ITC Tuesday Pizza Lunch Spring 2015 Schedule

The Institute for Theory and Computation (ITC) pizza lunch for Spring 2015 will be held on Tuesdays at 1:00 PM in Phillips unless stated otherwise. 

 

Date
Speaker
Affiliation
Topic
03 Feb, 1:00, Phillips
 Jonathan Tan
 University of Florida
 Magnetic Fields and Turbulence in Massive Star and Star Cluster
03 Feb, 1:30, Phillips
 Phil Myers
 CfA
 Filaments and N-pdfs in turbulent clouds
10 Feb, 1:00, Phillips
 Pat Slane
 CfA
 Postponed due to weather
10 Feb, 1:30, Phillips
 Laura Lopez
 CfA
 Postponed due to weather
18 Feb, 1:00, Phillips
 Meredith Hughes
 Wesleyan University
 Magnetic Fields and Turbulence in Protoplanetary Disks
18 Feb, 1:30, Phillips
 Xuening Bai
 CfA
 Magnetic Fields and Turbulence in Protoplanetary Disks
24 Feb, 1:00, Phillips
 Ofer Cohen
 CfA
 Stellar magnetic activity and space weather: perspectives from stars and planets 
24 Feb, 1:30, Phillips
 Jeremy Drake
 CfA
 Stellar magnetic activity and space weather: perspectives from stars and planets 
03 Mar, 1:00, Phillips
 Nick Murphy
 CfA
 Magnetic Recconection in Heliospheric, Labratory, and Astrophysical Plasmas
03 Mar, 1:30, Phillips
 Lorenzo Sironi
 CfA/ITC
 Magnetic Reconnection in Relativistic Astrophysical Jets
10 Mar, 1:00, Phillips
 Yanfei Jiang
 CfA/ITC
 Radiation MHD Simulations of Magneto rotational Instability in Accretion Disks
10 Mar, 1:30, Phillips
 Olek Sadowski
 CfA/ITC
 Jets and outflaws in black hole accretion disks
24 Mar, 1:00, Phillips
 Merav Opher
 Boston University
 Magnatized Jets Driven by the Sun: the Structure of the Heliosphere Revisited
24 Mar, 1:30, Phillips
 Pat Slane
 CfA
 Particle Accelaration in Super Nova Remnants: The Role of Magnetic Fields
31 Mar, 1:00, Phillips
 Josh Peek
 Columbia University
 GALFA-HI: new insights into the ISM paradigm and paradox
31 Mar, 1:30, Phillips
 Chat Hull
 CfA
 From filaments, to cores, to...filaments?! The role of magnetic fields in multi-scale, filamentary star formation.
07 Apr, 1:00, **Pratt**
 David Collins
 Florida State
 Turbulent Star Formation: a theoretical introduction
07 Apr, 1:30, **Pratt*
 Blakesley Burkhart
 CfA
How Well Does Turbulence Theory Describe the ISM?
14 Apr, 1:00, *Pratt*
 Antonia Savcheva
 CfA
 Using Magnetic Field Topology Analysis for Understanding Solar Eruptions
14 Apr, 1:30, *Pratt*
 Laura Lopez
 CfA
 Observational Tests of Cosmic-ray Diffusion in the Magellanic Clouds
21 Apr, 1:00, Phillips
 Dong Lai
 Cornell University
 Magnetic Star - Disk Interactions
21 Apr, 1:30, Phillips
 Alex Lazarian
 UW-Madison
 Cosmic ray acceleration and propagation in the presence of turbulence
28 Apr, 1:00, Phillips
 Mike McCourt
 CfA/ITC
 Do Galaxy Clusters Boil?
28 Apr, 1:30, Phillips
 Mark Bautz
 MIT
 TITLE