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<p class="MsoNormal"><span style="font-size:11.0pt;font-family:"Calibri",sans-serif;color:#1F497D;mso-fareast-language:EN-US">Physics colloquium at the University of Glasgow.<o:p></o:p></span></p>
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<p class="MsoNormal"><b><span lang="EN-US" style="font-size:11.0pt;font-family:"Calibri",sans-serif">From:</span></b><span lang="EN-US" style="font-size:11.0pt;font-family:"Calibri",sans-serif"> Sonja Franke-Arnold [mailto:Sonja.Franke-Arnold@glasgow.ac.uk]
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<b>Sent:</b> 22 November 2016 13:17<br>
<b>To:</b> phys-staff@glasgow.ac.uk; phas-pgall@glasgow.ac.uk; phas-hon-staff@glasgow.ac.uk<br>
<b>Cc:</b> Daniel Oi <daniel.oi@strath.ac.uk><br>
<b>Subject:</b> colloquium tomorrow, 23/11, 3pm, Thomas Neukirch on "Storms in Space"<o:p></o:p></span></p>
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<p class="MsoNormal"><span style="font-size:10.0pt;font-family:"Tahoma",sans-serif;color:black">Dear All,
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<p class="MsoNormal"><span style="font-size:10.0pt;font-family:"Tahoma",sans-serif;color:black">please remember tomorrow's colloquium by<o:p></o:p></span></p>
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<p class="MsoNormal"><span style="font-size:10.0pt;font-family:"Tahoma",sans-serif;color:black">Speaker: Thomas Neukirch, St.Andrews<o:p></o:p></span></p>
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<p class="MsoNormal"><span style="font-size:10.0pt;font-family:"Tahoma",sans-serif;color:black">Topic: Storms in Space - Aspects of Space Plasma Activity in the Solar System (abstract below)<o:p></o:p></span></p>
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<p class="MsoNormal"><span style="font-size:10.0pt;font-family:"Tahoma",sans-serif;color:black">Time: 3-4pm<br>
Location: Kelvin Building 247<o:p></o:p></span></p>
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<p class="MsoNormal"><span style="font-size:10.0pt;font-family:"Tahoma",sans-serif;color:black">The colloquium will be followed by discussions, doughnuts and coffee in the Common Room.<o:p></o:p></span></p>
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<p class="MsoNormal"><span style="font-size:10.0pt;font-family:"Tahoma",sans-serif;color:black">Hope to see you tomorrow!
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<p class="MsoNormal"><span style="font-size:10.0pt;font-family:"Tahoma",sans-serif;color:black">Sonja<o:p></o:p></span></p>
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<p class="MsoNormal"><span style="font-size:10.0pt;font-family:"Tahoma",sans-serif;color:black">___<o:p></o:p></span></p>
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<p class="MsoNormal"><span style="font-size:10.0pt;font-family:"Tahoma",sans-serif;color:black">abstract:<o:p></o:p></span></p>
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<p class="MsoNormal"><span style="font-size:10.0pt;font-family:"Tahoma",sans-serif;color:black">The interaction between the plasma permeating the solar system and the magnetic field of the Sun and the planets gives rise to many interesting activity processes.
The energy powering space plasma activity is often first stored as magnetic energy, which is then released and converted into other forms of energy, for example thermal energy, kinetic energy in the form of bulk flows or high-energy particle populations. In
this talk I will first give a broad overview of plasma processes occurring within the solar system and then focus on a few important of space plasma activity, for example magnetic reconnection.<o:p></o:p></span></p>
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