A Fast Bow Shock Location Predictor-Estimator From 2D and 3D Analytical Models: Application to Mars and the MAVEN Mission.

MAVEN mission Mars analytical empirical models bow shock magnetometer data

Journal

Journal of geophysical research. Space physics
ISSN: 2169-9380
Titre abrégé: J Geophys Res Space Phys
Pays: United States
ID NLM: 101661799

Informations de publication

Date de publication:
Jan 2022
Historique:
received: 06 09 2021
revised: 30 11 2021
accepted: 21 12 2021
entrez: 22 7 2022
pubmed: 23 7 2022
medline: 23 7 2022
Statut: ppublish

Résumé

We present fast algorithms to automatically estimate the statistical position of the bow shock from spacecraft data, using existing analytical two-dimensional (2D) and three-dimensional (3D) models of the shock surface. We derive expressions of the standoff distances in 2D and 3D and of the normal to the bow shock at any given point on it. Two simple bow shock detection algorithms are constructed, one solely based on a geometrical predictor from existing models, the other using this predicted position to further refine it with the help of magnetometer data, an instrument flown on many planetary missions. Both empirical techniques are applicable to any planetary environment with a defined shock structure. Applied to the Martian environment and the NASA/MAVEN mission, the predicted shock position is on average within 0.15 planetary radius

Identifiants

pubmed: 35865029
doi: 10.1029/2021JA029942
pii: JGRA56973
pmc: PMC9285960
doi:

Banques de données

figshare
['10.6084/m9.figshare.6356420']

Types de publication

Journal Article

Langues

eng

Pagination

e2021JA029942

Informations de copyright

©2022. The Authors.

Références

J Geophys Res Space Phys. 2022 Jan;127(1):e2021JA029942
pubmed: 35865029
Science. 1998 Mar 13;279(5357):1676-80
pubmed: 9497279

Auteurs

Cyril Simon Wedlund (C)

Space Research Institute Austrian Academy of Sciences Graz Austria.

Martin Volwerk (M)

Space Research Institute Austrian Academy of Sciences Graz Austria.

Arnaud Beth (A)

Department of Physics Umeå University Umeå Sweden.

Christian Mazelle (C)

Institut de Recherche en Astrophysique et Planétologie Université de Toulouse CNRS UPS CNES Toulouse France.

Christian Möstl (C)

Space Research Institute Austrian Academy of Sciences Graz Austria.

Jasper Halekas (J)

Department of Physics and Astronomy University of Iowa Iowa City IA USA.

Jacob R Gruesbeck (JR)

NASA Goddard Space Flight Center Laboratory for Planetary Magnetospheres Greenbelt MD USA.

Diana Rojas-Castillo (D)

Instituto de Geofísica Universidad Nacional Autónoma de México Coyoacán Mexico.

Classifications MeSH