Speaker: Susan Clark (Stanford)
Contact Information:
Title: Magnetism and morphology in the interstellar medium
Abstract: The interstellar medium (ISM) is a turbulent, multi-phase, magnetic environment. It is home to vastly different gas phases, from cold, dense clouds to hot, tenuous plasma. Magnetic fields thread this interstellar environment, helping to sculpt galaxies through their influence on a diverse range of physics, from cosmic ray propagation to star formation. The magnetic ISM is also a formidable foreground for experimental cosmology, especially for studies of the polarized cosmic microwave background. I will discuss new ways to probe interstellar magnetism, the phase structure of interstellar gas, and the link between the two, with a particular focus on morphology: how the spatial structure of gas and dust encodes information about the physics of the ISM.
Visitor's room: 123
If you're not meeting in the visitor's office (Room 123), please indicate your office number.
Wednesday:
9:30 a.m.:
10:00 a.m.: Shaunak Modak
10:30 a.m.: (optionally astro-coffee)
11:00 a.m.: Matt Coleman (visitor office, or wherever)
11:30 a.m.: Chris Carr (Peyton 104)
12:00 p.m.:
12:30 p.m.: Wunch
1:00 p.m.: Wunch
1:30 p.m.:
2:00 p.m.: Sal Fu (Peyton 116)
2:30 p.m.:
3:00 p.m.: Andrew Saydjari (Peyton 132)
3:30 p.m.:
4:00 p.m.:
4:30 p.m.:
Day of week: Wednesday, November 19
Faculty Host:
Postdoc Host: Andrew Saydjari
Ronan Hix
Matt Goodbred
Shaunak Modak
Jiaxuan Li
Minghao Guo
Speaker
STUDENTS HAVE PRIORITY.
PLEASE NO MORE THAN 8 PEOPLE (it is more difficult to properly interact with the speaker in larger groups).