Debris evolution in the EVOLVE model: application to DSMC modelling

Details Debris evolution in the EVOLVE model: application to DSMC modelling Debris evolution in the EVOLVE model: application to DSMC modelling

Oct 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001esasp.473..397s&link_type=abstract

In: Proceedings of the Third European Conference on Space Debris, 19 - 21 March 2001, Darmstadt, Germany. Ed.: Huguette Sawaya-L

Statistics

Methodology

Space Debris, Modelling

Scientific paper

Investigation is presented of the evolution of debris clouds generated by the EVOLVE model which has been recently updated. Simulation of debris clouds assumes perturbations due to the Earth's gravitational potential to degree 4, and aerodynamic drag. It is found that above an altitude of 700 km, a debris cloud has sufficient time to become fully developed, and that the orbital elements of Right Ascension of the Ascending Node and the Argument of Perifocus at epoch are lost. These conditions are those necessary for the Direct Simulation Monte Carlo method used to model debris risk. Below 700 km the methodology is still found to be justified when there has not been a recent injection of a substantial volume of debris below 700 km.

Affiliated with

Also associated with

No associations

Rating

Debris evolution in the EVOLVE model: application to DSMC modelling does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Debris evolution in the EVOLVE model: application to DSMC modelling, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Debris evolution in the EVOLVE model: application to DSMC modelling will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1105578