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20140414 - Filament data for 13 UTC
Available data for 20140414: »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  915 1667 (N29E27 L=238)   403     80        1 ( 865/1649- 949/1688)  36.9 E29-E24 N26-N30
      2  652 1523 (N13E37 L=228)   504    107        1 ( 602/1481- 703/1568)  66.8 E39-E35 N09-N16
      3 1005 1512 (N21E15 L=250)   491     75        1 ( 979/1476-1040/1550) -26.6 E18-E12 N19-N23
      4  550 1398 (N03E39 L=226)   306     82        0 ( 530/1358- 569/1432) -36.9 E40-E36 N01-N04
      5 1253 1370 (N20W03 L=268)   240     93        1 (1202/1339-1287/1391)   0.0 W00-W05 N18-N21
      6  465 1349 (S02E43 L=222)   357     88        1 ( 437/1328- 505/1372)   0.0 E45-E39 S03-N00
      7  903 1301 (N06E14 L=251)   406    113        1 ( 850/1248- 937/1336) -26.6 E17-E11 N03-N07
      8  779 1223 (S01E19 L=246)   633    211        2 ( 713/1190- 866/1291)   0.0 E24-E13 S02-N01
      9  201 1203 (S15E62 L=203)  1727    588        1 (  98/1123- 333/1286)  28.6 E73-E51 S20-S08
     10  256 1177 (S16E55 L=210)   713    195        1 ( 208/1112- 321/1241)  45.0 E58-E50 S19-S10
     11  370 1064 (S20E42 L=223)  2169    452        8 ( 310/ 939- 420/1227) -53.7 E51-E37 S27-S11
     12  682  853 (S24E15 L=250)   225     29        0 ( 659/ 837- 708/ 872)  14.0 E17-E13 S25-S23
     13 1014  795 (S18W06 L=271)   283     47        1 ( 987/ 776-1045/ 820)  14.0 W04-W08 S19-S17
     14 1396  487 (S24W41 L=306)   326    102        0 (1348/ 462-1437/ 506)   7.1 W36-W44 S24-S23
     15  863  421 (S46W11 L=276)   480     80        1 ( 838/ 389- 892/ 465) -33.7 W07-W13 S47-S43
     16  759  424 (S50W03 L=268)   403     87        0 ( 728/ 404- 809/ 458)   0.0 E01-W07 S50-S47
  
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.