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--- en:socis2014 [2014/04/16 18:49] – [Solar flares detection station] fluktuacia
+++ en:socis2014 [Unknown date] (current) – external edit (Unknown date) 127.0.0.1
@@ Line 82: / Line 82: @@
 === Cubesat automatic reception station ===
-Scalable design of our [[en:sdrx|software defined receiver]] gives opportunity to use multiple antenna  array for signal reception from Cubesat  satellites.  Cubesat development teams around the word are limited by signal reception from its home station or by volunteers which contributes by received data sets.
+Scalable design of our [[en:sdrx|software defined receiver]] gives opportunity to use multiple antenna array for signal reception from Cubesat satellites.  Cubesat development teams around the word are limited by signal reception from their home stations or by volunteers who contribute by received data sets.
-This amateur LEO satellite reception methods can be easily improved by use of multiple fixed antenna array and beam-forming algorithm on reception station.
+These amateur LEO satellite reception methods can easily be improved by the use of multiple fixed antenna array and beam-forming algorithm on reception station.
 {{ :cs:designs:measuring:arissat1.jpg?300 | A SSTV image taken from ARISSAT1 by SDRX01A }}
@@ Line 96: / Line 96: @@
 ==== Video meteor detection system ====
-Several projects of visual meteor detection software currently exist. But neither is open-source and all these softwares were poor results and big false positive detection rates. We need a quality video meteor detection system for evaluation our radio meteor detection metods.
+Several projects of visual meteor detection software currently exist. But neither is open-source and all of them have poor results and large false positive detection rates. We need a high quality video meteor detection system for evaluation of our radio meteor detection metods.
-Video data will be collected by our design of [[cs:vmds|visual meteor detection station (VMDS01A)]] in our project. Meteor trails must be detected in these video data in real-time. Meteor trails must be interpreted in physical context (meteoroid explosions, trail clouds coveradge, etc.). After this, geometric parameters can be delivered and orbit parameters can be calculated.
+Video data will be collected by our design of [[cs:vmds|visual meteor detection station (VMDS01A)]] (part of our project). Meteor trails within these video data have to be detected in real-time. Meteor trails must be interpreted in physical context (meteoroid explosions, trail clouds coveradge, etc.). Following this, geometric parameters can be delivered and orbit parameters can be calculated.
 {{ :cs:designs:measuring:meteor_trail.png?500 | A meteor trail captured by VMDS01A }}