Physics & Astronomy

Thayer School of Engineering

Engineering-Physics         

Plasma Seminars                      

Winter 2012
Tuesdays at 3:30pm

Room 200, Cummings Hall

Directions

  January 10     

Matthew Gilson    

"Simulations of the Nightside    

Proton Precipitation during Substorms    

using Global MHD and IMAGE    

Observations"    

January 17    

Binzheng Zhang     

"Effects of Soft Electron Precipitation on    

the Coupled Magnetosphere-Ionosphere-      Thermosphere"    

January 24  

David C. Montgomer  

"The Effects of Boundary Conditions    

on Turbulence"    

January 31 

Aleksandr y. Ukhorskiy 

"RBSP Mission: Understanding Particle  Accelerations and Electrodynamics of the  Inner Magnetosphere"

February 7 

Ellen Cousins 

"Small-Scale Electric Field Variability  

in the High-latitude Inospheres"  

February 14 

Micah Dombrowski      

"Interpreting High-Frequency Vector     

Electric Field Measurements in the     

Cusp: Bursty Langmuir Waves on the     

       TRICE Sounding Rocket Mission"     

February 21     

Jeremy Ouellette     

"Nightside Processes in Outflow     

Driven Sawtooth Substorms"      

February 28     

Josh Semeter     

"Substorm Imaging at 450 MHz: Recent        Results from PFISR"      

March 6      

Oliver Brambles      

Dartmouth College       

Tuesday, March 6

"Magnetotail-Ionosphere Coupling in Fast Flow Channels"

    Oliver Brambles    

Dartmouth College    

 ABSTRACT: The closure of open magnetic flux in the magnetotail by magnetic reconnection generates fast flows in the plasma sheet. These flows occur in a sequence of short bursts and have been found to be localized between 2100 and 0100 MLT, peaking in the duskside, pre-midnight sector. Auroral substorm expansions and the Alfvénic aurora show similar local time distributions to the fast flows in the plasma sheet. Controlled simulations using the LFM global model show that the dawn-dusk asymmetry of the fast flow channels and Alfvénic aurora is regulated by the spatial variation in ionospheric conductance. This asymmetry disappears when the conductance is taken to be spatially uniform. Furthermore, non-physical spatial variations in the ionospheric conductances can be used to produce fast flows which are predominantly on the dawn side. This talk will examine how the gradients in the ionospheric conductance affect the distribution of fast flows in the plasma sheet.


https://engineering.dartmouth.edu/plasmaseminar/w12.html