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20251223 - Filament data for 10 UTC
Available data for 20251223: »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  350 1430 (N27E47 L=  5)  1409    203        2 ( 252/1397- 455/1466)  -7.4 E60-E37 N24-N30
      2  449 1266 (N16E36 L= 16)   285     92        2 ( 415/1225- 477/1298) -45.0 E39-E33 N13-N18
      3 1827 1264 (N09W59 L=111)   392     14        0 (1810/1242-1845/1285)  56.3 W56-W61 N07-N10
      4  424 1187 (N11E38 L= 14)   287     64        0 ( 407/1159- 442/1232)  90.0 E38-E36 N09-N14
      5  378 1120 (N08E41 L= 11)   409    100        2 ( 345/1086- 424/1141)   9.5 E43-E37 N05-N08
      6  469 1052 (N03E35 L= 17)   505    123        0 ( 417/1017- 500/1101)  38.7 E38-E32 N01-N05
      7  296 1037 (N03E48 L=  4)   470     86        0 ( 276/ 993- 317/1087) -80.5 E50-E46 N00-N06
      8  236  779 (S11E58 L=354)  2594    325       14 ( 181/ 647- 299/ 908) -82.9 E64-E54 S19-S03
      9  417  816 (S11E41 L= 11)   850    214        3 ( 332/ 768- 475/ 901)  28.3 E48-E35 S13-S05
     10  327  711 (S16E51 L=  1)   861    164        3 ( 294/ 629- 351/ 783)  84.3 E53-E48 S21-S11
     11  694  718 (S18E23 L= 29)   264     84        0 ( 652/ 694- 738/ 745)  18.4 E25-E19 S19-S16
     12  842  636 (S24E14 L= 38)   974    222        3 ( 737/ 572- 929/ 690)  23.2 E22-E08 S27-S21
     13 1836  619 (S30W67 L=119)   574     68        0 (1799/ 603-1875/ 634)  10.3 W61-W74 S31-S29
     14  244  533 (S26E71 L=341)  1031    126        0 ( 207/ 511- 289/ 568)   3.0 E81-E62 S27-S24
     15 1621  425 (S43W50 L=102)   846    101        1 (1576/ 396-1663/ 469)  59.0 W44-W55 S45-S40
  
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.