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Abstract: Latitudinal structure of the heliospheric magnetic field and solar wind in the inner heliosphere: results of the first Solar Orbiter out of ecliptic orbit (AGU25)

Latitudinal structure of the heliospheric magnetic field and solar wind in the inner heliosphere: results of the first Solar Orbiter out of ecliptic orbit

Timothy Simon Horbury1, Stuart D Bale2, Andrei Fedorov3, Lorenzo Matteini4, Mathew James Owens5, Dr. Erika Palmerio6, Tamar Ervin7, Adam Finley8, Samuel Badman9, Yeimy Rivera10, Joseph Wang11, Philippe Louarn3, Christopher John Owen12, Michael Louis Stevens13, Roberto Livi14, Davin Larson9 and Phyllis Whittlesey14, (1)Imperial College London, Department of Physics, London, SW7, United Kingdom, (2)University of California Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, (3)CNRS - Institut de Recherche en Astrophysique et Planétologie, Toulouse, France, (4)Imperial College London, Department of Physics, London, United Kingdom, (5)University of Reading, Reading, United Kingdom, (6)Predictive Science Inc., San Diego, CA, United States, (7)Predictive Science Inc., San Diego, United States, (8)CEA Saclay DSM / LSCE, Gif sur Yvette, France, (9)University of California Berkeley, Berkeley, United States, (10)Harvard-Smithsonian Center for Astrophysics, Cambridge, United States, (11)Imperial College London, London, SW7, United Kingdom, (12)UCL, Mullard Space Science Laboratory, Dorking, United Kingdom, (13)Smithsonian Astrophysical Observatory, Cambridge, MA, United States, (14)University of California Berkeley, Space Sciences Laboratory, Berkeley, United States
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