18.1k citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- University of California, BerkeleyUS1.3k papers
- Goddard Space Flight CenterUS457 papers
- California Institute of TechnologyUS379 papers
- Centre National de la Recherche ScientifiqueFR367 papers
- Lawrence Berkeley National LaboratoryUS262 papers
- Jet Propulsion LaboratoryUS260 papers
- Commissariat à l'Énergie Atomique et aux Énergies AlternativesFR240 papers
- National Institute for AstrophysicsIT239 papers
- University of CambridgeGB208 papers
- Imperial College LondonGB203 papers
- Institut de Recherche en Astrophysique et PlanétologieFR195 papers
- Institut National de Physique Nucléaire et de Physique des ParticulesFR181 papers
18 papers · 2 filters
Observations of Energized Electrons in the Martian Magnetosheath
K. Horaites, L. Andersson, S. J. Schwartz +5
This observational study demonstrates that the magnitude and location of energization of electrons in the Martian magnetosheath is more complex than previous studies suggest. Elect…
Statistical analysis of orientation, shape, and size of solar wind switchbacks
Ronan Laker, Timothy S. Horbury, Stuart D. Bale +9
One of the main discoveries from the first two orbits of Parker Solar Probe (PSP) was the presence of magnetic switchbacks, whose deflections dominated the magnetic field measureme…
Turbulence characteristics of switchbacks and non-switchbacks intervals observed by \emph{Parker Solar Probe}
Sofiane Bourouaine, Jean C. Perez, Kristopher C. Klein +5
We use \emph{Parker Solar Probe} (\emph{PSP}) in-situ measurements to analyze the characteristics of solar wind turbulence during the first solar encounter covering radial distance…
Narrowband oblique whistler-mode waves: Comparing properties observed by Parker Solar Probe at <0.2 AU and STEREO at 1 AU
C. Cattell, B. Short, A. Breneman +15
AIM: Large amplitude narrowband obliquely propagating whistler-mode waves at frequencies of ~0.2 fce (electron cyclotron frequency) are commonly observed at 1 AU, and are most cons…
Cross Helicity of the November 2018 Magnetic Cloud Observed by the Parker Solar Probe
S. W. Good, E. K. J. Kilpua, M. Ala-Lahti +3
Magnetic clouds are large-scale transient structures in the solar wind with low plasma , low-amplitude magnetic field fluctuations, and twisted field lines with both ends often…
Electrostatic Waves and Electron Heating Observed over Lunar Crustal Magnetic Anomalies
F. Chu, J. S. Halekas, Xin Cao +3
Above lunar crustal magnetic anomalies, large fractions of solar wind electrons and ions can be scattered and stream back towards the solar wind flow, leading to a number of intere…
Small-scale Magnetic Flux Ropes in the First two Parker Solar Probe Encounters
Yu Chen, Qiang Hu, Lingling Zhao +15
Small-scale magnetic flux ropes (SFRs) are a type of structures in the solar wind that possess helical magnetic field lines. In a recent report (Chen & Hu 2020), we presented the r…
On the Scaling Properties of Magnetic Field Fluctuations Through the Inner Heliosphere
Tommaso Alberti, Monica Laurenza, Giuseppe Consolini +4
Although the interplanetary magnetic field variability has been extensively investigated in situ by means of data coming from several space missions, the newly launched missions pr…
Toward a Physics Based Model of Hypervelocity Dust Impacts
Paul J Kellogg, S. D. Bale, Keith Goetz +1
There has been important understanding of the process by which a hypersonic dust impact makes an electrical signal on a spacecraft sensor, leading to a fuller understanding of the…
Long-term variations of quasi-trapped and trapped electrons in the inner radiation belt observed by DEMETER and SAMPEX
Kun Zhang, Xinlin Li, Zheng Xiang +5
Electrons in the Earth's radiation belts can be categorized into three populations: precipitating, quasi-trapped and trapped. We use data from the DEMETER and SAMPEX missions and f…
ARTEMIS Observations of Plasma Waves in Laminar and Perturbed Interplanetary Shocks
L. Davis, C. A. Cattell, L. B. Wilson +3
The 'Acceleration, Reconnection, Turbulence and Electrodynamics of the Moon's Interaction with the Sun' (ARTEMIS) mission provides a unique opportunity to study the structure of in…
The STONE curve: A ROC-derived model performance assessment tool
Michael W. Liemohn, Abigail R. Azari, Natalia Ganushkina +1
A new model validation and performance assessment tool is introduced, the sliding threshold of observation for numeric evaluation (STONE) curve. It is based on the relative operati…
Radial Evolution of Magnetic Field Fluctuations in an Interplanetary Coronal Mass Ejection Sheath
S. W. Good, M. Ala-Lahti, E. Palmerio +2
The sheaths of compressed solar wind that precede interplanetary coronal mass ejections (ICMEs) commonly display large-amplitude magnetic field fluctuations. As ICMEs propagate rad…
Localized magnetic field structures and their boundaries in the near-Sun solar wind from Parker Solar Probe measurements
V. Krasnoselskikh, A. Larosa, O. Agapitov +18
One of the discoveries made by Parker Solar Probe during first encounters with the Sun is the ubiquitous presence of relatively small-scale structures standing out as sudden deflec…
Multi-scale coupling during magnetopause reconnection: the interface between the electron and ion diffusion regions
K. J. Genestreti, Y. -H. Liu, T. -D. Phan +15
Magnetospheric Multiscale (MMS) encountered the primary low-latitude magnetopause reconnection site when the inter-spacecraft separation exceeded the upstream ion inertial length.…
Shock Drift Acceleration of Ions in an Interplanetary Shock Observed by MMS
E. L. M. Hanson, O. V. Agapitov, I. Y. Vasko +6
An interplanetary (IP) shock wave was recorded crossing the Magnetospheric Multiscale (MMS) constellation on 2018 January 8. Plasma measurements upstream of the shock indicate effi…
Kinetic models of tangential discontinuities in the solar wind
T. Neukirch, I. Y. Vasko, A. V. Artemyev +1
Kinetic-scale current sheets observed in the solar wind are frequently approximately force-free despite the fact that their plasma is of the order of one. In-situ measurements…
Electron energy partition across interplanetary shocks: III. Analysis
L. B. Wilson, Li-Jen Chen, Shan Wang +10
Analysis of model fit results of 15,210 electron velocity distribution functions (VDFs), observed within 2 hours of 52 interplanetary (IP) shocks by the Wind spacecraft near 1…