Helioseismology
- 1 October 1995
- journal article
- Published by AIP Publishing in Physics Today
- Vol. 48 (10) , 32-38
- https://doi.org/10.1063/1.881453
Abstract
What powers the Sun? Why does it have spots? How long will it sustain life on Earth? Efforts to answer these questions about the astrophysical object that is of greatest importance to humanity have produced many advances in physics and helped lay the main foundations of astrophysics. The three questions, however, remain to be answered. For example, the best models of the Sun's nuclear power predict a significantly higher neutrino flux than is observed. (See PHYSICS TODAY April, page 19.) We do not know what causes sunspots and other solar activity or even why the Sun emits x rays. Modeling how stars evolve leads to age estimates for some stars that are greater than recent estimates of the age of the universe.Keywords
This publication has 13 references indexed in Scilit:
- Slow rotation of the Sun's interiorNature, 1995
- An instrument to observe low-degree solar oscillationsSolar Physics, 1995
- Progress and prospects in neutrino astrophysicsNature, 1995
- Properties of acoustic sources in the SunThe Astrophysical Journal, 1994
- Using solar p-modes to determine the convection zone depth and constrain diffusion-produced composition gradientsThe Astrophysical Journal, 1993
- The depth of the solar convection zoneThe Astrophysical Journal, 1991
- Inferring the sun's internal angular velocity from observed p-mode frequency splittingsThe Astrophysical Journal, 1989
- Speed of sound in the solar interiorNature, 1985
- Improvements in birefringent filters 6: Analog birefringent elementsApplied Optics, 1980
- The magneto-optical filterSolar Physics, 1978