Image of Rob Pfaff Launching a Rocket

"The dream of yesterday is the hope of today and the reality of tomorrow" -- R H Goddard

image of NASA Logo
Who Are We?
Home
Mission Statement
Branch Members
Associates
Where Are We?
LEP
SED
Sun-Earth Connect.
GSFC
NASA
What Do We Do?
Project Scientists and Directors
PI & Co-I Investigations
CCMC
Electric Fields Investigations
Magnetic Fields Investigations
Education and Public Outreach
Project Links
SEC
STP
LWS
Explorers
NMP
WIND
POLAR
MESSENGER
CNOFS
ST-5
THEMIS

frames version

Geospace Physics Branch, Code 612.3

Specializing in Mesospheric, Thermospheric, Ionospheric, and Magnetospheric Research


Mission Statement:
The Geospace Physics Branch's mission is to advance knowledge of the coupled solar wind - magnetosphere - ionosphere system by means of experimental and theoretical investigations and to provide leadership to NASA's Space Science Enterprise by serving as Project Scientists for Sun-Earth Connection Theme space flight programs.


April 18, 2005 - New Geospace GI Award:
Dr. Guan Le (612.3) has had a proposal to the Geospace Guest Investigator NRA selected by NASA HQ for 3 years of funding (Total Award: $293K). The title of the proposal is "An investigation of flux transfer events (FTEs) using multiple spacecraft and ground based observations using global MHD modeling". The main objective of Dr. Le's research project is to understand the nature of the time-varying reconnection that is responsible for FTE formation and evolution by using MHD simulations to place the local spacecraft observations in a global context.


August 10, 2005 - C/NOFS Satellite EMI Testing Underway:
The C/NOFS satellite is undergoing EMI testing at General Dynamics in Phoenix, Arizona this week (August 8-12). The Vector Electric Field Instrument (VEFI) built by Code 612.3 scientists Robert Pfaff and Doug Rowland, has performed well in all tests. Furthermore, this highly sensitive electric field detector has been used to unveil interference sources radiated by the satellite, including very small variations to the star sensor and other subsystems. For these tests, the output of the General Dyanmics EMI test antenna situated 1 meter from the spacecraft is fed back into the VEFI electric field detector burst memory input for high time/spectral resolution wave measurements and subsequent identification of the spacecraft interference.




Privacy, Security, Notices

Curator: Albert E. Davison, International Technology and Management, Inc.
E-mail:

Responsible NASA Representative: Dr. James A. Slavin
E-mail:

Last revised: June 28, 2004