Numerical simulation of 3-D flow around sounding rocket in the lower thermosphere

Numerical simulations using the Direct Simulation Monte Carlo (DSMC) method are known to be useful for analyses of aerodynamic effects on in-situ rocket measurements in the lower thermosphere, but the DSMC analysis of a spin modulation caused by an asymmetric flow around the rocket spin axis has...

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Main Authors: J. Kurihara, K.-I. Oyama, N. Iwagami, T. Takahashi
Format: Article
Language:English
Published: Copernicus Publications 2006-03-01
Series:Annales Geophysicae
Online Access:https://www.ann-geophys.net/24/89/2006/angeo-24-89-2006.pdf
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spelling doaj-cd05ec8bced64d379d28704135c3c8022020-11-24T20:46:40ZengCopernicus PublicationsAnnales Geophysicae0992-76891432-05762006-03-0124899510.5194/angeo-24-89-2006Numerical simulation of 3-D flow around sounding rocket in the lower thermosphereJ. Kurihara0K.-I. Oyama1N. Iwagami2T. Takahashi3Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara, Kanagawa 229-8510, JapanInstitute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara, Kanagawa 229-8510, JapanDept. of Earth and Planetary Science, Graduate School of Science, University of Tokyo, Bunkyo-ku, Tokyo 113-0033, JapanInformation Science Laboratory, Tokai University, Hiratsuka, Kanagawa 259-1292, JapanNumerical simulations using the Direct Simulation Monte Carlo (DSMC) method are known to be useful for analyses of aerodynamic effects on in-situ rocket measurements in the lower thermosphere, but the DSMC analysis of a spin modulation caused by an asymmetric flow around the rocket spin axis has been restricted to the two-dimensional and axially symmetric simulations in actual sounding rocket experiments. This study provides a quantitative analysis of the spin modulation using a three-dimensional (3-D) simulation of the asymmetric flow with the DSMC method. Clear spin modulations in the lower thermospheric N<sub>2</sub> density measurement by a rocket-borne instrument are simulated using the rocket attitude and velocity, the simplified payload structure, and the approximated atmospheric conditions. Comparison between the observed and simulated spin modulations show a very good agreement within 5% at around 100km. The results of the simulation are used to correct the spin modulations and derive the absolute densities in the background atmosphere.https://www.ann-geophys.net/24/89/2006/angeo-24-89-2006.pdf
collection DOAJ
language English
format Article
sources DOAJ
author J. Kurihara
K.-I. Oyama
N. Iwagami
T. Takahashi
spellingShingle J. Kurihara
K.-I. Oyama
N. Iwagami
T. Takahashi
Numerical simulation of 3-D flow around sounding rocket in the lower thermosphere
Annales Geophysicae
author_facet J. Kurihara
K.-I. Oyama
N. Iwagami
T. Takahashi
author_sort J. Kurihara
title Numerical simulation of 3-D flow around sounding rocket in the lower thermosphere
title_short Numerical simulation of 3-D flow around sounding rocket in the lower thermosphere
title_full Numerical simulation of 3-D flow around sounding rocket in the lower thermosphere
title_fullStr Numerical simulation of 3-D flow around sounding rocket in the lower thermosphere
title_full_unstemmed Numerical simulation of 3-D flow around sounding rocket in the lower thermosphere
title_sort numerical simulation of 3-d flow around sounding rocket in the lower thermosphere
publisher Copernicus Publications
series Annales Geophysicae
issn 0992-7689
1432-0576
publishDate 2006-03-01
description Numerical simulations using the Direct Simulation Monte Carlo (DSMC) method are known to be useful for analyses of aerodynamic effects on in-situ rocket measurements in the lower thermosphere, but the DSMC analysis of a spin modulation caused by an asymmetric flow around the rocket spin axis has been restricted to the two-dimensional and axially symmetric simulations in actual sounding rocket experiments. This study provides a quantitative analysis of the spin modulation using a three-dimensional (3-D) simulation of the asymmetric flow with the DSMC method. Clear spin modulations in the lower thermospheric N<sub>2</sub> density measurement by a rocket-borne instrument are simulated using the rocket attitude and velocity, the simplified payload structure, and the approximated atmospheric conditions. Comparison between the observed and simulated spin modulations show a very good agreement within 5% at around 100km. The results of the simulation are used to correct the spin modulations and derive the absolute densities in the background atmosphere.
url https://www.ann-geophys.net/24/89/2006/angeo-24-89-2006.pdf
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