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20260108 - Filament data for 08 UTC
Available data for 20260108: »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 1705 1634 (N39W61 L=263)   637     73        1 (1676/1611-1739/1656)   9.5 W54-W66 N37-N41
      2  715 1540 (N28E23 L=180)   245     41        2 ( 689/1519- 748/1557)   0.0 E24-E20 N26-N28
      3  922 1441 (N21E08 L=194)   630    193        1 ( 839/1401-1018/1477) -14.0 E13-E01 N18-N23
      4  633 1385 (N17E26 L=176)   368     87        1 ( 605/1342- 662/1437) -56.3 E28-E23 N14-N20
      5 1832 1267 (N15W58 L=260)   405     54        1 (1810/1249-1853/1291)  21.8 W55-W60 N13-N16
      6 1736 1203 (N10W47 L=249)   298     68        1 (1718/1169-1751/1237) -76.0 W45-W48 N07-N11
      7  180 1180 (N05E62 L=140)   486     97        1 ( 135/1162- 221/1207)  11.3 E67-E57 N04-N06
      8  446  990 (S07E37 L=165)   705    157        3 ( 383/ 918- 494/1044) -45.0 E41-E33 S10-S03
      9  902  866 (S14E07 L=195)   480    153        0 ( 877/ 801- 941/ 916)  74.1 E08-E04 S17-S10
     10  725  560 (S33E20 L=182)  4219    811       10 ( 557/ 446- 951/ 801) -43.5 E31-E03 S40-S17
     11 1606  724 (S19W40 L=243)   885    264        0 (1501/ 637-1708/ 798)  40.2 W34-W47 S25-S14
     12 1824  732 (S17W61 L=263)   533    106        0 (1798/ 684-1849/ 786)  74.1 W59-W62 S20-S13
     13 1701  501 (S33W59 L=261)   805    103        2 (1660/ 471-1746/ 528)  12.5 W53-W63 S34-S30
     14 1112  416 (S42W09 L=211)   520     83        2 (1064/ 402-1161/ 437)  15.9 W05-W13 S43-S40
     15  569  351 (S49E42 L=161)   740     99        1 ( 523/ 326- 627/ 379)  -4.8 E46-E34 S50-S46
     16  821  154 (S69E28 L=174)   806     78        1 ( 780/ 132- 853/ 185)  15.9 E40-E19 S71-S64
  
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.