Grating Lobes and Spatial Aliasing in Sparse Array Beampatterns
Calculated beam pattern in Fourier space of a unitary input given two sparsely sampled synthetic aperture arrays: 1. a regularly spaced array sampled at 2*lambda, where lambda is the wavelength of the 40 GHz signal, and 2. the regularly spaced array with random perturbations (of order ~
Resources
6 resources available
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PLAIN TEXT
Dataset use, references, and contact information
PLAIN TEXT -
ORGANIZED WITH X DATA GIVEN IN THE FIRST COLUMN AND, FOR LINE PLOTS, Y DATA GIVEN IN SUBSEQUENT COLUMNS OR, FOR SURFACE PLOTS, Y DATA GIVEN IN THE SECOND COLUMN AND Z OR COLOR DATA GIVEN IN THE THIRD COLUMN. COLUMN HEADERS DEFINE EACH AXIS WITH UNITS REPORTED AS "_UNITS".
Data to generate Fig. 21: Sparse Array Before and After Optimization
ORGANIZED WITH X DATA GIVEN IN THE FIRST COLUMN AND, FOR LINE PLOTS, Y DATA GIVEN IN SUBSEQUENT COLUMNS OR, FOR SURFACE PLOTS, Y DATA GIVEN IN THE SECOND COLUMN AND Z OR COLOR DATA GIVEN IN THE THIRD COLUMN. COLUMN HEADERS DEFINE EACH AXIS WITH UNITS REPORTED AS "_UNITS". -
MATLAB FUNCTION
Matlab function to compute 2D FFT
MATLAB FUNCTION -
MATLAB SCRIPT
Matlab code to recreate Fig. 20
MATLAB SCRIPT -
ORGANIZED WITH X DATA GIVEN IN THE FIRST COLUMN AND, FOR LINE PLOTS, Y DATA GIVEN IN SUBSEQUENT COLUMNS OR, FOR SURFACE PLOTS, Y DATA GIVEN IN THE SECOND COLUMN AND Z OR COLOR DATA GIVEN IN THE THIRD COLUMN. COLUMN HEADERS DEFINE EACH AXIS WITH UNITS REPORTED AS "_UNITS".
Data to generate Fig. 22: Optimized Sparse Array Beam Pattern
ORGANIZED WITH X DATA GIVEN IN THE FIRST COLUMN AND, FOR LINE PLOTS, Y DATA GIVEN IN SUBSEQUENT COLUMNS OR, FOR SURFACE PLOTS, Y DATA GIVEN IN THE SECOND COLUMN AND Z OR COLOR DATA GIVEN IN THE THIRD COLUMN. COLUMN HEADERS DEFINE EACH AXIS WITH UNITS REPORTED AS "_UNITS". -
ORGANIZED WITH X DATA GIVEN IN THE FIRST COLUMN AND, FOR LINE PLOTS, Y DATA GIVEN IN SUBSEQUENT COLUMNS OR, FOR SURFACE PLOTS, Y DATA GIVEN IN THE SECOND COLUMN AND Z OR COLOR DATA GIVEN IN THE THIRD COLUMN. COLUMN HEADERS DEFINE EACH AXIS WITH UNITS REPORTED AS "_UNITS".
Data to generate Fig. 20: Grating Lobes Due to Sparse Sampling Grid
ORGANIZED WITH X DATA GIVEN IN THE FIRST COLUMN AND, FOR LINE PLOTS, Y DATA GIVEN IN SUBSEQUENT COLUMNS OR, FOR SURFACE PLOTS, Y DATA GIVEN IN THE SECOND COLUMN AND Z OR COLOR DATA GIVEN IN THE THIRD COLUMN. COLUMN HEADERS DEFINE EACH AXIS WITH UNITS REPORTED AS "_UNITS".
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Complete Metadata
| @type | dcat:Dataset |
|---|---|
| accessLevel | public |
| accrualPeriodicity | irregular |
| bureauCode |
[
"006:55"
]
|
| contactPoint |
{
"fn": "Mohamed Hany",
"hasEmail": "mailto:mohamed.hany@nist.gov"
}
|
| description | Calculated beam pattern in Fourier space of a unitary input given two sparsely sampled synthetic aperture arrays: 1. a regularly spaced array sampled at 2*lambda, where lambda is the wavelength of the 40 GHz signal, and 2. the regularly spaced array with random perturbations (of order ~<lambda) to the (x,y) spatial location of each sample point. This dataset is published in "An Overview of Advances in Signal Processing Techniques for Classical and Quantum Wideband Synthetic Apertures" by Vouras, et al. in IEEE Selected Topics in Signal Processing Recent Advances in Wideband Signal Processing for Classical and Quantum Synthetic Apertures. |
| distribution |
[
{
"title": "Dataset use, references, and contact information",
"format": "plain text",
"mediaType": "text/plain",
"description": ""Readme" file provided additional information relating to "Grating Lobes and Spatial Aliasing in Sparse Array Beampatterns" simulation dataset.",
"downloadURL": "https://data.nist.gov/od/ds/mds2-2595/readme.txt"
},
{
"title": "Data to generate Fig. 21: Sparse Array Before and After Optimization",
"format": "Organized with x data given in the first column and, for line plots, y data given in subsequent columns or, for surface plots, y data given in the second column and z or color data given in the third column. Column headers define each axis with units reported as "_units".",
"mediaType": "text/csv",
"description": "A simple approach for mitigating grating lobes in a sparse lattice is to perturb the regularity of the grid spacing by applying a random offset to each spatial sample. These data compare the spatial locations of a regularly sampled sparse array labeled as "Before" to the randomly perturbed sparse array sample locations labeled as "After".",
"downloadURL": "https://data.nist.gov/od/ds/mds2-2595/Fig21_SparseArrayBeforeAndAfterOptimization.csv"
},
{
"title": "Matlab function to compute 2D FFT",
"format": "Matlab function",
"mediaType": "application/octet-stream",
"description": "Matlab function to compute the two-dimensional spatial Fast Fourier Transform (FFT) of an input spatially sampled array along x and y (input variables "array_x" and "array_y") given a wavelength ("lambda"), Fourier space sampling "U" and "V", and signal magnitude at each spatial location ("temp").",
"downloadURL": "https://data.nist.gov/od/ds/mds2-2595/compute_FFT.m"
},
{
"title": "Matlab code to recreate Fig. 20",
"format": "Matlab script",
"mediaType": "application/octet-stream",
"description": "Matlab script will generate the exact data provided in "Fig20_GratingLobesDueToSparseSamplingGrid.csv" and will plot the output. This script requires "compute_FFT.m" to be located in the same workspace or directory. To generate the output data given in "Fig22_OptimizedSparseArrayBeamPattern.csv", one can replace "sparse_array_x" (line 20) and "sparse_array_y" (line 21) with the first two columns of "Fig21_SparseArrayBeforeAndAfterOptimization.csv" ("Xposition_m" and "Yposition_m_After").",
"downloadURL": "https://data.nist.gov/od/ds/mds2-2595/Code_to_recreate_Figure_20.m"
},
{
"title": "Data to generate Fig. 22: Optimized Sparse Array Beam Pattern",
"format": "Organized with x data given in the first column and, for line plots, y data given in subsequent columns or, for surface plots, y data given in the second column and z or color data given in the third column. Column headers define each axis with units reported as "_units".",
"mediaType": "text/csv",
"description": "Periodicity in the beam pattern, here calculated and reported in Fourier space (u=sin(theta)cos(phi), v=sin(theta)sin(phi), where theta is the elevation angle and phi is the azimuth angle), is eliminated by the use of the randomly perturbed spatial sample locations of the sparse array. These simulated data show the outcome of using the sparse array labeled "After" in dataset "Fig21_SparseArrayBeforeAndAfterOptimization.csv" and provides a comparison to this randomized perturbation to the regular sampling output given in "Fig20_GratingLobesDueToSparseSamplingGrid.csv".",
"downloadURL": "https://data.nist.gov/od/ds/mds2-2595/Fig22_OptimizedSparseArrayBeamPattern.csv"
},
{
"title": "Data to generate Fig. 20: Grating Lobes Due to Sparse Sampling Grid",
"format": "Organized with x data given in the first column and, for line plots, y data given in subsequent columns or, for surface plots, y data given in the second column and z or color data given in the third column. Column headers define each axis with units reported as "_units".",
"mediaType": "text/csv",
"description": "Sparsely sampled lattices on a regular grid introduce grating lobes in the beampattern as demonstrated by this simulated dataset of the beam pattern observed in Fourier space (u=sin(theta)cos(phi), v=sin(theta)sin(phi), where theta is the elevation angle and phi is the azimuth angle) when a regularly sampled sparse array is used to acquire the signal.",
"downloadURL": "https://data.nist.gov/od/ds/mds2-2595/Fig20_GratingLobesDueToSparseSamplingGrid.csv"
}
]
|
| identifier | ark:/88434/mds2-2595 |
| keyword |
[
"millimeter-wave",
"sparse array",
"synthetic aperture"
]
|
| landingPage | https://data.nist.gov/od/id/mds2-2595 |
| language |
[
"en"
]
|
| license | https://www.nist.gov/open/license |
| modified | 2022-03-31 00:00:00 |
| programCode |
[
"006:045"
]
|
| publisher |
{
"name": "National Institute of Standards and Technology",
"@type": "org:Organization"
}
|
| theme |
[
"Advanced Communications:Wireless (RF)"
]
|
| title | Grating Lobes and Spatial Aliasing in Sparse Array Beampatterns |
