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20260201 - Filament data for 10 UTC
Available data for 20260201: »10 UTC   »11 UTC   »13 UTC  
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  Color  xc   yc  (LatLon LCarr)  Area Length Branches (  x0/y0     x1/y1  )  Tilt Location
      1  780 1866 (N47E41 L=204)   618     88        0 ( 769/1817- 792/1914) -42.5 E49-E36 N42-N53
      2  857 1710 (N35E24 L=221)   664     83        3 ( 818/1678- 902/1742)  -8.1 E27-E20 N32-N37
      3 1189 1639 (N35W01 L=246)   389     70        1 (1167/1614-1226/1669) -45.0 W00-W04 N32-N37
      4 1679 1404 (N28W40 L=285)   330     51        2 (1647/1383-1708/1422)   0.0 W37-W42 N26-N28
      5  191 1326 (N04E66 L=179)  1409    174        4 ( 135/1260- 239/1406)  58.0 E73-E60 N00-N08
      6 1710 1323 (N23W42 L=287)   512     96        1 (1690/1271-1730/1375) -80.5 W40-W43 N19-N26
      7 1565 1328 (N20W30 L=275)   239     94        0 (1526/1298-1605/1359) -18.4 W27-W33 N19-N21
      8 1368 1114 (N04W19 L=264)   250     73        1 (1345/1079-1400/1143)  56.3 W17-W20 N02-N05
      9 1889 1037 (N10W61 L=306)   483     65        1 (1870/1001-1908/1068)  53.1 W59-W63 N07-N11
     10  219  949 (S19E57 L=188)  1211    247        5 ( 131/ 912- 328/ 989)   0.0 E68-E45 S21-S16
     11 1304  809 (S14W20 L=265)  1239    376        3 (1214/ 674-1425/ 964)  70.7 W17-W24 S23-S03
     12 1791  741 (S09W58 L=303)   771    141        2 (1756/ 685-1823/ 791) -15.3 W53-W64 S11-S06
     13 1761  663 (S14W58 L=303)   396     50        0 (1745/ 631-1780/ 690) -56.3 W56-W60 S15-S12
     14 1569  550 (S25W46 L=291)  1268    354        0 (1376/ 503-1699/ 604)  28.6 W33-W55 S31-S18
     15  982  579 (S33W04 L=249)   312     93        2 ( 929/ 568-1030/ 597)   8.1 W00-W07 S34-S31
     16 1257  267 (S50W40 L=285)   684     89        1 (1203/ 248-1305/ 290)  11.3 W34-W45 S51-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.