Magnetospheric Science Objectives of the Juno Mission

F Bagenal, A Adriani, F Allegrini, SJ Bolton… - Space Science …, 2017 - Springer
Abstract In July 2016, NASA's Juno mission becomes the first spacecraft to enter polar orbit
of Jupiter and venture deep into unexplored polar territories of the magnetosphere. Focusing …

Report of the IAU working group on cartographic coordinates and rotational elements: 2009

BA Archinal, MF A'Hearn, E Bowell, A Conrad… - Celestial Mechanics and …, 2011 - Springer
Every three years the IAU Working Group on Cartographic Coordinates and Rotational
Elements revises tables giving the directions of the poles of rotation and the prime meridians …

[PDF][PDF] The configuration of Jupiter's magnetosphere

KK Khurana, MG Kivelson, VM Vasyliunas… - Jupiter. The planet …, 2004 - lasp.colorado.edu
A magnetosphere is a" sphere" of influence around a planet in which the forces associated
with the magnetic field of the planet prevail over all other forces. The magnetic field of the …

[PDF][PDF] Jupiter's aurora

JT Clarke, D Grodent, SWH Cowley… - Jupiter: The planet …, 2004 - lasp.colorado.edu
Auroral processes are exhibited by every planet and satellite with a collisionally thick
atmosphere and an internal magnetic field sufficiently strong to stand off the solar wind or …

A search for radio emission from extrasolar planets

TS Bastian, GA Dulk, Y Leblanc - The Astrophysical Journal, 2000 - iopscience.iop.org
All magnetized planets in the solar system emit intense cyclotron maser radiation. Like
Jupiter, extrasolar giant planets are probably magnetized. If, in addition, there is a source of …

Model of the Jovian magnetic field topology constrained by the Io auroral emissions

SLG Hess, B Bonfond, P Zarka… - Journal of Geophysical …, 2011 - Wiley Online Library
The determination of the internal magnetic field of Jupiter has been the object of many
studies and publications. These models have been computed from the Pioneer, Voyager …

Time variation of Jupiter's internal magnetic field consistent with zonal wind advection

KM Moore, H Cao, J Bloxham, DJ Stevenson… - Nature …, 2019 - nature.com
Determination of the time dependency (secular variation) of a planet's magnetic field
provides a window into understanding the dynamo responsible for generating its field …

[PDF][PDF] Plasma interaction of Io with its plasma torus

J Saur, FM Neubauer, JEP Connerney… - Jupiter: The planet …, 2004 - researchgate.net
Io's plasma interaction with its torus is an exceptionally interesting case of magnetospheric
plasma flowing past a body with a tenuous atmosphere. Major progress in our …

Statistical analysis of 26 yr of observations of decametric radio emissions from Jupiter

MS Marques, P Zarka, E Echer, VB Ryabov… - Astronomy & …, 2017 - aanda.org
Jupiter is a complex and at the same time very powerful radio source in the decameter
wavelength range. The emission is anisotropic, intrinsically variable at millisecond to hour …

Modeling the Jovian magnetic field and its secular variation using all available magnetic field observations

VA Ridley, R Holme - Journal of Geophysical Research …, 2016 - Wiley Online Library
We present new models of Jupiter's internal magnetic field and secular variation from all
available direct measurements from three decades of spacecraft observation. A regularized …