30. Spectrum Module¶

The Spectrum module aims at providing support for modeling the frequency-dependent aspects of communications in ns-3. The model was first introduced in [Baldo2009Spectrum], and has been enhanced and refined over the years.

_images/spectrum-analyzer-example.png — Spectrogram produced by a spectrum analyzer in a scenario involving wifi signals interfered by a microwave oven, as simulated by the example `adhoc-aloha-ideal-phy-with-microwave-oven`.¶

30.1. Model Description¶

The module provides:

a set of classes for modeling signals and
a Channel/PHY interface based on a power spectral density signal representation that is technology-independent
two technology-independent Channel implementations based on the Channel/PHY interface
a set of basic PHY model implementations based on the Channel/PHY interface

The source code for the spectrum module is located at src/spectrum.

30.1.1. Design¶

30.1.1.1. Signal model¶

The signal model is implemented by the SpectrumSignalParameters class. This class provides the following information for a signal being transmitted/received by PHY devices:

a reference to the transmitting PHY device
a reference to the antenna model used by the transmitting PHY device to transmit this signal
the duration of the signal
the Power Spectral Density (PSD) of the signal, which is assumed to be constant for the duration of the signal
the frequency domain 3D spectrum channel matrix that is needed for MIMO computations when multiple streams are transmitted
the 3D precoding matrix that is needed for MIMO computations when multiple streams are transmitted.

The PSD is represented as a set of discrete scalar values each corresponding to a certain subband in frequency. The set of frequency subbands to which the PSD refers to is defined by an instance of the SpectrumModel class. The PSD itself is implemented as an instance of the SpectrumValue class which contains a reference to the associated SpectrumModel class instance. The SpectrumValue class provides several arithmetic operators to allow to perform calculations with PSD instances. Additionally, the SpectrumConverter class provides means for the conversion of SpectrumValue instances from one SpectrumModel to another.

The frequency domain 3D channel matrix is needed in MIMO systems in which multiple transmit and receive antenna ports can exist, hence the PSD is multidimensional. The dimensions are: the number of receive antenna ports, the number of transmit antenna ports, and the number of subbands in frequency (or resource blocks).

The 3D precoding matrix is also needed in MIMO systems to be able to correctly perform the calculations of the received signal and interference. The dimensions are: the number of transmit antenna ports, the number of transmit streams, and the number of subbands (or resource blocks).

For a more formal mathematical description of the signal model just described, the reader is referred to [Baldo2009Spectrum].

The SpectrumSignalParameters class is meant to include only information that is valid for all signals; as such, it is not meant to be modified to add technology-specific information (such as type of modulation and coding schemes used, info on preambles and reference signals, etc). Instead, such information shall be put in a new class that inherits from SpectrumSignalParameters and extends it with any technology-specific information that is needed. This design is intended to model the fact that in the real world we have signals of different technologies being simultaneously transmitted and received over the air.

30.1.1.2. Channel/PHY interface¶

The spectrum Channel/PHY interface is defined by the base classes SpectrumChannel and SpectrumPhy. Their interaction simulates the transmission and reception of signals over the medium. The way this interaction works is depicted in Sequence diagram showing the interaction between SpectrumPhy and SpectrumChannel:

_images/spectrum-channel-phy-interface.png — Sequence diagram showing the interaction between SpectrumPhy and SpectrumChannel¶

30.1.1.3. Spectrum Channel implementations¶

The module provides two SpectrumChannel implementations: SingleModelSpectrumChannel and MultiModelSpectrumChannel. They both provide this functionality:

Propagation loss modeling, in three forms:

you can plug models based on PropagationLossModel on these channels. Only linear models (where the loss value does not depend on the transmission power) can be used. These models are single-frequency in the sense that the loss value is applied equally to all components of the power spectral density.

you can plug models based on SpectrumPropagationLossModel on these channels. These models can have frequency-dependent loss, i.e., a separate loss value is calculated and applied to each component of the power spectral density.

you can plug models based on PhasedArraySpectrumPropagationLossModel on these channels. These models can have frequency-dependent loss, i.e., a separate loss value is calculated and applied to each component of the power spectral density. Additionally, these models support the phased antenna array at the transmitter and the receiver, i.e., ns-3 antenna type PhasedArrayModel.

Propagation delay modeling, by plugging a model based on PropagationDelayModel. The delay is independent of frequency and applied to the signal as a whole. Delay modeling is implemented by scheduling the StartRx event with a delay respect to the StartTx event.

SingleModelSpectrumChannel and MultiModelSpectrumChannel are quite similar, the main difference is that MultiModelSpectrumChannel allows to use different SpectrumModel instances with the same channel instance, by automatically taking care of the conversion of PSDs among the different models.

30.1.1.4. Example model implementations¶

The spectrum module provides some basic implementation of several components that are mainly intended as a proof-of-concept and as an example for building custom models with the spectrum module. Here is a brief list of the available implementations:

SpectrumModel300Khz300GhzLog and SpectrumModelIsm2400MhzRes1Mhz are two example SpectrumModel implementations

HalfDuplexIdealPhy: a basic PHY model using a gaussian interference model (implemented in SpectrumInterference) together with an error model based on Shannon capacity (described in [Baldo2009Spectrum] and implemented in SpectrumErrorModel. This PHY uses the GenericPhy interface. Its additional custom signal parameters are defined in HalfDuplexIdealPhySignalParameters.

WifiSpectrumValueHelper is an helper object that makes it easy to create SpectrumValues representing PSDs and RF filters for the wifi technology.

AlohaNoackNetDevice: a minimal NetDevice that allows to send packets over HalfDuplexIdealPhy (or other PHY model based on the GenericPhy interface).

SpectrumAnalyzer, WaveformGenerator and MicrowaveOven are examples of PHY models other than communication devices - the names should be self-explaining.

30.1.2. References¶

[Baldo2009Spectrum] (1,2,3)

N. Baldo and M. Miozzo, “Spectrum-aware Channel and PHY layer modeling for ns3”, Proceedings of ICST NSTools 2009, Pisa, Italy

30.2. Usage¶

The main use case of the spectrum model is for developers who want to develop a new model for the PHY layer of some wireless technology to be used within ns-3. Here are some notes on how the spectrum module is expected to be used.

SpectrumPhy and SpectrumChannel are abstract base classes. Real code will use classes that inherit from these classes.

If you are implementing a new model for some wireless technology of your interest, and want to use the spectrum module, you’ll typically create your own module and make it depend on the spectrum module. Then you typically have to implement:

a child class of SpectrumModel which defines the (sets of) frequency subbands used by the considered wireless technology. Note: instances of SpectrumModel are typically statically allocated, in order to allow several SpectrumValue instances to reference the same SpectrumModel instance.

a child class of SpectrumPhy which will handle transmission and reception of signals (including, if appropriate, interference and error modeling).

a child class of SpectrumSignalParameters which will contain all the information needed to model the signals for the wireless technology being considered that is not already provided by the base SpectrumSignalParameters class. Examples of such information are the type of modulation and coding schemes used, the PHY preamble format, info on the pilot/reference signals, etc.

The available SpectrumChannel implementations (SingleModelSpectrumChannel and MultiModelSpectrumChannel, are quite generic. Chances are you can use them as-is. Whether you prefer one or the other it is just a matter of whether you will have a single SpectrumModel or multiple ones in your simulations.

Typically, there will be a single SpectrumChannel instance to which several SpectrumPhy instances are plugged. The rule of thumb is that all PHYs that are interfering with each other shall be plugged on the same channel. Multiple SpectrumChannel instances are expected to be used mainly when simulating completely orthogonal channels; for example, when simulating the uplink and downlink of a Frequency Division Duplex system, it is a good choice to use two SpectrumChannel instances in order to reduce computational complexity.

Different types of SpectrumPhy (i.e., instances of different child classes) can be plugged on the same SpectrumChannel instance. This is one of the main features of the spectrum module, to support inter-technology interference. For example, if you implement a WifiSpectrumPhy and a BluetoothSpectrumPhy, and plug both on a SpectrumChannel, then you’ll be able to simulate interference between wifi and bluetooth and vice versa.

Different child classes of SpectrumSignalParameters can coexist in the same simulation, and be transmitted over the same channel object. Again, this is part of the support for inter-technology interference. A PHY device model is expected to use the DynamicCast<> operator to determine if a signal is of a certain type it can attempt to receive. If not, the signal is normally expected to be considered as interference.

Many propagation loss and delay models can be added to these channels. The base class SpectrumChannel provides an AssignStreams() method to allow the deterministic configuration of random variable stream numbers with a single API call. See the ns-3 Manual chapter on random variables for more information.

30.2.1. Helpers¶

The helpers provided in src/spectrum/helpers are mainly intended for the example implementations described in Example model implementations. If you are developing your custom model based on the spectrum framework, you will probably prefer to define your own helpers.

30.2.2. Attributes¶

Both SingleModelSpectrumChannel and MultiModelSpectrumChannel have an attribute MaxLossDb which can use to avoid propagating signals affected by very high propagation loss. You can use this to reduce the complexity of interference calculations. Just be careful to choose a value that does not make the interference calculations inaccurate.

The example implementations described in Example model implementations also have several attributes.

30.2.3. Output¶

Both SingleModelSpectrumChannel and MultiModelSpectrumChannel provide a trace source called PathLoss which is fired whenever a new path loss value is calculated. Note: only single-frequency path loss is accounted for, see the attribute description.

The example implementations described in Example model implementations also provide some trace sources.

The helper class SpectrumAnalyzerHelper can be conveniently used to generate an output text file containing the spectrogram produced by a SpectrumAnalyzer instance. The format is designed to be easily plotted with gnuplot. For example, if your run the example adhoc-aloha-ideal-phy-with-microwave-oven you will get an output file called spectrum-analyzer-output-3-0.tr. From this output file, you can generate a figure similar to Spectrogram produced by a spectrum analyzer in a scenario involving wifi signals interfered by a microwave oven, as simulated by the example adhoc-aloha-ideal-phy-with-microwave-oven. by executing the following gnuplot commands:

unset surface
set pm3d at s
set palette
set key off
set view 50,50
set xlabel "time (ms)"
set ylabel "freq (MHz)"
set zlabel "PSD (dBW/Hz)" offset 15,0,0
splot "./spectrum-analyzer-output-3-0.tr" using ($1*1000.0):($2/1e6):(10*log10($3))

30.2.4. Examples¶

The example programs in src/spectrum/examples/ allow to see the example implementations described in Example model implementations in action.

30.2.5. Troubleshooting¶

Disclaimer on inter-technology interference: the spectrum model makes it very easy to implement an inter-technology interference model, but this does not guarantee that the resulting model is accurate. For example, the gaussian interference model implemented in the SpectrumInterference class can be used to calculate inter-technology interference, however the results might not be valid in some scenarios, depending on the actual waveforms involved, the number of interferers, etc. Moreover, it is very important to use error models that are consistent with the interference model. The responsibility of ensuring that the models being used are correct is left to the user.

30.3. Testing¶

In this section we describe the test suites that are provided within the spectrum module.

30.3.1. SpectrumValue test¶

The test suite spectrum-value verifies the correct functionality of the arithmetic operators implemented by the SpectrumValue class. Each test case corresponds to a different operator. The test passes if the result provided by the operator implementation is equal to the reference values which were calculated offline by hand. Equality is verified within a tolerance of $10^{-6}$ which is to account for numerical errors.

30.3.2. SpectrumConverter test¶

The test suite spectrum-converter verifies the correct functionality of the SpectrumConverter class. Different test cases correspond to the conversion of different SpectrumValue instances to different SpectrumModel instances. Each test passes if the SpectrumValue instance resulting from the conversion is equal to the reference values which were calculated offline by hand. Equality is verified within a tolerance of $10^{-6}$ which is to account for numerical errors.

Describe how the model has been tested/validated. What tests run in the test suite? How much API and code is covered by the tests? Again, references to outside published work may help here.

30.3.3. Interference test¶

The test suite spectrum-interference verifies the correct functionality of the SpectrumInterference and ShannonSpectrumErrorModel in a scenario involving four signals (an intended signal plus three interferers). Different test cases are created corresponding to different PSDs of the intended signal and different amount of transmitted bytes. The test passes if the output of the error model (successful or failed) coincides with the expected one which was determine offline by manually calculating the achievable rate using Shannon’s formula.

30.3.4. IdealPhy test¶

The test verifies that AlohaNoackNetDevice and HalfDuplexIdealPhy work properly when installed in a node. The test recreates a scenario with two nodes (a TX and a RX) affected by a path loss such that a certain SNR is obtained. The TX node transmits with a pre-determined PHY rate and with an application layer rate which is larger than the PHY rate, so as to saturate the channel. PacketSocket is used in order to avoid protocol overhead. Different test cases correspond to different PHY rate and SNR values. For each test case, we calculated offline (using Shannon’s formula) whether the PHY rate is achievable or not. Each test case passes if the following conditions are satisfied:

if the PHY rate is achievable, the application throughput shall be within $1\%$ of the PHY rate;

if the PHY rate is not achievable, the application throughput shall be zero.

30.4. Additional Models¶

30.4.1. TV Transmitter Model¶

A TV Transmitter model is implemented by the TvSpectrumTransmitter class. This model enables transmission of realistic TV signals to be simulated and can be used for interference modeling. It provides a customizable power spectral density (PSD) model, with configurable attributes including the type of modulation (with models for analog, 8-VSB, and COFDM), signal bandwidth, power spectral density level, frequency, and transmission duration. A helper class, TvSpectrumTransmitterHelper, is also provided to assist users in setting up simulations.

30.4.1.1. Main Model Class¶

The main TV Transmitter model class, TvSpectrumTransmitter, provides a user-configurable PSD model that can be transmitted on the SpectrumChannel. It inherits from SpectrumPhy and is comprised of attributes and methods to create and transmit the signal on the channel.

_images/spectrum-tv-cofdm.png — 8K COFDM signal spectrum generated from `TvSpectrumTransmitter` (Left) and theoretical COFDM signal spectrum [KoppCOFDM] (Right)¶

One of the user-configurable attributes is the type of modulation for the TV transmitter to use. The options are 8-VSB (Eight-Level Vestigial Sideband Modulation) which is notably used in the North America ATSC digital television standard, COFDM (Coded Orthogonal Frequency Division Multiplexing) which is notably used in the DVB-T and ISDB-T digital television standards adopted by various countries around the world, and analog modulation which is a legacy technology but is still being used by some countries today. To accomplish realistic PSD models for these modulation types, the signals’ PSDs were approximated from real standards and developed into models that are scalable by frequency and power. The COFDM PSD is approximated from Figure 12 (8k mode) of [KoppCOFDM], the 8-VSB PSD is approximated from Figure 3 of [Baron8VSB], and the analog PSD is approximated from Figure 4 of [QualcommAnalog]. Note that the analog model is approximated from the NTSC standard, but other analog modulation standards such as PAL have similar signals. The approximated COFDM PSD model is in 8K mode. The other configurable attributes are the start frequency, signal/channel bandwidth, base PSD, antenna type, starting time, and transmit duration.

TvSpectrumTransmitter uses IsotropicAntennaModel as its antenna model by default, but any model that inherits from AntennaModel is selectable, so directional antenna models can also be used. The propagation loss models used in simulation are configured in the SpectrumChannel that the user chooses to use. Terrain and spherical Earth/horizon effects may be supported in future ns-3 propagation loss models.

After the attributes are set, along with the SpectrumChannel, MobilityModel, and node locations, the PSD of the TV transmitter signal can be created and transmitted on the channel.

30.4.1.2. Helper Class¶

The helper class, TvSpectrumTransmitterHelper, consists of features to assist users in setting up TV transmitters for their simulations. Functionality is also provided to easily simulate real-world scenarios.

_images/spectrum-tv-8vsb.png — North America ATSC channel 19 & 20 signals generated using `TvSpectrumTransmitterHelper` (Left) and theoretical 8-VSB signal [Baron8VSB] (Right). Note that the theoretical signal is not shown in dB while the ns-3 generated signals are.¶

Using this helper class, users can easily set up TV transmitters right after configuring attributes. Multiple transmitters can be created at a time. Also included are real characteristics of specific geographic regions that can be used to run realistic simulations. The regions currently included are North America, Europe, and Japan. The frequencies and bandwidth of each TV channel for each these regions are provided.

_images/spectrum-tv-rand-geo-points.png — Plot from MATLAB implementation of CreateRegionalTvTransmitters method in `TvSpectrumTransmitterHelper`. Shows 100 random points on Earth’s surface (with altitude 0) corresponding to TV transmitter locations within a 2000 km radius of 35° latitude and -100° longitude.¶

A method (CreateRegionalTvTransmitters) is provided that enables users to randomly generate multiple TV transmitters from a specified region with a given density within a chosen radius around a point on Earth’s surface. The region, which determines the channel frequencies of the generated TV transmitters, can be specified to be one of the three provided, while the density determines the amount of transmitters generated. The TV transmitters’ antenna heights (altitude) above Earth’s surface can also be randomly generated to be within a given maximum altitude. This method models Earth as a perfect sphere, and generated location points are referenced accordingly in Earth-Centered Earth-Fixed Cartesian coordinates. Note that bodies of water on Earth are not considered in location point generation–TV transmitters can be generated anywhere on Earth around the origin point within the chosen maximum radius.

30.4.1.3. Examples¶

Two example simulations are provided that demonstrate the functionality of the TV transmitter model. tv-trans-example simulates two 8-VSB TV transmitters with adjacent channel frequencies. tv-trans-regional-example simulates randomly generated COFDM TV transmitters (modeling the DVB-T standard) located around the Paris, France area with channel frequencies and bandwidths corresponding to the European television channel allocations.

30.4.1.4. Testing¶

The tv-spectrum-transmitter test suite verifies the accuracy of the spectrum/PSD model in TvSpectrumTransmitter by testing if the maximum power spectral density, start frequency, and end frequency comply with expected values for various test cases.

The tv-helper-distribution test suite verifies the functionality of the method in TvSpectrumTransmitterHelper that generates a random number of TV transmitters based on the given density (low, medium, or high) and maximum number of TV channels. It verifies that the number of TV transmitters generated does not exceed the expected bounds.

The CreateRegionalTvTransmitters method in TvSpectrumTransmitterHelper described in Helper Class uses two methods from the GeographicPositions class in the Mobility module to generate the random Cartesian points on or above earth’s surface around an origin point which correspond to TV transmitter positions. The first method converts Earth geographic coordinates to Earth-Centered Earth-Fixed (ECEF) Cartesian coordinates, and is tested in the geo-to-cartesian test suite by comparing (with 10 meter tolerance) its output with the output of the geographic to ECEF conversion function [MatlabGeo] of the MATLAB Mapping Toolbox for numerous test cases. The other used method generates random ECEF Cartesian points around the given geographic origin point, and is tested in the rand-cart-around-geo test suite by verifying that the generated points do not exceed the given maximum distance radius from the origin point.

30.4.2. 3GPP TR 38.901 fast fading model¶

The framework described by TR 38.901 [TR38901] is a 3D statistical Spatial Channel Model supporting different propagation environments (e.g., urban, rural, indoor), multi-antenna operations and the modeling of wireless channels between 0.5 and 100 GHz. The overall channel is represented by the matrix $H(t,\tau)$ , in which each entry H _u,s $(t,\tau)$ corresponds to the impulse response of the channel between the s-th element of the transmitting antenna and the u-th element of the receiving antenna. H _u,s $(t,\tau)$ is generated by the superposition of N different multi-path components, called clusters, each of which composed of M different rays. The channel matrix generation procedure accounts for large and small scale propagation phenomena. The classes ThreeGppSpectrumPropagationLossModel and ThreeGppChannelModel included in the spectrum module take care of the generation of the channel coefficients and the computation of the frequency-dependent propagation loss.

30.4.2.1. Implementation¶

Our implementation is described in [Zugno]. It is based on the model described in [Zhang], but the code has been refactored, extended, and aligned to TR 38.901 [TR38901]. The fundamental assumption behind this model is the channel reciprocity, i.e., the impulse response of the channel between node a and node b is the same as between node b and node a. To deal with the equivalence of the channel between a and b, no matter who is the transmitter and who is the receiver, the model considers the pair of nodes to be composed by one “s” and one “u” node. The channel matrix, as well as other parameters, are saved and used under the assumption that, within a pair, the definition of the “s” and “u” node will always be the same. For more details, please have a look at the documentation of the classes ThreeGppChannelModel and ThreeGppSpectrumPropagationLossModel.

Note:

Currently, no error model is provided; a link-to-system campaign may be needed to incorporate it in existing modules.

The model does not include any spatial consistency update procedure (see [TR38901], Sec. 7.6.1). The implementation of this feature is left as future work.

Issue regarding the blockage model: according to 3GPP TR 38.901 v15.0.0 (2018-06) section 7.6.4.1, the blocking region for self-blocking is provided in LCS.

However, here, clusterAOA and clusterZOA are in GCS and blocking check is performed for self-blocking similar to non-self blocking, that is in GCS. One would expect the angles to be transposed to LCS before checking self-blockage.

30.4.2.2. ThreeGppSpectrumPropagationLossModel¶

The class ThreeGppSpectrumPropagationLossModel implements the PhasedArraySpectrumPropagationLossModel interface and enables the modeling of frequency dependent propagation phenomena while taking into account the specific pair of the phased antenna array at the transmitter and the receiver. The main method is DoCalcRxPowerSpectralDensity, which takes as input the SpectrumSignalParameters structure, which contains, among others, the power spectral density (PSD) of the transmitted signal, and the precoding matrix of the transmitter which is needed for MIMO computations. Other input parameters are the mobility models of the transmitting and receiving node, and the phased antenna array of the transmitting and receiving node. DoCalcRxPowerSpectralDensity computes the PSD of the received signal (used in case of single stream transmission), and the frequency domain 3D channel matrix between receive and transmit antenna ports (needed for MIMO computations when multiple streams are transmitted). Finally, it returns the SpectrumSignalParameters which contains the received PSD and the frequency domain 3D spectrum channel matrix.

Procedure used to compute the PSD of the received signal and the frequency domain 3D spectrum channel matrix:

1. Retrieve the beamforming vectors To account for the beamforming, ThreeGppSpectrumPropagationLossModel has to retrieve the beamforming vectors of the transmitting and receiving antennas. The method DoCalcRxPowerSpectralDensity uses the antenna objects that are passed as parameters for both the transmitting and receiving devices, and calls the method GetBeamformingVector to retrieve the beamforming vectors of these antenna objects.

2. Retrieve the channel matrix and the channel params The ThreeGppSpectrumPropagationLossModel relies on the ThreeGppChannelModel class to obtain the channel matrix and channel parameters. In particular, it makes use of the method GetChannel, which returns a ChannelMatrix object containing the channel matrix, the generation time, the node pair, and the phased antenna array pair among which is created this channel matrix. Additionally, it makes use of the method GetParams which returns a ChannelParams object containing the channel parameters. Notice that the channel information is split into these two structures (ChannelMatrix and ChannelParams) to support multiple collocated phased antenna arrays at TX/RX node. ChannelParams (also its specialization ThreeGppChannelParams structure) contains parameters which are common for all the channels among the same RX/TX node pair, while ChannelMatrix contains the channel matrix for the specific pair of the phased antenna arrays of TX/RX nodes. For example, if the TX and the RX node have multiple collocated antenna arrays, then there will be multiple channel matrices among this pair of nodes for different pairs of antenna arrays of the TX and the RX node. These channel matrices that are among the same pair of nodes have common channel parameters, i.e., they share the same channel condition, cluster powers, cluster delays, AoD, AoA, ZoD, ZoA, K_factor, delay spread, etc. On the other hand, each pair of TX and RX antenna arrays has a specific channel matrix and fading, which depends on the actual antenna element positions and field patterns of each pair of antenna array subpartitions. The ThreeGppChannelModel instance is automatically created in the ThreeGppSpectrumPropagationLossModel constructor and it can be configured by using the method SetChannelModelAttribute.

Notice that in MultiModelSpectrumChannel it is checked whether the TX/RX SpectrumPhy instances belong to different TX/RX nodes. This is needed to avoid pathloss models calculations among the phased antenna arrays of the same node, because there are no models yet in ns-3 that support the calculation of this kind of interference.

4. Compute the long term component The method GetLongTerm returns the long term component obtained by multiplying the channel matrix and the beamforming vectors. The function CalculateLongTermComponent calculates the long term component per RX and TX port pair. Finally, GetLongTerm returns a 3D long term channel matrix whose dimensions are the number of the receive antenna ports, the number transmit antenna ports, and the number of clusters. When multiple ports are being configured note that the sub-array partition model is adopted for TXRU virtualization, as described in Section 5.2.2 of 3GPP TR 36.897 [TR36897], and so equal beam weights are used for all the ports. Support of the full-connection model for TXRU virtualization would need extensions. To reduce the computational load, the long term components associated to the different channels are stored in the m_longTermMap and recomputed only if the associated channel matrix is updated or if the transmitting and/or receiving beamforming vectors have changed. Given the channel reciprocity assumption, for each node pair a single long term component is saved in the map.

5. Apply the small scale fading, calculate the channel gain, generate the frequency domain 3D spectrum channel matrix, and finally compute the received PSD The method CalcBeamformingGain computes the channel gain in each sub-band and applies it to the PSD of the transmitted signal to obtain the received PSD. To compute the sub-band gain, it accounts for the Doppler phenomenon and the time dispersion effect on each cluster. In order to reduce the computational load, the Doppler component of each cluster is computed considering only the central ray. Also, as specified here, it is possible to account for the effect of environmental scattering following the model described in Sec. 6.2.3 of 3GPP TR 37.885. This is done by deviating the Doppler frequency by a random value, whose distribution depends on the parameter $v_{scatt}$ . The value of $v_{scatt}$ can be configured using the attribute “vScatt” (by default it is set to 0, so that the scattering effect is not considered). Function GenSpectrumChannelMatrix generates the received PSD for each pair of the transmit and receive antenna ports. It creates a frequency domain 3D spectrum channel matrix whose dimensions are the number of receive antenna ports, the number of transmit antenna ports, and the number of resource blocks. Finally, the frequency domain 3D spectrum channel matrix is used to obtain the received PSD. In case of multiple ports at the transmitter the PSD is calculated by summing per each RB the real parts of the diagonal elements of the (H*P)^h * (H*P), where H is the frequency domain spectrum channel matrix and P is the precoding matrix.

30.4.2.3. ThreeGppChannelModel¶

The class ThreeGppChannelModel implements the channel matrix generation procedure described in Sec. of [TR38901]. The main method is GetChannel, which takes as input the mobility models of the transmitter and receiver nodes, the associated antenna objects, and returns a ChannelMatrix object containing:

the channel matrix of size UxSxN, where U is the number of receiving antenna elements, S is the number of transmitting antenna elements and N is the number of clusters
the clusters delays, as an array of size N
the clusters arrival and departure angles, as a 2D array in which each row corresponds to a direction (AOA, ZOA, AOD, ZOD) and each column corresponds to a different cluster
a time stamp indicating the time at which the channel matrix was generated
the node IDs
other channel parameters

The ChannelMatrix objects are saved in the map m_channelMap and updated when the coherence time expires, or in case the LOS/NLOS channel condition changes. The coherence time can be configured through the attribute “UpdatePeriod”, and should be chosen by taking into account all the factors that affects the channel variability, such as mobility, frequency, propagation scenario, etc. By default, it is set to 0, which means that the channel is recomputed only when the LOS/NLOS condition changes. It is possible to configure the propagation scenario and the operating frequency of interest through the attributes “Scenario” and “Frequency”, respectively.

Blockage model: 3GPP TR 38.901 also provides an optional feature that can be used to model the blockage effect due to the presence of obstacles, such as trees, cars or humans, at the level of a single cluster. This differs from a complete blockage, which would result in an LOS to NLOS transition. Therefore, when this feature is enabled, an additional attenuation is added to certain clusters, depending on their angle of arrival. There are two possible methods for the computation of the additional attenuation, i.e., stochastic (Model A) and geometric (Model B). In this work, we used the implementation provided by [Zhang], which uses the stochastic method. In particular, the model is implemented by the method CalcAttenuationOfBlockage, which computes the additional attenuation. The blockage feature can be disable through the attribute “Blockage”. Also, the attributes “NumNonselfBlocking”, “PortraitMode” and “BlockerSpeed” can be used to configure the model.

30.4.2.4. Testing¶

The test suite ThreeGppChannelTestSuite includes five test cases:

ThreeGppChannelMatrixComputationTest checks if the channel matrix has the correct dimensions and if it correctly normalized
ThreeGppChannelMatrixUpdateTest, which checks if the channel matrix is correctly updated when the coherence time exceeds
ThreeGppSpectrumPropagationLossModelTest, which tests the functionalities of the class ThreeGppSpectrumPropagationLossModel. It builds a simple network composed of two nodes, computes the power spectral density received by the receiving node, and
1. Checks if the long term components for the direct and the reverse link are the same,
2. Checks if the long term component is updated when changing the beamforming vectors,
3. Checks if the long term is updated when changing the channel matrix
ThreeGppCalcLongTermMultiPortTest, which tests that the channel matrices are correctly generated when multiple transmit and receive antenna ports are used.
ThreeGppMimoPolarizationTest, which tests that the channel matrices are correctly generated when dual-polarized antennas are being used.

Note: TR 38.901 includes a calibration procedure that can be used to validate the model, but it requires some additional features which are not currently implemented, thus is left as future work.

30.4.2.5. References¶

[Baron8VSB] (1,2)

Baron, Stanley. “First-Hand:Digital Television: The Digital Terrestrial Television Broadcasting (DTTB) Standard.” IEEE Global History Network. <http://www.ieeeghn.org/wiki/index.php/First-Hand:Digital_Television:_The_Digital_Terrestrial_Television_Broadcasting_(DTTB)_Standard>.

[KoppCOFDM] (1,2)

Kopp, Carlo. “High Definition Television.” High Definition Television. Air Power Australia. <http://www.ausairpower.net/AC-1100.html>.

[MatlabGeo]

“Geodetic2ecef.” Convert Geodetic to Geocentric (ECEF) Coordinates. The MathWorks, Inc. <http://www.mathworks.com/help/map/ref/geodetic2ecef.html>.

[QualcommAnalog]

Stephen Shellhammer, Ahmed Sadek, and Wenyi Zhang. “Technical Challenges for Cognitive Radio in the TV White Space Spectrum.” Qualcomm Incorporated.

[TR38901] (1,2,3,4,5,6,7,8,9,10,11)

3GPP. 2018. TR 38.901. Study on channel for frequencies from 0.5 to 100 GHz. V.15.0.0. (2018-06).

[Zhang] (1,2)

Menglei Zhang, Michele Polese, Marco Mezzavilla, Sundeep Rangan, Michele Zorzi. “ns-3 Implementation of the 3GPP MIMO Channel Model for Frequency Spectrum above 6 GHz”. In Proceedings of the Workshop on ns-3 (WNS3 ‘17). 2017.

[Zugno]

Tommaso Zugno, Michele Polese, Natale Patriciello, Biljana Bojovic, Sandra Lagen, Michele Zorzi. “Implementation of a Spatial Channel Model for ns-3”. Submitted to the Workshop on ns-3 (WNS3 ‘20). 2020. Available: https://arxiv.org/abs/2002.09341

[TR36897]

3GPP. 2015. TR 36.897. Study on elevation beamforming / Full-Dimension (FD) Multiple Input Multiple Output (MIMO) for LTE. V13.0.0. (2015-06)

30.4.3. Two-Ray fading model¶

The model aims to provide a performance-oriented alternative to the 3GPP TR 38.901 framework [TR38901] which is implemented in the ThreeGppSpectrumPropagationLossModel and ThreeGppChannelModel classes and whose implementation is described in [Zugno2020]. The overall design described in [Pagin2023] follows the general approach of [Polese2018], with aim of providing the means for computing a 3GPP TR 38.901-like end-to-end channel gain by combining several statistical terms. The frequency range of applicability is the same as that of [TR38901], i.e., 0.5 - 100 GHz.

30.4.3.1. Use-cases¶

The use-cases for this channel model comprise large-scale MIMO simulations involving a high number of nodes (100+), such as multi-cell LTE and 5G deployments in dense urban areas, for which the full 3GPP TR 38.901 does not represent a viable option.

30.4.3.2. Implementation - `TwoRaySpectrumPropagationLossModel`¶

The computation of the channel gain is taken care of by the TwoRaySpectrumPropagationLossModel class. In particular, the latter samples a statistical term which combines:

The array and beamforming gain, computed as outlined in [Rebato2018] using the CalcBeamformingGain function. This term supports the presence of multiple antenna elements both at the transmitter and at the receiver and arbitrary antenna radiation patterns. Specifically, the array gain is compute as:

$G_{\mathrm{AA}}(\theta, \varphi)=\left|\boldsymbol{a}^{\mathrm{T}}(\theta, \varphi) \boldsymbol{w}\left(\theta_0, \varphi_0\right)\right|^2=\left|\mathrm{AF}_{\mathrm{v}}(\theta, \varphi)\right|^2\left|\mathrm{AF}_{\mathrm{h}}(\theta, \varphi)\right|^2 G(\theta, \varphi),$

where:

$\operatorname{AF}_{\mathrm{v}}(\theta, \varphi)=\frac{1}{\sqrt{N_{\mathrm{v}}}} \sum_{m=0}^{N_{\mathrm{v}}-1} e^{j k d_{\mathrm{v}} m\left(\cos \theta-\cos \theta_0\right)}$

and:

$\operatorname{AF}_{\mathrm{h}}(\theta, \varphi)=\frac{1}{\sqrt{N_{\mathrm{h}}}} \sum_{n=0}^{N_{\mathrm{h}}-1} e^{j k d_{\mathrm{h}} n\left(\sin \theta \sin \varphi-\sin \theta_0 \sin \varphi_0\right)}$

In turn, $N_h$ , $N_v$ are the number of horizontal and vertical antenna elements respectively, $d_h$ , $d_v$ are the element spacing in the horizontal and vertical direction respectively. The figures below depict the resulting array radiation pattern versus the relative azimuth of transmitter and receiver, for antenna arrays featuring 3GPP TR 38.901 (ThreeGppAntennaModel, top) and isotropic (IsotropicAntennaModel, bottom) antenna elements, respectively. These figures match the corresponding plots of [Asplund].

_images/two-ray-spectrum-loss-model-3gpp-radiation-pattern.png — Radiation pattern produced by the `CalcBeamformingGain` method when using antenna arrays featuring `ThreeGppAntennaModel` antenna elements, for various Uniform Planar Array (UPA) configurations.¶

_images/two-ray-spectrum-loss-model-iso-radiation-pattern.png — Radiation pattern produced by the `CalcBeamformingGain` method when using antenna arrays featuring `IsotropicAntennaModel` antenna elements, for various Uniform Planar Array (UPA) configurations.¶

Whenever the link is in NLOS, a penalty factor is introduced, to account for beam misalignment due to the lack of a dominant multipath component [Kulkarni].

A fast fading term, sampled using the Fluctuating Two Ray (FTR) model distribution [Romero]. The latter is a fading model which is more general than typical ones, taking into account two dominant specular components and a mixture of scattered paths. As, a consequence it has been shown to provide a better fit to fading phenomena at mmWaves. The model parameters are automatically picked once the simulation scenario is set, using a lookup table which associates the simulation parameters (such as carrier frequency and LOS condition) to the FTR parameters providing the best fit to the corresponding TR 38.901 channel statistics. As a consequence, this channel model can be used for all the frequencies which are supported by the 38.901 model, i.e., 0.5-100 GHz. The calibration has been done by first obtaining the statistics of the channel gain due to the small-scale fading in the 3GPP model, using an ad hoc simulation script (src/spectrum/examples/three-gpp-two-ray-channel-calibration.cc). Then, this information has been used as a reference to estimate the FTR parameters yielding the closest (in a goodness-of-fit sense) fading realizations, using a custom Python script (src/spectrum/utils/two-ray-to-three-gpp-ch-calibration.py).

Note:

To then obtain a full channel model characterization, the model is intended to be used in conjunction of the path loss and shadowing capability provided by the ThreeGppPropagationLossModel class. Indeed, the goal of this model is to provide channel realizations which are as close as possible to ones of [TR38901], but at a fraction of the complexity. Since the path loss and shadowing terms are not computationally demanding anyway, the ones of [Zugno2020] have been kept;

Currently, the value of NLoS beamforming factor penalty factor is taken from the preliminary work of [Kulkarni] and it is scenario-independent; As future work, the possibility of using scenario-dependent penalty factors will be investigated.

30.4.3.3. Calibration¶

The purpose of the calibration procedures is to compute offline a look-up table which associates the FTR fading model parameters with the simulation parameters. In particular, the [TR38901] fading distributions depend on:

The scenario (RMa, UMa, UMi-StreetCanyon, InH-OfficeOpen, InH-OfficeMixed);
The LOS condition (LoS/NLoS); and
The carrier frequency.

As a consequence, the calibration output is a map which associates LoS condition and scenario to a list of carrier frequency-FTR parameters values. The latter represent the FTR parameters yielding channel realizations which exhibit the closest statistics to [TR38901].

The actual calibration is a two-step procedure which:

1. First generates reference channel gain curves using the src/spectrum/examples/three-gpp-two-ray-channel-calibration.cc simulation script. Specifically, the script samples numRealizations channel realizations and computes for each of them the end-to-end channel gain by setting the speed of the TX and RX pair to $0$ , disabling the shadowing and fixing the LOS condition. In such a way, any variation around the mean is due to the small-scale fading only. The channel gain samples are produced, and returned on output conditioned on the value of enableOutput, for each combination of LoS condition, channel model scenario and carrier frequency. The latter cover the whole [TR38901] frequency range of 0.5 - 100 GHz with a relatively sparse resolution (500 MHz), since the dependency of the fading distribution with respect to the carrier frequency is actually relatively weak.

_images/three-gpp-gain-reference-gain-vs-fc.png — Empirical CDF of the reference channel gains obtained using the `three-gpp-two-ray-channel-calibration` simulation script when keeping a fixed LoS condition and channel scenario and varying the carrier frequency only.¶

2. Then, the output of the above script is parsed by the two-ray-to-three-gpp-ch-calibration.py Python companion script. In particular, reference ECDFs are obtained from the channel gains sampled using the model of [TR38901]. In turn, the reference ECDFs (one for each LoS condition, channel model scenario and carrier frequency combination) are compared to FTR distributions ECDFs obtained using different values of the parameters. Finally, the parameters which provide the best fit (in a goodness-of-fit sense) for the specific scenario, LOS condition and carrier frequency are found. The parameters to test are picked initially by performing an exhaustive search within a discrete grid of possible values, and then by iteratively refining the previous search runs by scanning the neighborhood of the most recent identified values. In such regard, the Anderson-Darling statistical test is used to rank the various FTR distributions and eventually pick the one providing the closest approximation to the reference statistics.

30.4.3.4. Testing¶

The test suite TwoRaySplmTestSuite includes three test cases:

FtrFadingModelAverageTest, which checks that the average of the Fluctuating Two Ray (FTR) fading model realizations is consistent with the theoretical value provided in [Romero].
ArrayResponseTest, which checks that the overall array response at boresight computed by the ù CalcBeamformingGain function coincides with the expected theoretical values.
OverallGainAverageTest, which checks that the average overall channel gain obtained using the DoCalcRxPowerSpectralDensity method of the TwoRaySpectrumPropagationLossModel class is close (it is, after all, a simplified and performance-oriented model) to the one obtained using the ThreeGppSpectrumPropagationLossModel and ThreeGppChannelModel classes.

30.4.3.5. References¶

[Pagin2023]

Pagin, Matteo, Sandra Lagen, Biljana Bojovic, Michele Polese, Michele Zorzi. 2023. “Improving the Efficiency of MIMO Simulations in ns-3” In Proceedings of the 2023 Workshop on ns-3, pp. 1–9. 2023

[Zugno2020] (1,2)

Zugno, Tommaso, Michele Polese, Natale Patriciello, Biljana Bojović, Sandra Lagen, Michele Zorzi. “Implementation of a spatial channel model for ns-3.” In Proceedings of the 2020 Workshop on ns-3, pp. 49-56. 2020.

[Polese2018]

Michele Polese, Michele Zorzi. “Impact of channel models on the end-to-end performance of mmwave cellular networks”. In: 2018 IEEE 19th International Workshop on Signal Processing Advances in Wireless Communications (SPAWC).

[Rebato2018]

Rebato, Mattia, Laura Resteghini, Christian Mazzucco, Michele Zorzi. “Study of realistic antenna patterns in 5G mmWave cellular scenarios”. In: 2018 IEEE International Conference on Communications (ICC).

[Romero] (1,2)

Romero-Jerez, Juan M., F. Javier Lopez-Martinez, José F. Paris, Andrea J. Goldsmith. “The fluctuating two-ray fading model: Statistical characterization and performance analysis”. In: IEEE Transactions on Wireless Communications 16.7 (2017).

[Kulkarni] (1,2)

Kulkarni, Mandar N., Eugene Visotsky, Jeffrey G. Andrews. “Correction factor for analysis of MIMO wireless networks with highly directional beamforming.”, IEEE Wireless Communications Letters, 2018

[Asplund]

Asplund, Henrik, David Astely, Peter von Butovitsch, Thomas Chapman, Mattias Frenne, Farshid Ghasemzadeh, Måns Hagström et al. Advanced Antenna Systems for 5G Network Deployments: Bridging the Gap Between Theory and Practice. Academic Press, 2020.

30.4.4. 3GPP TR 38.811 Non-Terrestrial Networks¶

3GPP with [3GPPTR38811] has extended the channel model presented in [3GPPTR38901] to support the so called Non-Terrestrial Networks (NTN), i.e. communication scenarios where the propagation of the signal travels through the atmosphere. The channel spectrum estimation procedure is the same as the one described in [3GPPTR38901], with a new set of parameters.

30.4.4.1. Use-cases¶

The use-cases for this channel model include simulations in 3D/vertical environments with communicating nodes placed in different types of orbit, in the atmosphere and/or on the ground.

30.4.4.2. Implementation¶

The channel spectrum estimation procedure is already implemented (as described in [ns3Zugno] ) into the classes ThreeGppChannelModel and ThreeGppSpectrumPropagationLossModel, that have been extended to support NTN through the introduction of the appropriate parameters. 3GPP considers two frequencies of interest: S-band (2GHz) and Ka-band (20/30GHz). Many channel parameters are dependent on the frequency band in use, but no specific range of frequencies of these bands has been given by 3GPP. Hence, this implementation considers S-band anything below 13GHz, and Ka-band anything above it. Four propagation scenarios are identified, in decreasing order of building height and density: Dense Urban, Urban, Suburban and Rural. Channel estimation parameters are scenario-dependent. Note: For satellite, the parameters that describe the departure angle spread are 0. Thus, in the logarithmic scale at which these parameters are represented is $-\infty$ .

30.4.4.3. References¶

[ns3Zugno]

Zugno Tommaso, Michele Polese, Natale Patriciello, Biljana Bojović, Sandra Lagen, Michele Zorzi. “Implementation of a spatial channel model for ns-3.” In Proceedings of the 2020 Workshop on ns-3, pp. 49-56. 2020.

[3GPPTR38901] (1,2)