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20140930 - Filament data for 10 UTC
Available data for 20140930: »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 1454 1719 (N32W55 L=247)   945    188        1 (1391/1700-1525/1737) -24.4 W49-W60 N28-N34
      2 1690 1561 (N15W64 L=256)   471     60        0 (1660/1537-1722/1586) -51.3 W61-W66 N12-N17
      3 1047 1442 (N29W14 L=206)   357     96        0 (1007/1413-1105/1465)  -9.5 W10-W17 N28-N30
      4 1507 1421 (N14W41 L=233)  2758    614        5 (1254/1383-1727/1454) -22.4 W24-W58 N05-N21
      5  734 1272 (N28E11 L=181)   501    132        1 ( 699/1215- 781/1338) -90.0 E12-E07 N24-N32
      6 1868 1186 (S10W63 L=255)  1240    205        3 (1822/1107-1896/1250) -90.0 W58-W66 S15-S06
      7 1152 1144 (N10W10 L=202)   411    149        0 (1137/1067-1172/1220)  49.4 W07-W13 N05-N13
      8 1796 1086 (S13W51 L=243)  2204    470        7 (1735/ 973-1858/1176) -74.1 W45-W57 S20-S06
      9 1195 1027 (N02W09 L=202)   466     71        3 (1145/1003-1252/1058) -38.7 W06-W12 N00-N04
     10  338  957 (N19E46 L=146)   366     73        1 ( 323/ 913- 349/ 999)  78.7 E47-E44 N16-N21
     11 1555  790 (S22W25 L=217)  1783    384        3 (1476/ 643-1592/ 944)  87.1 W21-W27 S30-S10
     12  471  556 (S07E48 L=144)   387     89        1 ( 442/ 522- 516/ 588) -59.0 E50-E45 S09-S04
     13  285  531 (S05E69 L=123)   933     94        0 ( 254/ 499- 321/ 564) -59.0 E72-E64 S07-S02
     14  703  458 (S18E36 L=156)   491    206        0 ( 662/ 394- 737/ 534)  36.0 E41-E30 S21-S13
     15  866  315 (S32E33 L=159)   429     55        0 ( 832/ 296- 901/ 336) -11.3 E36-E30 S32-S30
     16  733  251 (S33E47 L=146)  1254    289        2 ( 698/ 193- 790/ 308)  20.6 E54-E38 S37-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.