logo kso logo uni graz

20140307 - Filament data for 14 UTC
Available data for 20140307: »07 UTC   »08 UTC   »09 UTC   »10 UTC   »11 UTC   »12 UTC   »13 UTC   »14 UTC   »15 UTC  
Click on image to open sensitive map!
 
  Color  xc   yc  (LatLon LCarr)  Area Length Branches (  x0/y0     x1/y1  )  Tilt Location
      1 1224 1369 (N17W03 L= 48)   219     88        2 (1196/1332-1245/1405) -36.9 W00-W04 N15-N19
      2  329 1178 (S13E48 L=357)  1323    258        4 ( 277/1078- 396/1237)  63.4 E53-E43 S19-S09
      3 1817 1046 (N16W51 L= 96)   767    157        3 (1787/ 971-1844/1123) -45.0 W47-W55 N12-N20
      4  691 1022 (S15E19 L= 26)   569    217        1 ( 636/ 925- 745/1118) -45.0 E24-E14 S19-S10
      5 1384  949 (S02W22 L= 68)   996    230        1 (1291/ 898-1486/1027)   0.0 W14-W29 S04-N00
      6 1879  987 (N15W59 L=104)   579    146        2 (1849/ 963-1904/1020)  68.2 W55-W61 N13-N18
      7  880  881 (S19E05 L= 41)   180     34        0 ( 868/ 852- 891/ 907) -56.3 E05-E03 S20-S17
      8 1790  818 (N03W55 L=101)   942    147        1 (1762/ 743-1820/ 887) -60.3 W52-W59 S01-N07
      9  424  829 (S32E35 L= 11)  1107    325        0 ( 295/ 801- 545/ 856)  10.8 E46-E25 S35-S29
     10 1199  702 (S21W19 L= 64)   251     92        0 (1147/ 686-1250/ 715)  26.6 W16-W22 S22-S19
     11 1455  656 (S16W36 L= 81)   567    208        0 (1360/ 631-1550/ 694)  28.6 W29-W40 S18-S11
     12 1726  580 (S11W60 L=106)   498     52        0 (1701/ 550-1752/ 609)  78.7 W58-W62 S13-S08
     13 1664  569 (S14W55 L=101)   344     47        1 (1638/ 548-1686/ 597)  90.0 W53-W57 S15-S12
     14 1161  543 (S31W23 L= 68)   595    125        0 (1090/ 519-1234/ 569)  36.9 W18-W26 S33-S27
     15 1678  500 (S17W60 L=106)  2520    422        6 (1586/ 450-1771/ 560)  47.5 W54-W69 S22-S10
  
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.