Search Publications

Scaling laws for the energy transfer in space plasma turbulence
DOI: 10.1016/j.physrep.2022.12.001 Bibcode: 2023PhR..1006....1M

Sorriso-Valvo, Luca; Marino, Raffaele

One characteristic trait of space plasmas is the multi-scale dynamics resulting from non-linear transfers and conversions of various forms of energy. Routinely evidenced in a range from the large-scale solar structures down to the characteristic scales of ions and electrons, turbulence is a major cross-scale energy transfer mechanism in space plas…

2023 Physics Reports
Cluster 54
HelioSwarm: A Multipoint, Multiscale Mission to Characterize Turbulence
DOI: 10.1007/s11214-023-01019-0 Bibcode: 2023SSRv..219...74K

Verscharen, Daniel; Retinò, Alessandro; Alexandrova, Olga +47 more

HelioSwarm (HS) is a NASA Medium-Class Explorer mission of the Heliophysics Division designed to explore the dynamic three-dimensional mechanisms controlling the physics of plasma turbulence, a ubiquitous process occurring in the heliosphere and in plasmas throughout the universe. This will be accomplished by making simultaneous measurements at ni…

2023 Space Science Reviews
Cluster 36
Particle Acceleration by Magnetic Reconnection in Geospace
DOI: 10.1007/s11214-023-01011-8 Bibcode: 2023SSRv..219...75O

Khotyaintsev, Yuri; Drake, James F.; Oka, Mitsuo +7 more

Particles are accelerated to very high, non-thermal energies during explosive energy-release phenomena in space, solar, and astrophysical plasma environments. While it has been established that magnetic reconnection plays an important role in the dynamics of Earth's magnetosphere, it remains unclear how magnetic reconnection can further explain pa…

2023 Space Science Reviews
Cluster 19
An Anisotropic Density Turbulence Model from the Sun to 1 au Derived from Radio Observations
DOI: 10.3847/1538-4357/acf6c1 Bibcode: 2023ApJ...956..112K

Kontar, Eduard P.; Chen, Xingyao; Chrysaphi, Nicolina +5 more

Solar radio bursts are strongly affected by radio-wave scattering on density inhomogeneities, changing their observed time characteristics, sizes, and positions. The same turbulence causes angular broadening and scintillation of galactic and extragalactic compact radio sources observed through the solar atmosphere. Using large-scale simulations of…

2023 The Astrophysical Journal
Cluster 18
Laboratory Study of Collisionless Magnetic Reconnection
DOI: 10.1007/s11214-023-01024-3 Bibcode: 2023SSRv..219...76J

Yamada, M.; Burch, J.; Egedal, J. +13 more

A concise review is given on the past two decades' results from laboratory experiments on collisionless magnetic reconnection in direct relation with space measurements, especially by the Magnetospheric Multiscale (MMS) mission. Highlights include spatial structures of electromagnetic fields in ion and electron diffusion regions as a function of u…

2023 Space Science Reviews
Cluster 14
Simultaneous Global Ionospheric Disturbances Associated With Penetration Electric Fields During Intense and Minor Solar and Geomagnetic Disturbances
DOI: 10.1029/2023GL104250 Bibcode: 2023GeoRL..5004250Z

Nishimura, Yukitoshi; Zhang, Shun-Rong; Vierinen, Juha +8 more

A new observational phenomenon, named Simultaneous Global Ionospheric Density Disturbance (SGD), is identified in GNSS total electron content (TEC) data during periods of three typical geospace disturbances: a Coronal Mass Ejection-driven severe disturbance event, a high-speed stream event, and a minor disturbance day with a maximum Kp of 4. SGDs …

2023 Geophysical Research Letters
Cluster 13
Electron Heating Scales in Collisionless Shocks Measured by MMS
DOI: 10.1029/2022GL100400 Bibcode: 2023GeoRL..5000400J

Johlander, Andreas; Khotyaintsev, Yuri V.; Dimmock, Andrew P. +2 more

Electron heating at collisionless shocks in space is a combination of adiabatic heating due to large-scale electric and magnetic fields and non-adiabatic scattering by high-frequency fluctuations. The scales at which heating happens hints to what physical processes are taking place. In this letter, we study electron heating scales with data from t…

2023 Geophysical Research Letters
Cluster 12
The evolving paradigm of the subauroral geospace
DOI: 10.3389/fspas.2023.1118758 Bibcode: 2023FrASS..1018758M

Mishin, Evgeny V.

An assessment of the status quo of fast subauroral flows—subauroral ion drifts (SAID) and subauroral polarization streams (SAPS), is presented. For a few decades, their development has been interpreted in terms of the voltage and current magnetospheric generators based largely on the drift motion of test particles. Recent multispacecraft observati…

2023 Frontiers in Astronomy and Space Sciences
Cluster 12
Global Structure of Magnetotail Reconnection Revealed by Mining Space Magnetometer Data
DOI: 10.1029/2022JA031066 Bibcode: 2023JGRA..12831066S

Sitnov, M. I.; Genestreti, K. J.; Tsyganenko, N. A. +5 more

Reconnection in the magnetotail occurs along so-called X-lines, where magnetic field lines tear and detach from plasma on microscopic spatial scales (comparable to particle gyroradii). In 2017-2020, the Magnetospheric MultiScale (MMS) mission detected X-lines in the magnetotail enabling their investigation on local scales. However, the global stru…

2023 Journal of Geophysical Research (Space Physics)
Cluster 10
Evidence for lunar tide effects in Earth's plasmasphere
DOI: 10.1038/s41567-022-01882-8 Bibcode: 2023NatPh..19..486X

Zong, Qiugang; Guo, Ruilong; Xiao, Chao +18 more

Tides are universal and affect spatially distributed systems, ranging from planetary to galactic scales. In the Earth-Moon system, effects caused by lunar tides were reported in the Earth's crust, oceans, neutral gas-dominated atmosphere (including the ionosphere) and near-ground geomagnetic field. However, whether a lunar tide effect exists in th…

2023 Nature Physics
Cluster 10