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20260314 - Latest Filament data
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 1300 1693 (N41E03 L= 63)   383     83        0 (1254/1675-1348/1711)  15.9 E06-W01 N39-N42
      2  851 1616 (N22E27 L= 39)   507    133        1 ( 787/1577- 907/1639)   0.0 E31-E22 N20-N23
      3 1037 1417 (N15E10 L= 56)   337    106        1 ( 994/1394-1083/1442)  45.0 E12-E07 N13-N17
      4  961 1368 (N10E12 L= 54)   229    103        0 ( 925/1334-1007/1394)  -8.1 E15-E08 N09-N11
      5  457 1329 (S03E42 L= 24)   234     52        1 ( 444/1295- 476/1355) -76.0 E43-E40 S05-S01
      6 1875 1266 (N33W56 L=122)   589     58        1 (1848/1249-1910/1280)  15.3 W52-W63 N31-N35
      7  678 1183 (S07E23 L= 42)   484    140        1 ( 625/1139- 744/1227)  54.5 E26-E20 S10-S02
      8 1237 1165 (N06W08 L= 74)   276    136        0 (1195/1128-1302/1204)   0.0 W04-W12 N05-N07
      9  604 1034 (S17E25 L= 41)   767    188        1 ( 567/ 979- 672/1119) -29.1 E28-E19 S19-S12
     10  340 1087 (S19E45 L= 21)   336    117        0 ( 295/1067- 384/1111)  20.6 E49-E41 S21-S17
     11  112 1000 (S28E73 L=353)   799     80        2 (  72/ 972- 148/1023)   6.0 E86-E66 S29-S26
     12 1059  904 (S13W05 L= 71)   984    273        6 ( 922/ 874-1171/ 940)  24.8 E02-W11 S17-S08
     13 1850  730 (N02W65 L=131)   905     97        2 (1821/ 691-1872/ 765)  90.0 W60-W69 N00-N04
     14 1686  514 (S14W61 L=127)  1140     96        2 (1652/ 466-1721/ 570) -13.0 W55-W68 S16-S12
     15  561  374 (S62E18 L= 48)   812     76        1 ( 531/ 338- 595/ 416) -50.2 E22-E13 S64-S57
     16 1156  152 (S54W60 L=126)   443     48        0 (1142/ 124-1168/ 184) -17.1 W53-W66 S55-S51
  
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.