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20260831 - Filament data for 09 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  510 1530 (N50E31 L=308)   451    115        0 ( 458/1497- 558/1569)  15.3 E36-E25 N47-N51
      2 1054 1446 (N31W12 L=351)   433     93        2 (1008/1415-1094/1479) -51.3 W10-W14 N29-N34
      3 1824 1396 (N07W69 L= 48)  1356    195        3 (1797/1332-1853/1467)  63.4 W63-W75 N03-N11
      4  662 1300 (N31E18 L=321)  1139    252        3 ( 599/1209- 751/1397) -59.0 E21-E12 N23-N38
      5 1232 1305 (N19W19 L=357)  1030    258        1 (1124/1251-1355/1353) -45.0 W13-W25 N12-N23
      6 1559 1269 (N09W39 L= 17)   836    128        1 (1534/1203-1581/1332)  69.4 W36-W41 N04-N12
      7  123 1075 (N24E74 L=265)   813     45        2 (  94/1050- 145/1096)  -4.4 E82-E69 N22-N25
      8 1804 1028 (S12W52 L= 31)   506     54        0 (1783/ 994-1825/1055)  45.0 W50-W54 S13-S10
      9  313  877 (N11E51 L=288)   504    138        0 ( 277/ 814- 337/ 937) -69.4 E53-E49 N06-N14
     10  152  814 (N08E72 L=266)  1071     63        4 ( 115/ 793- 180/ 837) -10.3 E81-E67 N06-N09
     11  685  762 (S01E25 L=313)   767    217        1 ( 635/ 668- 751/ 825)  37.9 E29-E20 S06-N01
     12 1227  617 (S21W03 L=342)   759    250        2 (1147/ 558-1351/ 682)  12.1 E02-W12 S23-S19
     13 1615  550 (S37W31 L= 10)   367     39        0 (1589/ 533-1640/ 567)   0.0 W28-W33 S38-S35
     14  596  484 (S17E40 L=298)   319     54        0 ( 575/ 455- 627/ 511)  31.0 E42-E37 S18-S15
     15 1291  442 (S35W04 L=342)  1518    305        1 (1159/ 358-1419/ 503)   8.1 E07-W14 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.