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Continuing its long history of influential scientific publishing,
Phil. Trans. R. Soc. A publishes high quality theme issues on
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Philosophical Transactions A
ISSN 1364-503X
© The Royal Society, 2015
Except as otherwise permitted under the
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Cover image
A direct numerical simulation of incompressible magnetohydrodynamic plasma turbulence in the presence of a strong guide field. The resolution
of the simulation is 2048x2048x128. The image shows the presence and development of strong current sheets and instabilities in the current
density, in one of the planes perpendicular to the guide field. Overlaid on this is an image of a solar prominence eruption observed by the NASA
Solar Dynamics Observatory (SDO) on March 16, 2013. Simulation image is provided by Dr. Romain Meyrand and the SDO image is from the SDO
Gallery, image 187 [http://sdo.gsfc.nasa.gov/gallery/main/item/187].
Typeset in India by Techset Composition Limited. Printed in the UK by Cambrian Printers.
This paper meets the requirements of ISO 9706:1994(E) and ANSI/NISO Z39.48-1992 (Permanence of Paper) effective with volume 338,
issue 1649, 1992.
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ISSN 1364-503X | Volume 373 | Issue 2041 | 13 May 2015
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Dissipation and heating in solar wind turbulence
Theme issue compiled and edited by Khurom H. Kiyani, Kareem T. Osman and Sandra C. Chapman
Dissipation and heating in solar wind turbulence
• Supporting outstanding science
Phil. Trans. R. Soc. A | Volume 373 | Issue 2041 | 13 May 2015
The Royal Society is a self-governing Fellowship
of many of the world’s most distinguished scientists
drawn from all areas of science, engineering, and
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has been since its foundation in 1660, is to recognise,
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encourage the development and use of science for
the benefit of humanity.
1364-503X(20150513)373:2041
ISBN 978-1-78252-129-7
ISSN 1364-503X
The Royal Society Registered Charity No 207043
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