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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Copernicus Publications
2006-03-01
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Series: | Annales Geophysicae |
Online Access: | https://www.ann-geophys.net/24/89/2006/angeo-24-89-2006.pdf |
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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 |
work_keys_str_mv |
AT jkurihara numericalsimulationof3dflowaroundsoundingrocketinthelowerthermosphere AT kioyama numericalsimulationof3dflowaroundsoundingrocketinthelowerthermosphere AT niwagami numericalsimulationof3dflowaroundsoundingrocketinthelowerthermosphere AT ttakahashi numericalsimulationof3dflowaroundsoundingrocketinthelowerthermosphere |
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1716811894348578816 |