A brief selection of problems occurring in the interpretation of planetary atmospheres, the resolution of which demands a knowledge of atomic collision processes, is presented. The selection is largely arbitrary.Physic
As the search for Earth-like exoplanets gathers pace, in order to understand them, we need comprehen...
Part I: This thesis consists of two chapters concerning photochemical processes in the atmosphe...
The paper discusses the following: 1. F + Cl2 Kinetics. Absolute rate constant for the reaction F(P-...
We propose to establish a long-term program of critical evaluation by domain experts of the rates an...
Progress in the following research supported under NSG 7386 is reported: (1) measurement of differen...
Spacecraft and groundbased observations of the atmospheres of solar system objects have provided a d...
The present state of planetary exospheres is determined largely by satellite and ground based obser...
The emphasis of this book is on comparative aspects of planetary atmospheres, generally meaning comp...
Abstract In this chapter we describe the current knowledge of a selection of collision processes and...
An analysis of the collisional transition between the lower atmosphere and the collisionless exosphe...
In this chapter we describe the current knowledge of a selection of collision processes and chemical...
The modeling of atmospheric gas, interacting with the space vehicles in re-entry conditions in plane...
More than half of the planets so far discovered have masses between Earth andNeptune. These ‘Super-E...
All nine planets, four moons, and most comets have atmospheres. These gaseous envelopes are remarka...
Planetary atmosphere composition, temperature, and pressure of Mars, Venus, and Jupite
As the search for Earth-like exoplanets gathers pace, in order to understand them, we need comprehen...
Part I: This thesis consists of two chapters concerning photochemical processes in the atmosphe...
The paper discusses the following: 1. F + Cl2 Kinetics. Absolute rate constant for the reaction F(P-...
We propose to establish a long-term program of critical evaluation by domain experts of the rates an...
Progress in the following research supported under NSG 7386 is reported: (1) measurement of differen...
Spacecraft and groundbased observations of the atmospheres of solar system objects have provided a d...
The present state of planetary exospheres is determined largely by satellite and ground based obser...
The emphasis of this book is on comparative aspects of planetary atmospheres, generally meaning comp...
Abstract In this chapter we describe the current knowledge of a selection of collision processes and...
An analysis of the collisional transition between the lower atmosphere and the collisionless exosphe...
In this chapter we describe the current knowledge of a selection of collision processes and chemical...
The modeling of atmospheric gas, interacting with the space vehicles in re-entry conditions in plane...
More than half of the planets so far discovered have masses between Earth andNeptune. These ‘Super-E...
All nine planets, four moons, and most comets have atmospheres. These gaseous envelopes are remarka...
Planetary atmosphere composition, temperature, and pressure of Mars, Venus, and Jupite
As the search for Earth-like exoplanets gathers pace, in order to understand them, we need comprehen...
Part I: This thesis consists of two chapters concerning photochemical processes in the atmosphe...
The paper discusses the following: 1. F + Cl2 Kinetics. Absolute rate constant for the reaction F(P-...
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