The problem of secular growth of the inter-satellite induced by the J2 perturbations has been widely exploredin the literature. In this paper, we study the influence of altitude and initial mean anomaly of the chief on theinter-satellite distance growth in a classical trailing formation. Mean elements are converted into osculatingones and then in Cartesian coordinates that are propagated together in the ECI frame. Preliminary resultsshows that zonal harmonics are responsible for a steep distance drift when the formation is inserted inthe vicinity of ±45 and ±135 degrees of mean anomaly in a polar orbit. Distance-invariant solutions aredetermined in term of the mean anomaly and characterized in terms of the difference between the averagerela...
Paper given at Dynamics and Control of Systems and Structures in Space (DCSSS), 6th conference, Ri...
Generally, any initially-close satellites-chief and deputy-moving on orbits with slightly different ...
AbstractThree techniques for station keeping an orbiting constellation of satellites in an elliptica...
The inclusion of the linearized J2 effect in the Hill equations of relative motion gives greater in...
Formation flying is a new satellite mission concept that is concerned with clusters of satellites in...
The purpose of this thesis is to examine the secular effects of the J2 oblateness perturbation on cl...
We study the dynamics of the relative motion of satellites in the gravitational field of the Earth,...
Several methods are presented for the design of satellite formations for science missions in high-ec...
In the latest years there has been a growing interest in satellite formation flight and distributed ...
The problem of Earth satellite constellation and formation flight is investigated in the context of ...
The aim of this paper is to present the analysis conducted by CNES for the maintenance of a formatio...
The initial conditions that generate bounded motion in eccentric reference orbit are determined for ...
This paper addresses the problem of bringing two satellites on different orbital planes together and...
With high-precision DEM (Digital Elevation Model) and GMTI (Ground Moving Target Indicator) as the d...
The Centre for Large Space Structures and Systems Inc. (CLS3) is planning a low Earth orbit formati...
Paper given at Dynamics and Control of Systems and Structures in Space (DCSSS), 6th conference, Ri...
Generally, any initially-close satellites-chief and deputy-moving on orbits with slightly different ...
AbstractThree techniques for station keeping an orbiting constellation of satellites in an elliptica...
The inclusion of the linearized J2 effect in the Hill equations of relative motion gives greater in...
Formation flying is a new satellite mission concept that is concerned with clusters of satellites in...
The purpose of this thesis is to examine the secular effects of the J2 oblateness perturbation on cl...
We study the dynamics of the relative motion of satellites in the gravitational field of the Earth,...
Several methods are presented for the design of satellite formations for science missions in high-ec...
In the latest years there has been a growing interest in satellite formation flight and distributed ...
The problem of Earth satellite constellation and formation flight is investigated in the context of ...
The aim of this paper is to present the analysis conducted by CNES for the maintenance of a formatio...
The initial conditions that generate bounded motion in eccentric reference orbit are determined for ...
This paper addresses the problem of bringing two satellites on different orbital planes together and...
With high-precision DEM (Digital Elevation Model) and GMTI (Ground Moving Target Indicator) as the d...
The Centre for Large Space Structures and Systems Inc. (CLS3) is planning a low Earth orbit formati...
Paper given at Dynamics and Control of Systems and Structures in Space (DCSSS), 6th conference, Ri...
Generally, any initially-close satellites-chief and deputy-moving on orbits with slightly different ...
AbstractThree techniques for station keeping an orbiting constellation of satellites in an elliptica...