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20260314 - Filament data for 08 UTC
Available data for 20260314: »07 UTC   »08 UTC   »09 UTC  
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  Color  xc   yc  (LatLon LCarr)  Area Length Branches (  x0/y0     x1/y1  )  Tilt Location
      1 1298 1693 (N41E03 L= 63)   402     88        0 (1251/1675-1347/1712)  15.9 E06-W01 N39-N42
      2  846 1618 (N22E28 L= 38)   622    137        1 ( 782/1567- 904/1649)  -5.7 E32-E22 N20-N23
      3  723 1568 (N16E33 L= 33)   394    111        2 ( 705/1503- 750/1611) -60.3 E34-E30 N12-N19
      4 1035 1418 (N15E10 L= 56)   401    103        2 ( 992/1392-1084/1445)  45.0 E12-E07 N13-N17
      5  454 1331 (S03E42 L= 24)   337     48        1 ( 439/1295- 475/1360) -63.4 E43-E41 S05-S01
      6 1884 1260 (N34W58 L=124)  1017     89        3 (1842/1229-1922/1284)   8.1 W51-W65 N31-N35
      7  675 1186 (S07E24 L= 42)   618    155        0 ( 616/1139- 743/1234)  53.1 E26-E20 S10-S02
      8 1236 1166 (N06W08 L= 74)   323    148        0 (1187/1130-1306/1207)   0.0 W04-W12 N05-N07
      9  598 1041 (S17E25 L= 41)   914    202        2 ( 561/ 980- 668/1140) -33.7 E28-E19 S19-S11
     10  325 1085 (S20E47 L= 20)   279     89        0 ( 291/1068- 368/1108)  26.6 E49-E43 S20-S17
     11  111 1000 (S28E73 L=353)   884     76        3 (  72/ 970- 147/1024)   6.3 E86-E66 S29-S26
     12 1049  904 (S13W05 L= 71)  1240    278        4 ( 908/ 874-1168/ 943)  28.3 E02-W11 S17-S09
     13 1849  732 (N02W65 L=131)   938    101        2 (1820/ 691-1870/ 769)  90.0 W60-W68 N00-N04
     14 1682  517 (S14W61 L=127)  1211     88        1 (1639/ 468-1718/ 570) -13.0 W54-W68 S16-S12
     15 1253  464 (S31W33 L= 99)   229     59        0 (1217/ 451-1282/ 476)  14.0 W30-W34 S32-S29
     16  559  376 (S62E18 L= 48)   865     62        1 ( 528/ 343- 595/ 419) -74.1 E23-E13 S64-S57
  
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.