Abstract
The physical processes in the heliospace are a direct consequence of the Sun’s mass and electromagnetic emissions. There has been enormous progress in studying these processes since the dawn of the space age half a century ago. The heliospace serves as a great laboratory to study numerous physical processes, using the vast array of ground and space-based measurements of various physical quantities. The observational capabilities collectively form the Great Observatory to make scientific investigations not envisioned by individual instrument teams. The International Heliophysical Year (IHY) program has been promoting scientific investigations on the universality of physical processes such as shocks, particle acceleration, dynamo, magnetic reconnection, magnetic flux ropes, plasma-neutral matter interactions, turbulence, and several other topics. This chapter highlights scientific deliberations on these and related topics that took place during the IAGA session on “Universal Heliophysical Processes” in Sopron, Hungary. The session featured several invited and contributed papers that focused on observations, theory and modeling of the universal heliophysical processes.
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Acknowledgements
The author thanks Drs. K. Kecskeméety, B. Vršnak and B. J. Thompson for their help in convening the IAGA session. He also thanks Dr. P. Mäkelä for proof reading the manuscript.
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Gopalswamy, N. (2011). Universal Heliophysical Processes. In: Miralles, M., Sánchez Almeida, J. (eds) The Sun, the Solar Wind, and the Heliosphere. IAGA Special Sopron Book Series, vol 4. Springer, Dordrecht. https://doi.org/10.1007/978-90-481-9787-3_2
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