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The Magnetosphere and Plasmasphere CSI 769 3 rd section, Oct. – Nov. 2005 J. Guillory
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The Magnetosphere and Plasmasphere

Dec 31, 2015

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The Magnetosphere and Plasmasphere. CSI 769 3 rd section, Oct. – Nov. 2005 J. Guillory. Lecture 8 (Oct.25) Bow shock scattering; Magnetosphere structure, charged particle orbits Advance reading: Gombosi Ch.1 & 6 (and/or Parks Ch. 4, 8 &10). - PowerPoint PPT Presentation
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Page 1: The Magnetosphere and Plasmasphere

The Magnetosphere and Plasmasphere

CSI 769

3rd section, Oct. – Nov. 2005

J. Guillory

Page 2: The Magnetosphere and Plasmasphere

• Lecture 8 (Oct.25) • Bow shock scattering; Magnetosphere structure, charged particle orbits

– Advance reading: Gombosi Ch.1 & 6 (and/or Parks Ch. 4, 8 &10).and Sci. Am. Apr. 1991: Collisionless Shock Waves

• Lecture 9 (Nov. 1) • Dawn-dusk electric field; gyrokinetic codes; magnetotail & current sheet

– Advance reading: Gombosi Ch. 7 & 14, Parks Sec. 7.8 & 11.5)

• Lecture 10 (Nov. 8)• MHD codes & boundary conditions; parallel E-fields & precipitation; satellite

diagnostics– Advance reading: Gombosi Ch. 4 , Parks Sec. 7.7

• In conjunction with the last topic: – Joel Fedder (NRL) is scheduled for a Space Sciences Seminar on his MHD

magnetosphere code, Wed. 10/26, 3:00 p.m., 206– Please attend.

Page 3: The Magnetosphere and Plasmasphere

Incoming particle scattering

• Stochastic Injection of Energetic Particles from Bow Shock and from Tailward reconnection region

• Nonadiabatic because gyroradius ~ B scale-length locally

• Particle orbit diffusion due to field fluctuations

Page 4: The Magnetosphere and Plasmasphere

Magnetic field geometry

Page 5: The Magnetosphere and Plasmasphere

Charged particle orbits, static B:

• Fast gyration about field line

• North-south bounce due to “magnetic mirror” force

• Slow east-west drift due to inhomogeneous magnetic field

• ExB drifts due to electric fields

Page 6: The Magnetosphere and Plasmasphere

Magnetosphere Simulation

• Particle codes, incl. gyro-averaged particle followers (e.g. Mary Hudson’s at Dartmouth)

• Fluid (MHD) codes– Fedder-Lyon-Mobarry code (NRL)– Spicer’s code(s): Odin etc.– BATSRUS (U. Michigan)

• Hybrid (particles and MHD) codes– Rice MSM code

Page 7: The Magnetosphere and Plasmasphere

• Models are available for community use:– CCMC: http://ccmc.gsfc.nasa.gov/– UCLA: http://www-ggcm2.igpp.ucla.edu/

• Source codes in public domain:– GEDAS (Japan, T. Ogino) (Japan, T.)

http://gedas22.stelab.nagoya-u.ac.jp/simulation/jst2k/hpf02.html

– BATSRUS: http://csem.engin.umich.edu/– NRL: http://www.lcp.nrl.navy.mil/hpcc-ess/software.html

• FCTMHD3D (C.R. DeVore)• AMRMHD3D (P. MacNeice)

– Zeus 3D MHD (Michael Norman): http://zeus.ncsa.uiuc.edu:8080/lca_intro_zeus3d.html

– CFD Codes: http://icemcfd.com/cfd/CFD_codes.html

Page 8: The Magnetosphere and Plasmasphere

Satellite sensors

Page 9: The Magnetosphere and Plasmasphere

Living With A Star Research Network

Solar Dynamics Observatory

Pole Sitter

Radiation Belt Mappers

Ionospheric Mappers

L1 Solar Sentinel

L2

Distributed network of spacecraft providing continuous observations

•Geospace Dynamics Nework with constellations of smallsats in key regions of geospace.

Page 10: The Magnetosphere and Plasmasphere

Cluster & Vortex

Page 11: The Magnetosphere and Plasmasphere

Cluster & Doublestar (DSP)

Page 12: The Magnetosphere and Plasmasphere

Image Satellite ENA sensors