Atmospheric escape processes and planetary atmospheric evolution
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 …
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 …
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 …
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
Recent observations by the Juno spacecraft have shown that electrons contributing to
Jupiter's main auroral emission appear to be frequently characterized by broadband …
Jupiter's main auroral emission appear to be frequently characterized by broadband …
In situ observations connected to the Io footprint tail aurora
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 …
altitudes on multiple occasions. The transits covered longitudinal separations of …
Jupiter's aurora observed with HST during Juno orbits 3 to 7
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 …
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 …
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 …
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 …
caused by energetic electrons precipitating from the magnetosphere into the atmosphere …
Statistical analysis of 26 yr of observations of decametric radio emissions from Jupiter
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 …
wavelength range. The emission is anisotropic, intrinsically variable at millisecond to hour …