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Determining the Beaming of Io Decametric Emissions: A Remote Diagnostic to Probe the Io-Jupiter Interaction
DOI: 10.1029/2021JA030160 Bibcode: 2022JGRA..12730160L

Kurth, W. S.; Cecconi, B.; Lamy, L. +8 more

We investigate the beaming of 11 Io-Jupiter decametric (Io-DAM) emissions observed by Juno/Waves, the Nançay Decameter Array, and NenuFAR. Using an up-to-date magnetic field model and three methods to position the active Io Flux Tube (IFT), we accurately locate the radiosources and determine their emission angle θ from the local magnetic field vec…

2022 Journal of Geophysical Research (Space Physics)
eHST 13
Radial and Local Time Variations in the Thickness of Jupiter's Magnetospheric Current Sheet
DOI: 10.1029/2022JA030664 Bibcode: 2022JGRA..12730664K

Hospodarsky, G. B.; Khurana, K. K.; Paranicas, C. P. +1 more

The magnetic field observations from the Galileo, Ulysses, Voyager 1 and 2, and Pioneer 10 and 11 spacecraft are analyzed to understand the structures and thickness of the Jovian magnetospheric current sheet. Using a new technique that can determine the motion of the spacecraft relative to the current sheet, we have built the first global map of t…

2022 Journal of Geophysical Research (Space Physics)
Ulysses 11
Scale-Dependent Kurtosis of Magnetic Field Fluctuations in the Solar Wind: A Multi-Scale Study With Cluster 2003-2015
DOI: 10.1029/2021JA029483 Bibcode: 2022JGRA..12729483R

Alexandrova, O.; Lion, S.; Nakamura, R. +9 more

During the lifetime of the Cluster mission, the inter-spacecraft distances in the solar wind have changed from the large, fluid, scales (∼104 km), down to the scales of protons (∼102 km). As part of the guest investigator campaign, the mission achieved a formation where a pair of spacecraft were separated by ∼7 km. The small …

2022 Journal of Geophysical Research (Space Physics)
Cluster 10
Discrete Aurora on the Nightside of Mars: Occurrence Location and Probability
DOI: 10.1029/2021JA029716 Bibcode: 2022JGRA..12729716F

Luhmann, Janet; Fang, Xiaohua; Jakosky, Bruce +7 more

This paper represents the first attempt to predict the occurrence location and probability of discrete electron aurora on the nightside of Mars. We run a 3-D time-dependent magnetohydrodynamic model to characterize the spatial and temporal dynamics of magnetic field and plasma distributions over the course of one planetary rotation. We perform eig…

2022 Journal of Geophysical Research (Space Physics)
MEx 9
Decadal and Annual Variations in Meteoric Flux From Ulysses, Wind, and SOFIE Observations
DOI: 10.1029/2022JA030749 Bibcode: 2022JGRA..12730749H

Malaspina, David; Hunziker, Silvan; Sterken, Veerle +3 more

Our solar system is filled with meteoric particles, or cosmic dust, which is either interplanetary or interstellar in origin. Interstellar dust (ISD) enters the heliosphere due to the relative motion of the sun and the interstellar flow. Interplanetary dust (IPD) comes primarily from asteroid collisions or comet sublimation, and comprises the bulk…

2022 Journal of Geophysical Research (Space Physics)
Ulysses 9
Pitch Angle Distribution of MeV Electrons in the Magnetosphere of Jupiter
DOI: 10.1029/2022JA030627 Bibcode: 2022JGRA..12730627N

Witasse, O.; Kollmann, P.; Nénon, Q. +3 more

The magnetosphere of Jupiter harbors the most extreme fluxes of MeV electrons in the solar system and therefore provides a testbed of choice to understand the origin, transport, acceleration, and loss of energetic electrons in planetary magnetospheres. Along this objective, the Pitch Angle Distribution (PAD) of energetic electrons may reveal signa…

2022 Journal of Geophysical Research (Space Physics)
Ulysses 9
Three-Dimensional Structure of the Corona During WHPI Campaign Rotations CR-2219 and CR-2223
DOI: 10.1029/2022JA030406 Bibcode: 2022JGRA..12730406L

Lamy, P.; Gilardy, H.; Nuevo, F. A. +6 more

Differential emission measure tomography (DEMT) and white light (WL) tomography were applied to study the three-dimensional (3D) structure of the global solar corona for two Whole Heliosphere and Planetary Interactions campaign periods, Carrington rotations 2219 and 2223. With DEMT, Solar Dynamics Observatory/Atmospheric Imaging Assembly images we…

2022 Journal of Geophysical Research (Space Physics)
SOHO 8
A Climatology of Long-Duration High 2-MeV Electron Flux Periods in the Outer Radiation Belt
DOI: 10.1029/2022JA030661 Bibcode: 2022JGRA..12730661M

Artemyev, A. V.; Agapitov, O. V.; Mourenas, D. +1 more

Since the advent of the Space Age, the importance of understanding and forecasting relativistic electron fluxes in the Earth's radiation belts has been steadily growing due to the threat that such particles pose to satellite electronics. Here, we provide a model of long-duration periods of high time-integrated 2-MeV electron flux deep inside the o…

2022 Journal of Geophysical Research (Space Physics)
INTEGRAL 8
Massive Multi-Mission Statistical Study and Analytical Modeling of the Earth's Magnetopause: 3. An Asymmetric Non Indented Magnetopause Analytical Model
DOI: 10.1029/2021JA030112 Bibcode: 2022JGRA..12730112N

Lavraud, B.; Jeandet, A.; Aunai, N. +3 more

In a companion statistical study, we showed that the expression of the magnetopause surface as a power law of an elliptic function of the zenith angle θ holds at lunar distances, that the flaring of the magnetopause surface is influenced by the Interplanetary Magnetic Field (IMF) By component and that the IMF Bx component had…

2022 Journal of Geophysical Research (Space Physics)
Cluster DoubleStar 7
Extreme Energy Spectra of Relativistic Electron Flux in the Outer Radiation Belt
DOI: 10.1029/2022JA031038 Bibcode: 2022JGRA..12731038M

Artemyev, A. V.; Angelopoulos, V.; Mourenas, D. +1 more

Electron diffusion by whistler-mode chorus waves is one of the key processes controlling the dynamics of relativistic electron fluxes in the Earth's radiation belts. It is responsible for the acceleration of sub-relativistic electrons injected from the plasma sheet to relativistic energies as well as for their precipitation and loss into the atmos…

2022 Journal of Geophysical Research (Space Physics)
Cluster 7