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20251123 - Filament data for 09 UTC
Available data for 20251123: »07 UTC   »08 UTC   »09 UTC   »10 UTC   »11 UTC   »12 UTC   »13 UTC  
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  Color  xc   yc  (LatLon LCarr)  Area Length Branches (  x0/y0     x1/y1  )  Tilt Location
      1  705 1795 (N61E08 L= 79)   509     80        0 ( 668/1762- 734/1832)  35.5 E13-E04 N58-N64
      2  561 1768 (N63E30 L= 58)  1011    124        0 ( 520/1731- 610/1791)  -7.6 E37-E20 N59-N66
      3  886 1732 (N50W08 L= 95)   577    142        1 ( 829/1682- 949/1779)  17.1 W01-W14 N46-N52
      4 1010 1717 (N45W17 L=105)   422     48        1 ( 991/1684-1038/1747)  51.3 W14-W18 N42-N47
      5  854 1514 (N34E01 L= 87)   340     96        0 ( 808/1478- 895/1543) -59.0 E03-W01 N31-N36
      6  391 1417 (N37E39 L= 49)   377     68        0 ( 352/1394- 431/1442) -24.0 E43-E34 N35-N39
      7  494 1099 (N16E31 L= 57)   347    116        0 ( 457/1060- 529/1149)  33.7 E34-E28 N13-N17
      8  248 1107 (N20E52 L= 36)   345     38        2 ( 226/1083- 268/1129)  56.3 E54-E49 N18-N21
      9 1720  913 (S18W43 L=131)   430    108        1 (1676/ 891-1781/ 935)   0.0 W39-W48 S18-S16
     10 1657  701 (S30W37 L=125)  1649    389        0 (1543/ 589-1773/ 854)  31.0 W27-W47 S35-S22
     11 1234  729 (S19W07 L= 95)   291     92        1 (1219/ 695-1258/ 785) -90.0 W05-W07 S21-S15
     12 1245  626 (S26W06 L= 94)   209     78        0 (1210/ 603-1278/ 655)  21.8 W03-W08 S26-S24
     13  731  589 (S18E27 L= 61)   681    174        1 ( 657/ 516- 777/ 644) -73.3 E29-E24 S23-S13
     14  390  545 (S15E53 L= 35)  1124    196        2 ( 348/ 470- 429/ 629)  78.7 E57-E50 S19-S09
     15  323  534 (S14E61 L= 27)  1476    188        3 ( 267/ 466- 355/ 613) -84.3 E65-E56 S18-S08
  
Data will be available after one hour of observations. 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.