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20251227 - Filament data for 12 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  521 1653 (N41E39 L=319)   496    140        0 ( 460/1635- 597/1666)   0.0 E45-E31 N39-N41
      2  867 1552 (N31E09 L=349)   302     34        1 ( 848/1527- 889/1579) -56.3 E10-E07 N29-N32
      3  966 1557 (N31E02 L=356)   456    108        2 ( 916/1530-1023/1574)   8.1 E05-W02 N29-N32
      4 1119 1520 (N28W08 L=  6)   288     35        0 (1090/1497-1144/1538) -33.7 W06-W09 N26-N29
      5  197 1337 (N21E63 L=295)  2230    194        4 ( 163/1252- 246/1420) -57.5 E71-E56 N15-N26
      6 1307 1316 (N14W18 L= 17)   309     56        2 (1278/1286-1338/1342) -26.6 W16-W20 N12-N15
      7 1159 1200 (N08W09 L=  7)   833    197        4 (1078/1127-1226/1269)  29.1 W03-W12 N03-N11
      8  226 1169 (N10E56 L=303)   355     30        1 ( 208/1146- 246/1196) -71.6 E57-E53 N08-N11
      9  130 1042 (N03E67 L=291)   592     82        2 ( 105/1006- 158/1080)  26.6 E71-E62 N01-N05
     10 1730  920 (S10W47 L= 45)   294     32        1 (1709/ 896-1750/ 944) -71.6 W45-W48 S11-S08
     11  222  844 (S09E58 L=300)   336     52        0 ( 198/ 824- 243/ 864) -11.3 E60-E55 S10-S08
     12  256  812 (S11E55 L=303)   424     72        2 ( 239/ 780- 277/ 861)  78.7 E57-E52 S13-S08
     13  201  705 (S17E65 L=293)  4399    315       12 ( 120/ 579- 269/ 832) -72.6 E73-E58 S25-S09
     14 1531  802 (S17W32 L= 30)   262     97        0 (1476/ 778-1575/ 828)  23.2 W28-W35 S18-S15
     15  209  793 (S12E61 L=298)   480     44        1 ( 187/ 771- 229/ 814)  11.3 E63-E58 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.