Solar wind interaction with small bodies. 1: Whistler wing signatures near to Gaspra and Ida

Details Solar wind interaction with small bodies. 1: Whistler wing signatures near to Gaspra and Ida Solar wind interaction with small bodies. 1: Whistler wing signatures near to Gaspra and Ida

Aug 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995adspr..16...47w&link_type=abstract

Advances in Space Research (ISSN 0273-1177), vol. 16, no. 4, p. (4)47-(4)57

Computer Science

9

Asteroids, Flyby Missions, Interactions, Interplanetary Magnetic Fields, Magnetic Field Configurations, Magnetohydrodynamics, Solar Wind, Whistlers, Computerized Simulation, Data Reduction, Galileo Spacecraft, Magnetic Signatures, Phase Velocity, Solar Wind Velocity

Scientific paper

Data from Galileo's two asteroid flybys reveal magnetic fluctuations that we interpret as perturbations of the solar wind magnetic field caused by an interaction with the nearby asteroid. The scale sizes of the bodies (approximately 14 km for Gaspra and approximately 30 km for Ida) are intermediate between the ion and electron gyroradii, which implies that the asteroid-imposed perturbations propagate in the whistler mode. Special properties of the whistler mode include phase phase velocities that can exceed the solar wind speed and confinement of the disturbance to directions nearly aligned with the magnetic field. These features of the interaction impose a structure on the solar wind disturbance that differs greatly from the forms familiar for either magnetized or unmagnetized bodies of magnetohydrodynamic spatial scales. We examine both data and computer simulations of the interaction with special attention to what can be inferred about the interaction itself from analysis of the data.

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