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20140416 - Filament data for 08 UTC
Available data for 20140416: »05 UTC   »06 UTC   »07 UTC   »08 UTC   »09 UTC   »10 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  456 1518 (N08E51 L=190)   885    189        2 ( 382/1482- 531/1566)  37.9 E56-E46 N05-N12
      2 1220 1521 (N29E03 L=238)   271     17        0 (1194/1501-1244/1536)  18.4 E04-E01 N27-N30
      3 1312 1387 (N23W06 L=248)   409     80        0 (1293/1346-1333/1434) -68.2 W04-W07 N20-N25
      4  271 1179 (S15E54 L=187)  1161    289        0 ( 183/1093- 330/1305)  61.9 E61-E50 S21-S06
      5 1227 1160 (N07W07 L=249)   321    139        1 (1175/1124-1287/1198)  -7.1 W03-W11 N06-N08
      6  327  911 (S30E43 L=198)   384     97        1 ( 307/ 853- 343/ 959) -56.3 E45-E41 S33-S27
      7  670  876 (S23E17 L=225)   435    117        0 ( 643/ 818- 710/ 920)  81.9 E18-E15 S26-S19
      8  184  792 (S41E57 L=184)   553    136        0 ( 154/ 774- 214/ 810)   8.1 E60-E53 S41-S39
      9 1409  704 (S12W32 L=273)   304     74        1 (1373/ 675-1449/ 732)  45.0 W29-W33 S13-S09
     10  970  689 (S26W07 L=248)   216     56        1 ( 943/ 667-1003/ 715) -11.3 W04-W09 S26-S24
     11  800  670 (S32E03 L=238)   318     79        0 ( 750/ 647- 835/ 690)   0.0 E06-W00 S32-S30
     12 1688  506 (S13W63 L=304)   505    123        0 (1665/ 461-1701/ 558) -63.4 W59-W64 S15-S09
     13  819  398 (S49W09 L=250)   595    141        0 ( 798/ 346- 853/ 456) -33.7 W05-W14 S52-S44
     14  944  315 (S50W23 L=265)  1114    242        5 ( 914/ 260- 992/ 390) -39.3 W17-W29 S54-S45
     15 1233  356 (S37W38 L=280)   444     67        2 (1208/ 332-1259/ 387) -18.4 W35-W41 S38-S35
     16 1077  309 (S46W32 L=274)   458     55        1 (1054/ 284-1102/ 341) -38.7 W29-W35 S47-S43
  
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.