Search Publications

Global Response of Martian Plasma Environment to an Interplanetary Structure: From Ena and Plasma Observations at Mars
DOI: 10.1007/s11214-006-9026-9 Bibcode: 2006SSRv..126..315F

Barabash, S.; Lundin, R.; Futaana, Y. +4 more

As a part of the global plasma environment study of Mars and its response to the solar wind, we have analyzed a peculiar case of the subsolar energetic neutral atom (ENA) jet observed on June 7, 2004 by the Neutral Particle Detector (NPD) on board the Mars Express satellite. The "subsolar ENA jet" is generated by the interaction between the solar …

2006 Space Science Reviews
MEx 21
Shocks: Commonalities in Solar-Terrestrial Chains
DOI: 10.1007/s11214-006-9093-y Bibcode: 2006SSRv..124..333S

Schwartz, Steven J.

Shocks are found throughout the heliosphere, wherever supersonic (or super-magnetosonic) flows encounter obstacles or other, slowly moving, media. Although some of the physical parameters are in different regimes, all shocks heat and decelerate the media incident upon them. Most shocks must propagate in a collisionless plasma, thereby adding impor…

2006 Space Science Reviews
Cluster 13
Asymmetries in Mars' Exosphere. Implications for X-ray and ENA Imaging
DOI: 10.1007/s11214-006-9036-7 Bibcode: 2006SSRv..126..435H

Holmström, Mats

Observations and simulations show that Mars' atmosphere has large seasonal variations. Total atmospheric density can have an order of magnitude latitudinal variation at exobase heights. By numerical simulations we show that these latitude variations in exobase parameters induce asymmetries in the hydrogen exosphere that propagate to large distance…

2006 Space Science Reviews
MEx 13
Energisation of O+ and O+ 2 Ions at Mars: An Analysis of a 3-D Quasi-Neutral Hybrid Model Simulation
DOI: 10.1007/s11214-006-9120-z Bibcode: 2006SSRv..126...39K

Kallio, E.; Fedorov, A.; Janhunen, P. +12 more

We have studied the loss of O+ and O+2 ions at Mars with a numerical model. In our quasi-neutral hybrid model ions (H+, He++, O+, O+2) are treated as particles while electrons form a massless charge-neutralising fluid. The employed model version does not includ…

2006 Space Science Reviews
MEx 12
Substorms and Their Solar Wind Causes
DOI: 10.1007/s11214-006-9131-9 Bibcode: 2006SSRv..124...91N

Nakamura, Rumi

Consequences of the solar wind input observed as large scale magnetotail dynamics during substorms are reviewed, highlighting results from statistical studies as well as global magnetosphere/ionosphere observations. Among the different solar wind input parameters, the most essential one to initiate reconnection relatively close to the Earth is a s…

2006 Space Science Reviews
Cluster 11
Observations of the Martian Subsolar ENA Jet Oscillations
DOI: 10.1007/s11214-006-9121-y Bibcode: 2006SSRv..126..299G

Fedorov, A.; Barabash, S.; Futaana, Y. +1 more

The Neutral Particle Detector (NPD) of the ASPERA-3 experiment (Analyser of Space Plasmas and Energetic Atoms) on board the Mars Express (MEX) spacecraft observed an intense flux of H ENAs (energetic neutral atoms) with average energy of about 1.5 keV emitted anisotropically from the subsolar region of Mars. The NPD detected the ENA jet near the b…

2006 Space Science Reviews
MEx 11
Review of Ionospheric Effects of Solar Wind Magnetosphere Coupling in the Context of the Expanding Contracting Polar Cap Boundary Model
DOI: 10.1007/s11214-006-9132-8 Bibcode: 2006SSRv..124..117L

Wild, J. A.; Lester, M.; Milan, S. E. +1 more

This paper reviews the coupling between the solar wind, magnetosphere and ionosphere. The coupling between the solar wind and Earth’s magnetosphere is controlled by the orientation of the Interplanetary Magnetic Field (IMF). When the IMF has a southward component, the coupling is strongest and the ionospheric convection pattern that is generated i…

2006 Space Science Reviews
Cluster 8
Cross-Scale Coupling Within Rolled-Up MHD-Scale Vortices and Its Effect on Large Scale Plasma Mixing Across the Magnetospheric Boundary
DOI: 10.1007/s11214-006-7768-z Bibcode: 2006SSRv..122....3F

Hasegawa, H.; Fujimoto, M.; Nakamura, T. K. M.

Kelvin-Helmholtz Instability (KHI) is an MHD-scale instability that grows in a velocity shear layer such as the low-latitude boundary layer of the magnetosphere. KHI is driven unstable when a velocity shear is strong enough to overcome the stabilization effect of magnetic field. When the shear is significantly strong, vortices in the nonlinear sta…

2006 Space Science Reviews
Cluster 6
Supermassive Black Holes in Galactic Nuclei: Past, Present and Future Research
DOI: 10.1007/s11214-005-3947-6 Bibcode: 2005SSRv..116..523F

Ford, Holland; Ferrarese, Laura

This review discusses the current status of supermassive black hole research, as seen from a purely observational standpoint. Since the early ‘90s, rapid technological advances, most notably the launch of the Hubble Space Telescope, the commissioning of the VLBA and improvements in near-infrared speckle imaging techniques, have not only given us i…

2005 Space Science Reviews
eHST 852
The Foreshock
DOI: 10.1007/s11214-005-3824-3 Bibcode: 2005SSRv..118...41E

Eastwood, J. P.; Lucek, E. A.; Narita, Y. +4 more

2005 Space Science Reviews
Cluster 272