Comment on Relation to Solar Activity of Intense Aurorae in Sunlight and Darkness
We applaud the excellent effort and far-reaching results of Newell et al. (1998).
Aurorae Solar Activity atmosphere nightside interp↗
Engineering topics
Tsurutani, B.
Publications and source records attributed to Tsurutani, B..
A CME Loop and the January 10, 1997 First Substorm
The January 10, 1997 interplanetary high-speed stream and the resultant first substorm is studied using Wind interplanetary data and Polar UV images, respectively.
substorm Polar UV images interplanetary data↗
Energetic Particle Cross-Field Diffusion: Interaction with Magnetic Decreases (MDs)
Charged particle interactions with magnetic field magnitude changes lead to particle guiding center displacements and hence particle cross-field diffusion.
cross-field diffusion↗
Plasma Microstructure in the Solar Wind
We review some of the new NASA/ESA Ulysses solar wind microscale results.
Interplanetary Space Plasma Microstructure Solar W↗
Solar/Interplanetary Plasma Phenomena Causing Geomagnetic Activity at Earth
Solar wind phenomena leading to different types of geomagnetic activity are discussed.
solar winds geomagnetic substorms storms aurora Ea↗
Broadband Plasma Waves in the Boundary Layers
Boundary layers are commonly encountered in space and astrophysical plasmas.
broadband plasma waves boundary layer↗
The Jovian Magnetopause Boundary Layer
There are plasma boundary layers at the magnetopause of Juputer and the Earth.
Magnetosphere Jovian↗
Energetic Particle Transport at Corotating Interaction Regions (CIRs)
We examine energetic particle transport at or near Corotating Interaction Regions (CIRs).
Corotating Interaction Regions (CIRs) energetic pa↗
CIR Morphology, Turbulence, Discontinuities, and Energetic Particles
Corotating interaction regions (CIRs) in the middle heliosphere have distinct morphological features and associated patterns of turbulence and energetic particles.
CIRs turbulence discontinuities↗
Substorms, Pseudobreakups and Quiescent Events Caused by Interplanetary Shocks
We use WIND solar wind data and POLAR UV imaging data to study magnetospheric responses and substorm triggering mechanisms during and after interplanetary (IP) shock events.
Substorm Interplanetary Shock↗
Rapid Intensification and Propagation of the Dayside Aurora: Large Scale Interplanetary Pressure Pulses (fast shocks)
We study cases of abrupt dayside auroral brightenings and very fast auroral propagation using the POLAR UV imaging data.
waves↗
Here Comes Solar Prove!
Flying a trajectory perpendicular to the Earth-Sun line during its perihelion passage, Solar Probe will use in-situ and imaging instruments to provide the first three dimentional viewing of the corona, direct observations of solar polar regions, and local sampling of the solar environment. These primary observations are complemented by context-setting cruise measurements and Earth-based observations.
solar corona solar wind solar probe heliosphere ph↗
Solar Probe: A Mission to the Sun and the Inner Core of the Heliosphere
Following a brief review of out current knowledge of the solar wind and processes on the solar surface, we describe the baseline Solar Probe mission, its prime scientific objectives and its strawman instrument payload.
Solar Probe Sun Corona magnetic fields poles solar↗
The Role of Waves in Substorm Onsets
Explore the source record for details and available documents.
neutral line substorm onsets instabilities plasmas↗
Arc Polarized Discontinuities in the Solar Wind: Ulysses
Explore the source record for details and available documents.
polarizations discontinuities ambient magnetic fie↗
Nonlinear Electromagnetic Waves and Spherical Arc-Polarized Waves in Space Plasmas
We review observations of nonlinear plasma waves detected by interplanetary spacecraft. For this paper we will focus primarily on the phase-steepened properties of such waves. Plasma waves at comet Giacobini-Zinner measured by the International Cometary Explorer (ICE), at comets Halley and Grigg-Skjellerup measured by Giotto, and interplanetary Alfven waves measured by Ulysses, will be discussed and intercompared.
Nonliner Plasma waves↗
Reply .. to Cliver
Explore the source record for details and available documents.
Solar Cycle Coronal holes↗
Latitudinal Structure of the Heliospheric Current Sheet and Corotating Streams Measured by WIND and ULYSSES
All heliospheric current sheet (HCS) crossings and corotating solar wind streams detectedby both WIND and ULYSSES have been identified.
heliosphecic current sheet (HCS) corotating solar ↗