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20260826 - Filament data for 12 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 1068 1643 (N44W20 L= 63)   297      9        0 (1049/1621-1087/1664)  36.9 W18-W22 N42-N45
      2 1451 1526 (N26W42 L= 85)   415    125        0 (1397/1488-1498/1545)   0.0 W36-W45 N24-N27
      3 1348 1407 (N22W29 L= 72)   358    104        1 (1293/1391-1398/1421) -15.9 W25-W32 N20-N23
      4 1616 1325 (N11W45 L= 88)  1348    295        1 (1508/1216-1713/1404) -59.0 W39-W49 N02-N17
      5  259 1265 (N34E56 L=347)  2735    298        2 ( 163/1142- 321/1370) -24.4 E80-E47 N25-N41
      6 1243 1090 (N06W14 L= 57)   513    180        0 (1207/1040-1271/1172)  76.0 W10-W15 N03-N11
      7 1347 1152 (N08W22 L= 64)   212     56        0 (1313/1137-1381/1165)   0.0 W19-W23 N06-N08
      8  335  998 (N17E47 L=356)   937    222        0 ( 271/ 928- 417/1070) -42.3 E52-E40 N11-N21
      9  265  945 (N14E54 L=348)   737    123        1 ( 232/ 878- 286/ 994) -74.1 E57-E51 N10-N17
     10  598  908 (N08E28 L= 15)   834    160        2 ( 569/ 837- 634/ 983)  45.0 E31-E24 N03-N11
     11  373  678 (S03E50 L=353)  1502    318        1 ( 268/ 574- 497/ 737) -32.0 E59-E43 S10-N01
     12  928  602 (S16E14 L= 28)   380     82        2 ( 910/ 554- 948/ 651)  74.1 E15-E13 S19-S12
     13  463  414 (S21E55 L=347)   852    136        0 ( 407/ 393- 531/ 440)   0.0 E62-E47 S22-S19
     14  858  403 (S28E25 L= 18)   249     24        0 ( 839/ 386- 882/ 418)   0.0 E26-E23 S29-S26
     15  619  265 (S35E53 L=349)  1337    163        1 ( 545/ 228- 702/ 292)   7.1 E69-E43 S37-S33
  
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.