Search Publications

Effects from dayside magnetosphere to distant tail unleashed by a bifurcated, non-reconnecting interplanetary current sheet
DOI: 10.3389/fphy.2022.942486 Bibcode: 2022FrP....10.2486F

Berchem, J.; Wing, S.; Farrugia, C. J. +6 more

Global magnetospheric effects resulting from the passage at Earth of large-scale structures have been well studied. The effects of common and short-term features, such as discontinuities and current sheets (CSs), have not been studied in the same depth. Herein we show how a seemingly unremarkable interplanetary feature can cause widespread effects…

2022 Frontiers in Physics
Cluster 4
Comparing Quasi-Parallel and Quasi-Perpendicular Configuration in the Terrestrial Magnetosheath: Multifractal Analysis
DOI: 10.3389/fphy.2022.903632 Bibcode: 2022FrP....10.3632G

Sorriso-Valvo, Luca; Burgess, David; Yordanova, Emiliya +4 more

The terrestrial magnetosheath is characterized by large-amplitude magnetic field fluctuations. In some regions, and depending on the bow-shock geometry, these can be observed on several scales, and show the typical signatures of magnetohydrodynamic turbulence. Using Cluster data, magnetic field spectra and flatness are observed in two intervals se…

2022 Frontiers in Physics
Cluster 3
Data Mining Reconstruction of Magnetotail Reconnection and Implications for Its First-Principle Modeling
DOI: 10.3389/fphy.2021.644884 Bibcode: 2021FrP.....9...90S

Sitnov, Mikhail; Stephens, Grant; Motoba, Tetsuo +1 more

Magnetic reconnection is a fundamental process providing topological changes of the magnetic field, reconfiguration of space plasmas and release of energy in key space weather phenomena, solar flares, coronal mass ejections and magnetospheric substorms. Its multiscale nature is difficult to study in observations because of their sparsity. Here we …

2021 Frontiers in Physics
Cluster 25
Concurrent empirical magnetic reconstruction of storm and substorm spatial scales using data mining and virtual spacecraft
DOI: 10.3389/fphy.2021.653111 Bibcode: 2021FrP.....9..210S

Stephens, Grant K.; Sitnov, Mikhail I.

Data-mining (DM) has ushered in a new era of empirical magnetic reconstructions of the 4 magnetosphere via application of the k-nearest neighbors (kNN) method. In this approach, 5 the combined magnetosphere storm-substorm state is characterized by the Sym-H and AL IMF 6 indices, their time derivatives, and the solar wind electric field vBz . Howev…

2021 Frontiers in Physics
Cluster 9
Kelvin-Helmholtz Instability Associated with Reconnection and Ultra Low Frequency Waves at the Ground: A Case Study
DOI: 10.3389/fphy.2021.738988 Bibcode: 2021FrP.....9..700K

Grigorenko, E. E.; Kronberg, E. A.; Nykyri, K. +7 more

The Kelvin-Helmholtz instability (KHI) and its effects relating to the transfer of energy and mass from the solar wind into the magnetosphere remain an important focus of magnetospheric physics. One such effect is the generation of Pc4-Pc5 ultra low frequency (ULF) waves (periods of 45-600 s). On 3 July 2007 at ~0500 magnetic local time the Cluste…

2021 Frontiers in Physics
Cluster 7
On the Origin of High–Frequency Magnetic Fluctuations in the Interplanetary Medium: A Brownian–like Approach
DOI: 10.3389/fphy.2021.613759 Bibcode: 2021FrP.....9...18C

Vecchio, Antonio; Chiappetta, Federica; Lepreti, Fabio +2 more

Low–frequency fluctuations in the interplanetary medium have been extensively investigated and described in the framework of turbulence, and the observed universal scaling behavior represents a clear signature of the underlying energy cascade. On the contrary, the interpretation of observations of plasma fluctuations at high frequencies, where wav…

2021 Frontiers in Physics
Cluster 5
High-latitude cold ion outflow inferred from the Cluster wake observations in the magnetotail lobes and the polar cap region
DOI: 10.3389/fphy.2021.743316 Bibcode: 2021FrP.....9..620L

André, Mats; Li, Kun; Wei, Yong +3 more

Cold ions with low (a few eV) thermal energies and also often low bulk drift energies, dominate the ion population in the Earth's magnetosphere. These ions mainly originate from the ionosphere. Here we concentrate on cold ions in the high latitude polar regions, where magnetic field lines are open and connected to the magnetotail. Outflow from the…

2021 Frontiers in Physics
Cluster 1
AME: A Cross-scale Constellation of CubeSats to Explore Magnetic Reconnection in the Solar-Terrestrial Relation
DOI: 10.3389/fphy.2020.00089 Bibcode: 2020FrP.....8...89D

Dunlop, Malcolm; Khotyaintsev, Yuri; Phan, Tai +25 more

A major subset of solar-terrestrial relations, responsible in particular for the driver of space weather phenomena, is the interaction between the Earth's magnetosphere and the solar wind. As one of the most important modes of the solar-wind-magnetosphere interaction, magnetic reconnection regulates the energy transport and energy release in the s…

2020 Frontiers in Physics
Cluster 24
A Note on Capon's Minimum Variance Projection for Multi-Spacecraft Data Analysis
DOI: 10.3389/fphy.2019.00008 Bibcode: 2019FrP.....7....8N

Narita, Yasuhito

Capon's minimum variance projection for the multi-point measurements is revisited using the method of likelihood function to derive the minimum variance projection and a simplified error estimate analytically. Theoretical construction of the minimum variance projection assumes a Gaussian form of the likelihood function and also regards the data co…

2019 Frontiers in Physics
Cluster 4
Ion-Scale Sideband Waves and Filament Formation: Alfvénic Impact on Heliospheric Plasma Turbulence
DOI: 10.3389/fphy.2017.00008 Bibcode: 2017FrP.....5....8N

Motschmann, Uwe; Narita, Yasuhito

A mini-review is given about two recent discoveries in the solar wind turbulence research on ion-kinetic scales: the existence of sideband waves (or breakdown of the linear mode wave picture) and the wavevector anisotropy leading to a persistent filament formation in a wide range of plasma beta.

2017 Frontiers in Physics
Cluster 5