NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
Fast Plasma Instrument for MMS: Simulation ResultsMagnetospheric Multiscale (MMS) mission will study small-scale reconnection structures and their rapid motions from closely spaced platforms using instruments capable of high angular, energy, and time resolution measurements. The Dual Electron Spectrometer (DES) of the Fast Plasma Instrument (FPI) for MMS meets these demanding requirements by acquiring the electron velocity distribution functions (VDFs) for the full sky with high-resolution angular measurements every 30 ms. This will provide unprecedented access to electron scale dynamics within the reconnection diffusion region. The DES consists of eight half-top-hat energy analyzers. Each analyzer has a 6 deg. x 11.25 deg. Full-sky coverage is achieved by electrostatically stepping the FOV of each of the eight sensors through four discrete deflection look directions. Data compression and burst memory management will provide approximately 30 minutes of high time resolution data during each orbit of the four MMS spacecraft. Each spacecraft will intelligently downlink the data sequences that contain the greatest amount of temporal structure. Here we present the results of a simulation of the DES analyzer measurements, data compression and decompression, as well as ground-based analysis using as a seed re-processed Cluster/PEACE electron measurements. The Cluster/PEACE electron measurements have been reprocessed through virtual DES analyzers with their proper geometrical, energy, and timing scale factors and re-mapped via interpolation to the DES angular and energy phase-space sampling measurements. The results of the simulated DES measurements are analyzed and the full moments of the simulated VDFs are compared with those obtained from the Cluster/PEACE spectrometer using a standard quadrature moment, a newly implemented spectral spherical harmonic method, and a singular value decomposition method. Our preliminary moment calculations show a remarkable agreement within the uncertainties of the measurements, with the results obtained by the Cluster/PEACE electron spectrometers. The data analyzed was selected because it represented a potential reconnection event as currently published.
Document ID
20090005975
Acquisition Source
Goddard Space Flight Center
Document Type
Conference Paper
Authors
Figueroa-Vinas, Adolfo
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Adrian, Mark L.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Lobell, James V.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Simpson, David G.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Barrie, Alex
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Winkert, George E.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Yeh, Pen-Shu
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Moore, Thomas E.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
August 24, 2013
Publication Date
December 15, 2008
Subject Category
Geophysics
Meeting Information
Meeting: American Geophysical Union Conference
Location: San Francisco, CA
Country: United States
Start Date: December 15, 2008
End Date: December 20, 2008
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

Available Downloads

There are no available downloads for this record.
No Preview Available