Modeling Heliospheric Phenomena with an Adaptive, MHD-Boltzmann Code
Principal Investigator: Nikolai Pogorelov
Affiliation: University of California–Riverside
Machine: Cray XT4
Allocation: 850,000 processor hours
Research Summary: The solar system, tucked inside a bubble created by the continuous stream of charged particles being emitted by the sun, is drifting through a thin cloud of gas that permeates our neighborhood of the galaxy. This project uses a carefully crafted combination of computational techniques to examine the bubble (known as the heliosphere) as it interacts with the cloud (known as the Local Interstellar Medium), focusing on changes in the relationship throughout the sun’s 11-year activity cycle.