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The Analyzer of Space Plasmas and Energetic Atoms (ASPERA-3) for the Mars Express Mission
DOI: 10.1007/s11214-006-9124-8 Bibcode: 2006SSRv..126..113B

Coates, A. J.; Kallio, E.; Fedorov, A. +39 more

The general scientific objective of the ASPERA-3 experiment is to study the solar wind - atmosphere interaction and to characterize the plasma and neutral gas environment with within the space near Mars through the use of energetic neutral atom (ENA) imaging and measuring local ion and electron plasma. The ASPERA-3 instrument comprises four sensor…

2006 Space Science Reviews
MEx 253
Plasma Morphology at Mars. Aspera-3 Observations
DOI: 10.1007/s11214-006-9039-4 Bibcode: 2006SSRv..126..209D

Barabash, S.; Lundin, R.; Winningham, J. D. +6 more

A total of about of 400 orbits during the first year of the ASPERA-3 operation onboard the Mars Express spacecraft were analyzed to obtain a statistical pattern of the main plasma domains in the Martian space environment. The environment is controlled by the direct interaction between the solar wind and the planetary exosphere/ionosphere which res…

2006 Space Science Reviews
MEx 109
Cosmic Rays at High Heliolatitudes
DOI: 10.1007/s11214-006-9085-y Bibcode: 2006SSRv..127..117H

Potgieter, M. S.; Heber, B.

The Ulysses spacecraft has been the first to orbit the Sun over its poles and to explore the heliosphere at these high heliolatitudes. It has now completed two fast latitude scans, one 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, …

2006 Space Science Reviews
Ulysses 88
Coronal Observations of CMEs. Report of Working Group A
DOI: 10.1007/s11214-006-9016-y Bibcode: 2006SSRv..123..127S

Schwenn, R.; Pick, M.; Reiner, M. +15 more

CMEs have been observed for over 30 years with a wide variety of instruments. It is now possible to derive detailed and quantitative information on CME morphology, velocity, acceleration and mass. Flares associated with CMEs are observed in X-rays, and several different radio signatures are also seen. Optical and UV spectra of CMEs both on the dis…

2006 Space Science Reviews
SOHO 80
Thin Current Sheets in the Magnetotail Observed by Cluster
DOI: 10.1007/s11214-006-6219-1 Bibcode: 2006SSRv..122...29N

Nakamura, R.; Baumjohann, W.; Asano, Y. +1 more

The dynamics of the current sheet is one of the most essential elements in magnetotail physics. Particularly, thin current sheets, which we define here as those with a thickness of less than several ion inertia lengths, are known to play an important role in the energy conversion process in the magnetotail. With its capability of multi-point obser…

2006 Space Science Reviews
Cluster 79
Locations of Atmospheric Photoelectron Energy Peaks Within the Mars Environment
DOI: 10.1007/s11214-006-9119-5 Bibcode: 2006SSRv..126..389F

Coates, A. J.; Kallio, E.; Barabash, S. +13 more

By identifying peaks in the photoelectron spectrum produced by photoionization of CO2 in the Martian atmosphere, we have conducted a pilot study to determine the locations of these photoelectrons in the space around Mars. The significant result of this study is that these photoelectrons populate a region around Mars bounded externally b…

2006 Space Science Reviews
MEx 78
Plasma Moments in the Environment of Mars. Mars Express ASPERA-3 Observations
DOI: 10.1007/s11214-006-9115-9 Bibcode: 2006SSRv..126..165F

Coates, A. J.; Fedorov, A.; Barabash, S. +7 more

We present the first electron and ion moment maps (density, velocity and temperature) of the martian plasma environment, using data from the ELS and IMA sensors of the ASPERA-3 experiment onboard Mars Express. Moments are calculated by integration and by Gaussian fits to the phase space distribution. The methods of calculation and the calibration …

2006 Space Science Reviews
MEx 76
Energetic Particle Observations
DOI: 10.1007/s11214-006-9018-9 Bibcode: 2006SSRv..123..217K

Simnett, G. M.; Lario, D.; Klecker, B. +14 more

The characteristics of solar energetic particles (SEP) as observed in interplanetary space provide fundamental information about the origin of these particles, and the acceleration and propagation processes at the Sun and in interplanetary space. Furthermore, energetic particles provide information on the development and structure of coronal mass …

2006 Space Science Reviews
SOHO Ulysses 55
Observations of Vertical Reflections from the Topside Martian Ionosphere
DOI: 10.1007/s11214-006-9113-y Bibcode: 2006SSRv..126..373N

Gurnett, D. A.; Morgan, D. D.; Orosei, R. +7 more

The Martian ionosphere has for the first time been probed by a low frequency topside radio wave sounder experiment (MARSIS) (Gurnett et al., 2005). The density profiles in the Martian ionosphere have for the first time been observed for solar zenith angles less than 48 degrees. The sounder spectrograms typically have a single trace of echoes, whic…

2006 Space Science Reviews
MEx 53
Bursty Bulk Flow Driven Turbulence in the Earth's Plasma Sheet
DOI: 10.1007/s11214-006-6987-7 Bibcode: 2006SSRv..122..301V

Nakamura, R.; Baumjohann, W.; Volwerk, M. +2 more

During the last several years significant progress has been made in understanding MHD turbulence in the Earth’s plasma sheet. Due to the statistically transitory properties of fluctuations, finite size and boundary effects, however, issues of fundamental importance remain unresolved. Here we concentrate on such intrinsic features of plasma sheet t…

2006 Space Science Reviews
Cluster 46