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20141019 - Filament data for 11 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 1506 1416 (N13W40 L=341)   398    179        0 (1459/1365-1579/1454)   5.2 W35-W46 N11-N13
      2 1099 1234 (N15W10 L=311)   302    100        0 (1043/1203-1154/1265) -50.2 W07-W12 N12-N18
      3  296 1150 (N31E46 L=255)  1218    306        2 ( 219/1068- 381/1235) -47.1 E52-E39 N23-N37
      4 1145 1055 (N04W07 L=308)   400    121        0 (1103/1013-1198/1106)  23.2 W04-W11 N02-N05
      5 1002 1070 (N09E00 L=301)   508    148        1 ( 921/1052-1073/1085) -29.7 E04-W03 N06-N10
      6  700 1023 (N14E18 L=282)   596    136        1 ( 639/ 993- 770/1045)  -6.3 E22-E13 N12-N16
      7  429  931 (N15E39 L=262)   422    153        0 ( 372/ 910- 492/ 965) -26.6 E42-E33 N12-N17
      8 1374  853 (S13W15 L=316)   309    138        0 (1359/ 784-1393/ 926)  63.4 W13-W17 S17-S09
      9 1666  867 (S22W35 L=336)   249     54        0 (1643/ 842-1683/ 896)  26.6 W32-W36 S22-S20
     10  127  853 (N16E71 L=230)  1246    211        2 (  92/ 814- 159/ 888) -20.6 E76-E66 N13-N17
     11  327  790 (N09E51 L=250)   315     70        1 ( 314/ 752- 342/ 825) -90.0 E51-E48 N06-N11
     12 1197  596 (S23E02 L=299)  1664    312        3 (1151/ 452-1260/ 738)  47.0 E09-W05 S31-S16
     13  382  567 (S05E55 L=246)   694    143        3 ( 336/ 530- 431/ 611) -54.5 E57-E52 S08-S01
     14  517  539 (S09E45 L=256)  1263    223        3 ( 465/ 457- 568/ 611)  73.3 E49-E41 S14-S04
     15  607  454 (S17E43 L=258)   326     10        0 ( 584/ 432- 628/ 473) -63.4 E44-E41 S17-S15
     16  501  358 (S20E57 L=244)   991    177        3 ( 464/ 299- 537/ 397)  66.8 E60-E53 S24-S17
  
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.