User Tools

Site Tools


en:socis2014

Differences

This shows you the differences between two versions of the page.

Link to this comparison view

Both sides previous revisionPrevious revision
Next revisionBoth sides next revision
en:socis2014 [2014/04/16 18:44] – [General purpose radio-astronomy station software] fluktuaciaen:socis2014 [2014/04/16 18:49] – [Solar flares detection station] fluktuacia
Line 68: Line 68:
 === Solar flares detection station === === Solar flares detection station ===
  
-Combination of radio-observer with the Basic radio astronomy station design gets opportunity to detect radio bursts exited by solar flares. These data are useful for Heliophysics. But Solar radio burst is weak compared to local man made noise and signal must be cleared before detection and classification. +Combination of radio-observer with the Basic radio astronomy station design brings opportunity to detect radio bursts exited by solar flares. These data are useful for Heliophysics. However, a solar radio burst is weak compared to the local man-made noise and signal must therefore be cleared of this noise before the detection and classification. 
  
 {{ :cs:designs:measuring:ionosphere.jpg?500 | Ionosphere measurement by SDRX01B}} {{ :cs:designs:measuring:ionosphere.jpg?500 | Ionosphere measurement by SDRX01B}}
en/socis2014.txt · Last modified: 2014/04/16 22:54 (external edit)