Research
Focus
Target
Description: This task challenges proposers to characterize the
properties of the solar dynamo that determine the strength of the solar
activity cycle and its terrestrial consequences (e.g,. through
irradiance changes and geomagnetic effects). Recent advances in
modeling promise to provide accurate forecasts of the strength and
timing of solar cycles. Now Cycle 23, a longer than average and
somewhat peculiar cycle, is ending, and the new Cycle 24, which has
widely different predictions for its maximum activity level from
different models, is beginning. In order to be useful for future cycle
forecasting, models need to be constrained and related more closely to
LWS impacts. Interpretation of available data from the SOlar and
Heliospheric Observatory (SOHO), Global Oscillation Network Group
(GONG), Synoptic Optical Long-term Investigations of the Sun (SOLIS),
other space- and ground-based sources, and the upcoming Solar Dynamics
Observatory (SDO) mission toward this resolution is timely and may lead
to new observational strategies as the solar activity level increases.
Goals and Measures of
Success: Successful investigations should help us to
discriminate between and improve dynamo models. This requires improved
measurements of critical subsurface flows, including the expected deep
meridional flow, detection of the subsurface magnetic fields, and a
determination of the influences of the solar polar properties on the
dynamo. The connections between dynamo operation and the properties of
the active regions that give rise to terrestrial effects also require
clarification. Solar irradiance variations are determined by both
sunspot and plage areas. What in the dynamo action determines this
combination? Similarly, significant eruptive events can occur during
both large and small activity cycles. An understanding of what aspect
of dynamo action gives rise to eruptive regions is needed.
Types of investigations:
• Development of methods to discriminate between subsurface magnetic
fields and thermal structures;
• Determination of the properties of the deep meridional return flow;
• Analyses revealing how the magnetic and dynamic characteristics of
the solar poles affect the dynamo and the solar activity cycle; and
• Use of observations to discriminate between models that forecast the
properties of Cycle 24.