Suprathermal particles in the planetary atmospheres
A non-equilibrium state of the atmospheric multi-component gas as an
open thermodynamical system is triggered and
maintained by the incident solar EUV and corpuscular radiation, with the
involvement of successive collisional relaxation and numerous chemical
reactions responsible for the system evolution. The original photolytic and
energetic electron impact processes of interaction and the physical and
chemical evolutionary processes can be described by a set of nonlinear
Boltzmann type equations with the source term. Instead of a direct solution of
these equations facing many obstacles, a special technique of stochastic
simulation and Monte-Carlo algorithms were used for the numerical computer
evaluation of such a system. This powerful technique allowed to study in detail
the non-equilibrium state of the rarefied atmospheric gas at both microscopic
(molecular) and macroscopic (continuum) levels and, in particular, to estimate
the input of nonthermal particles into the composition, energetics,
and dynamics of the planetary upper atmospheres. The main objectives were to
reveal specific effects of the processes of non-equilibrium kinetics in terms
of their domain and/or significant contribution to the macroscopic state of the
atmospheric system. These included:
-the detailed quantitative study of the
kinetics of photolysis and energetic electron impacts involving estimates of
the dissociation and ionization production rates and formation of molecules and
atoms in different states of excitation:
Numerical stochastic simulation of kinetics of atmospheric
photochemistry.
In:
Marov M. (Ed.) Mathematical problems of applied aeronomy, 1987, Keldysh
Inst. of Applied Math., Moscow, 199-209, (in Russian).
-the multichannel
processes of the formation, collisional relaxation, and transport of the
"hot" particles of photochemical origin (superthermal
H, C, N, and O) leading to the formation of hot planetary coronas:
Kinetic approach to the
mathematical modelling of collisional physical and
chemical processes in planetary atmospheres (abstract).
In: Rarefied gas dynamics;
Proceedings of the 17th International Symposium,
1991,
Numerical kinetic
simulation of the upper atmosphere photochemistry and dynamics (abstract).
Advances Space Res., 1992, 12,
303.
Superthermal particles in the planetary atmosphere.
In: Massevitch
A.G. (Ed.) Non-stable processes in the Universe,
Nonequilibrium
processes in the planetary and cometary atmospheres. A kinetic approach to modeling.
Space Science Reviews, 1996, 76,
Nos. 1/2, 1-202.
Nonequilibrium
processes in the planetary and cometary atmospheres:
Theory and Applications.
1997, Kluwer Academic Publishers,
Earth:
-the photochemistry of odd-nitrogen and its influence on the composition
of the lower thermosphere of the Earth:
Non-thermal nitrogen atoms in the
earth's thermosphere. I - Kinetics of hot N(4S) (abstract).
Geophysical Research
Letters, 1991, 18, 1691.
Non-thermal nitrogen atoms in the
earth's thermosphere. II - A source of nitric oxide (abstract).
Geophysical
Research Letters, 1991,18, 1695.
The
thermospheric odd nitrogen photochemistry
: role of non-thermal N(4S) atoms (abstract).
Ann.
Geophys., 1992, 10, 792.
Effect of hot N(4S)
atoms on the NO solar cycle variation in the lower thermosphere(abstract).
J. Geophys. Res., 1993, 98, 11581.
The
role of fast N(4S) atoms and photoelectrons on the
distribution of NO in the thermosphere(abstract).
In: The Upper Mesosphere and Lower Thermosphere: A
Review of Experiment and Theory, Geophysical Monograph 87,
1995, American Geophysical
An
updated model of the hot nitrogen atom kinetics and thermospheric
nitric oxide(abstract).
J. Geophys. Res., 1997, 102, No.A1, 285.
TITAN:
- kinetics and dynamics of hot nitrogen in the
upper atmosphere:
Kinetic modeling of superthermal nitrogen atoms in the Titan's atmosphere.I.
Sources (
abstract).
Solar System Research (English
translation of "Astronomicheskij Vestnik"), 1998,32,
No.5 , 384.
Titan's
atmospheric haze: the case for HCN incorporation (abstract).
Astronomy and Astrophysics, 1999, 341,
312-317.
COMETS:
-the kinetic effects and peculiarities of the subliming gas flow in the
near-surface (Knudsen) layer of the cometary nucleus:
· Bisikalo, D. V.; Marov,
M. Ya.; Shematovich, and V. I.; Strel'Nitskij,
V. S.
The flow of the subliming gas in the
near-nuclear (Knudsen) layer of the cometary coma(abstract).
Advances Space Res., 1989, 9,
53.
Kinetic investigations
of the near-surface phenomena in the gas and dust envelopes of small celestial
bodies.
In: Rarefied
Gas Dynamics-19 (ed. by J. Harvey and G. Lord), 1995,
-the photochemistry and dynamics of the rarefied gas in the inner cometary coma:
· Bisikalo, D. V.; Shematovich, V. I.
Numerical
modeling of the nonequilibrium flow of a rarefied gas
in the inner coma of a comet (abstract).
Solar System Research
(English translation of "Astonomicheskij Vestnik"), 1999, 33, No.1, 36.
·
Pyarnpuu, A.A., Shematovich, V.I., Svirschevsky
S.B., and Titov E.V.
Nonequilibrium
jet flows in the coma of a comet
In: Rarefied
Gas Dynamics 20 (ed. by Shen Ching),
1997,