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20260308 - Filament data for 12 UTC
Available data for 20260308: »06 UTC   »07 UTC   »08 UTC   »09 UTC   »10 UTC   »11 UTC   »12 UTC   »13 UTC   »14 UTC   »15 UTC  
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  Color  xc   yc  (LatLon LCarr)  Area Length Branches (  x0/y0     x1/y1  )  Tilt Location
      1  718 1819 (N34E49 L= 94)  1734    187        2 ( 649/1756- 776/1870) -15.3 E62-E40 N29-N37
      2  983 1699 (N32E23 L=121)   322     70        0 ( 944/1678-1025/1718)   9.5 E25-E19 N30-N32
      3  545 1618 (N16E47 L= 96)   843    123        0 ( 479/1594- 605/1637)  26.6 E51-E42 N13-N17
      4  927 1399 (N11E15 L=128)   284     72        0 ( 899/1369- 966/1429)  63.4 E15-E13 N09-N13
      5  836 1260 (N01E16 L=127)   428     87        0 ( 803/1221- 861/1306)  78.7 E17-E14 S01-N04
      6 1715 1215 (N23W38 L=182)   969    147        0 (1652/1185-1777/1243)  20.0 W33-W44 N18-N24
      7 1744 1007 (N12W45 L=188)  1143    294        0 (1693/ 919-1773/1165)  90.0 W42-W47 N05-N21
      8 1866  994 (N15W57 L=200)  2087    287        5 (1827/ 878-1905/1156) -45.0 W51-W65 N09-N23
      9  646 1061 (S14E23 L=121)   494    102        2 ( 619/1021- 677/1101)  90.0 E24-E20 S16-S11
     10 1591  942 (N03W35 L=178)   484    126        1 (1544/ 916-1637/ 981)   7.1 W30-W38 N01-N05
     11 1399  892 (S05W24 L=167)   484    142        1 (1378/ 820-1426/ 955) -69.4 W22-W26 S08-N00
     12  325  836 (S34E44 L= 99)  1973    322        2 ( 181/ 778- 469/ 888)  15.7 E63-E31 S39-S28
     13 1119  725 (S21W13 L=157)   363    142        0 (1048/ 712-1186/ 740)  20.6 W09-W17 S23-S19
     14 1466  614 (S17W38 L=181)   255     52        2 (1438/ 594-1498/ 638)  26.6 W36-W40 S18-S15
     15 1547  490 (S21W51 L=194)   304     97        1 (1513/ 457-1572/ 542) -80.5 W48-W52 S23-S17
     16  728  487 (S47E04 L=139)   236     36        0 ( 710/ 471- 755/ 505)  45.0 E06-E02 S48-S45
     17 1614  452 (S21W59 L=202)   696    128        3 (1567/ 416-1657/ 504) -81.9 W55-W62 S24-S17
  
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.