The ‘Particles-in-a-box’ (PIB) model introduced by Talent (1992) removed the need for computer-intensive Monte Carlo simulation to predict the gross characteristics of an evolving debris environment. The PIB model was described using a differential equation that allows the stability of the low Earth orbit (LEO) environment to be tested by a straightforward analysis of the equation’s coefficients. As part of an ongoing research effort to investigate more efficient approaches to evolutionary modelling and to develop a suite of educational tools, a new PIB model has been developed. The model, entitled Fast Debris Evolution (FaDE), employs a first-order differential equation to describe the rate at which new objects ?10 cm) are added and remove...
Over 120 cases of on-orbit breakups have now been recorded. Many more undetected events are believed...
It is well known that the increasing space activities pose a serious threat to future missions. This...
Current debris evolutionary models usually neglect fragments smaller than 10 cm because of the high ...
The ‘Particles-in-a-box’ (PIB) model introduced by Talent (1992) removed the need for computer-inten...
The GEO regime represents a growing debris environment that poses a significant long-term collision ...
Orbital space debris is a threat to space operations and for this reason numerous studies have been ...
The space debris population is similar to the asteroid belt, since it is subject to a process of hig...
The importance of modelling the historical evolution of the orbital debris environment is discussed....
During the past 60 years the number of objects on Earth orbits has increased. So has the risk of col...
Several numerical approaches exist to simulate the evolution of the space debris environment. These ...
Orbital debris environment models are essential in predicting the characteristics of the entire debr...
The space debris model MASTER-2009 is based on the simulation of historical fragmentation events tha...
Over the last two decades the rise of NewSpace has led to a transition away from traditional space o...
As the space debris population continues to increase, there is a growing need to develop models that...
This work presents a source-sink debris evolutionary model of the Low Earth Orbit (LEO) with a propo...
Over 120 cases of on-orbit breakups have now been recorded. Many more undetected events are believed...
It is well known that the increasing space activities pose a serious threat to future missions. This...
Current debris evolutionary models usually neglect fragments smaller than 10 cm because of the high ...
The ‘Particles-in-a-box’ (PIB) model introduced by Talent (1992) removed the need for computer-inten...
The GEO regime represents a growing debris environment that poses a significant long-term collision ...
Orbital space debris is a threat to space operations and for this reason numerous studies have been ...
The space debris population is similar to the asteroid belt, since it is subject to a process of hig...
The importance of modelling the historical evolution of the orbital debris environment is discussed....
During the past 60 years the number of objects on Earth orbits has increased. So has the risk of col...
Several numerical approaches exist to simulate the evolution of the space debris environment. These ...
Orbital debris environment models are essential in predicting the characteristics of the entire debr...
The space debris model MASTER-2009 is based on the simulation of historical fragmentation events tha...
Over the last two decades the rise of NewSpace has led to a transition away from traditional space o...
As the space debris population continues to increase, there is a growing need to develop models that...
This work presents a source-sink debris evolutionary model of the Low Earth Orbit (LEO) with a propo...
Over 120 cases of on-orbit breakups have now been recorded. Many more undetected events are believed...
It is well known that the increasing space activities pose a serious threat to future missions. This...
Current debris evolutionary models usually neglect fragments smaller than 10 cm because of the high ...