Search Publications

VLF Transmitter Signals Observed by the Cluster Spacecraft Over a Wide Range of Latitudes
DOI: 10.1029/2024JA033621 Bibcode: 2025JGRA..13033621N

Santolík, O.; Němec, F.; Albert, J. M.

Very low frequency transmitter signals can penetrate through the ionosphere and propagate in the inner magnetosphere, being observed by spacecraft instruments with sufficient frequency resolution and range. We use 23 years of measurements performed by the Waves of High frequency and Sounder for Probing of Electron density by Relaxation instrument …

2025 Journal of Geophysical Research (Space Physics)
Cluster 0
Solar Wind Current Sheets: MVA Inaccuracy and Recommended Single-Spacecraft Methodology
DOI: 10.1029/2023JA032215 Bibcode: 2024JGRA..12932215W

Wang, R.; Phan, T. D.; Mozer, F. S. +1 more

We present the analysis of 1,831 current sheets (CS) observed aboard four Cluster spacecraft in a pristine solar wind. Four-spacecraft estimates of the CS normal and propagation velocity are compared with different single-spacecraft estimates. The Minimum Variance Analysis (MVA) of the magnetic field is shown to be highly inaccurate in estimating …

2024 Journal of Geophysical Research (Space Physics)
Cluster 10
New Chorus Diffusion Coefficients for Radiation Belt Modeling
DOI: 10.1029/2023JA031607 Bibcode: 2024JGRA..12931607W

Meredith, Nigel P.; Wong, Jin-Mann; Horne, Richard B. +2 more

Whistler mode chorus is an important magnetospheric wave emission playing a major role in radiation belt dynamics, where it contributes to both the acceleration and loss of relativistic electrons. In this study we compute bounce and drift averaged chorus diffusion coefficients for 3.0 < L* < 6.0, using the TS04 external magnetic field model,…

2024 Journal of Geophysical Research (Space Physics)
Cluster DoubleStar 8
Storm-Time Very-Near-Earth Magnetotail Reconnection: A Statistical Perspective
DOI: 10.1029/2024JA032434 Bibcode: 2024JGRA..12932434B

Angelopoulos, V.; Beyene, F.

The ring current, an equatorial near-Earth current, fluctuates in response to solar wind plasma interactions with Earth's magnetosphere. Despite extensive research on storm-time ring current energization, direct evidence of the energy transport into the inner-magnetosphere that powers this current remains scarce. Recent observations revealing that…

2024 Journal of Geophysical Research (Space Physics)
Cluster 5
Key Factors Determining Nightside Energetic Electron Losses Driven by Whistler-Mode Waves
DOI: 10.1029/2023JA032351 Bibcode: 2024JGRA..12932351T

Ma, Qianli; Zhang, Xiao-Jia; Agapitov, Oleksiy +4 more

Energetic electron losses by pitch-angle scattering and precipitation to the atmosphere from the radiation belts are controlled, to a great extent, by resonant wave particle interactions with whistler-mode waves. The efficacy of such precipitation is primarily modulated by wave intensity, although its relative importance, compared to other wave an…

2024 Journal of Geophysical Research (Space Physics)
Cluster 5
Reconnection Inside a Dipolarization Front of a Diverging Earthward Fast Flow
DOI: 10.1029/2023JA031976 Bibcode: 2024JGRA..12931976H

Escoubet, C. P.; Fazakerley, A. N.; Le Contel, O. +18 more

We examine a Dipolarization Front (DF) event with an embedded electron diffusion region (EDR), observed by the Magnetospheric Multiscale (MMS) spacecraft on 08 September 2018 at 14:51:30 UT in the Earth's magnetotail by applying multi-scale multipoint analysis methods. In order to study the large-scale context of this DF, we use conjunction observ…

2024 Journal of Geophysical Research (Space Physics)
Cluster 4
Global Environmental Constraints on Magnetic Reconnection at the Magnetopause From In Situ Measurements
DOI: 10.1029/2023JA032098 Bibcode: 2024JGRA..12932098M

Lavraud, B.; Génot, V.; Jeandet, A. +5 more

Progress in locating the X-line on the magnetopause beyond the atypical due south interplanetary magnetic field (IMF) condition is hampered by the fact that the global plasma and field spatial distributions constraining where reconnection could develop on the magnetopause are poorly known. This work presents global maps of the magnetic shear, curr…

2024 Journal of Geophysical Research (Space Physics)
Cluster DoubleStar 2
The April 2023 SYM-H = −233 nT Geomagnetic Storm: A Classical Event
DOI: 10.1029/2024JA032986 Bibcode: 2024JGRA..12932986H

Henri, Pierre; Hajra, Rajkumar; Horne, Richard B. +8 more

The 23-24 April 2023 double-peak (SYM-H intensities of −179 and −233 nT) intense geomagnetic storm was caused by interplanetary magnetic field southward component Bs associated with an interplanetary fast-forward shock-preceded sheath (Bs of 25 nT), followed by a magnetic cloud (MC) (Bs of 33 nT), respectively. The…

2024 Journal of Geophysical Research (Space Physics)
Cluster 2
On the Contribution of Latitude-Dependent ULF Waves to the Radial Transport of Off-Equatorial Relativistic Electrons in the Radiation Belts
DOI: 10.1029/2024JA032905 Bibcode: 2024JGRA..12932905S

Angelopoulos, Vassilis; Li, Xinlin; Ergun, Robert E. +15 more

Ultra-low frequency (ULF) waves radially diffuse hundreds-keV to few-MeV electrons in the magnetosphere, as the range of drift frequencies of such electrons overlaps with the wave frequencies, leading to resonant interactions. Theoretically this process is described by analytic expressions of the resonant interactions between electrons and ULF wav…

2024 Journal of Geophysical Research (Space Physics)
Cluster 1
Magnetic Field in the Earth's Magnetosheath: Models Versus Observations
DOI: 10.1029/2023JA032393 Bibcode: 2024JGRA..12932393V

Vandas, M.; Romashets, E.

Magnetic field measurements in the Earth's magnetosheath are compared with four analytical models, namely Kobel and Flückiger (1994), (https://doi.org/10.1029/94ja01778), Romashets and Vandas (2019), (https://doi.org/10.1029/2018ja026006), Vandas and…

2024 Journal of Geophysical Research (Space Physics)
Cluster 1