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20260104 - Filament data for 12 UTC
Available data for 20260104: »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 1346 1755 (N46W28 L=281)   523     92        1 (1296/1742-1404/1774)  -5.7 W23-W33 N45-N47
      2 1148 1640 (N36W09 L=262)   930    146        3 (1078/1585-1209/1678) -33.7 W03-W12 N32-N38
      3 1437 1492 (N26W28 L=281)   272     81        1 (1396/1470-1476/1511) -18.4 W24-W30 N24-N27
      4  287 1303 (N14E52 L=201)  2177    406        2 ( 192/1183- 386/1485) -32.8 E75-E41 N06-N26
      5 1689 1139 (N05W43 L=296)   247     58        0 (1660/1112-1718/1172)  31.0 W40-W45 N03-N06
      6 1577  980 (S05W35 L=288)   309     97        0 (1532/ 938-1614/1005)  33.7 W31-W37 S07-S03
      7 1616  921 (S08W38 L=291)   449     76        1 (1571/ 902-1666/ 937)   8.1 W34-W41 S09-S07
      8 1625  832 (S14W40 L=293)  1197    221        5 (1569/ 740-1686/ 907)  59.0 W35-W43 S19-S09
      9 1177  742 (S20W10 L=263)   926    283        0 (1151/ 618-1201/ 876)  86.4 W08-W11 S27-S11
     10  902  789 (S17E07 L=246)   343    118        1 ( 854/ 749- 945/ 830)  39.8 E10-E04 S19-S14
     11  317  768 (S18E50 L=203)   442     79        0 ( 290/ 741- 335/ 808)  45.0 E52-E47 S19-S15
     12  269  616 (S27E60 L=193)  2158    326        3 ( 214/ 519- 308/ 773)  79.4 E67-E55 S33-S17
     13 1320  313 (S50W29 L=282)   483    100        1 (1276/ 283-1370/ 345) -21.0 W23-W36 S52-S47
     14 1305  198 (S61W38 L=291)   531     27        0 (1283/ 172-1327/ 224) -22.6 W32-W44 S63-S58
     15  684  160 (S66E56 L=197)   793     59        1 ( 660/ 131- 713/ 183)   7.9 E80-E44 S68-S62
  
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.