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Research needed to improve solar flare and particle forecasting
1Department of Physics, The University of Alabama in Huntsville 35899, USA.
Advances in Space Research : the Official Journal of the Committee on Space Research (COSPAR)
|October 1, 1994
Summary
Understanding solar transient active phenomena is key to predicting space weather. Further research is needed to improve our physical models for energy buildup and release, enhancing prediction capabilities for near-Earth space.
Area of Science:
- Solar physics
- Space weather
- Plasma physics
Background:
- Transient active phenomena on the Sun, such as solar flares and coronal mass ejections, are driven by the buildup and release of magnetic energy.
- Accurate prediction of these events is crucial for mitigating their impact on technological systems and astronauts in the near-Earth environment.
Purpose of the Study:
- To review the current physical understanding of energy processes in solar transient active phenomena.
- To identify critical research areas needed to improve predictive capabilities for these events and their space weather effects.
Main Methods:
- Review of existing literature and theoretical models concerning solar energy buildup and release mechanisms.
- Analysis of the requirements for enhanced predictive models of solar transient events.
Main Results:
- The current physical understanding of energy buildup and release in solar transient active phenomena is summarized.
- Key gaps in knowledge and areas requiring further investigation are identified.
Conclusions:
- Improved physical understanding of solar energy dynamics is essential for advancing space weather prediction.
- Targeted research efforts are necessary to enhance our ability to forecast solar transient events and their interplanetary consequences.