dor_id: 51601

506.#.#.a: Público

590.#.#.d: Los artículos enviados a la Revista Mexicana de Astronomía y Astrofísica se juzgan por medio de un proceso de revisión por pares

510.0.#.a: Consejo Nacional de Ciencia y Tecnología (CONACyT), Sistema Regional de Información en Línea para Revistas Científicas de América Latina, el Caribe, España y Portugal (Latindex), Scientific Electronic Library Online (SciELO), Science Citation Index, Astronomy and Astrophysics Abstracts, Physics Briefs (RMxAC), Astronomy and Astrophysics Monthly Index, PERIODICA, La Red de Revistas Científicas de América Latina y el Caribe, España y Portugal (RedALyC)

561.#.#.u: https://www.astroscu.unam.mx/IA/index.php?lang=es

650.#.4.x: Físico Matemáticas y Ciencias de la Tierra

336.#.#.b: article

336.#.#.3: Artículo de Investigación

336.#.#.a: Artículo

351.#.#.6: http://www.revistas.unam.mx/index.php/revmexaa/index

351.#.#.b: Revista Mexicana de Astronomía y Astrofísica

351.#.#.a: Artículos

harvesting_group: RevistasUNAM

270.1.#.p: Revistas UNAM. Dirección General de Publicaciones y Fomento Editorial, UNAM en revistas@unam.mx

590.#.#.c: Open Journal Systems (OJS)

270.#.#.d: MX

270.1.#.d: México

590.#.#.b: Concentrador

883.#.#.u: http://www.revistas.unam.mx/front/

883.#.#.a: Revistas UNAM

590.#.#.a: Coordinación de Difusión Cultural, UNAM

883.#.#.1: https://www.publicaciones.unam.mx/

883.#.#.q: Dirección General de Publicaciones y Fomento Editorial, UNAM

850.#.#.a: Universidad Nacional Autónoma de México

856.4.0.u: http://www.revistas.unam.mx/index.php/revmexaa/article/view/31419/29749

100.1.#.a: Aceves, H.; Reyes Ruiz, M.; Chavez, C. E.

524.#.#.a: Aceves, H., et al. (2012). Effects of Magnetic Turbulence on the Dynamics of Pickup Ions in the Ionosheath of Mars. Revista Mexicana de Astronomía y Astrofísica; Vol 48, No 1, 2012; 137-148. Recuperado de https://repositorio.unam.mx/contenidos/51601

245.1.0.a: Effects of Magnetic Turbulence on the Dynamics of Pickup Ions in the Ionosheath of Mars

502.#.#.c: Universidad Nacional Autónoma de México

561.1.#.a: Instituto de Astronomía, UNAM

264.#.0.c: 2012

264.#.1.c: 2012-04-24

506.1.#.a: La titularidad de los derechos patrimoniales de esta obra pertenece a las instituciones editoras. Su uso se rige por una licencia Creative Commons BY-NC-ND 4.0 Internacional, https://creativecommons.org/licenses/by-nc-nd/4.0/legalcode.es, fecha de asignación de la licencia 2012-04-24, para un uso diferente consultar al responsable jurídico del repositorio por medio del correo electrónico rmaa@astro.unam.mx

884.#.#.k: http://www.revistas.unam.mx/index.php/revmexaa/article/view/31419

001.#.#.#: oai:ojs.phoenicis.tic.unam.mx:article/31419

041.#.7.h: eng

520.3.#.a: We study some of the effects that magnetic turbulent fluctuations have on the dynamics of pickup O+ ions in the magnetic polar regions of the Mars ionosheath. In particular we study their effect on the bulk velocity profiles of ions as a function of altitude over the magnetic poles, in order to compare them with recent Mars Express data; that indicate that their average velocity is very low and essentially in the anti-sunward direction. We find that, while magnetic field fluctuations do give rise to deviations from simple E × B-drift gyromotion, even fluctuation amplitudes much greater than those of in situ measurements are not able to reproduce the vertical velocity profile of O+ ions. We conclude that other physical mechanisms, different from a pure charged particle dynamics, are acting on pickup ions at the Martian terminator. A possibility is a viscous-like interaction between the Solar Wind and the Martian ionosphere at low altitudes.We study some of the effects that magnetic turbulent fluctuations have on the dynamics of pickup O+ ions in the magnetic polar regions of the Mars ionosheath. In particular we study their effect on the bulk velocity profiles of ions as a function of altitude over the magnetic poles, in order to compare them with recent Mars Express data; that indicate that their average velocity is very low and essentially in the anti-sunward direction. We find that, while magnetic field fluctuations do give rise to deviations from simple E × B-drift gyromotion, even fluctuation amplitudes much greater than those of in situ measurements are not able to reproduce the vertical velocity profile of O+ ions. We conclude that other physical mechanisms, different from a pure charged particle dynamics, are acting on pickup ions at the Martian terminator. A possibility is a viscous-like interaction between the Solar Wind and the Martian ionosphere at low altitudes.

773.1.#.t: Revista Mexicana de Astronomía y Astrofísica; Vol 48, No 1 (2012); 137-148

773.1.#.o: http://www.revistas.unam.mx/index.php/revmexaa/index

046.#.#.j: 2021-08-03 00:00:00.000000

022.#.#.a: ISSN impreso: 0185-1101

310.#.#.a: Semestral

300.#.#.a: Páginas: 137-148

264.#.1.b: Instituto de Astronomía, UNAM

758.#.#.1: http://www.revistas.unam.mx/index.php/revmexaa/index

handle: 00bb6fd892ea4e17

harvesting_date: 2019-02-06 00:00:00.0

856.#.0.q: application/pdf

245.1.0.b: Effects of Magnetic Turbulence on the Dynamics of Pickup Ions in the Ionosheath of Mars

last_modified: 2021-08-12 16:00:00

license_url: https://creativecommons.org/licenses/by-nc-nd/4.0/legalcode.es

license_type: by-nc-nd

_deleted_conflicts: 2-3c648d041cb344f0eec6e13e4181dd1e

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