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20260829 - Filament data for 12 UTC
Available data for 20260829: »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  387 1509 (N50E46 L=317)   593    105        1 ( 339/1478- 441/1536)   8.7 E53-E39 N48-N51
      2  619 1398 (N38E20 L=343)  1772    460        2 ( 438/1298- 782/1457) -29.7 E37-E09 N28-N44
      3 1758 1381 (N09W60 L= 63)  1145    122        3 (1695/1351-1813/1415) -28.6 W54-W66 N06-N12
      4  369 1239 (N32E43 L=321)  1104    277        2 ( 339/1120- 423/1355) -69.4 E46-E37 N23-N39
      5 1628 1200 (N03W42 L= 45)   422    155        0 (1561/1165-1668/1223) -23.2 W36-W44 N00-N04
      6  887 1148 (N17E06 L=358)   645    247        3 ( 773/1083- 973/1191) -39.3 E12-E01 N11-N21
      7 1220 1106 (N08W13 L= 16)   624    150        1 (1191/1033-1242/1181)  63.4 W10-W15 N03-N11
      8  755 1049 (N14E15 L=348)   310    137        0 ( 728/ 987- 778/1098) -90.0 E16-E14 N10-N17
      9 1809 1034 (S11W53 L= 56)   452     18        1 (1786/1013-1832/1057) -36.9 W50-W55 S12-S09
     10  639  923 (N08E25 L=338)   207     52        0 ( 612/ 910- 669/ 942) -33.7 E26-E23 N07-N09
     11  315  884 (N11E50 L=313)   358     58        0 ( 300/ 849- 327/ 920)  68.2 E51-E48 N08-N13
     12  379  695 (S01E49 L=314)   879    139        2 ( 323/ 646- 436/ 732)  14.0 E56-E44 S03-N00
     13 1426  574 (S29W16 L= 19)   242     46        0 (1401/ 553-1446/ 594)  33.7 W14-W17 S30-S27
     14  928  520 (S21E17 L=346)   544    105        1 ( 877/ 497- 982/ 549)   0.0 E20-E12 S22-S19
     15  723  453 (S22E32 L=331)  1147    271        1 ( 634/ 410- 839/ 494) -24.8 E37-E24 S25-S17
     16  976  339 (S35E21 L=343)  1489    275        1 ( 869/ 276-1112/ 385)   7.8 E31-E09 S37-S32
  
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.