663 citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Centre National de la Recherche ScientifiqueFR14 papers
- Goddard Space Flight CenterUS14 papers
- Johns Hopkins University Applied Physics LaboratoryUS14 papers
- The University of Texas at San AntonioUS12 papers
- Sorbonne UniversitéFR11 papers
- University of Alaska AnchorageUS10 papers
- University of New HampshireUS10 papers
- University of SouthamptonGB10 papers
- Instituto de Astrofísica de CanariasES9 papers
- Universidad de La LagunaES9 papers
- University of California, Los AngelesUS9 papers
- Centro de AstrobiologíaES8 papers
17 papers · 1 filter
The Gannon Storm: Citizen science observations during the geomagnetic superstorm of 10 May 2024
Maxime Grandin, Emma Bruus, Vincent E. Ledvina +12
The 10 May 2024 geomagnetic storm, referred to as the Gannon Storm in this paper, was one of the most extreme to have occurred in over 20 years. In the era of smartphones and socia…
The Localized 12-hour Wave Over Alaska: Leveraging Meridional Wind Measurements From the Sodium Lidar
Sophie R. Phillips, Katrina Bossert, Komal Kumari +3
The 12-h wave in meridional winds in the mesosphere and lower thermosphere (MLT) during the solar minimum 2018-2019 Arctic winter is investigated using sodium lidar observations at…
Advancing Heliophysics and Space Weather Modeling through Open Science
C. Corti, M. M. Kuznetsova, M. A. Reiss +85
We present a community-wide effort to develop a strategy and action plan to advance heliophysics and space weather modeling through open science. While open science has the potenti…
Corotation-bounce resonance of ions in Jupiter's magnetosphere
Y. Sarkango, J. R. Szalay, P. A. Damiano +6
Banded energy distributions of H, O, S, and O or S ions between 100 eV to ~20 keV are consistently observed in Jupiter's magnetosphere mapping to M-…
Space Plasma Physics: A Review
Bruce T. Tsurutani, Gary P. Zank, Veerle J. Sterken +13
Owing to the ever-present solar wind, our vast solar system is full of plasmas. The turbulent solar wind, together with sporadic solar eruptions, introduces various space plasma pr…
Regression to the Mean can Explain Saturation of Geomagnetic Storms
Nithin Sivadas, David Sibeck, Varsha Subramanyan +4
Extreme space weather events on Earth occur during intervals of strong solar wind driving. The solar wind drives plasma convection and currents in the near-Earth space environment.…
A Turbulent Heating Model Combining Diffusion and Advection Effects for Giant Planet Magnetospheres
C. S. Ng, B. R. Neupane, P. A. Delamere +1
The ion temperature of the magnetospheres of Jupiter and Saturn was observed to increase substantially from about 10 to 30 planet radii. Different heating mechanisms have been prop…
Observations of an Electron-cold Ion Component Reconnection at the Edge of an Ion-scale Antiparallel Reconnection at the Dayside Magnetopause
S. Q. Zhao, H. Zhang, Terry Z. Liu +11
Solar wind parameters play a dominant role in reconnection rate, which controls the solar wind-magnetosphere coupling efficiency at Earth's magnetopause. Besides, low-energy ions f…
Direct Multipoint Observations Capturing the Reformation of a Supercritical Fast Magnetosonic Shock
D. L. Turner, L. B. Wilson, K. A. Goodrich +12
Using multipoint Magnetospheric Multiscale (MMS) observations in an unusual string-of-pearls configuration, we examine in detail observations of the reformation of a fast magnetoso…
Magnetospheric Multiscale (MMS) observations of foreshock transients at their very early stage
Terry Z. Liu, Xin An, Hui Zhang +1
Foreshock transients are ion kinetic structures in the ion foreshock. Due to their dynamic pressure perturbations, they can disturb the bow shock and magnetosphere-ionosphere syste…
How Jupiter's Unusual Magnetospheric Topology Structures Its Aurora
Binzheng Zhang, Peter A. Delamere, Zhonghua Yao +10
Jupiter's bright persistent polar aurora and Earth's dark polar region indicate that the planets' magnetospheric topologies are very different. High-resolution global simulations s…
Electron acceleration by magnetosheath jet-driven bow waves
Terry Z. Liu, Heli Hietala, Vassilis Angelopoulos +2
Magnetosheath jets are localized fast flows with enhanced dynamic pressure. When they supermagnetosonically compress the ambient magnetosheath plasma, a bow wave or shock can form…
Statistical study of magnetosheath jet-driven bow waves
Terry Z. Liu, Heli Hietala, Vassilis Angelopoulos +3
When a magnetosheath jet (localized dynamic pressure enhancements) compresses ambient magnetosheath at a (relative) speed faster than the local magnetosonic speed, a bow wave or sh…
Dayside magnetospheric and ionospheric responses to a foreshock transient on June 25, 2008: 2. 2-D evolution based on dayside auroral imaging
Boyi Wang, Yukitoshi Nishimura, Heli Hietala +8
The foreshock region involves localized and transient structures such as foreshock cavities and hot flow anomalies due to solar wind-bow shock interactions, and foreshock transient…
Radial transport and plasma heating in Jupiter's magnetodisc
C. S. Ng, P. A. Delamere, V. Kaminker +1
The ion temperature of the magnetosphere of Jupiter derived from Galileo PLS data was observed to increase by about an order of magnitude from 10 to 40 Jupiter radii. This suggests…
Observations of kinetic-size magnetic holes in the magnetosheath
S. T. Yao, X. G. Wang, Q. Q. Shi +25
Magnetic holes (MHs), with a scale much greater than \r{ho}i (proton gyroradius), have been widely reported in various regions of space plasmas. On the other hand, kinetic-size mag…
Electrostatic Structures in Space Plasmas: Stability of Two-dimensional Magnetic Bernstein-Greene-Kruskal Modes
C. S. Ng, S. J. Soundararajan, E. Yasin
Electrostatic structures have been observed in many regions of space plasmas, including the solar wind, the magnetosphere, the auroral acceleration region, and in association with…