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walkerDelta

Create Walker-Delta constellation in satellite scenario

Description

example

sat = walkerDelta(scenario,radius,inclination,totalSatellites,geometryPlanes,phasing) creates an array of satellites, sat, inside the satellite scenario scenario using specified geometric properties such as radius, radius, inclination, inclination, total number of satellites, totalSatellites, number of geometry planes, geometryPlanes, and phasing between satellites, phasing. For more information on Walker-Delta constellations, see Algorithms.

sat = walkerDelta(__,Name=Value) creates an array of satellites using one or more optional Name=Value arguments. Use this option with any of the input argument combinations in the previous syntax.

Examples

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Model a Galileo constellation as a Walker-Delta constellation that contains 24 satellites in three planes inclined at 56 degrees (56:24/3/1) in a 29599.8 km orbit. Provide an initial argument of latitude offset of 15 degrees.

Create a default satellite scenario object.

sc = satelliteScenario;

Create Walker-Delta constellation that contains 24 satellites in three planes inclined at 56 degrees (56:24/3/1) in a 29599.8 kilometer orbit.

sat = walkerDelta(sc, 29599.8e3, 56, 24, 3, 1, ...
       ArgumentOfLatitude=15, Name="Galileo");

Visualize the scenario using the Satellite Scenario Viewer.

satelliteScenarioViewer(sc);

Input Arguments

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Satellite scenario, specified as a satelliteScenario object.

Orbital radius, specified as a scalar, in meters.

Data Types: double

Inclination, specified as a scalar, in degrees.

Data Types: double

Total number of satellites, specified as a scalar positive integer.

Data Types: double

Number of equally spaced geometry planes, specified as a scalar positive integer.

Data Types: double

Phasing between satellites in adjacent planes, specified as a scalar integer greater than or equal to 0 and less than geometryPlanes. The change in true anomaly for equivalent satellites in neighboring planes is calculated as:

(phasing*360/totalSatellites).

Data Types: double

Name-Value Arguments

Specify optional pairs of arguments as Name1=Value1,...,NameN=ValueN, where Name is the argument name and Value is the corresponding value. Name-value arguments must appear after other arguments, but the order of the pairs does not matter.

Example: sat = walkerDelta(sc,29599.8e3,56, 24,3,1,Name="Galileo") creates an array of satellites named Galileo.

Right ascension of ascending node, specified as a scalar value from 0 to 360. RAAN is the angle in the equatorial plane from the x-axis to the location of the ascending node, point at which the satellite crosses the equator from south to north, in degrees. The function uses this value as the starting point for distribution of the satellites along the equator.

Data Types: double

Argument of latitude, specified as a scalar value from 0 to 360. ArgumentOfLatitude is the angle between the ascending node and the body. The function uses this value as the starting point for distribution of satellites along the first orbital track.

Data Types: double

Constellation name, specified as a scalar.

Individual satellite names within the constellation use the constellation name appended with increasing whole numbers starting with 1, for example, Name_1, Name_2, and so forth.

Data Types: char | string

Name of orbit propagator used for propagating satellite position and velocity, specified as:

  • "two-body-keplerian" — Two-Body-Keplerian orbit propagator based on the relative two-body model that assumes a spherical gravity field for the Earth and neglects third body effects and other environmental perturbations. It is considered the least accurate.

  • "sgp4" — Simplified General Perturbations-4 orbit propagator.

  • "sdp4" — Simplified Deep-Space Perturbations-4 orbit propagator.

Data Types: string | char

Output Arguments

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Satellite in scenario, returned as an array of Satellite objects.

Algorithms

Walker-Delta constellations are a common solution for maximizing geometric coverage over Earth while minimizing the number of satellites required to perform the mission. Walker-Delta constellation patterns use the notation:

I:T/P/F.
where:

  • I — Orbital inclination

  • T — Total number of satellites, which must be divisible by F

  • P — Number of equally spaced geometric planes

  • F — Phasing between satellites in adjacent planes

To define the radial height of the circular orbit (with respect to the Earth center), the function also requires a radius r.

In addition:

  • The ascending nodes of the orbital planes of a Walker-Delta constellation are uniformly distributed at intervals of 360/P deg around the equator.

  • The number of satellites per plane, satellitesPerPlane, is defined as

    satellitesPerPlane=T/P.

    The satellites in each orbital plane are distributed at intervals of 360/satellitesPerPlane deg. F represents the interplane phasing, the number of empty slots between the first satellites in each orbital plane.

Version History

Introduced in R2022a