logo kso logo uni graz

20150618 - Latest Filament data
Available data for 20150618: »13 UTC  
Click on image to open sensitive map!
 
  Color  xc   yc  (LatLon LCarr)  Area Length Branches (  x0/y0     x1/y1  )  Tilt Location
      1  829 1448 (N26E18 L=330)  2280    591        4 ( 615/1291-1013/1615) -24.6 E38-E03 N17-N35
      2 1277 1494 (N34W13 L=  1)   237     55        0 (1244/1472-1304/1511) -26.6 W10-W15 N32-N34
      3  507 1298 (N13E37 L=310)   358    116        2 ( 459/1242- 536/1350)  66.8 E39-E35 N09-N16
      4 1701 1206 (N19W46 L= 33)  2867    579        7 (1526/1030-1795/1345) -36.0 W31-W54 N08-N26
      5  993 1187 (N11E04 L=344)   442    134        0 ( 954/1136-1047/1243) -45.0 E06-W00 N08-N14
      6 1754  869 (S02W53 L= 41)   309     91        0 (1717/ 854-1786/ 884)   8.1 W49-W56 S02-N00
      7 1449  746 (S12W30 L= 18)   633    163        5 (1390/ 712-1510/ 785) -11.3 W25-W35 S13-S09
      8 1613  762 (S09W42 L= 30)   337    140        1 (1554/ 747-1666/ 778)  12.5 W37-W46 S10-S08
  
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.