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20260405 - Filament data for 12 UTC
Available data for 20260405: »06 UTC   »07 UTC   »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  337 1514 (N04E61 L= 73)  1593    196        4 ( 278/1460- 426/1570)  -5.7 E70-E50 N01-N07
      2 1671 1529 (N46W31 L=165)   382     23        0 (1647/1512-1694/1546)  33.7 W28-W34 N43-N48
      3 1199 1457 (N23E03 L=131)   265     42        0 (1175/1430-1220/1490) -78.7 E03-E01 N20-N25
      4 1174 1339 (N15E01 L=133)   280     67        1 (1154/1312-1199/1376) -56.3 E01-W01 N13-N17
      5 1414 1216 (N15W16 L=150)   320    150        0 (1375/1141-1458/1263) -26.6 W12-W20 N12-N16
      6  169 1169 (S19E66 L= 68)  1725    194        1 (  89/1125- 236/1220)  11.8 E82-E57 S21-S14
      7 1049 1111 (S01E01 L=133)   602    154        2 (1018/1032-1077/1176) -63.4 E03-W01 S04-N02
      8 1806 1020 (N18W50 L=184)   357     68        0 (1786/ 987-1829/1051)  78.7 W48-W52 N15-N20
      9 1710  942 (N10W43 L=177)   268     84        0 (1691/ 903-1721/ 986) -63.4 W41-W44 N07-N12
     10 1370  912 (S02W22 L=156)   477    142        0 (1314/ 867-1420/ 957)  74.1 W20-W24 S06-N01
     11 1075  611 (S27W16 L=150)   301     85        0 (1038/ 595-1123/ 630)  18.4 W13-W19 S28-S26
     12  897  585 (S34W06 L=140)   427    118        0 ( 832/ 562- 950/ 603)  12.5 W01-W10 S36-S31
     13  311  543 (S56E51 L= 83)   413     59        0 ( 283/ 522- 343/ 569)  18.4 E59-E44 S58-S53
     14  419  539 (S53E34 L=100)   315     47        0 ( 399/ 520- 445/ 564) -26.6 E36-E30 S54-S51
     15 1499  473 (S21W49 L=183)   404     99        0 (1453/ 440-1545/ 498)  51.3 W47-W51 S23-S18
     16 1252  374 (S35W40 L=174)   944    206        0 (1168/ 319-1326/ 443)  74.7 W36-W41 S39-S28
  
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.