3/2/2024 0 Comments Jim raines his solar orbiterJournal of Geophysical Research: Space Physics 127 (12) (2022) Ganymede's Auroral Footprint Latitude: Comparison With Magnetodisc Model Reconstruction of the magnetic connection from Mercury to the solar corona during enhancements in the solar proton fluxes at MercuryĪ. Journal of Space Weather and Space Climate 12 3 (2022) The Great Aurora of 4 February 1872 observed by Angelo Secchi in Rome The Jovian Energetic Ion Environment of Ganymede: Planetary Space Weather Considerations in View of the JUICE MissionĬhristina Plainaki, Stefano Massetti, Xianzhe Jia, et al. IOP Conference Series: Earth and Environmental Science 988 (2) 022017 (2022) Jack Diab, Mohit Melwani Daswani and Julie Castillo-RogezĮ N Prokofeva, A V Vostrikov, H A Nekrasov, N E Bragin and M O Malcev Alberti, et al.īulk composition and thermal evolution constrain the formation of organics in Ceres' subsurface ocean via geochemical modeling The CAESAR Project for the ASI Space Weather Infrastructure Corso, Denis Garoli, Giuseppe Emanuele Lio, Marco Manente, Giulio Favaro, Marco Bazzan, Giampaolo Piotto, Nicola Andriolli, Lucanos Strambini, Daniele Pavarin, Leonardo Badia, Remo Proietti Zaccaria, Philip Lubin, Roberto Ragazzoni and Maria G. Swarm of lightsail nanosatellites for Solar System exploration Wimmer‐Schweingruber, Marco Pinto, Richard Moissl, Johannes Benkhoff, Hermann Opgenoorth, Uli Auster, Jos de Brujine, Peter Collins, Guido De Marchi, David Fischer, Yoshifumi Futaana, James Godfrey, Daniel Heyner, Mats Holmstrom, Andrew Johnstone, Simon Joyce, Daniel Lakey, Santa Martinez, David Milligan, et al. Knutsen, Dikshita Meggi, Shayla Viet, Mark Lester, Robert F. Solar Energetic Particle Events Detected in the Housekeeping Data of the European Space Agency's Spacecraft Flotilla in the Solar Systemīeatriz Sánchez‐Cano, Olivier Witasse, Elise W. Planetary Exploration Horizon 2061 331 (2023) Taylor, Johan De Keyser, et al.įrontiers in Astronomy and Space Sciences 10 (2023)īernard Foing, Jonathan Lewis, Aurore Hutzler, et al. We will also provide an overview of the available data and accessibility of the public datasets.This article has been cited by the following article(s): 36 articles Space plasma physics science opportunities for the lunar orbital platform - Gateway We discuss how SWA-HIS will enable linkages between the Sun and the solar wind to reveal the nature of the acceleration and release of the solar wind and the sources and structure of the solar wind. We present measurements of heavy ion composition from SWA-HIS taken during the cruise phase of the mission to highlight the capabilities of the instrument and the observations we expect to collect over the next 10 years. The SWA-Heavy Ion Sensor (HIS) is optimized to measure heavy ions in the solar wind, pickup ions, and suprathermal ions in an energy range spanning from 0.5- 75keV/e. The Solar Wind Analyser (SWA) is a suite of instruments that provide in-situ measurements of solar wind electrons, protons, alpha particles, and heavy ions. During its orbit, periods of quasi-corotation with the Sun will enable determination of the source regions on the Sun for solar wind structures. The Solar Orbiter mission was launched in 2020 into an orbit that will explore the inner heliosphere.
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