Asymptotics for spherical particle motion in a spherically expanding flow
Autor: | Stavro Ivanovski, Alessandra Rotundi, V. Della Corte, Vladimir Zakharov, Jean-François Crifo, Marco Fulle |
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Přispěvatelé: | Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA (UMR_8109)), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Istituto di Astrofisica e Planetologia Spaziali - INAF (IAPS), Istituto Nazionale di Astrofisica (INAF), Dipartimento di Scienze e Tecnologie [Napoli] (DIST), Universita degli studi di Napoli 'Parthenope' [Napoli], IMPEC - LATMOS, Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS), Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), INAF - Osservatorio Astronomico di Trieste (OAT), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), PLANETO - LATMOS, Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS) |
Jazyk: | angličtina |
Rok vydání: | 2018 |
Předmět: |
Physics
010504 meteorology & atmospheric sciences Terminal velocity [SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph] Mathematical analysis Comets: General Astronomy and Astrophysics Context (language use) Parameter space dust dynamics 01 natural sciences Numerical integration numerical simulations Methods: Numerical simulations Flow (mathematics) Space and Planetary Science Comets: General Dust dynamics Methods: Numerical simulations Ordinary differential equation 0103 physical sciences comets 010303 astronomy & astrophysics Magnetosphere particle motion 0105 earth and related environmental sciences Dimensionless quantity |
Zdroj: | Icarus Icarus, Elsevier, 2018, 312, pp.121-127. ⟨10.1016/j.icarus.2018.04.030⟩ |
ISSN: | 0019-1035 1090-2643 |
DOI: | 10.1016/j.icarus.2018.04.030⟩ |
Popis: | International audience; In the context of an increasing number of complex multiparametric dust coma models it was found convenient to construct an elementary model with a minimum number of parameters selected to represent the key processes acting on the dust. The models outputs can be used as a reference evaluation of these processes with rough estimates of the resulting dust properties e.g. velocity.The present work introduces three, universal, dimensionless parameters which characterize the dust motion in an expanding flow, and computes as a function of these parameters the dust terminal velocity, the time it takes to acquire it, and the distance at which it is acquired.The motion of dust grains is presented as a system of dimensionless ordinary differential equations the solution of which depends upon the above mentioned three parameters. The numerical integration of this system was performed over a wide range of parameter space covering the whole range of physically possible conditions.Precomputed results of dust terminal velocity, time and distance where it is reached are presented in dimensionless form. To obtain dimensional values for a particular case it is sufficient to perform algebraic operations. |
Databáze: | OpenAIRE |
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