logo kso logo uni graz

20131107 - Filament data for 13 UTC
Available data for 20131107: »06 UTC   »07 UTC   »08 UTC   »09 UTC   »10 UTC   »11 UTC   »12 UTC   »13 UTC   »14 UTC  
Click on image to open sensitive map!
 
  Color  xc   yc  (LatLon LCarr)  Area Length Branches (  x0/y0     x1/y1  )  Tilt Location
      1 1239 1764 (N42W43 L=229)   432     61        0 (1214/1732-1266/1797)  12.5 W38-W47 N39-N43
      2  992 1670 (N43W18 L=205)   565    107        2 ( 957/1628-1042/1706)   6.3 W14-W23 N40-N44
      3 1311 1554 (N26W33 L=220)   239     75        1 (1275/1534-1346/1568)  -9.5 W29-W35 N25-N27
      4  455 1315 (N34E31 L=156)  1064    182        3 ( 392/1256- 531/1376)  18.4 E37-E24 N30-N36
      5 1011 1283 (N18W05 L=192)   421    119        0 ( 989/1214-1032/1342)  49.4 W02-W08 N14-N21
      6 1532 1285 (N06W37 L=224)   315     82        0 (1493/1267-1585/1300) -15.9 W33-W40 N04-N06
      7  192 1255 (N36E61 L=126)   513     43        0 ( 156/1241- 221/1270)  -5.2 E67-E56 N34-N37
      8 1878 1082 (S15W61 L=248)   590     85        1 (1855/1043-1901/1120)  31.0 W57-W64 S17-S13
      9 1906  952 (S24W64 L=250)  1846    129        2 (1872/ 908-1953/1007) -36.0 W58-W74 S27-S19
     10 1529  779 (S23W25 L=212)   360     71        0 (1509/ 734-1543/ 822) -90.0 W23-W25 S25-S19
     11  204  766 (N06E64 L=123)   593     61        0 ( 174/ 741- 234/ 792) -38.7 E67-E60 N04-N08
     12 1707  706 (S33W39 L=226)  1077    180        0 (1651/ 642-1745/ 790)  41.2 W33-W43 S36-S28
     13  851  700 (S10E18 L=169)   314     70        1 ( 822/ 674- 890/ 723) -45.0 E19-E15 S12-S08
     14  826  642 (S13E21 L=166)   214     41        0 ( 798/ 628- 855/ 658) -14.0 E22-E18 S14-S12
     15  500  292 (S28E66 L=121)   617     45        1 ( 475/ 263- 523/ 315)  63.4 E68-E62 S30-S26
  
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.