The Juno waves investigation
Jupiter is the source of the strongest planetary radio emissions in the solar system.
Variations in these emissions are symptomatic of the dynamics of Jupiter's magnetosphere …
Variations in these emissions are symptomatic of the dynamics of Jupiter's magnetosphere …
The Radio & Plasma Wave Investigation (RPWI) for the JUpiter ICy moons Explorer (JUICE)
JE Wahlund, JES Bergman, L Åhlén, W Puccio… - Space Science …, 2025 - Springer
Abstract The Radio & Plasma Wave Investigation (RPWI) onboard the ESA JUpiter ICy
moons Explorer (JUICE) is described in detail. The RPWI provides an elaborate set of state …
moons Explorer (JUICE) is described in detail. The RPWI provides an elaborate set of state …
Mapper of the IGM spin temperature: instrument overview
RA Monsalve, C Altamirano, V Bidula… - Monthly Notices of …, 2024 - academic.oup.com
The observation of the global 21 cm signal produced by neutral hydrogen gas in the
intergalactic medium (IGM) during the Dark Ages, Cosmic Dawn, and Epoch of Reionization …
intergalactic medium (IGM) during the Dark Ages, Cosmic Dawn, and Epoch of Reionization …
Beam current oscillations driven by cyclotron instabilities in a minimum-B electron cyclotron resonance ion source plasma
Experimental observation of cyclotron instabilities in a minimum-B confined electron
cyclotron resonance ion source plasma is reported. The instabilities are associated with …
cyclotron resonance ion source plasma is reported. The instabilities are associated with …
Auroral processes at the giant planets: Energy deposition, emission mechanisms, morphology and spectra
SV Badman, G Branduardi-Raymont, M Galand… - Space Science …, 2015 - Springer
The ionospheric response to auroral precipitation at the giant planets is reviewed, using
models and observations. The emission processes for aurorae at radio, infrared, visible …
models and observations. The emission processes for aurorae at radio, infrared, visible …
A space-based observational strategy for characterizing the first stars and galaxies using the redshifted 21 cm global spectrum
JO Burns, R Bradley, K Tauscher… - The Astrophysical …, 2017 - iopscience.iop.org
A Space-based Observational Strategy for Characterizing the First Stars and Galaxies Using
the Redshifted 21 cm Global Spectrum - IOPscience This site uses cookies. By continuing to …
the Redshifted 21 cm Global Spectrum - IOPscience This site uses cookies. By continuing to …
How is the Jovian main auroral emission affected by the solar wind?
The influence of the solar wind on Jupiter's magnetosphere is studied via three‐dimensional
global MHD simulations. We especially examine how solar wind density variations affect the …
global MHD simulations. We especially examine how solar wind density variations affect the …
LuSEE'Night': The Lunar Surface Electromagnetics Experiment
The Lunar Surface Electromagnetics Explorer'LuSEE Night'is a low frequency radio
astronomy experiment that will be delivered to the farside of the Moon by the NASA …
astronomy experiment that will be delivered to the farside of the Moon by the NASA …
Influence of axial mirror ratios on the kinetic instability threshold in electron cyclotron resonance ion source plasma
V Toivanen, BS Bhaskar, H Koivisto, L Maunoury… - Physics of …, 2022 - pubs.aip.org
Electron Cyclotron Resonance (ECR) ion source plasmas are prone to kinetic instabilities.
The onset of the instabilities manifests as emission of microwaves, bursts of electrons …
The onset of the instabilities manifests as emission of microwaves, bursts of electrons …
Dynamic regimes of cyclotron instability in the afterglow mode of minimum-B electron cyclotron resonance ion source plasma
The paper is concerned with the dynamic regimes of cyclotron instabilities in non-
equilibrium plasma of a minimum-B electron cyclotron resonance ion source operated in …
equilibrium plasma of a minimum-B electron cyclotron resonance ion source operated in …