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Ohm's Law, the Reconnection Rate, and Energy Conversion in Collisionless Magnetic Reconnection
DOI: 10.1007/s11214-025-01142-0 Bibcode: 2025SSRv..221...16L

Phan, Tai; Cassak, Paul A.; Hoshino, Masahiro +12 more

Magnetic reconnection is a ubiquitous plasma process that transforms magnetic energy into particle energy during eruptive events throughout the universe. Reconnection not only converts energy during solar flares and geomagnetic substorms that drive space weather near Earth, but it may also play critical roles in the high energy emissions from the …

2025 Space Science Reviews
Cluster 8
Jets Downstream of Collisionless Shocks: Recent Discoveries and Challenges
DOI: 10.1007/s11214-024-01129-3 Bibcode: 2025SSRv..221....4K

Raptis, Savvas; Blanco-Cano, Xóchitl; Karlsson, Tomas +19 more

Plasma flows with enhanced dynamic pressure, known as magnetosheath jets, are often found downstream of collisionless shocks. As they propagate through the magnetosheath, they interact with the surrounding plasma, shaping its properties, and potentially becoming geoeffective upon reaching the magnetopause. In recent years (since 2016), new researc…

2025 Space Science Reviews
Cluster 3
The Role of Kinetic Instabilities and Waves in Collisionless Magnetic Reconnection
DOI: 10.1007/s11214-024-01133-7 Bibcode: 2025SSRv..221...20G

Khotyaintsev, Yu. V.; Graham, D. B.; Steinvall, K. +13 more

Magnetic reconnection converts magnetic field energy into particle energy by breaking and reconnecting magnetic field lines. Magnetic reconnection is a kinetic process that generates a wide variety of kinetic waves via wave-particle interactions. Kinetic waves have been proposed to play an important role in magnetic reconnection in collisionless p…

2025 Space Science Reviews
Cluster 2
From Foreshock 30-Second Waves to Magnetospheric Pc3 Waves
DOI: 10.1007/s11214-025-01152-y Bibcode: 2025SSRv..221...26T

Kajdič, Primož; Pfau-Kempf, Yann; Turc, Lucile +7 more

Ultra-low frequency waves, with periods between 1-1000 s, are ubiquitous in the near-Earth plasma environment and play an important role in magnetospheric dynamics and in the transfer of electromagnetic energy from the solar wind to the magnetosphere. A class of those waves, often referred to as Pc3 waves when they are recorded from the ground, wi…

2025 Space Science Reviews
Cluster 0
Magnetic Reconnection at Planetary Bodies and Astrospheres
DOI: 10.1007/s11214-023-01017-2 Bibcode: 2024SSRv..220....7G

Stawarz, Julia E.; Phan, Tai D.; Harada, Yuki +11 more

Magnetic reconnection is a fundamental mechanism for the transport of mass and energy in planetary magnetospheres and astrospheres. While the process of reconnection is itself ubiquitous across a multitude of systems, the techniques used for its analysis can vary across scientific disciplines. Here we frame the latest understanding of reconnection…

2024 Space Science Reviews
Cluster 10
Global-Scale Processes and Effects of Magnetic Reconnection on the Geospace Environment
DOI: 10.1007/s11214-024-01067-0 Bibcode: 2024SSRv..220...34F

Eastwood, J. P.; Lavraud, B.; Nakamura, R. +14 more

Recent multi-point measurements, in particular from the Magnetospheric Multiscale (MMS) spacecraft, have advanced the understanding of micro-scale aspects of magnetic reconnection. In addition, the MMS mission, as part of the Heliospheric System Observatory, combined with recent advances in global magnetospheric modeling, have furthered the unders…

2024 Space Science Reviews
Cluster 9
The Interplay Between Collisionless Magnetic Reconnection and Turbulence
DOI: 10.1007/s11214-024-01124-8 Bibcode: 2024SSRv..220...90S

Hasegawa, H.; Khotyaintsev, Yu. V.; Graham, D. B. +13 more

Alongside magnetic reconnection, turbulence is another fundamental nonlinear plasma phenomenon that plays a key role in energy transport and conversion in space and astrophysical plasmas. From a numerical, theoretical, and observational point of view there is a long history of exploring the interplay between these two phenomena in space plasma env…

2024 Space Science Reviews
Cluster 4
Heavy Molecular and Metallic Ions in the Magnetosphere
DOI: 10.1007/s11214-024-01114-w Bibcode: 2024SSRv..220...82Y

Yamauchi, M.; Wurz, P.; Dandouras, I. +11 more

Observations and present knowledge of heavy ions with mass ≥ 27 in the magnetosphere are reviewed. There are four ultimate sources of these heavy ions: the solar wind (mainly high charge-state atomic ions), the ionosphere (mainly molecular ions), the atmospheric metal layers that originate ultimately from ablation of meteoroids and possibly space …

2024 Space Science Reviews
Cluster SOHO 0
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