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20251227 - Filament data for 10 UTC
Available data for 20251227: »07 UTC   »08 UTC   »09 UTC   »10 UTC   »11 UTC   »12 UTC   »13 UTC  
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  Color  xc   yc  (LatLon LCarr)  Area Length Branches (  x0/y0     x1/y1  )  Tilt Location
      1  850 1550 (N31E10 L=349)   365     47        1 ( 831/1520- 874/1583) -63.4 E11-E08 N28-N33
      2  941 1556 (N31E04 L=356)   434     99        0 ( 887/1537- 993/1572)   0.0 E07-W00 N29-N32
      3 1100 1519 (N28W07 L=  6)   284     50        1 (1072/1499-1127/1538) -18.4 W05-W08 N26-N29
      4  177 1388 (N24E69 L=290)   721     77        2 ( 159/1349- 200/1412)  90.0 E73-E65 N21-N25
      5 1674 1393 (N18W46 L= 46)   284     60        0 (1639/1381-1707/1405)  -9.5 W43-W49 N17-N19
      6  190 1320 (N20E63 L=296)  1533    108        5 ( 140/1264- 240/1363)  45.0 E72-E57 N16-N22
      7 1289 1315 (N14W17 L= 17)   203     60        1 (1265/1289-1311/1344) -56.3 W15-W18 N12-N15
      8 1141 1200 (N08W08 L=  7)   777    207        2 (1058/1126-1220/1264)  21.8 W02-W12 N03-N11
      9  214 1169 (N10E57 L=302)   385     42        2 ( 191/1144- 237/1196) -56.3 E59-E54 N08-N11
     10  122 1040 (N03E68 L=291)   602     87        0 (  98/1004- 152/1079)  24.0 E72-E63 N01-N05
     11 1715  921 (S10W46 L= 45)   359     70        1 (1670/ 900-1747/ 942)   8.1 W41-W48 S11-S08
     12  235  825 (S10E57 L=303)   941    140        3 ( 185/ 780- 285/ 865) -21.8 E62-E52 S13-S07
     13 1514  801 (S17W31 L= 30)   226     95        0 (1462/ 779-1555/ 825)  18.4 W27-W33 S18-S15
     14  196  699 (S18E66 L=293)  4265    312       13 ( 119/ 575- 268/ 823) -72.6 E73-E59 S25-S09
     15  201  792 (S12E62 L=298)   501     37        1 ( 180/ 767- 220/ 814)  36.9 E64-E59 S13-S10
  
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.