Magnetic connectivity of the ecliptic plane within 0.5 AU : PFSS modelling of the early PSP encounters
Magnetic connectivity of the ecliptic plane within 0.5 AU : PFSS modelling of the early PSP encounters
Samuel Timothy Badman1, Stuart D Bale2, Juan Carlos Martinez Oliveros3, Olga Panasenco4, Marco Velli5, David Stansby6, Juan Camilo Buitrago-Casas3, Victor Réville7,8, Marc Pulupa2, David Malaspina9, John W Bonnell2, Peter Harvey2, Keith Goetz10, Thierry Dudok de Wit11, Robert J MacDowall12, Justin Christophe Kasper13, Anthony W Case14, Kelly E Korreck15, Davin E Larson3, Roberto Livi1, Michael Louis Stevens16 and Phyllis L Whittlesey1, (1)University of California Berkeley, Berkeley, CA, United States, (2)University of California, Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, (3)Space Sciences Laboratory, Berkeley, CA, United States, (4)Advanced Heliophysics, Pasadena, CA, United States, (5)University of California Los Angeles, Los Angeles, CA, United States, (6)Imperial College London, London, SW7, United Kingdom, (7)IRAP, Toulouse, France, (8)University of California Los Angeles, Los Angeles, United States, (9)University of Colorado, Boulder, Laboratory for Atmospheric and Space Physics, Boulder, CO, United States, (10)University of Minnesota, Minneapolis, MN, United States, (11)LPC2E, CNRS and University of Orléans, Orléans, France, (12)NASA/Goddard Space Flight Center, Greenbelt, United States, (13)University of Michigan, Ann Arbor, MI, United States, (14)Smithsonian Astrophysical Observatory, Cambridge, MA, United States, (15)Smithsonian Observatory, Cambridge, MA, United States, (16)Smithsonian Astrophysics Observatory, Cambridge, MA, United States
