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--- en:socis2014 [2014/04/16 18:41] – [Station maintenance software] fluktuacia
+++ en:socis2014 [2014/04/16 18:49] – [Solar flares detection station] fluktuacia
@@ Line 58: / Line 58: @@
 ==== General purpose radio-astronomy station software ====
-[[http://mlab-project.github.io/radio-observer/|radio-observer]] should be used for other radio astronomy measurements using our designs of Basic or Advanced radio astronomy stations or well known [[http://www.haystack.mit.edu/edu/undergrad/srt/index.html| Small Radio Telescope design]]
+[[http://mlab-project.github.io/radio-observer/|Radio-observer]] should be used for other radio astronomy measurements using our designs of Basic or Advanced radio astronomy stations or well known [[http://www.haystack.mit.edu/edu/undergrad/srt/index.html| Small Radio Telescope design]]
 == Knowledge prerequisites ==
   * Basic knowledge of signal analysis
-  * Good math skills, at least has to know what Fourier transform does.
+  * Good math skills, at least the knowledge what Fourier transform does.
-  * Knowledge of most used data structures and algorithms, networking and thread programming.
+  * Knowledge of the most frequently used data structures and algorithms, networking and thread programming.
 === 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}}