Abstract
Magnetic reconnection at Earth’s dayside magnetopause plays a crucial role in space weather-related phenomena. The response of the magnetosphere to input from interplanetary space differs greatly depending on where reconnection happens and how efficiently it reconnects magnetic flux from interplanetary space. This chapter is a pedagogical treatment of dayside reconnection. Introductory topics include a guide to the magnetosphere for the uninitiated and a brief history of the field. Technical topics include qualitative properties of dayside reconnection, such as where reconnection occurs and what it looks like, and how reconnection quantitatively depends on ambient conditions, including the effect of asymmetries, the diamagnetic drift, and flow shear. Both observational and theoretical aspects are discussed. The chapter is closed with a discussion of open questions and the outlook for the future of dayside reconnection research.
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Acknowledgements
The authors dedicate this chapter to Gene Parker, whose insight into the field of reconnection cannot be overestimated. Special thanks go out to Walter Gonzalez, who organized the Parker Reconnection Workshop in Saõ Jose dos Campos and was the driving force behind the production of this book. The authors thank Christopher Doss, Colin Komar and Karlheinz Trattner for the use of figures they made and/or assisted with. Helpful conversations with James Drake, Stefan Eriksson, Ramon Lopez, Kittipat Malakit, Michael Shay, and Marc Swisdak are acknowledged.
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Cassak, P.A., Fuselier, S.A. (2016). Reconnection at Earth’s Dayside Magnetopause. In: Gonzalez, W., Parker, E. (eds) Magnetic Reconnection. Astrophysics and Space Science Library, vol 427. Springer, Cham. https://doi.org/10.1007/978-3-319-26432-5_6
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