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Driving the dynamo via magnetic helicity flux: how differential rotation makes large scale magnetic fields

Event Details

Event Dates: 

Monday, April 28, 2014 - 4:00pm

Seminar Location: 

  • JILA Auditorium

Speaker Name(s): 

Ethan Vishniac

Speaker Affiliation(s): 

University of Saskatchewan
Seminar Type/Subject

Scientific Seminar Type: 

  • Astrophysical & Planetary Sciences Colloquia

Event Details & Abstract: 

Large scale magnetic fields are found everywhere in the universe, from the scales of planets to galactic disks (or larger). Understanding their generation and maintenance has proven to be unexpectedly difficult. I will discuss topological constraints on the growth of such fields, and argue that they are inconsistent with kinematic dynamo theory. Instead, I propose a modified version of mean field dynamo theory in which field growth is not exponential, but can grow from infinitestimal seeds in a very short time. I compare the predictions of the model to observations of stellar magnetic fields.

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