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20260116 - Filament data for 13 UTC
Available data for 20260116: »08 UTC   »09 UTC   »10 UTC   »11 UTC   »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  768 1729 (N40E26 L= 68)   398     43        0 ( 745/1702- 794/1752) -76.0 E28-E24 N37-N41
      2 1216 1684 (N39W09 L=103)   328     43        1 (1193/1660-1246/1706)  36.9 W07-W11 N37-N41
      3  392 1496 (N21E49 L= 45)   550    123        0 ( 368/1435- 418/1551) -60.3 E50-E46 N17-N24
      4  326 1431 (N17E53 L= 42)  2126    315        7 ( 279/1314- 389/1550) -78.7 E59-E45 N09-N24
      5  490 1241 (N05E35 L= 59)   308     85        1 ( 450/1220- 519/1275)  36.9 E37-E33 N04-N07
      6  678 1177 (N02E22 L= 72)   676    147        1 ( 647/1115- 712/1249) -66.8 E24-E19 S01-N06
      7 1792 1120 (N08W51 L=146)  1140    224        1 (1689/1093-1879/1174)  17.5 W42-W61 N05-N12
      8  372 1004 (S09E42 L= 52)  1554    408        6 ( 293/ 893- 435/1153) -56.3 E49-E37 S15-N00
      9  168 1078 (S05E62 L= 32)   452     51        0 ( 152/1053- 185/1111)  53.1 E64-E60 S06-S02
     10  485 1050 (S06E34 L= 60)   442     77        0 ( 455/1017- 533/1078)  31.0 E35-E30 S07-S04
     11  289  937 (S13E50 L= 45)   865    183        2 ( 207/ 909- 333/ 999)  17.1 E58-E45 S14-S09
     12 1930  953 (N00W69 L=164)   711     83        0 (1896/ 920-1961/ 973)  16.7 W64-W75 S02-N01
     13 1387  895 (S10W23 L=117)   240     26        0 (1371/ 869-1406/ 921)  90.0 W21-W24 S11-S07
     14 1462  680 (S22W32 L=126)   328     75        1 (1432/ 653-1499/ 707)  53.1 W29-W33 S23-S19
     15  903  437 (S43E04 L= 90)   218     54        0 ( 878/ 418- 933/ 451)  26.6 E06-E02 S44-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.