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20251210 - Filament data for 11 UTC
Available data for 20251210: »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 1515 1736 (N38W54 L=277)  2019    194        6 (1425/1673-1593/1770) -30.3 W45-W62 N32-N41
      2 1297 1717 (N40W33 L=255)   441     74        1 (1265/1692-1333/1743) -53.1 W30-W34 N37-N42
      3  440 1659 (N49E45 L=178)   510     50        2 ( 424/1626- 458/1688) -35.5 E49-E41 N46-N51
      4  539 1309 (N22E28 L=195)   617    175        0 ( 451/1285- 602/1338) -20.0 E34-E23 N20-N25
      5 1682 1270 (N06W46 L=269)   266     80        0 (1645/1249-1726/1285)   8.1 W42-W49 N05-N07
      6 1812 1230 (N03W57 L=280)   416     91        0 (1784/1192-1846/1254)  20.6 W53-W61 N00-N04
      7  309 1115 (N13E46 L=176)   520     98        0 ( 280/1066- 341/1163) -56.3 E49-E43 N10-N16
      8 1854  976 (S13W58 L=281)  5457    430       14 (1725/ 895-1948/1066) -15.1 W45-W72 S17-S06
      9 1654  843 (S18W39 L=262)  1058    183        2 (1625/ 763-1673/ 945)  84.8 W36-W41 S23-S12
     10 1720  901 (S15W45 L=267)   379     56        2 (1702/ 863-1738/ 934)  90.0 W43-W46 S17-S13
     11 1790  862 (S19W52 L=274)   299     60        0 (1778/ 831-1801/ 897) -76.0 W50-W52 S20-S16
     12 1344  649 (S27W16 L=239)   747    229        0 (1271/ 575-1403/ 753)  45.0 W10-W20 S30-S20
     13 1132  655 (S24W02 L=225)   354    115        1 (1101/ 603-1162/ 705)  56.3 W00-W04 S26-S20
     14  429  522 (S23E50 L=173)   394     46        1 ( 411/ 497- 447/ 556) -90.0 E52-E47 S24-S20
     15  861  314 (S44E25 L=198)   301     78        1 ( 822/ 293- 895/ 340)   0.0 E28-E21 S45-S41
  
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.