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20151115 - Filament data for 09 UTC
Available data for 20151115: »07 UTC   »08 UTC   »09 UTC   »10 UTC  
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  Color  xc   yc  (LatLon LCarr)  Area Length Branches (  x0/y0     x1/y1  )  Tilt Location
      1  484 1555 (N48E29 L=139)   422    118        1 ( 460/1505- 502/1592) -63.4 E32-E26 N44-N52
      2  926 1549 (N36W07 L=176)   864    179        1 ( 853/1501-1021/1580)  -9.5 W01-W13 N33-N37
      3  335 1455 (N45E43 L=125)   373     99        2 ( 302/1440- 370/1476)   0.0 E46-E39 N43-N46
      4 1812 1393 (N05W65 L=234)   832    126        2 (1770/1353-1850/1443) -60.3 W61-W68 N01-N08
      5 1617 1316 (N06W43 L=212)   420     60        1 (1583/1282-1650/1345) -63.4 W41-W45 N03-N07
      6  205 1181 (N29E54 L=114)   572    188        0 ( 148/1160- 248/1199) -16.7 E60-E50 N27-N30
      7 1305  939 (S08W14 L=182)  2209    529        5 (1191/ 717-1366/1110)  82.6 W08-W18 S20-N03
      8  298 1070 (N20E47 L=122)   301    112        0 ( 263/1043- 336/1092) -33.7 E49-E43 N18-N22
      9 1091  927 (S04W02 L=170)  1197    393        3 (1009/ 724-1160/1081)  50.5 E07-W08 S14-N03
     10 1593 1025 (S10W34 L=202)   260     89        0 (1559/1008-1634/1045) -36.9 W31-W36 S11-S08
     11  233  952 (N15E55 L=114)   364     80        1 ( 203/ 930- 255/ 974) -36.9 E57-E52 N13-N16
     12 1426  700 (S25W17 L=186)   646    160        1 (1344/ 653-1506/ 740)   0.0 W11-W23 S26-S23
     13 1195  670 (S21W02 L=170)   252     92        0 (1153/ 633-1232/ 713)  26.6 E01-W05 S22-S19
     14  741  363 (S30E37 L=132)   815    167        2 ( 717/ 303- 765/ 436)  56.3 E40-E32 S34-S25
     15 1396  343 (S51W10 L=178)   413     62        1 (1374/ 313-1419/ 377)  51.3 W07-W12 S53-S47
     16  440  320 (S27E63 L=105)   720    134        2 ( 421/ 282- 457/ 353)  51.3 E65-E60 S29-S24
  
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.