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20251223 - Filament data for 09 UTC
Available data for 20251223: »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  346 1431 (N27E48 L=  5)  1424    228        3 ( 250/1400- 453/1483)  -7.4 E60-E37 N24-N31
      2  820 1385 (N21E11 L= 42)   199     48        0 ( 790/1369- 846/1404)  18.4 E12-E09 N19-N22
      3  437 1273 (N16E37 L= 15)   275     75        1 ( 405/1244- 472/1303) -45.0 E39-E34 N14-N18
      4  416 1177 (N11E38 L= 14)   227     21        0 ( 399/1157- 434/1199)  71.6 E39-E36 N09-N12
      5  373 1117 (N07E42 L= 11)   380     87        1 ( 342/1084- 416/1137)   9.5 E44-E38 N05-N08
      6  295 1056 (N05E48 L=  4)   626    138        0 ( 270/ 996- 327/1126)  69.4 E50-E45 N00-N08
      7  464 1052 (N03E35 L= 18)   429     81        0 ( 419/1020- 492/1088)  31.0 E38-E32 N01-N05
      8  366  768 (S13E46 L=  7)  1798    410        6 ( 287/ 629- 467/ 917)  43.3 E54-E36 S21-S04
      9  228  782 (S11E59 L=354)  2710    263       13 ( 169/ 660- 292/ 904) -86.2 E66-E54 S18-S03
     10 1184  768 (S18W08 L= 61)   188     42        1 (1163/ 740-1199/ 794) -71.6 W07-W09 S19-S16
     11  686  717 (S18E23 L= 29)   202     84        0 ( 646/ 701- 728/ 742)   9.5 E26-E20 S19-S16
     12  834  634 (S24E15 L= 38)   968    225        5 ( 727/ 570- 923/ 694)  23.2 E22-E08 S27-S21
     13 1832  619 (S30W66 L=119)   714     60        1 (1798/ 598-1874/ 637)   4.8 W61-W74 S31-S29
     14  241  532 (S26E71 L=341)   978    129        0 ( 206/ 512- 285/ 567)   0.0 E79-E63 S27-S24
     15 1617  426 (S43W49 L=102)   835    104        2 (1572/ 394-1659/ 470)  68.2 W44-W54 S45-S40
  
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.