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20260831 - Filament data for 05 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 1014 1443 (N32W09 L=350)   469    119        1 ( 947/1403-1060/1483) -50.2 W06-W12 N28-N35
      2 1812 1422 (N09W70 L= 50)  1183    113        0 (1786/1376-1847/1468) -90.0 W66-W73 N05-N11
      3 1536 1278 (N10W37 L= 18)  1003    201        2 (1506/1191-1558/1389)  57.5 W34-W42 N04-N15
      4  635 1290 (N31E20 L=321)  1010    225        3 ( 574/1209- 719/1380) -58.4 E23-E14 N24-N37
      5 1822 1346 (N05W66 L= 46)   708     73        1 (1792/1316-1848/1376) -59.0 W63-W69 N02-N07
      6 1200 1292 (N19W17 L=357)   948    271        0 (1094/1234-1322/1340) -45.0 W11-W22 N12-N23
      7  116 1081 (N24E76 L=264)   885     66        1 (  92/1053- 138/1108)  16.7 E84-E71 N22-N26
      8 1807 1037 (S11W53 L= 34)   491     39        1 (1785/1010-1825/1061)  11.3 W50-W55 S13-S09
      9  300  860 (N10E52 L=288)   420    121        0 ( 277/ 803- 321/ 913) -74.1 E53-E51 N06-N13
     10  142  820 (N09E74 L=266)  1562     99        2 ( 104/ 792- 173/ 857) -14.0 E84-E68 N06-N10
     11  667  765 (S01E27 L=314)   723    216        1 ( 604/ 696- 761/ 823)  14.0 E32-E20 S04-N01
     12 1201  609 (S21W02 L=342)   728    234        0 (1115/ 557-1315/ 669)   8.7 E04-W09 S23-S19
     13 1590  538 (S37W29 L= 10)   306     42        0 (1565/ 521-1614/ 553)   0.0 W26-W31 S38-S35
     14  463  500 (S14E50 L=290)   358     44        1 ( 443/ 470- 480/ 526)  76.0 E51-E48 S16-S12
     15 1262  432 (S35W02 L=342)  1549    316        0 (1131/ 347-1392/ 492)   8.1 E09-W12 S38-S33
  
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.