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20260831 - Filament data for 13 UTC
Available data for 20260831: »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  755 1497 (N42E07 L=329)   232     42        0 ( 736/1470- 776/1521)  26.6 E09-E05 N39-N42
      2  998 1502 (N36W10 L=347)   240     97        0 ( 955/1480-1048/1518) -38.7 W07-W13 N33-N37
      3 1095 1448 (N30W15 L=351)   222     26        1 (1077/1425-1118/1473)  56.3 W13-W16 N28-N31
      4  694 1306 (N30E15 L=321)  1080    243        2 ( 627/1213- 780/1392) -60.3 E19-E10 N23-N37
      5 1266 1317 (N18W21 L=358)  1326    284        2 (1155/1243-1386/1384) -52.4 W15-W26 N11-N24
      6 1586 1282 (N09W41 L= 17)   822    112        2 (1558/1222-1607/1342)  74.1 W38-W43 N05-N12
      7  133 1075 (N24E72 L=264)   779     48        1 ( 108/1053- 159/1096) -11.3 E77-E66 N22-N25
      8 1811 1031 (S12W53 L= 29)   562     31        1 (1784/1001-1831/1057) -90.0 W50-W55 S13-S10
      9  324  901 (N12E49 L=287)   656    164        1 ( 268/ 825- 365/ 965) -56.3 E53-E46 N07-N16
     10  723  775 (S01E23 L=313)   707    172        1 ( 669/ 706- 791/ 832)  24.0 E27-E17 S04-N01
     11 1262  631 (S21W06 L=342)   741    241        1 (1183/ 579-1384/ 695)   8.1 W00-W14 S23-S19
     12 1630  552 (S37W33 L=  9)   378     33        1 (1608/ 529-1653/ 575) -51.3 W30-W35 S39-S34
     13  508  511 (S14E46 L=290)   283     45        0 ( 494/ 488- 524/ 538)  45.0 E47-E43 S15-S12
     14 1330  460 (S35W07 L=343)  1340    258        0 (1223/ 393-1445/ 521)   6.7 E01-W16 S37-S32
     15  623  491 (S17E38 L=298)   313     65        0 ( 599/ 460- 653/ 517)  31.0 E40-E34 S18-S15
  
Download FITS filament maps as tar archive

» All Filament Data of 20260831 ...
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.