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20260210 - Filament data for 14 UTC
Available data for 20260210: »07 UTC   »08 UTC   »09 UTC   »10 UTC   »14 UTC  
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  Color  xc   yc  (LatLon LCarr)  Area Length Branches (  x0/y0     x1/y1  )  Tilt Location
      1 1212 1613 (N33W01 L=125)   507     85        1 (1188/1565-1238/1649) -63.4 E01-W02 N29-N35
      2  308 1501 (N12E60 L= 64)  2632    244       11 ( 233/1406- 376/1591)  63.4 E68-E55 N05-N18
      3 1393 1512 (N30W15 L=139)  1422    291        3 (1276/1421-1500/1586) -15.5 W05-W23 N25-N33
      4 1403 1132 (N06W20 L=145)  1226    353        0 (1251/1050-1530/1219) -11.3 W09-W29 N04-N08
      5  136 1148 (S11E69 L= 56)  1868    147        4 (  81/1100- 190/1195)   6.3 E79-E61 S13-S07
      6 1839 1128 (N16W54 L=178)   329     43        1 (1811/1107-1859/1146)   0.0 W50-W56 N15-N17
      7 1931 1071 (N16W67 L=191)  2069    166        7 (1883/1015-1976/1118) -13.0 W59-W77 N13-N19
      8  608 1022 (S13E25 L=100)   407    125        0 ( 557/ 979- 660/1058)  50.2 E27-E21 S16-S10
      9 1749 1033 (N08W46 L=171)   271     40        0 (1730/1014-1771/1052)  45.0 W44-W48 N07-N09
     10  772  947 (S15E14 L=111)   343    110        0 ( 711/ 922- 821/ 977)  29.7 E17-E10 S17-S12
     11 1634  797 (S07W42 L=167)   687    131        1 (1579/ 741-1676/ 834)  -6.3 W38-W47 S09-S04
     12  708  701 (S31E15 L=110)  1414    359        0 ( 559/ 636- 883/ 760)  30.6 E25-E03 S37-S24
     13 1700  568 (S18W58 L=182)   600    116        0 (1681/ 533-1729/ 620) -59.0 W54-W61 S19-S14
     14  396  592 (S43E42 L= 82)   403     26        1 ( 372/ 570- 422/ 612)  31.0 E45-E39 S44-S41
     15 1354  444 (S34W37 L=161)  1700    333        5 (1219/ 346-1484/ 524)  62.1 W31-W42 S43-S26
     16 1739  442 (S23W74 L=198)  1175    102        3 (1707/ 399-1784/ 468)  50.2 W69-W81 S26-S20
  
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.