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20140930 - Filament data for 11 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 1456 1722 (N32W55 L=247)  1088    150        1 (1390/1699-1527/1741) -31.0 W49-W60 N28-N34
      2 1056 1445 (N29W15 L=206)   325     97        1 (1015/1413-1108/1467)   0.0 W11-W18 N27-N30
      3 1511 1425 (N14W42 L=233)  2751    620        6 (1248/1381-1731/1459) -23.8 W24-W58 N05-N21
      4  741 1278 (N28E10 L=181)   479    139        1 ( 707/1233- 788/1350) -90.0 E11-E07 N25-N33
      5 1868 1196 (S10W63 L=254)  1198    196        6 (1834/1111-1896/1263) -90.0 W59-W67 S15-S05
      6 1179 1089 (N06W10 L=202)   820    278        1 (1145/1009-1252/1222)  85.6 W07-W13 N00-N13
      7 1792 1118 (S11W52 L=243)  1459    229        5 (1741/1068-1858/1167) -37.9 W46-W58 S14-S07
      8 1704 1090 (S09W43 L=235)   274     41        1 (1691/1063-1719/1116) -90.0 W42-W45 S11-S07
      9 1812 1014 (S18W51 L=242)   391    103        2 (1789/ 980-1841/1060) -90.0 W48-W53 S20-S14
     10  342  949 (N19E46 L=146)   401    110        1 ( 330/ 887- 357/ 999)  63.4 E47-E43 N15-N21
     11 1561  793 (S22W26 L=217)  1841    414        4 (1470/ 641-1600/ 951) -90.0 W21-W28 S31-S09
     12 1002  579 (S18E14 L=178)   208     62        0 ( 970/ 546-1028/ 603) -78.7 E14-E12 S20-S15
     13  484  553 (S07E47 L=144)   421    111        1 ( 446/ 521- 539/ 594) -56.3 E48-E44 S10-S04
     14  287  534 (S05E68 L=123)   871    124        1 ( 260/ 506- 322/ 569) -59.0 E72-E63 S07-S02
     15  709  461 (S18E36 L=156)   480    183        0 ( 669/ 401- 740/ 531)  31.0 E40-E30 S20-S14
     16  785  276 (S32E41 L=151)  1767    421        3 ( 697/ 196- 918/ 344)  11.3 E53-E28 S36-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.