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The multi-scale nature of the solar wind
The solar wind is a magnetized plasma and as such exhibits collective plasma behavior
associated with its characteristic spatial and temporal scales. The characteristic length …
associated with its characteristic spatial and temporal scales. The characteristic length …
Solar wind electron proton alpha monitor (SWEPAM) for the Advanced Composition Explorer
Abstract The Solar Wind Electron Proton Alpha Monitor (SWEPAM) experiment provides the
bulk solar wind observations for the Advanced Composition Explorer (ACE). These …
bulk solar wind observations for the Advanced Composition Explorer (ACE). These …
First in situ measurements of electron density and temperature from quasi-thermal noise spectroscopy with Parker Solar Probe/FIELDS
Heat transport in the solar corona and wind is still a major unsolved astrophysical problem.
Because of the key role played by electrons, the electron density and temperature (s) are …
Because of the key role played by electrons, the electron density and temperature (s) are …
A comprehensive review of Electric Solar Wind Sail concept and its applications
Abstract The Electric Solar Wind Sail (E-sail) is an innovative propellantless propulsion
system conceived by Pekka Janhunen in 2004 for use in interplanetary space. An E-sail …
system conceived by Pekka Janhunen in 2004 for use in interplanetary space. An E-sail …
Space Weather: From solar origins to risks and hazards evolving in time
Space Weather is the portion of space physics that has a direct effect on humankind. Space
Weather is an old branch of space physics that originates back to 1808 with the publication …
Weather is an old branch of space physics that originates back to 1808 with the publication …
Magnetohydrodynamic modeling of the solar corona during Whole Sun Month
The Whole Sun Month campaign (August 10 to September 8, 1996) brought together a wide
range of space‐based and ground‐based observations of the Sun and the interplanetary …
range of space‐based and ground‐based observations of the Sun and the interplanetary …
Motion of the footpoints of heliospheric magnetic field lines at the Sun: Implications for recurrent energetic particle events at high heliographic latitudes
LA Fisk - Journal of Geophysical Research: Space Physics, 1996 - Wiley Online Library
The interplay between the differential rotation of the footpoints of heliospheric magnetic field
lines in the photosphere and the subsequent nonradial expansion of these same field lines …
lines in the photosphere and the subsequent nonradial expansion of these same field lines …
The solar magnetic field
The magnetic field of the Sun is the underlying cause of the many diverse phenomena
combined under the heading of solar activity. Here we describe the magnetic field as it …
combined under the heading of solar activity. Here we describe the magnetic field as it …
The structure of the large-scale heliosphere as seen by current models
This review summarizes the current state of research aiming at a description of the global
heliosphere using both analytical and numerical modeling efforts, particularly in view of the …
heliosphere using both analytical and numerical modeling efforts, particularly in view of the …
Three‐dimensional propagation of coronal mass ejections (CMEs) in a structured solar wind flow: 1. CME launched within the streamer belt
D Odstrčil, VJ Pizzo - Journal of Geophysical Research: Space …, 1999 - Wiley Online Library
A three‐dimensional (3‐D) numerical hydrodynamic model is used to investigate the
temporal and spatial evolution of large‐scale solar wind structures. A tilted‐dipole outflow …
temporal and spatial evolution of large‐scale solar wind structures. A tilted‐dipole outflow …