On the relation between auroral morphologies and compression conditions of Jupiter's magnetopause: Observations from Juno and the Hubble Space Telescope
Jupiter displays the most powerful auroral emissions in our solar system, which result from
strong energy dissipation in Jupiter's surrounding space environment. Although mass and …
strong energy dissipation in Jupiter's surrounding space environment. Although mass and …
On the relation between Jupiter's aurora and the dawnside current sheet
Jupiter's auroral emission is a spectacular phenomenon that provides insight into energy
release processes related to the coupling of its magnetosphere and ionosphere. This energy …
release processes related to the coupling of its magnetosphere and ionosphere. This energy …
Energy flux and characteristic energy of electrons over Jupiter's main auroral emission
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 …
A high spatial and spectral resolution study of Jupiter's mid-infrared auroral emissions and their response to a solar wind compression
We present mid-infrared spectroscopy of Jupiter's mid-to-high latitudes using the Gemini-
North/Texas Echelon Cross Echelle Spectrograph on 2017 March 17–19. These …
North/Texas Echelon Cross Echelle Spectrograph on 2017 March 17–19. These …
Reconnection‐and dipolarization‐driven auroral dawn storms and injections
Jupiter displays many distinct auroral structures, among which auroral dawn storms and
auroral injections are often observed contemporaneously. However, it is unclear if the …
auroral injections are often observed contemporaneously. However, it is unclear if the …
Planetary Exploration Horizon 2061 Report, Chapter 4: From planetary exploration goals to technology requirements
This chapter reviews for each province and destination of the Solar System the
representative space missions that will have to be designed and implemented by 2061 to …
representative space missions that will have to be designed and implemented by 2061 to …
Periodicities and plasma density structure of Jupiter's dawnside magnetosphere
Ability to quantify variations in magnetic field topology and density within Jupiter's
magnetosphere is an important step in understanding the overall structure and dynamics …
magnetosphere is an important step in understanding the overall structure and dynamics …
Magnetotail reconnection at Jupiter: A survey of Juno magnetic field observations
At Jupiter, tail reconnection is thought to be driven by an internal mass loading and release
process called the Vasyliunas cycle. Galileo data have shown hundreds of reconnection …
process called the Vasyliunas cycle. Galileo data have shown hundreds of reconnection …
Six pieces of evidence against the corotation enforcement theory to explain the main aurora at Jupiter
The most remarkable feature of the ultraviolet auroras at Jupiter is the ever‐present and
almost continuous curtain of bright emissions centered on each magnetic pole and called …
almost continuous curtain of bright emissions centered on each magnetic pole and called …
Relation of Jupiter's dawnside main emission intensity to magnetospheric currents during the Juno mission
JD Nichols, SWH Cowley - Journal of Geophysical Research …, 2022 - Wiley Online Library
We compare Jupiter's dawn‐side main auroral emission intensity observed by the Hubble
Space Telescope with the simultaneous magnitude of the dawn‐side magnetospheric …
Space Telescope with the simultaneous magnitude of the dawn‐side magnetospheric …