Authors: Lidiya Ahmed; Michael Stevens; Samuel Badman; Aileen Niesta Most solar-wind prediction methods rely on boundary conditions specified at a fixed inner radius, typically derivedView More
Authors: Lidiya Y. Ahmed1,2 , Michael L. Stevens1, Sam Badman1, Yeimy Rivera1, Kristoff Paulson1, Srijan Das1. 1 Smithsonian Astrophysical Observatory 2 Harvard University Parker SolarView More
Authors: Lidiya Y. Ahmed (Smithsonian Astrophysical Observatory, Harvard University), Michael L. Stevens (Smithsonian Astrophysical Observatory), Kristoff Paulson (Smithsonian Astrophysical Observatory), Sam Badman (Smithsonian Astrophysical Observatory),View More
Authors: Lidiya Y. Ahmed1,2 , Michael L. Stevens1, Kristoff Paulson1, Anthony Case1 1 Smithsonian Astrophysical Observatory 2 Harvard University Solar wind parameters such as density,View More