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--- en:algorithms [2019/04/11 17:15] – fluktuacia
+++ en:algorithms [2019/04/11 17:15] – [Data from DVB-T] fluktuacia
@@ Line 57: / Line 57: @@
 In case of positive detection, model parameters to calculate the replica have to be extracted from the signal.
-Calculation of path will be carried out using several methods. First is the [[https://en.wikipedia.org/wiki/Multilateration|multilateration]] based on different records’ time shifts on individual stations. Time shifts have to be obtained by time correlations of recorded data. This correlation can be carried out either in signal time-space or using Fourier transformations (?? Fourierov obraz). In both cases, it is first necessary to isolate the useful signal of meteor in the noise.
+Calculation of path will be carried out using several methods. First is the [[https://en.wikipedia.org/wiki/Multilateration|multilateration]] based on different records’ time shifts on individual stations. Time shifts have to be obtained by time correlations of recorded data. This correlation can be carried out either in signal time-space or using Fourier transformations. In both cases, it is first necessary to isolate the useful signal of meteor in the noise.
 Next step is a measurement of doppler parameters of meteor’s head-echo, which determines the inclination and speed of the path.
@@ Line 74: / Line 74: @@
   * Command assignment to individual stations.
-  * Start re-planing due to unsuccessful launch (??vypuštení) or rejection from station.
+  * Start re-planing due to unsuccessful launch or rejection from station.
   * Control of a potential violation of airspace and prohibited zones.