Environments, needs and opportunities for future space photovoltaic power generation: A review
A Bermudez-Garcia, P Voarino, O Raccurt - Applied Energy, 2021 - Elsevier
This paper aims to assess the potential and requirements of photovoltaic arrays to provide
energy for more than 30 mission types to explore 14 celestial bodies in our solar system …
energy for more than 30 mission types to explore 14 celestial bodies in our solar system …
Jupiter science enabled by ESA's Jupiter icy moons explorer
Abstract ESA's Jupiter Icy Moons Explorer (JUICE) will provide a detailed investigation of the
Jovian system in the 2030s, combining a suite of state-of-the-art instruments with an orbital …
Jovian system in the 2030s, combining a suite of state-of-the-art instruments with an orbital …
Revealing the source of Jupiter's x-ray auroral flares
Jupiter's rapidly rotating, strong magnetic field provides a natural laboratory that is key to
understanding the dynamics of high-energy plasmas. Spectacular auroral x-ray flares are …
understanding the dynamics of high-energy plasmas. Spectacular auroral x-ray flares are …
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 …
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 …
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 …
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 …
A study of Jupiter's UV Great Dark Spot and tropopause to stratosphere winds in the high northern latitudes as seen by Cassini imaging
Images of Jupiter taken during the year 2000 Cassini flyby revealed the early stages and
evolution of a high northern-latitude UV Great Dark Spot over a three-month period. They …
evolution of a high northern-latitude UV Great Dark Spot over a three-month period. They …
Long-term variability of Jupiter's northern auroral 8-μm CH4 emissions
We present a study of the long term variability of Jupiter's mid-infrared CH 4 auroral
emissions. 7.7–7.9 μ m images of Jupiter recorded by NASA's Infrared Telescope Facility …
emissions. 7.7–7.9 μ m images of Jupiter recorded by NASA's Infrared Telescope Facility …
Comparisons between Jupiter's X‐ray, UV and radio emissions and in‐situ solar wind measurements during 2007
We compare Chandra and XMM‐Newton X‐ray observations of Jupiter during 2007 with a
rich multi‐instrument data set including upstream in situ solar wind measurements from the …
rich multi‐instrument data set including upstream in situ solar wind measurements from the …