A Cool Solar Core?

Date: 24 Apr 1998
Satellite: SOHO
Depicts: Solar Interior
Copyright: See below

From long-lasting observations by these instruments, scientists deduce information about the Sun's interior precise enough to put the theories of how the Sun works to a severe test.

In red coloured layers, sound travels faster than predicted by the theories, implying that the temperature is higher then expected. The conspicuous red layer, about a third of the way down from the surface to the Sun's centre, shows unexpectedly high temperatures at the transition zone between the turbulent outer region (convection zone) and the more stable region inside it (radiative zone).

Here MDI/SOI has measured a rapid change in the speed of rotation about the Sun's axis, between the faster-turning outer region and the slower interior. This shear layer may generate the magnetism that battles with the gas in the outer layer and causes frenzied activity at the visible surface, where MDI/SOI also charts sunspots (left). Resulting storms in the solar atmosphere can affect the Earth.

In blue coloured layers the sound speed is lower than expected, and temperatures are lower too. Most notable in this respect is the very core of the Sun, where the temperature may be 0.1 per cent cooler than the expected 15 million degrees C. Although the discrepancy seems small, it implies that the thermonuclear reactions in the core that power the Sun could be underperforming at present. If confirmed by prolonged observations by SOHO, the cool core may leave theorists wondering if the Sun varies its power-generation over long periods.

Built in Europe for the European Space Agency, SOHO carries twelve sets of instruments provided by European and American investigators and it was despatched into space on 2 December 1995 by a NASA launcher. SOHO is a project of international cooperation between ESA and NASA.

Credit: SOHO (ESA & NASA), MDI/SOI and VIRGO data imaged by A. Kosovichev, Stanford University