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20260831 - Filament data for 08 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  507 1529 (N50E31 L=308)   407    118        0 ( 459/1497- 554/1568)  15.3 E36-E25 N47-N51
      2 1156 1353 (N23W16 L=355)  1572    480        3 ( 976/1254-1328/1488) -55.7 W08-W23 N13-N35
      3 1819 1430 (N09W71 L= 50)   874     83        0 (1795/1398-1848/1467) -78.7 W68-W74 N06-N11
      4  657 1295 (N30E18 L=321)  1179    250        3 ( 591/1204- 746/1390) -60.3 E22-E13 N23-N37
      5 1825 1356 (N05W67 L= 46)   590     83        2 (1796/1326-1851/1385) -53.1 W62-W69 N03-N07
      6 1553 1267 (N09W38 L= 17)   830    120        1 (1529/1200-1574/1328)  69.4 W35-W40 N04-N12
      7  121 1078 (N24E75 L=264)   826     61        1 (  93/1052- 142/1105)  -9.5 E82-E70 N22-N25
      8 1805 1032 (S11W52 L= 31)   428     30        1 (1785/1011-1824/1057)  33.7 W50-W54 S13-S10
      9  307  876 (N11E51 L=288)   526    144        0 ( 271/ 811- 331/ 939) -69.4 E53-E49 N06-N14
     10  152  813 (N08E72 L=267)  1154     56        4 ( 114/ 791- 180/ 836)  -4.8 E81-E67 N06-N09
     11  681  758 (S02E26 L=313)   838    267        2 ( 627/ 648- 771/ 823)  45.0 E30-E19 S08-N01
     12 1220  615 (S21W03 L=342)   744    235        1 (1137/ 562-1340/ 676)   8.7 E02-W11 S23-S19
     13 1609  546 (S37W31 L= 10)   379     49        0 (1581/ 526-1633/ 570)   0.0 W28-W33 S38-S35
     14  590  486 (S17E41 L=298)   301     60        1 ( 569/ 458- 618/ 511)  26.6 E43-E37 S18-S15
     15 1280  439 (S35W03 L=342)  1539    317        0 (1145/ 356-1412/ 499)   5.4 E08-W13 S38-S32
  
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.