Search Publications

Energetic Charged Particles in the Terrestrial Magnetosphere: Cluster/RAPID Results
DOI: 10.1029/2021JA029273 Bibcode: 2021JGRA..12629273K

Daly, P. W.; Klecker, B.; Malykhin, A. Yu. +3 more

In this work, we review the results of observations by the Cluster/Research with Adaptive Particle Imaging Detectors (RAPID) energetic charged particle detector (∼>40 keV-∼1 MeV). The origin of energetic ions in the region upstream of the Earth's bow shock is compared under different solar wind conditions. We give a brief overview of the accele…

2021 Journal of Geophysical Research (Space Physics)
Cluster 5
Global Magnetosphere Response to Solar Wind Dynamic Pressure Pulses During Northward IMF Using the Heliophysics System Observatory
DOI: 10.1029/2020JA028587 Bibcode: 2021JGRA..12628587V

Moldwin, M. B.; Vidal-Luengo, S. E.

We analyzed the magnetospheric global response to dynamic pressure pulses (DPPs) using the Heliophysics System Observatory (HSO) and ground magnetometers. During northward Interplanetary Magnetic Field (IMF) Bz conditions, the magnetosphere acts as a closed "cavity" and reacts to solar wind DPPs more simply than during southward IMF. In this study…

2021 Journal of Geophysical Research (Space Physics)
Cluster 5
The Structure of the Cusp Diamagnetic Cavity and Test Particle Energization in the GAMERA Global MHD Simulation
DOI: 10.1029/2021JA029738 Bibcode: 2021JGRA..12629738B

Merkin, V.; Otto, A.; Nykyri, K. +4 more

Electrons with energies ≥40 keV can be found at low density in many different regions of Earth's magnetosphere. A litany of fundamental questions in space physics have focused on the acceleration mechanism of these particles, given that the sources of plasma are the relatively cool ionosphere and solar wind (∼1-100s eV). Upgraded global solar wind…

2021 Journal of Geophysical Research (Space Physics)
Cluster 5
Morphology of Jupiter's Polar Auroral Bright Spot Emissions via Juno UVS Observations
DOI: 10.1029/2020JA028586 Bibcode: 2021JGRA..12628586H

Bonfond, B.; Vogt, M. F.; Gérard, J. -C. +12 more

Since 2016, the Juno UVS (Ultraviolet Spectrograph) instrument has been taking spectral images of Jupiter's auroras in their full extent, including the nightside, which cannot be viewed from Earth. We present a systematic analysis of features in Jupiter's polar auroras called auroral bright spots, which were observed by Juno UVS during the first 2…

2021 Journal of Geophysical Research (Space Physics)
eHST 5
Simultaneous Observation of an Auroral Dawn Storm With the Hubble Space Telescope and Juno
DOI: 10.1029/2020JA028717 Bibcode: 2021JGRA..12628717S

Wilson, R. J.; Kurth, W. S.; Bagenal, F. +7 more

On July 13, 2016, the Hubble Space Telescope observed the onset of a dawn storm in Jupiter's northern ultraviolet aurora, while the NASA Juno spacecraft simultaneously traversed the dawnside outer magnetosphere. This represents the first concurrent auroral and in situ magnetospheric observations of the onset of a dawn storm at Jupiter. Mapping the…

2021 Journal of Geophysical Research (Space Physics)
eHST 5
Cluster Multi-Probing of the Aurora During Two Decades
DOI: 10.1029/2021JA029497 Bibcode: 2021JGRA..12629497M

Lindqvist, Per-Arne; Marklund, Göran

The Cluster spacecraft, launched in the year 2000, were pioneers using multi-point measurements to explore the dynamic space plasma environment of Earth. This capability offered a new, powerful approach to study in situ fundamental space plasma processes of the solar-terrestrial interaction. Although not a major science objective of the mission, t…

2021 Journal of Geophysical Research (Space Physics)
Cluster 5
The 3D Structure of Saturn Magnetospheric Neutral Tori Produced by the Enceladus Plumes
DOI: 10.1029/2020JA028775 Bibcode: 2021JGRA..12628775S

Richardson, John D.; Smith, Howard Todd

This research provides updated and validated spatial distributions of Enceladus generated H2O, OH, and O neutral tori. These tori are produced by the primary neutral source, Enceladus, and consist of populations of coorbiting neutral particles that provide the bulk of heavy molecules to Saturn's (neutral particle dominant) magnetosphere…

2021 Journal of Geophysical Research (Space Physics)
Cassini eHST 5
Magnetic Reconnection Inside Solar Wind Rotational Discontinuity During Its Interaction With the Quasi-Perpendicular Bow Shock and Magnetosheath
DOI: 10.1029/2021JA029979 Bibcode: 2021JGRA..12629979G

Wang, Xueyi; Lin, Yu; Du, Aimin +1 more

Using a three-dimensional global hybrid simulation, we investigate the formation and evolution of ion-scale magnetic reconnection inside an interplanetary rotational discontinuity (RD) owing to its interaction with the quasi-perpendicular (Q-⊥) bow shock and the magnetosphere. The interplanetary magnetic field (IMF) is initially predominantly nort…

2021 Journal of Geophysical Research (Space Physics)
Cluster 4
A Complete Data Set of Equatorial Projections of Saturn's Energetic Neutral Atom Emissions Observed by Cassini-INCA
DOI: 10.1029/2020JA028908 Bibcode: 2021JGRA..12628908B

Mitchell, D. G.; Paranicas, C.; Badman, S. V. +3 more

Observations of energetic neutral atoms (ENAs) are a useful tool for analyzing ion and neutral abundances in planetary magnetospheres. They are created when hot plasma, originating for example from magnetic reconnection sites, charge-exchanges with the ambient neutral population surrounding the planet. The motion of ENAs is not governed by the mag…

2021 Journal of Geophysical Research (Space Physics)
Cassini 4
Discovery of Alfvén Waves Planetward of Saturn's Rings
DOI: 10.1029/2020JA028473 Bibcode: 2021JGRA..12628473S

Dougherty, M. K.; Cao, H.; Southwood, D. J. +3 more

Between April and September 2017 in the final stages of the Cassini Saturn Orbiter mission the spacecraft executed 22 orbits passing planetward of the innermost ring, the D ring. During all periapsis passes oscillations were detected in the azimuthal magnetic field components on typical time scales of a few minutes. We argue that these time varyin…

2021 Journal of Geophysical Research (Space Physics)
Cassini 4