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20251210 - Filament data for 07 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 1487 1728 (N38W51 L=276)  1723    165        6 (1408/1684-1560/1757) -33.7 W43-W57 N34-N41
      2 1266 1711 (N40W30 L=255)   366     44        0 (1244/1680-1290/1740) -90.0 W28-W31 N37-N42
      3  423 1654 (N49E48 L=177)   565     64        1 ( 404/1619- 446/1684) -68.2 E51-E44 N46-N51
      4 1644 1510 (N21W51 L=276)   408     78        1 (1609/1489-1683/1529) -21.8 W47-W55 N19-N22
      5  516 1299 (N22E30 L=195)   459    120        0 ( 457/1281- 577/1320)   0.0 E34-E25 N20-N23
      6 1731 1242 (N04W50 L=274)  1246    316        2 (1598/1162-1854/1283)  -9.9 W39-W62 N00-N07
      7 1873  959 (S14W61 L=286)  2929    306       16 (1800/ 845-1936/1078) -56.3 W52-W70 S21-S06
      8 1704  926 (S14W44 L=268)   654    188        3 (1670/ 849-1736/1009)  71.6 W40-W46 S18-S09
      9 1625  835 (S18W37 L=262)   993    237        1 (1594/ 740-1641/ 964)  85.9 W34-W38 S24-S10
     10 1769  852 (S19W50 L=274)   344     76        1 (1752/ 814-1787/ 892)  78.7 W48-W51 S21-S16
     11 1814  859 (S19W54 L=279)   342     44        2 (1800/ 837-1839/ 881)  26.6 W52-W57 S20-S17
     12 1107  661 (S23W01 L=225)   207     94        0 (1087/ 614-1132/ 703)  59.0 E01-W02 S25-S20
     13 1308  619 (S28W13 L=238)   538    148        1 (1255/ 564-1353/ 686)  45.0 W09-W16 S31-S24
     14  596  465 (S29E39 L=186)   442    147        0 ( 537/ 445- 664/ 489) -18.4 E43-E33 S30-S26
     15  847  314 (S44E26 L=198)   404    106        1 ( 799/ 289- 899/ 341)  10.3 E31-E20 S45-S42
  
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.