-E28 S25-S16
     13  800  784 (S25E07 L=249)   235     38        0 ( 775/ 768- 826/ 803)  33.7 E09-E04 S25-S25
     14 1577  576 (S13W49 L=305)   388    101        0 (1558/ 532-1589/ 628) -56.3 W45-W53 S15-S11
     15  891  361 (S49W18 L=273)   437     94        1 ( 845/ 326- 930/ 397)  -9.5 W12-W24 S50-S48
     16  981  368 (S45W24 L=279)   449     78        0 ( 941/ 338-1009/ 394)   0.0 W19-W28 S46-S45
  
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.