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Version 8 (MERIOCHAUD, Antoine, 12/13/2015 09:58 PM) → Version 9/43 (MERIOCHAUD, Antoine, 12/13/2015 10:07 PM)
h1. Report
h2. Introduction
Satellites are a quite new and growing way to improve different ways to communicate all over the world. In order to establish this communication, signals must be transmitted between a satellite and the ground station. To be readable on the two ways, these signals must comply some specifications and to check that this is the case, we can use for example a signal analyser.
Signal analyser
Assess quality of signals
Figure of merit, characteristics
h2. Scope and objectives
Labview
ni-USRP 2950 R : characteristics, block diagram
Antenna : Ku band, X-band ?
Satellites to target
Measurements to carry out : Analogic vs digital
h2. Implementation
h3. Definition of inputs and ways to compute the outputs
To be able to use the USRP, we first need to set it in LabView. We have to configure the device name (RIO0 with the PCI express card), the IQ sampling rate (twice the symbol rate), the carrier frequency and the antenna to use on the USRP. These parameters are really importants because if we put for example a wrong sampling rate, we will not be able to observe a good constellation.
Once we have our signal coming from the USRP, we have to compute the expected results. To observe the spectrum of the signal we just need to put the power spectrum block of LabView with the good parameters. This allows us to compute the power of the signal and the power of the noise. Indeed if we set the carrier frequency of the USRP centered on our signal, we just have to do a peak detection to measure the power of the signal plus the noise. Then we have the power of the noise in taking a carrier frequency completely out the bandwidth of the satellite. Now we have the power of the noise and the power of the signal so we can easily compute the signal to noise ratio (SNR).
Now, let's have a look to digital results. We want to observe the constellation of the signal and some results like mean error vector magnitude or mean phase error. Our signal analyser does not determine automatically what is the constellation used to transmit the signal, we have to know it before and to enter it in the program as a parameter. Then we can observe the received constellation, the mean error vector magnitude, the mean phase error, and the mean magnitude error. <warning>mettre schéma du calcul</warning>
h3. Simulation
First we decided to design our signal analyser and to test it with simulated signals generated automatically such as sine wave.
To do this we first created a VI able to generate a noisy signal. This signal correspond to the addition of three basic signals and a white Gaussian noise. For each basic signal we can set the signal type, the frequency, the amplitude and the offset. For the noise, we can set the noise standard deviation.
Consequently we can insert the noisy signal into our signal analyser to test it.
For example if we set 3 sine waves with different frequencies and amplitudes we observe this spectrum <warning>mettre photo</warning>
We can also observe the spectrum of a noisy sine wave <warning>mettre photo</warning>
In the two cases, the spectrum match with the expected values (frequencies and amplitudes)
h3. Moving from simulation to acquisition of real signals
To replace the generated signal by a real signal received by an antenna, we first need to set the USRP and
Definition of inputs and computation models of the outputs
Simulation
Generation of a noisy signal + analogic and digital measurements ⇒ do the results match what is expected ?
Expected issues when we move to the acquisition of the real signal ?
h2. Tests and results
Explanation of the commands and operations to reach the presented results + comparison between what is display by the signal analyser and by Labview + explanations
h2. Introduction
Satellites are a quite new and growing way to improve different ways to communicate all over the world. In order to establish this communication, signals must be transmitted between a satellite and the ground station. To be readable on the two ways, these signals must comply some specifications and to check that this is the case, we can use for example a signal analyser.
Signal analyser
Assess quality of signals
Figure of merit, characteristics
h2. Scope and objectives
Labview
ni-USRP 2950 R : characteristics, block diagram
Antenna : Ku band, X-band ?
Satellites to target
Measurements to carry out : Analogic vs digital
h2. Implementation
h3. Definition of inputs and ways to compute the outputs
To be able to use the USRP, we first need to set it in LabView. We have to configure the device name (RIO0 with the PCI express card), the IQ sampling rate (twice the symbol rate), the carrier frequency and the antenna to use on the USRP. These parameters are really importants because if we put for example a wrong sampling rate, we will not be able to observe a good constellation.
Once we have our signal coming from the USRP, we have to compute the expected results. To observe the spectrum of the signal we just need to put the power spectrum block of LabView with the good parameters. This allows us to compute the power of the signal and the power of the noise. Indeed if we set the carrier frequency of the USRP centered on our signal, we just have to do a peak detection to measure the power of the signal plus the noise. Then we have the power of the noise in taking a carrier frequency completely out the bandwidth of the satellite. Now we have the power of the noise and the power of the signal so we can easily compute the signal to noise ratio (SNR).
Now, let's have a look to digital results. We want to observe the constellation of the signal and some results like mean error vector magnitude or mean phase error. Our signal analyser does not determine automatically what is the constellation used to transmit the signal, we have to know it before and to enter it in the program as a parameter. Then we can observe the received constellation, the mean error vector magnitude, the mean phase error, and the mean magnitude error. <warning>mettre schéma du calcul</warning>
h3. Simulation
First we decided to design our signal analyser and to test it with simulated signals generated automatically such as sine wave.
To do this we first created a VI able to generate a noisy signal. This signal correspond to the addition of three basic signals and a white Gaussian noise. For each basic signal we can set the signal type, the frequency, the amplitude and the offset. For the noise, we can set the noise standard deviation.
Consequently we can insert the noisy signal into our signal analyser to test it.
For example if we set 3 sine waves with different frequencies and amplitudes we observe this spectrum <warning>mettre photo</warning>
We can also observe the spectrum of a noisy sine wave <warning>mettre photo</warning>
In the two cases, the spectrum match with the expected values (frequencies and amplitudes)
h3. Moving from simulation to acquisition of real signals
To replace the generated signal by a real signal received by an antenna, we first need to set the USRP and
Definition of inputs and computation models of the outputs
Simulation
Generation of a noisy signal + analogic and digital measurements ⇒ do the results match what is expected ?
Expected issues when we move to the acquisition of the real signal ?
h2. Tests and results
Explanation of the commands and operations to reach the presented results + comparison between what is display by the signal analyser and by Labview + explanations