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20260308 - Filament data for 13 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  713 1830 (N35E51 L= 92)  1646    166        2 ( 651/1774- 787/1870)   0.0 E61-E44 N30-N37
      2  766 1771 (N31E41 L=101)   333     24        0 ( 747/1749- 784/1794) -63.4 E43-E39 N29-N33
      3  582 1626 (N17E45 L= 98)   673     69        0 ( 549/1600- 628/1651)   9.5 E47-E41 N15-N19
      4  277 1524 (N06E68 L= 75)   976     91        7 ( 233/1487- 309/1557)  18.4 E73-E63 N03-N08
      5  880 1314 (N05E15 L=128)   709    292        1 ( 807/1215- 980/1425)  75.1 E16-E12 S01-N14
      6 1720 1211 (N23W39 L=181)   980    160        0 (1659/1175-1775/1241)  21.8 W34-W44 N19-N25
      7 1868  991 (N15W58 L=200)  2030    297        5 (1824/ 877-1900/1153) -45.0 W51-W64 N09-N23
      8 1751 1000 (N12W45 L=188)  1122    222        0 (1700/ 916-1777/1113)  90.0 W42-W47 N05-N18
      9  654 1058 (S14E22 L=121)   457     80        1 ( 626/1019- 683/1095) -63.4 E24-E19 S16-S11
     10 1599  941 (N04W35 L=178)   501    140        1 (1549/ 912-1645/ 983)   8.1 W31-W38 N02-N05
     11 1408  887 (S05W25 L=168)   497    154        1 (1388/ 815-1435/ 953) -69.4 W23-W27 S08-N00
     12  332  835 (S34E44 L= 99)  1974    320        2 ( 185/ 779- 476/ 887)  15.3 E63-E30 S39-S28
     13 1120  722 (S21W14 L=156)   351    140        0 (1049/ 708-1188/ 738)  20.6 W09-W17 S23-S19
     14 1552  485 (S21W51 L=194)   345     96        0 (1518/ 453-1574/ 535) -68.2 W49-W53 S23-S18
     15  734  484 (S47E04 L=139)   265     38        0 ( 715/ 464- 762/ 503)   0.0 E05-E01 S48-S45
     16 1619  451 (S21W59 L=202)   678    107        3 (1581/ 414-1659/ 499) -71.6 W56-W63 S23-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.