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Open AccessJournal ArticleDOI

A statistical study of the cross‐shock electric potential at low Mach number, quasi‐perpendicular bow shock crossings using Cluster data

TLDR
In this article, the cross-shock electrostatic potential at the front of collisionless shocks plays a key role in the distribution of energy at the shock front, and a statistical study of the crossshock potential calculated for around 50 crossings of the terrestrial bow shock is presented.
Abstract
[1] The cross-shock electrostatic potential at the front of collision-less shocks plays a key role in the distribution of energy at the shock front. Multipoint measurements such as those provided by the Cluster II mission provide an ideal framework for the study of the cross-shock potential because of their ability to distinguish between temporal and spacial variations at the shock front. We present a statistical study of the cross-shock potential calculated for around 50 crossings of the terrestrial bow shock. The statistical dependency of the normalized (with resect to upstream ion kinetic energy) cross-shock potential (ΦK) on the upstream Alfven Mach number is in good agreement with analytical results that predict decrease of Φk with increasing Mach number.

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Citations
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Journal ArticleDOI

The Dynamic Quasiperpendicular Shock: Cluster Discoveries

TL;DR: In this paper, the authors address a subset of unresolved problems in collisionless shock physics from experimental point of view making use of multi-point observations onboard Cluster satellites, including determination of scales of fields and of a scale of electron heating, identification of energy source of precursor wave train, an estimate of the role of anomalous resistivity in energy dissipation process by means of measuring short scale wave fields, and direct observation of reformation process during one single shock front crossing.
Journal ArticleDOI

Quantified energy dissipation rates in the terrestrial bow shock: 2. Waves and dissipation

TL;DR: In this paper, the first quantified measure of the energy dissipation rates due to wave-particle interactions, in the transition region of the Earth's collisionless bow shock using data from the Time History of Events and Macroscale Interactions during Substorms spacecraft was presented.
Journal ArticleDOI

The statistical mapping of magnetosheath plasma properties based on THEMIS measurements in the magnetosheath interplanetary medium reference frame

TL;DR: In this paper, a study of magnetosheath plasma properties using 5 years of THEMIS and OMNI data was performed to produce statistical maps of fundamental magneto-heath properties.
Journal ArticleDOI

Quantified energy dissipation rates in the terrestrial bow shock: 1. Analysis techniques and methodology

TL;DR: In this paper, a detailed outline and discussion of the analysis techniques used to compare the relevance of different energy dissipation mechanisms at collisionless shock waves is presented. And the authors show that high-frequency, large-amplitude (>100 mV/m and/or > 1 nT) waves are ubiquitous in the transition region of collisionless shocks.
References
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Journal ArticleDOI

Magnetopause structure and attitude from Explorer 12 observations.

TL;DR: In this article, satellite magnetometer data at a magnetopause penetration can be used to determine the vector normal to the magnetopsause current layer and the magnetic-field component along this normal.
Book ChapterDOI

Solar Wind Electron Proton Alpha Monitor (SWEPAM) for the Advanced Composition Explorer

TL;DR: The solar wind Electron Proton Alpha Monitor (SWEPAM) experiment provides the bulk solar wind observations for the Advanced Composition Explorer (ACE) as discussed by the authors, which provides the context for elemental and isotopic composition measurements made on ACE as well as allowing the direct examination of numerous solar wind phenomena such as coronal mass ejections, interplanetary shocks, and solar wind fine structure, with advanced, 3-D plasma instrumentation.
Book ChapterDOI

The ace magnetic fields experiment

TL;DR: The magnetic field experiment on ACE provides continuous measurements of the local magnetic field in the interplanetary medium as discussed by the authors, which are essential in the interpretation of simultaneous ACE observations of energetic and thermal particles distributions.
Journal ArticleDOI

Electron velocity distributions near the Earth's bow shock

TL;DR: A survey of electron velocity distributions measured near the earth's bow shock between October 1977 and December 1978 using the Los Alamos/Garching plasma instrumentation aboard ISEE 2 is presented in this article.
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