Search Publications

Geochemical Consequences of Widespread Clay Mineral Formation in Mars' Ancient Crust
DOI: 10.1007/s11214-012-9930-0 Bibcode: 2013SSRv..174..329E

Ehlmann, Bethany L.; Mangold, Nicolas; Chassefière, Eric +7 more

Clays form on Earth by near-surface weathering, precipitation in water bodies within basins, hydrothermal alteration (volcanic- or impact-induced), diagenesis, metamorphism, and magmatic precipitation. Diverse clay minerals have been detected from orbital investigation of terrains on Mars and are globally distributed, indicating geographically wid…

2013 Space Science Reviews
MEx 104
Quantitative Assessments of the Martian Hydrosphere
DOI: 10.1007/s11214-012-9946-5 Bibcode: 2013SSRv..174..155L

Mangold, Nicolas; Mousis, Olivier; Hauber, Ernst +6 more

In this paper, we review current estimates of the global water inventory of Mars, potential loss mechanisms, the thermophysical characteristics of the different reservoirs that water may be currently stored in, and assess how the planet's hydrosphere and cryosphere evolved with time. First, we summarize the water inventory quantified from geologic…

2013 Space Science Reviews
MEx 76
Kinetic Structure of Current Sheets in the Earth Magnetotail
DOI: 10.1007/s11214-012-9954-5 Bibcode: 2013SSRv..178..419A

Zelenyi, Lev; Artemyev, Anton

In this paper we present a short review of kinetic models of the thin current sheet and corresponding Cluster observations in the Earth magnetotail. We concentrate mainly on manifestations of non-fluid ion kinetic effects. We discuss the different approaches to model description of the proton component and show that current sheets observed by Clus…

2013 Space Science Reviews
Cluster 61
Cosmic Rays in the Inner Heliosphere: Insights from Observations, Theory and Models
DOI: 10.1007/s11214-011-9750-7 Bibcode: 2013SSRv..176..165P

Potgieter, M. S.

The global modulation of galactic cosmic rays in the inner heliosphere is determined by four major mechanisms: convection, diffusion, particle drifts (gradient, curvature and current sheet drifts), and adiabatic energy losses. When these processes combine to produce modulation, the complexity increases significantly especially when one wants to de…

2013 Space Science Reviews
Ulysses 54
Solar Drivers of 11-yr and Long-Term Cosmic Ray Modulation
DOI: 10.1007/s11214-011-9746-3 Bibcode: 2013SSRv..176....3C

Richardson, I. G.; Ling, A. G.; Cliver, E. W.

In the current paradigm for the modulation of galactic cosmic rays (GCRs), diffusion is taken to be the dominant process during solar maxima while drift dominates at minima. Observations during the recent solar minimum challenge the pre-eminence of drift at such times. In 2009, the ∼2 GV GCR intensity measured by the Newark neutron monitor increas…

2013 Space Science Reviews
Ulysses 53
Methods for Characterising Microphysical Processes in Plasmas
DOI: 10.1007/s11214-013-9974-9 Bibcode: 2013SSRv..178..665D

Alexandrova, O.; Dudok de Wit, T.; Sorriso-Valvo, L. +2 more

Advanced spectral and statistical data analysis techniques have greatly contributed to shaping our understanding of microphysical processes in plasmas. We review some of the main techniques that allow for characterising fluctuation phenomena in geospace and in laboratory plasma observations. Special emphasis is given to the commonalities between d…

2013 Space Science Reviews
Cluster 49
Microphysics of Quasi-parallel Shocks in Collisionless Plasmas
DOI: 10.1007/s11214-013-9969-6 Bibcode: 2013SSRv..178..513B

Scholer, M.; Burgess, D.

Shocks in collisionless plasmas require dissipation mechanisms which couple fields and particles at scales much less than the conventional collisional mean free path. For quasi-parallel geometries, where the upstream magnetic field makes a small angle to the shock normal direction, wave-particle coupling produces a broad transition zone with large…

2013 Space Science Reviews
Cluster 40
Solar Surface and Atmospheric Dynamics. The Photosphere
DOI: 10.1007/s11214-013-9967-8 Bibcode: 2013SSRv..178..141M

Martínez Pillet, V.

Various aspects of the magnetism of the quiet sun are reviewed. The suggestion that a small scale dynamo acting at granular scales generates what we call the quiet sun fields is studied in some detail. Although dynamo action has been proved numerically, it is argued that current simulations are still far from achieving the complexity that might be…

2013 Space Science Reviews
Hinode 36
Solar Wind Conditions and Composition During the Genesis Mission as Measured by in situ Spacecraft
DOI: 10.1007/s11214-013-9960-2 Bibcode: 2013SSRv..175..125R

Neugebauer, Marcia; Wiens, Roger C.; Zurbuchen, Thomas H. +4 more

We describe the Genesis mission solar-wind sample collection period and the solar wind conditions at the L1 point during this 2.3-year period. In order to relate the solar wind samples to solar composition, the conditions under which the samples were collected must be understood in the context of the long-term solar wind. We find that the state of…

2013 Space Science Reviews
Ulysses 36
Cosmic Rays Through the Solar Hale Cycle. Insights from Ulysses
DOI: 10.1007/s11214-011-9784-x Bibcode: 2013SSRv..176..265H

Heber, B.

The Ulysses spacecraft had been the first to orbit the Sun over its poles and to explore the heliosphere at these high heliolatitudes. It has now completed three fast latitude scans, two at solar minimum and one at solar maximum. Since its launch in October 1990, this mission has led to several surprising discoveries concerning energetic particles…

2013 Space Science Reviews
Ulysses 34