Beatriz Sánchez-Cano, Lina Z Hadid, Sae Aizawa, Go Murakami, Yumi Bamba, Shota Chiba, Takuya Hara, Daniel Heyner, George Ho, Kazumasa Iwai, Emilia Kilpua, Gaku Kinoshita, Benoit Lavraud, Yoshizumi Miyoshi, Marco Pinto, Daniel Schmid, Daikou Shiota, Rami Vainio, Nicolas Andre, Alessandro Aronica, Sami Asmar, Hans-Ulrich Auster, Stas Barabash, Alain Barthe, Wolfgang Baumjohann, Johannes Benkhoff, Mark Bentley, Emma Bunce, Paolo Cappuccio, Dominique Delcourt, Ivan di Stefano, Irene Doria, Nina Dresing, Andrei Fedorov, David Fischer, Bjorn Fiethe, Markus Fränz, Jan Gieseler, Franz Giner, Gabriel Giono, Yuki Harada, Hauke Hussmann, Luciano Iess, Takeshi Imamura, Harald Jeszenszky, Geraint Jones, Bruno Katra, Adrian Kazakov, Alexander Kozyrev, Gunter Laky, Carlo Lefevre, Herbert Lichtenegger, Simon Lindsay, Marco Lucente, Carmelo Magnafico, Werner Magnes, Adrian Martindale, Ayako Matsuoka, Anna Milillo, Igor Mitrofanov, Gaku Nishiyama, Philipp Oleynik, Stefano Orsini, Meegyeong Paik, Christian Palmroos, Christina Plainaki, Emanuel Penou, Moa Persson, Francesco Quarati, Eric Quémerais, Ingo Richter, Rozenn Robidel, Mathias Rojo, Yoshifumi Saito, Francesco Santoli, Alexander Stark, Mirko Stumpo, Rong Tian, Ali Varsani, Christopher Verdeil, Hayley Williamson, Olivier Witasse, Shoichiro Yokota
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BepiColombo cruise science: overview of the mission contribution to heliophysics.
BepiColombo, the joint ESA/JAXA mission to Mercury, was launched in October 2018 and is scheduled to arrive at Mercury in November 2026 after an 8-year cruise. Like other planetary missions, its scientific objectives focus mostly on the nominal, orbiting phase of the mission. However, due to the long duration of the cruise phase covering distances between 1.2 and 0.3 AU, the BepiColombo mission has been able to outstandingly contribute to characterise the solar wind and transient events encountered by the spacecraft, as well as planetary environments during the flybys of Earth, Venus, and Mercury, and contribute to the characterisation of the space radiation environment in the inner Solar System and its evolution with solar activity. In this paper, we provide an overview of the cruise observations of BepiColombo, highlighting the most relevant science cases, with the aim of demonstrating the importance of planetary missions to perform cruise observations, to contribute to a broader understanding of Space Weather in the Solar System, and in turn, increase the scientific return of the mission.
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Earth, Planets and Space (EPS) covers scientific articles in Earth and Planetary Sciences, particularly geomagnetism, aeronomy, space science, seismology, volcanology, geodesy, and planetary science. EPS also welcomes articles in new and interdisciplinary subjects, including instrumentations. Only new and original contents will be accepted for publication.
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