Can we detect convection in the Sun? Journal Article

Overview

abstract

• AbstractWe investigate the possibility of detecting deep convection in the Sun by computing travel-time shifts induced by convective flows interacting with propagating waves. The convection zone is modeled using a velocity profile taken from an Anelastic convection simulation. We present results obtained from a ray calculation of travel-time shifts. We compare these results with a full 3D calculation of the wave-flow interaction.

CU Boulder Authors

• Miesch, Mark Steven

publication date

• August 1, 2006

has restriction

• bronze

Date in CU Experts

• June 3, 2024 11:56 AM

Full Author List

• Hanasoge SM; Duvall TL; Derosa ML; Miesch MS

author count

• 4

published in

• Proceedings of the International Astronomical Union  Journal

Other Profiles

International Standard Serial Number (ISSN)

• 1743-9213

Electronic International Standard Serial Number (EISSN)

• 1743-9221

Digital Object Identifier (DOI)

• https://doi.org/10.1017/s1743921307000737

Additional Document Info

start page

• 364

end page

• 369

volume

• 2

issue

• S239