Effects of core mixing on solar oscillation frequencies (open access)

Effects of core mixing on solar oscillation frequencies

This paper discusses predicted p- and g-mode periods for two solar models provided by Schatzman and Maeder (1981). One model has no mixing while the other has turbulent diffusion mixing (allowed for by a Reynolds number of 100). The resulting g-mode period spacings allow a very close look at the central solar structure which, like the p-mode period splittings, indicate little or no mixing over the lifetime of the sun.
Date: July 27, 1984
Creator: Cox, A. N. & Kidman, R. B.
Object Type: Article
System: The UNT Digital Library
Texas Register, Volume 9, Number 56, Pages 4045-4100, July 27, 1984 (open access)

Texas Register, Volume 9, Number 56, Pages 4045-4100, July 27, 1984

A weekly publication, the Texas Register serves as the journal of state agency rulemaking for Texas. Information published in the Texas Register includes proposed, adopted, withdrawn and emergency rule actions, notices of state agency review of agency rules, governor's appointments, attorney general opinions, and miscellaneous documents such as requests for proposals. After adoption, these rulemaking actions are codified into the Texas Administrative Code.
Date: July 27, 1984
Creator: Texas. Secretary of State.
Object Type: Journal/Magazine/Newsletter
System: The Portal to Texas History