Modeling the Corona-Heliosphere Interface in Anticipation of the Murchison Wide-field Array

Computer Science – Performance

Scientific paper

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2101 Coronal Mass Ejections (7513), 7509 Corona, 7524 Magnetic Fields, 7534 Radio Emissions, 7827 Kinetic And Mhd Theory

Scientific paper

The Murchison Widefield Array (MWA) is an 8,000-antenna, 80-300 MHz, imaging radio array under construction in Western Australia that features a large field of view, high sensitivity, and accurate polarization and intensity calibration. An MWA prototype has been deployed in the field and construction of the full array will begin in mid-2009 after the performance of the prototype is evaluated. Understanding the connection between the upper corona and the inner heliosphere with novel low-frequency radio observations is a primary objective of the MWA Solar, Heliospheric, and Ionospheric (SHI) science consortium. This presentation covers progress by the SHI consortium's theory and modeling effort. We show simulations of how Faraday rotation, interplanetary scintillation, and radio burst measurements can track and constrain the transport of magnetic fields, density, and energetic electrons into the heliosphere.

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