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20141019 - Filament data for 13 UTC
Available data for 20141019: »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 1435 1673 (N29W49 L=349)   425     96        1 (1389/1638-1487/1701) -63.4 W47-W51 N25-N31
      2 1109 1248 (N15W11 L=311)   390    142        1 (1032/1213-1177/1284) -45.0 W07-W14 N12-N19
      3  310 1151 (N30E44 L=255)   969    274        3 ( 241/1071- 389/1222) -45.0 E50-E38 N24-N36
      4 1159 1063 (N04W08 L=308)   359    112        1 (1120/1023-1211/1106)  23.2 W05-W12 N02-N05
      5 1021 1078 (N09W01 L=301)   521    153        3 ( 934/1062-1091/1096) -35.5 E03-W05 N06-N11
      6  707 1021 (N13E18 L=282)   693    244        1 ( 600/ 961- 824/1051)  -3.6 E26-E10 N11-N15
      7  443  937 (N15E37 L=262)   438    145        1 ( 386/ 911- 508/ 969) -24.0 E41-E32 N12-N17
      8 1388  873 (S13W16 L=316)   240    119        0 (1374/ 807-1408/ 932)  60.3 W14-W18 S16-S09
      9 1683  887 (S21W37 L=336)   405     81        2 (1659/ 841-1707/ 930)  38.7 W34-W39 S23-S18
     10  146  842 (N15E69 L=231)  1905    374        3 (  91/ 795- 220/ 891) -17.4 E76-E60 N11-N17
     11 1212  601 (S24E01 L=299)  1601    333        2 (1160/ 447-1276/ 745)  48.8 E08-W06 S32-S16
     12  364  597 (S03E55 L=245)   359    103        1 ( 323/ 565- 402/ 633) -38.7 E57-E52 S04-N00
     13  529  540 (S10E44 L=256)  1141    247        5 ( 478/ 460- 571/ 615)  73.3 E48-E41 S14-S04
     14  437  473 (S12E55 L=245)   496    133        2 ( 394/ 449- 487/ 499) -20.6 E59-E51 S14-S09
     15  619  460 (S17E42 L=258)   304     20        0 ( 596/ 442- 642/ 478) -45.0 E43-E40 S17-S15
     16  505  354 (S21E57 L=243)   989    186        3 ( 473/ 293- 535/ 406)  71.6 E60-E52 S25-S16
  
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.