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Duration and extent of the great auroral storm of 1859.
The great geomagnetic storm of August 28 through September 3, 1859 is, arguably, the greatest and most famous space weather event in the last two hundred years. For the first time observations showed… Expand
On the origin of whistler mode radiation in the plasmasphere
 The origin of whistler mode radiation in the plasmasphere is examined from 3 years of plasma wave observations from the Dynamics Explorer and the Imager for Magnetopauseto-Aurora Global… Expand
Seasonal and solar cycle dynamics of the auroral kilometric radiation source region
 Several year's worth of observations from the plasma wave instruments on both Magnetopause-to-Aurora Global Exploration (IMAGE) and Polar spacecraft are used to study the seasonal and solar cycle… Expand
Electron Bulk Acceleration and Thermalization at Earth's Quasiperpendicular Bow Shock.
Electron heating at Earth's quasiperpendicular bow shock has been surmised to be due to the combined effects of a quasistatic electric potential and scattering through wave-particle interaction. Here… Expand
Evolution of the Aurora during the Great Geomagnetic Storm of 1859
We present a multi-instrument study of a hot flow anomaly ( HFA ) observed by the Venus Express spacecraft in the Venusian foreshock , on 22 March 2008 , incorporating both Venus Express Magnetometer…
 We present a multi-instrument study of a hot flow anomaly (HFA) observed by the Venus Express spacecraft in the Venusian foreshock, on 22 March 2008, incorporating both Venus Express Magnetometer… Expand
Association of kilometric continuum radiation with plasmaspheric structures
 A year's worth of observations of kilometric continuum (KC) from the plasma wave instrument (PWI) on GEOTAIL and extreme ultraviolet (EUV) images of the plasmasphere from IMAGE are compared. In… Expand
Observations of upstream ultra-low-frequency waves in the Mercury's foreshock
- G. Le, P. Chi, +4 authors H. Korth
- XXXIth URSI General Assembly and Scientific…
- 1 September 2014
We report the observational results of upstream ULF waves in the Mercury's foreshock using high-time resolution magnetic field data, 20 samples per second, from the MESSENGER spacecraft. The… Expand
ISTP catalog of preliminary solar wind events
Cyclic reformation of a quasi‐parallel bow shock at Mercury: MESSENGER observations
 We here document with magnetic field observations a passage of the MErcury Surface, Space ENvironment, GEochemistry, and Ranging (MESSENGER) spacecraft through Mercury's magnetosphere under… Expand