Search Publications

Multi-Spacecraft Magnetic Field Reconstructions: A Cross-Scale Comparison of Methods
DOI: 10.1029/2023EA003369 Bibcode: 2024E&SS...1103369B

Klein, K. G.; Broeren, T.; TenBarge, J. M.

Space plasma studies frequently use in situ magnetic field measurements taken from many spacecraft simultaneously. A useful data product of these measurements is the reconstructed magnetic field in a volume near the spacecraft observatory. We compare a standard Linear method of computing the magnetic field at arbitrary spatial points to two novel …

2024 Earth and Space Science
Cluster 2
A Database for Simultaneous Observations of the Earth's Magnetosheath by Cluster and MMS Between 2017 and 2021
DOI: 10.1029/2024EA003638 Bibcode: 2024E&SS...1103638M

Voitcu, Gabriel; Echim, Marius; Munteanu, Costel +4 more

This paper describes a catalog of simultaneous observations of the Earth's magnetosheath by ESA's Cluster and NASA's MMS missions. The catalog is built from a visual inspection of summary plots provided by the two missions complemented by an analysis of high-resolution magnetic field data. The catalog includes 117 events when Cluster 4 and MMS 4 c…

2024 Earth and Space Science
Cluster 0
An Integrated Nonlinear Analysis (INA) Software for Space Plasma Turbulence
DOI: 10.1029/2022EA002692 Bibcode: 2023E&SS...1002692M

Echim, Marius; Munteanu, Costel; Kovács, Péter

We built an integrated nonlinear analysis software (INA)-designed to study space plasma turbulence and intermittency. The MATLAB programming environment was used for the algorithmic development and implementation of methods for spectral analysis, multiscale fluctuations and multifractal analysis. The performance of INA is demonstrated using magnet…

2023 Earth and Space Science
Cluster Ulysses 1
Classifying Interplanetary Discontinuities Using Supervised Machine Learning
DOI: 10.1029/2023EA002960 Bibcode: 2023E&SS...1002960D

Munteanu, Costel; Dumitru, Daniel

Directional discontinuities (DDs) are defined as abrupt changes of the magnetic field orientation. We use observations from ESA's Cluster mission to compile a database of events: Four thousand two hundred and sixteen events are identified in January-April 2007, and 5,194 in January-April 2008. Localized time scale images depicting angular changes …

2023 Earth and Space Science
Cluster 1
Compiling Magnetosheath Statistical Data Sets Under Specific Solar Wind Conditions: Lessons Learnt From the Dayside Kinetic Southward IMF GEM Challenge
DOI: 10.1029/2020EA001095 Bibcode: 2020E&SS....701095D

Dimmock, A. P.; Hietala, H.; Zou, Y.

The Geospace Environmental Modelling (GEM) community offers a framework for collaborations between modelers, observers, and theoreticians in the form of regular challenges. In many cases, these challenges involve model-data comparisons to provide wider context to observations or validate model results. To perform meaningful comparisons, a statisti…

2020 Earth and Space Science
Cluster 9
Open-Source Software Analysis Tool to Investigate Space Plasma Turbulence and Nonlinear DYNamics (ODYN)
DOI: 10.1029/2019EA001004 Bibcode: 2020E&SS....701004T

Echim, M. M.; Teodorescu, E.

We have designed and built a versatile modularized software library—ODYN—that wraps a comprehensive set of advanced data analysis methods meant to facilitate the study of turbulence, nonlinear dynamics, and complexity in space plasmas. The Python programming language is used for the algorithmic implementation of models and methods devised to under…

2020 Earth and Space Science
Cluster Ulysses 6
Robust Adaptive Spacecraft Array Derivative Analysis
DOI: 10.1029/2019EA000953 Bibcode: 2020E&SS....700953V

Vogt, J.; Blagau, A.; Pick, L.

Multispacecraft missions such as Cluster, Themis, Swarm, and MMS contribute to the exploration of geospace with their capability to produce gradient and curl estimates from sets of spatially distributed in situ measurements. This paper combines all existing estimators of the reciprocal vector family for spatial derivatives and their errors. The re…

2020 Earth and Space Science
Cluster 4
Intermittency in Solar Wind Turbulence From Fluid to Kinetic Scales
DOI: 10.1029/2018EA000535 Bibcode: 2019E&SS....6..656B

Bruno, Roberto

Solar wind is a highly turbulent medium exhibiting fluctuations ranging from the solar sidereal rotation period to proton and electron gyroperiods. Their amplitudes show remarkable scalings with frequency across more than seven decades, suggesting a self-similar nature for these fluctuations. However, these fluctuations are not globally scale inva…

2019 Earth and Space Science
Cluster 46