Atmospheric escape processes and planetary atmospheric evolution

G Gronoff, P Arras, S Baraka, JM Bell… - Journal of …, 2020 - Wiley Online Library
The habitability of the surface of any planet is determined by a complex evolution of its
interior, surface, and atmosphere. The electromagnetic and particle radiation of stars drive …

[HTML][HTML] Discrete and broadband electron acceleration in Jupiter's powerful aurora

BH Mauk, DK Haggerty, C Paranicas, G Clark… - Nature, 2017 - nature.com
The most intense auroral emissions from Earth's polar regions, called discrete for their
sharply defined spatial configurations, are generated by a process involving coherent …

Juno observations of energetic charged particles over Jupiter's polar regions: Analysis of monodirectional and bidirectional electron beams

BH Mauk, DK Haggerty, C Paranicas… - Geophysical …, 2017 - Wiley Online Library
Juno obtained unique low‐altitude space environment measurements over Jupiter's poles
on 27 August 2016. Here Jupiter Energetic‐particle Detector Instrument observations are …

Jovian auroral electron precipitation budget—A statistical analysis of diffuse, mono‐energetic, and broadband auroral electron distributions

A Salveter, J Saur, G Clark… - Journal of Geophysical …, 2022 - Wiley Online Library
Recent observations by the Juno spacecraft have shown that electrons contributing to
Jupiter's main auroral emission appear to be frequently characterized by broadband …

In situ observations connected to the Io footprint tail aurora

JR Szalay, B Bonfond, F Allegrini… - Journal of …, 2018 - Wiley Online Library
The Juno spacecraft crossed flux tubes connected to the Io footprint tail at low Jovian
altitudes on multiple occasions. The transits covered longitudinal separations of …

Jupiter's aurora observed with HST during Juno orbits 3 to 7

D Grodent, B Bonfond, Z Yao, JC Gérard… - Journal of …, 2018 - Wiley Online Library
A large set of observations of Jupiter's ultraviolet aurora was collected with the Hubble
Space Telescope concurrently with the NASA‐Juno mission, during an eight‐month period …

[HTML][HTML] Scientific problems addressed by the Spektr-UV space project (world space Observatory—Ultraviolet)

AA Boyarchuk, BM Shustov, IS Savanov, ME Sachkov… - Astronomy Reports, 2016 - Springer
The article presents a review of scientific problems and methods of ultraviolet astronomy,
focusing on perspective scientific problems (directions) whose solution requires UV space …

Diverse electron and ion acceleration characteristics observed over Jupiter's main aurora

BH Mauk, DK Haggerty, C Paranicas… - Geophysical …, 2018 - Wiley Online Library
Two new Juno‐observed particle features of Jupiter's main aurora demonstrate substantial
diversity of processes generating Jupiter's mysterious auroral emissions. It was previously …

Energy flux and characteristic energy of electrons over Jupiter's main auroral emission

F Allegrini, B Mauk, G Clark… - Journal of …, 2020 - Wiley Online Library
Jupiter's ultraviolet (UV) aurorae, the most powerful and intense in the solar system, are
caused by energetic electrons precipitating from the magnetosphere into the atmosphere …

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 …