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20260826 - Filament data for 07 UTC
Available data for 20260826: »05 UTC   »06 UTC   »07 UTC   »08 UTC   »09 UTC   »10 UTC   »11 UTC   »12 UTC   »13 UTC   »14 UTC   »15 UTC   »16 UTC  
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  Color  xc   yc  (LatLon LCarr)  Area Length Branches (  x0/y0     x1/y1  )  Tilt Location
      1 1065 1644 (N44W20 L= 66)   344     19        1 (1044/1622-1089/1666)  14.0 W18-W22 N42-N45
      2 1431 1515 (N26W40 L= 85)   345    113        0 (1384/1496-1484/1528) -14.0 W35-W43 N24-N27
      3 1305 1389 (N22W26 L= 71)   389    128        0 (1244/1372-1366/1405) -14.0 W21-W29 N20-N23
      4 1602 1296 (N10W43 L= 88)  1302    325        3 (1488/1170-1693/1390) -67.6 W37-W47 N00-N17
      5  240 1260 (N34E58 L=347)  2777    264        5 ( 156/1151- 298/1367) -23.6 E84-E49 N26-N40
      6 1303 1133 (N08W19 L= 64)   191     71        0 (1265/1118-1338/1147)   0.0 W16-W20 N06-N08
      7 1198 1057 (N05W11 L= 56)   321     84        0 (1166/1025-1227/1100)  36.9 W08-W13 N03-N07
      8  312  988 (N16E49 L=356)  1025    213        1 ( 246/ 916- 390/1063) -42.3 E55-E43 N11-N21
      9  558  895 (N08E31 L= 15)   806    178        1 ( 530/ 831- 600/ 976)  49.4 E33-E26 N03-N11
     10 1182  956 (N00W08 L= 53)   195     88        1 (1141/ 943-1215/ 975) -14.0 W05-W09 N00-N01
     11 1745  924 (S15W45 L= 91)   494    103        1 (1712/ 898-1792/ 952)   7.1 W42-W50 S16-S13
     12  345  674 (S03E53 L=353)  1630    337        1 ( 243/ 567- 468/ 740) -36.3 E62-E45 S10-N01
     13  894  569 (S18E17 L= 28)   345     86        1 ( 877/ 522- 913/ 607)  59.0 E19-E15 S20-S15
     14  437  412 (S21E59 L=347)   927    128        2 ( 383/ 391- 497/ 438)   0.0 E64-E50 S22-S19
     15  814  403 (S27E28 L= 17)   276     46        0 ( 791/ 381- 839/ 429) -71.6 E29-E26 S29-S25
  
Download FITS filament maps as tar archive

» All Filament Data of 20260826 ...
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.