Article
Geosciences, Multidisciplinary
Brandon L. Burkholder, Li-Jen Chen, Stephen Fuselier, Daniel Gershman, Conrad Schiff, Jason Shuster, Ying Zou, Brian M. Walsh, Patricia Reiff, Steve Petrinec, Anthony Sciola
Summary: Observations by the MMS Mission reveal the existence of multiple magnetopause boundary layers near the southern cusp during storm-time intervals around winter solstice. This provides an opportunity to study the microphysics of the solar wind-magnetosphere interaction during storms. The observations suggest the presence of active reconnection near closed magnetic flux regions in the boundary layer.
GEOPHYSICAL RESEARCH LETTERS
(2022)
Article
Astronomy & Astrophysics
Q. Y. Xiong, S. Y. Huang, Z. G. Yuan, K. Jiang, S. B. Xu, Y. Y. Wei, J. Zhang, Z. Wang, L. Yu, R. T. Lin, Y. Y. Li
Summary: This study investigates the changes in electron energy during magnetic reconnection using full kinetic particle-in-cell simulation. The results reveal that the electron energy gain rate is dependent on the traveling time and path in the inner electron diffusion region.
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS
(2022)
Article
Geosciences, Multidisciplinary
Y. Ren, L. Dai, C. Wang, W. Li, X. Tao, B. Lavraud, O. Le Contel
Summary: Analysis of Magnetospheric Multiscale (MMS) data reveals characteristics in the frequency spectrum of whistler waves near the diffusion region of magnetopause reconnection, with electron temperature anisotropy playing a role in the occurrence rate of these waves.
GEOPHYSICAL RESEARCH LETTERS
(2021)
Article
Physics, Multidisciplinary
Kyunghwan Dokgo, Kyoung-Joo Hwang, James L. Burch, Peter H. Yoon
Summary: This study investigates the nature of high-frequency waves inside a flux rope with a crater-shaped magnetic depression. Two electrostatic wave modes, parallel and perpendicular, are identified with distinct locations and frequencies. The parallel mode can be generated by an electron beam and effectively thermalize electrons, while the generation mechanism of the perpendicular mode remains unclear and requires further study.
FRONTIERS IN PHYSICS
(2021)
Article
Astronomy & Astrophysics
S. L. Robertson, J. P. Eastwood, J. E. Stawarz, H. Hietala, T. D. Phan, B. Lavraud, J. L. Burch, B. Giles, D. J. Gershman, R. Torbert, P. -A. Lindqvist, R. E. Ergun, C. T. Russell, R. J. Strangeway
Summary: Flux ropes have been proposed as a important site for particle energization during magnetic reconnection, and the evidence of electron trapping in the structures support this idea. Potential formation mechanisms and evolutionary states of the structures are compared and analyzed.
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS
(2021)
Editorial Material
Physics, Fluids & Plasmas
Julia E. E. Stawarz, Kevin J. J. Genestreti
Summary: NASA's MMS mission, consisting of four satellites, has been providing unparalleled measurements of local plasma dynamics in near-Earth space for the past 8 years. With advanced space plasma instrumentation, it can measure electromagnetic fields and particle distribution functions at unprecedented speeds, significantly enhancing our understanding of Earth's magnetosphere and plasma physics.
PHYSICS OF PLASMAS
(2023)
Article
Astronomy & Astrophysics
G-W Chen, L-N Hau
Summary: Observations of multiple X line magnetic reconnection (MR) events in Earth's magnetotail have been reported for the first time using the Grad-Shafranov reconstruction model, showing 2D structures with multiple X lines and magnetic islands on a smaller spatial scale. Additionally, findings from this study suggest that MR events with firehose-type temperature anisotropy result in smaller magnetic islands compared to isotropic cases.
ASTROPHYSICAL JOURNAL
(2022)
Article
Physics, Fluids & Plasmas
Seung Choi, Naoki Bessho, Shan Wang, Li-Jen Chen, Michael Hesse
Summary: In this study, a two-dimensional particle-in-cell simulation of asymmetric reconnection with a guide field is used to investigate electron distribution functions and wave intensities in the diffusion region. The analysis reveals the presence of whistler waves with frequencies below the electron cyclotron frequency, concentrated near the magnetospheric separatrix and spreading through the electron diffusion region. The asymmetry of the reconnection outflows is found to affect the wave intensity, with stronger waves observed in the side of the faster electron outflow. The study also examines the characteristics of whistler waves using different analytical techniques.
PHYSICS OF PLASMAS
(2022)
Article
Geosciences, Multidisciplinary
Q. Y. Xiong, S. Y. Huang, M. Zhou, Z. G. Yuan, X. H. Deng, K. Jiang, Y. Y. Wei, S. B. Xu, J. Zhang, R. T. Lin, L. Yu
Summary: Magnetic reconnection, a universal phenomenon, involves energy conversion. This study reports the occurrence of negative energy conversion on the inflow edge of the inner electron diffusion region, mainly contributed by the energy loss in the electron pressure tensor. This finding provides significant insights to expand the understanding of reconnection mechanisms.
GEOPHYSICAL RESEARCH LETTERS
(2022)
Article
Astronomy & Astrophysics
Ramiz A. Qudsi, Brian M. Walsh, Jeff Broll, Emil Atz, Stein Haaland
Summary: In this study, we analyze the observations from the Magnetospheric Multiscale (MMS) mission to determine the factors that affect the accuracy of magnetic reconnection models and are most strongly associated with dayside magnetopause reconnection.
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS
(2023)
Article
Physics, Fluids & Plasmas
Kevin J. Genestreti, Xiaocan Li, Yi-Hsin Liu, James L. Burch, Roy B. Torbert, Stephen A. Fuselier, Takuma Nakamura, Barbara L. Giles, Daniel J. Gershman, Robert E. Ergun, Christopher T. Russell, Robert J. Strangeway
Summary: In this study, the patchiness of energy conversion in electron diffusion regions (EDRs) observed by NASA's MMS mission is investigated. The results show that the patchiness is correlated with parameters describing the structure and stability of the asymptotic inflow regions, as well as the time-variability in the upstream magnetic field direction. The study also suggests that magnetopause reconnection may commonly exhibit patchy behavior at the electron scale.
PHYSICS OF PLASMAS
(2022)
Article
Geosciences, Multidisciplinary
Meng Zhou, Hengyan Man, Yan Yang, Zhihong Zhong, Xiaohua Deng
Summary: This paper evaluates quasi-viscous dissipation in the electron diffusion region at Earth's magnetopause and reveals intriguing findings, such as electrons being cooled rather than heated in a large portion of the diffusion region.
GEOPHYSICAL RESEARCH LETTERS
(2021)
Article
Astronomy & Astrophysics
Q. Lenouvel, V Genot, P. Garnier, S. Toledo-Redondo, B. Lavraud, N. Aunai, G. Nguyen, D. J. Gershman, R. E. Ergun, P. A. Lindqvist, B. Giles, J. L. Burch
Summary: This article identifies 18 magnetic reconnection electron diffusion region (EDR) candidates at the Earth's dayside magnetopause using a neural network algorithm, comparing them with previously reported EDRs and discussing the energy dissipation during the reconnection process as well as the distinction between inner and outer EDRs.
EARTH AND SPACE SCIENCE
(2021)
Article
Astronomy & Astrophysics
S. Hoilijoki, F. Pucci, R. E. Ergun, S. J. Schwartz, F. D. Wilder, S. Eriksson, A. Chasapis, N. Ahmadi, J. M. Webster, J. L. Burch, R. B. Torbert, R. J. Strangeway, B. L. Giles
Summary: During a dayside magnetopause crossing, the MMS mission observed a series of magnetic depletions in the total magnetic field, mainly due to fluctuations in the component normal to the magnetopause.
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS
(2021)
Article
Astronomy & Astrophysics
S. A. Fuselier, J. M. Webster, K. J. Trattner, S. M. Petrinec, K. J. Genestreti, K. R. Pritchard, K. LLera, J. M. Broll, J. L. Burch, R. J. Strangeway
Summary: Observations from the magnetospheric multiscale mission in or near electron diffusion regions (EDRs) at the Earth's magnetopause provide insights into the orientation of reconnection X-lines, highlighting the differences between component and anti-parallel reconnection, and the morphology of reconnection under open interplanetary magnetic field (IMF) conditions. The study also reveals quasi-two-dimensional structures at certain scales and the potential for longer X-lines in different scenarios.
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS
(2021)
Article
Astronomy & Astrophysics
Ari Le, Li-Jen Chen, Blake Wetherton, Brett Keenan, Adam Stanier
Summary: This paper further explores the right-hand instability using numerical solutions of the plasma dispersion relation and non-linear kinetic simulations, with parameters inspired by observations from NASA's MMS mission. The ion distributions in the simulations agree with the Magnetospheric Multiscale spacecraft data, showing the gyrophase bunching characteristic of the instability. The non-linear structures created by right-hand instability tend to be stronger when the plasma beta is lower, presenting planet-sized disturbances to the magnetosphere.
FRONTIERS IN ASTRONOMY AND SPACE SCIENCES
(2023)
Article
Astronomy & Astrophysics
Yan Yang, Francesco Pecora, William H. H. Matthaeus, Sohom Roy, Manuel Enrique Cuesta, Alexandros Chasapis, Tulasi Parashar, Riddhi Bandyopadhyay, D. J. Gershman, B. L. Giles, J. L. Burch
Summary: This study analyzes the distribution of energy in weakly collisional plasmas, focusing on the partitioning between different species and energy channels. The fractions of isotropic compressive, gyrotropic, and nongyrotropic heating for each species are quantified through the analysis of pressure-strain interaction. Comparisons are made between kinetic turbulence simulations and Magnetospheric Multiscale Mission observation data. The results show that compressive heating is stronger than incompressive heating in the magnetosheath, while incompressive heating is stronger in kinetic plasma turbulence simulations. Gyrotropic heating dominates for electrons, while nongyrotropic heating is enhanced for protons in both simulations and observations. The impact of plasma beta on heating variations is also discussed, indicating that increasing beta leads to more heating for protons.
ASTROPHYSICAL JOURNAL
(2023)
Article
Geosciences, Multidisciplinary
Yuri Y. Y. Shprits, Ingo Michaelis, Dedong Wang, Hayley Allison, Ruggero Vasile, Andrei Runov, Alexander Drozdov, Christopher T. Russell, Vladimir Kalegaev, Artem Smirnov
Summary: This study used measurements from the ELFIN-L suit of instruments on the Lomonosov spacecraft to distinguish between stably trapped and drift loss cone electrons. The results show that the loss at MeV energies mainly occurs on the dawn-side, consistent with loss induced by chorus waves.
GEOPHYSICAL RESEARCH LETTERS
(2023)
Article
Geosciences, Multidisciplinary
H. -W. Wang, B. -B. Tang, W. Y. Li, Y. -C. Zhang, D. B. Graham, Y. V. Khotyaintsev, C. -H. Gao, X. -C. Guo, C. Wang
Summary: In this study, detailed electron dynamics in strong guide-field reconnection are investigated. Observations show the presence of a large parallel electric field, with electrons being accelerated or decelerated depending on their direction of entry. We propose that electron beta is an important parameter in guide-field reconnection.
GEOPHYSICAL RESEARCH LETTERS
(2023)
Article
Geosciences, Multidisciplinary
J. Ng, B. M. Walsh, L. -j. Chen, Y. Omelchenko
Summary: Interactions between solar wind ions and neutral hydrogen atoms can produce soft X-rays in Earth's exosphere. Upcoming missions like SMILE and LEXI aim to study the global structure of the magnetosphere using soft X-ray imaging. However, current fluid simulations used to predict X-ray emissions often omit kinetic physics, which can drive the magnetosheath and dayside magnetopause. Our hybrid simulations under quasi-radial interplanetary magnetic fields show that ion-ion instabilities generate foreshock waves and turbulence in the magnetosheath, influencing the dynamics of the cusp and magnetopause. We simulate soft X-ray emission to assess the potential for identifying kinetic structures, but current instruments may lack the time resolution to detect them.
GEOPHYSICAL RESEARCH LETTERS
(2023)
Article
Physics, Fluids & Plasmas
Michael Gedalin, Andrew P. Dimmock, Christopher T. Russell, Nikolai V. Pogorelov, Vadim Roytershteyn
Summary: A collisionless shock is a self-organized structure that adjusts fields and particle distributions to ensure stable mass, momentum, and energy transfer from the upstream to the downstream region. The motion of charged particles generates fields inside the shock front, which in turn governs the particle motion. The overshoot compensates for the deceleration of ion flow by increasing the magnetic field, adjusting downstream ion temperature and pressure, speeding up collisionless relaxation, and reducing anisotropy.
JOURNAL OF PLASMA PHYSICS
(2023)
Article
Physics, Fluids & Plasmas
J. Ng, J. Yoo, L. -j. Chen, N. Bessho, H. Ji
Summary: The recent magnetic reconnection experiment observed short wavelength lower-hybrid waves near the electron diffusion region in strong guide field reconnection. A three-dimensional fully kinetic simulation is performed based on plasma parameters from the experiment to investigate the generation and effects of the lower-hybrid waves on the reconnection process. It is found that the low-beta regions around the reconnection site are unstable to the lower-hybrid drift instability, which is driven by the difference between the electron and ion outflows. These waves modify the electron distributions, causing periodic opening and closing of gaps in electron velocity space and contributing to the anomalous resistivity. The simulation results are discussed in the context of space observations and laboratory experiments.
PHYSICS OF PLASMAS
(2023)
Review
Astronomy & Astrophysics
Benjamin P. P. Weiss, Jose M. G. Merayo, Jodie B. B. Ream, Rona Oran, Peter Brauer, Corey J. J. Cochrane, Kyle Cloutier, Linda T. T. Elkins-Tanton, John L. L. Jorgensen, Clara Maurel, Ryan S. S. Park, Carol A. A. Polanskey, Maria de Soria Santacruz-Pich, Carol A. A. Raymond, Christopher T. T. Russell, Daniel Wenkert, Mark A. A. Wieczorek, Maria T. T. Zuber
Summary: The Psyche Magnetometry Investigation aims to test the hypothesis that asteroid (16) Psyche formed from a differentiated planetesimal. The instrument will measure the magnetic field around the asteroid to search for evidence of remanent magnetization. It consists of two three-axis fluxgate Sensor Units (SUs) mounted along a 2.15-m long boom, connected to Electronics Units (EUs) within the spacecraft bus. The Magnetometer will acquire data for the full duration of the mission to estimate Psyche's dipole moment.
SPACE SCIENCE REVIEWS
(2023)
Article
Astronomy & Astrophysics
N. Omidi, X. -Y. Zhou, C. T. Russell, V. Angelopoulos
Summary: In this study, the interaction between interplanetary shocks and the Moon is investigated using 3-D electromagnetic hybrid simulations and observations. The results show the formation and recovery of a density hole in the shock front on the Moon's dayside, as well as the broadening of the magnetic field shock front in the lunar tail. The interplanetary shock also accelerates energetic ions in the lunar tail. Comparisons between the measurements in the solar wind and lunar tail confirm the absence of a shock front in density and the expected broadening of the magnetic field profile.
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS
(2023)
Article
Astronomy & Astrophysics
Wenyi Sun, Yingjuan Ma, Christopher T. Russell, Janet Luhmann, Andrew Nagy, David Brain
Summary: Although photochemistry-enabled escape of oxygen is dominant at Mars today, ion outflow, including planetary proton loss, plays an important role in the atmosphere's long-term evolution. Improving the MHD model of Mars to differentiate between planetary and solar wind protons, we find that planetary proton escape rates exceed heavy ion loss rates and solar wind proton inflows. However, the contribution of planetary protons to hydrogen loss is limited. By considering different reactions, we conclude that H-O charge exchange affects low altitude densities while impact ionizations impact escape rates at higher altitudes. This research highlights the need to include specific treatment of proton origins in future studies on the fate of water on Mars.
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS
(2023)
Article
Astronomy & Astrophysics
Z. C. Tian, M. Zhou, H. Y. Man, Z. H. Zhong, X. H. Deng, D. J. Gershman, Y. V. Khotyaintsev, C. T. Russell
Summary: This paper presents the simultaneous observation of the inner and outer electron diffusion region (EDR) in magnetic reconnection with a large guide field at the dayside magnetopause by the magnetospheric multiscale (MMS) spacecraft. The inner EDR is characterized by positive J·E', while the outer EDR is manifested by negative J·E' and opposite out-of-plane electric field. The observation of bidirectional accelerated electron jets on the opposite side of the X-line is significant, and the fortuitous formation of MMS provides estimates for the length of the inner EDR and the reconnection rate.
ASTROPHYSICAL JOURNAL
(2023)
Article
Geosciences, Multidisciplinary
Tongkuai Li, Wenya Li, Binbin Tang, Yuri. V. Khotyaintsev, Daniel Bruce Graham, Akhtar Ardakani, J. L. Burch, D. J. Gershman, B. Lavraud, C. T. Russell, Quanming Lu, Xiaocheng Guo, Chi Wang
Summary: This study presents Magnetospheric Multiscale (MMS) observations of a K-H wave event accompanied by ongoing magnetic reconnection under southward IMF conditions. The nonlinear K-H waves exhibit quasi-periodic fluctuations, presence of low-density and high-speed ions, and variations in the boundary normal vectors. Through the identification of Alfvenic ion jets and the escape of energetic magnetospheric electrons, clear evidence of on-going magnetic reconnection is revealed. Notably, out of the 36 magnetopause current-sheet crossings in this event, 19 exhibit unambiguous signatures of reconnection at both the leading and trailing edges, indicating the compression effect resulting from the large-scale evolution of the K-H waves.
GEOPHYSICAL RESEARCH LETTERS
(2023)
Article
Physics, Fluids & Plasmas
Harry C. Lewis, Julia E. Stawarz, Luca Franci, Lorenzo Matteini, Kristopher Klein, Chadi S. Salem, James L. Burch, Robert E. Ergun, Barbara L. Giles, Christopher T. Russell, Per-Arne Lindqvist
Summary: Turbulence in space plasmas is analyzed using Magnetospheric Multiscale (MMS) measurements. Different linear and nonlinear processes are decomposed using the electric field dynamics measured by MMS. Spectral characteristics of the terms in generalized Ohm's law are identified, including the dominance of the Hall effect over MHD, constant amplitude ratio of electron pressure to Hall effect, and independent scaling of nonlinear and linear components. The findings provide insights into the relationship between fluctuation amplitudes and plasma conditions.
PHYSICS OF PLASMAS
(2023)
Article
Astronomy & Astrophysics
Ze-Fan Yin, Xu-Zhi Zhou, Ze-Jun Hu, Qiu-Gang Zong, Jian-Jun Liu, Chao Yue, Shan Wang, Xing-Xin Zhao, Hui-Gen Yang, Bin Li
Summary: Based on optical measurements from the high-latitude Yellow River Station and magnetic measurements from multiple ground-based stations, we investigated a periodic Poleward-moving auroral arcs (PMAAs) event at the postdawn sector. The observations showed long-duration periodic auroral arcs in multiple wavebands with a wide energy range of precipitating electrons. The auroral luminosity variations and ground-based magnetic pulsations exhibited consistent periodicity, indicating potential field line resonance driven by perturbations at the magnetopause boundary layer.
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS
(2023)