A Preliminary Analysis Places a Portion of the Dust Grains Detected by PSP on Prograde, Low-eccentricity Orbits in the Ecliptic
Brent Fairley Page1, Stuart D Bale1, John W Bonnell1, Thierry Dudok de Wit2, Keith Goetz3, Peter Harvey1, Robert J MacDowall4, David Malaspina5, Petr Pokorny6, Marc Pulupa1 and Jamey R Szalay7, (1)University of California, Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, (2)LPC2E, CNRS and University of Orléans, Orléans, France, (3)University of Minnesota, Minneapolis, MN, United States, (4)NASA/Goddard Space Flight Center, Greenbelt, United States, (5)University of Colorado, Boulder, Laboratory for Atmospheric and Space Physics, Boulder, CO, United States, (6)Catholic University of America, Department of Physics and Astronomy, Washington, DC, United States, (7)Princeton University, Department of Astrophysical Sciences, Princeton, NJ, United States