[HTML][HTML] Field-of-view guiding camera on the HISAKI (SPRINT-A) satellite
A Yamazaki, F Tsuchiya, T Sakanoi, K Uemizu… - Space Science …, 2014 - Springer
Abstract HISAKI (SPRINT-A) satellite is an earth-orbiting Extreme UltraViolet (EUV)
spectroscopic mission and launched on 14 Sep. 2013 by the launch vehicle Epsilon-1 …
spectroscopic mission and launched on 14 Sep. 2013 by the launch vehicle Epsilon-1 …
First detection of a diamagnetic cavity at comet 67P/Churyumov-Gerasimenko
C Goetz, C Koenders, I Richter, K Altwegg… - Astronomy & …, 2016 - aanda.org
Context. The Rosetta magnetometer RPC-MAG has been exploring the plasma environment
of comet 67P/Churyumov-Gerasimenko since August 2014. The first months were …
of comet 67P/Churyumov-Gerasimenko since August 2014. The first months were …
[HTML][HTML] Global upper-atmospheric heating on Jupiter by the polar aurorae
J O'Donoghue, L Moore, T Bhakyapaibul, H Melin… - Nature, 2021 - nature.com
Jupiter's upper atmosphere is considerably hotter than expected from the amount of sunlight
that it receives,–. Processes that couple the magnetosphere to the atmosphere give rise to …
that it receives,–. Processes that couple the magnetosphere to the atmosphere give rise to …
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 …
Structure and evolution of the diamagnetic cavity at comet 67P/Churyumov–Gerasimenko
C Goetz, C Koenders, KC Hansen… - Monthly Notices of …, 2016 - academic.oup.com
The long duration of the Rosetta mission allows us to study the evolution of the diamagnetic
cavity at comet 67P/Churyumov–Gerasimenko in detail. From 2015 April to 2016 February …
cavity at comet 67P/Churyumov–Gerasimenko in detail. From 2015 April to 2016 February …
Magnetic structure and propagation of two interacting CMEs from the Sun to Saturn
E Palmerio, T Nieves‐Chinchilla… - Journal of …, 2021 - Wiley Online Library
One of the grand challenges in heliophysics is the characterization of coronal mass ejection
(CME) magnetic structure and evolution from eruption at the Sun through heliospheric …
(CME) magnetic structure and evolution from eruption at the Sun through heliospheric …
[HTML][HTML] Automated Multi-Dataset Analysis (AMDA): An on-line database and analysis tool for heliospheric and planetary plasma data
V Génot, E Budnik, C Jacquey, M Bouchemit… - Planetary and Space …, 2021 - Elsevier
Accessing, visualizing and analyzing heterogeneous plasma datasets has always been a
tedious task that hindered students and senior researchers as well. Offering user friendly …
tedious task that hindered students and senior researchers as well. Offering user friendly …
[HTML][HTML] The plasma environment of comet 67P/Churyumov-Gerasimenko
The environment of a comet is a fascinating and unique laboratory to study plasma
processes and the formation of structures such as shocks and discontinuities from electron …
processes and the formation of structures such as shocks and discontinuities from electron …
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 …
Statistical validation of a solar wind propagation model from 1 to 10 AU
B Zieger, KC Hansen - Journal of Geophysical Research …, 2008 - Wiley Online Library
A one‐dimensional (1‐D) numerical magnetohydrodynamic (MHD) code is applied to
propagate the solar wind from 1 AU through 10 AU, ie, beyond the heliocentric distance of …
propagate the solar wind from 1 AU through 10 AU, ie, beyond the heliocentric distance of …