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20260826 - Filament data for 10 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 1066 1642 (N44W20 L= 64)   255     11        0 (1046/1626-1082/1664)  14.0 W18-W22 N42-N45
      2 1442 1519 (N26W41 L= 85)   412    122        1 (1384/1481-1496/1537)   0.0 W34-W45 N24-N27
      3 1329 1400 (N22W28 L= 72)   351    120        0 (1270/1382-1384/1413) -15.9 W23-W31 N20-N23
      4 1605 1317 (N11W44 L= 88)  1355    315        2 (1499/1202-1705/1402) -60.6 W38-W48 N01-N17
      5  250 1263 (N34E57 L=347)  2866    295        3 ( 157/1138- 313/1370) -23.8 E83-E48 N25-N40
      6 1328 1144 (N08W20 L= 64)   214     63        0 (1294/1127-1364/1157)   0.0 W17-W22 N06-N08
      7 1212 1058 (N05W11 L= 56)   525    161        2 (1149/1008-1254/1122)  35.5 W07-W14 N03-N08
      8  323  994 (N17E48 L=356)   933    217        0 ( 261/ 923- 405/1066) -39.8 E53-E41 N11-N21
      9 1039  963 (N03E00 L= 44)   207    106        0 (1000/ 931-1071/ 984) -45.0 E02-W01 N00-N04
     10  584  905 (N08E29 L= 15)   727    165        3 ( 553/ 840- 615/ 979)  49.4 E31-E25 N04-N11
     11  328  702 (S01E54 L=350)  1107    228        1 ( 256/ 634- 415/ 736) -26.6 E61-E47 S06-N01
     12  914  579 (S17E16 L= 28)   374     79        2 ( 881/ 536- 936/ 622)  63.4 E17-E13 S20-S14
     13  498  532 (S14E45 L=359)   309     48        0 ( 483/ 505- 520/ 561)  76.0 E46-E43 S15-S11
     14  446  411 (S21E57 L=347)   736    139        1 ( 394/ 392- 510/ 435)  -4.4 E63-E49 S22-S19
     15  611  264 (S35E55 L=349)  1271    174        1 ( 540/ 226- 690/ 292)   6.3 E71-E44 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.