46. The source of the slow solar wind revealed by heliospheric observations by Matt Owens (University of Reading) Heliospheric magnetic flux topology and connectivity deduced from suprathermal electrons sheds light on the slow wind formation.

http://www.uksolphys.org/?p=7936

~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ UKSP Nuggets are published on a monthly basis highlighting solar physics research led from the UK.

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Iain Hannah and Lyndsay Fletcher

~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ Dr. Iain G. Hannah Royal Society Research Fellow, Astronomy & Astrophysics Group, SUPA School of Physics & Astronomy, Kelvin Building, University of Glasgow, Glasgow, UK, G12 8QQ

Web: http://www.astro.gla.ac.uk/~iain/ Eml: iain.hannah@glasgow.ac.ukmailto:iain.hannah@glasgow.ac.uk Tel: +44 (0)141 330 6427 Fax: +44 (0)141 330 5183 ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~