Search Publications

Properties of Ground Level Enhancement Events and the Associated Solar Eruptions During Solar Cycle 23
DOI: 10.1007/s11214-012-9890-4 Bibcode: 2012SSRv..171...23G

Gopalswamy, N.; Yashiro, S.; Mäkelä, P. +3 more

Solar cycle 23 witnessed the most complete set of observations of coronal mass ejections (CMEs) associated with the Ground Level Enhancement (GLE) events. We present an overview of the observed properties of the GLEs and those of the two associated phenomena, viz., flares and CMEs, both being potential sources of particle acceleration. Although we…

2012 Space Science Reviews
SOHO 270
Particle Acceleration in the Magnetotail and Aurora
DOI: 10.1007/s11214-012-9874-4 Bibcode: 2012SSRv..173...49B

Zelenyi, L. M.; Baker, D. N.; Artemyev, A. V. +3 more

This paper deals with acceleration processes in the magnetotail and the processes that enhance particle precipitation from the tail into the ionosphere through electric fields in the auroral acceleration region, generating or intensifying discrete auroral arcs. Particle acceleration in the magnetotail is closely related to substorms and the occurr…

2012 Space Science Reviews
Cluster 180
Magnetic Reconnection in the Solar Wind
DOI: 10.1007/s11214-011-9747-2 Bibcode: 2012SSRv..172..187G

Gosling, J. T.

It is only within the last 5 years that we have learned how to recognize the unambiguous signature of magnetic reconnection in the solar wind in the form of roughly Alfvénic accelerated plasma flows embedded within bifurcated magnetic field reversal regions (current sheets). This paper provides a brief overview of what has since been learned about…

2012 Space Science Reviews
Cluster 131
Anisotropy in Space Plasma Turbulence: Solar Wind Observations
DOI: 10.1007/s11214-011-9821-9 Bibcode: 2012SSRv..172..325H

Horbury, T. S.; Chen, C. H. K.; Wicks, R. T.

The local magnetic field induces many types of anisotropy in plasma turbulence, changing the rate of energy transfer and affecting the propagation of energetic particles. It is challenging to measure this anisotropy in the solar wind due to the limited number of sampling points and measurement difficulties and many aspects remain poorly understood…

2012 Space Science Reviews
Cluster 110
Ion Acceleration at the Earth's Bow Shock
DOI: 10.1007/s11214-012-9901-5 Bibcode: 2012SSRv..173....5B

Möbius, E.; Scholer, M.; Burgess, D.

The Earth's bow shock is the most studied example of a collisionless shock in the solar system. It is also widely used to model or predict the behaviour at other astrophysical shock systems. Spacecraft observations, theoretical modelling and numerical simulations have led to a detailed understanding of the bow shock structure, the spatial organiza…

2012 Space Science Reviews
Cluster 109
What Are Special About Ground-Level Events?. Flares, CMEs, Active Regions and Magnetic Field Connection
DOI: 10.1007/s11214-012-9877-1 Bibcode: 2012SSRv..171...61N

Liu, Y.; Nitta, N. V.; Nightingale, R. W. +1 more

Ground level events (GLEs) occupy the high-energy end of gradual solar energetic particle (SEP) events. They are associated with coronal mass ejections (CMEs) and solar flares, but we still do not clearly understand the special conditions that produce these rare events. During Solar Cycle 23, a total of 16 GLEs were registered, by ground-based neu…

2012 Space Science Reviews
SOHO 57
Solar Wind Models from the Chromosphere to 1 AU
DOI: 10.1007/s11214-012-9887-z Bibcode: 2012SSRv..172...89H

Velli, Marco; Hansteen, Viggo H.

Recent models of the fast solar wind are characterized by low coronal electron temperatures while proton, α-particle, and minor ion temperatures are expected to be quite high and generally anisotropic, including large temperatures perpendicular to the magnetic field and parallel beams. This entails that the electric field should be relatively unim…

2012 Space Science Reviews
Ulysses 54
Observational Aspects of Particle Acceleration in Large Solar Flares
DOI: 10.1007/s11214-012-9897-x Bibcode: 2012SSRv..173..197R

Krucker, Säm; Raymond, John C.; Lin, Robert P. +1 more

Solar flares efficiently accelerate electrons to several tens of MeV and ions to 10 GeV. The acceleration is usually thought to be associated with magnetic reconnection occurring high in the corona, though a shock produced by the Coronal Mass Ejection (CME) associated with a flare can also accelerate particles. Diagnostic information comes from em…

2012 Space Science Reviews
SOHO 36
LCROSS (Lunar Crater Observation and Sensing Satellite) Observation Campaign: Strategies, Implementation, and Lessons Learned
DOI: 10.1007/s11214-011-9759-y Bibcode: 2012SSRv..167...93H

Terada, Hiroshi; de Pater, Imke; Vilas, Faith +84 more

NASA's LCROSS (Lunar Crater Observation and Sensing Satellite) mission was designed to explore the nature of previously detected enhanced levels of hydrogen near the lunar poles. The LCROSS mission impacted the spent upper stage of the launch vehicle into a permanently shadowed region of the lunar surface to create an ejecta plume. The resultant i…

2012 Space Science Reviews
eHST 19
Scalings, Cascade and Intermittency in Solar Wind Turbulence
DOI: 10.1007/s11214-012-9907-z Bibcode: 2012SSRv..172..343C

Carbone, Vincenzo

Investigating in situ fluctuations in the interplanetary space, offers us a unique challenge to study scaling properties in a turbulent medium which cover a wide range of scales. This includes not only the inertial range, where turbulence can be described within a fluid-like approach, but also the high-frequency region, where a kinetic approach is…

2012 Space Science Reviews
Cluster 16