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20260211 - Filament data for 13 UTC
Available data for 20260211: »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  738 1834 (N41E44 L= 67)   473     50        0 ( 723/1803- 759/1864) -56.3 E47-E41 N37-N43
      2 1510 1491 (N31W23 L=135)  2460    420        6 (1350/1364-1657/1598) -14.0 W10-W35 N24-N35
      3  429 1493 (N12E48 L= 64)   795    243        1 ( 366/1420- 484/1571)  84.8 E51-E44 N06-N17
      4  341 1337 (N02E50 L= 61)   395    104        0 ( 302/1321- 386/1369)  -7.1 E54-E46 N00-N03
      5  188 1121 (S12E61 L= 51)  1250    170        2 ( 126/1073- 260/1153)  19.7 E69-E53 S15-S10
      6  216 1036 (S17E57 L= 55)   340     44        0 ( 190/1020- 238/1051)   9.5 E60-E54 S18-S16
      7  373  957 (S20E42 L= 70)   302    108        0 ( 357/ 901- 392/1005)  90.0 E42-E40 S23-S17
      8 1872  963 (N08W60 L=172)   739     89        2 (1854/ 913-1897/ 999) -78.7 W57-W62 N05-N10
      9 1000  907 (S14W01 L=112)   181     39        1 ( 977/ 890-1023/ 925)   0.0 W00-W02 S14-S12
     10 1762  735 (S07W55 L=167)   917    121        2 (1709/ 683-1805/ 767)  -4.8 W49-W61 S09-S04
     11  887  654 (S31E02 L=110)  1974    478        3 ( 674/ 587-1109/ 725)  32.6 E15-W10 S38-S22
     12 1729  616 (S14W58 L=170)   672    165        0 (1671/ 586-1790/ 665)  41.2 W52-W62 S17-S10
     13 1420  582 (S24W35 L=147)   897    265        0 (1317/ 555-1541/ 610)  18.4 W27-W42 S26-S19
     14 1768  505 (S19W71 L=183)   807     66        3 (1740/ 475-1786/ 544) -45.0 W67-W75 S20-S16
     15 1405  351 (S38W47 L=159)  2901    404        5 (1221/ 252-1558/ 460)  62.4 W38-W54 S48-S27
     16 1117  251 (S53W33 L=145)   304     72        0 (1105/ 216-1129/ 290) -32.0 W28-W36 S55-S50
  
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.