Lunar precursor effects in the Terrestrial magnetosphere and solar wind

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ARTEMIS Science Working Team Meeting 9/14-16/2011 LUNAR PRECURSOR EFFECTS IN THE TERRESTRIAL MAGNETOSPHERE AND SOLAR WIND Jasper S. Halekas Space Sciences Laboratory University of California, Berkeley

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Lunar precursor effects in the Terrestrial magnetosphere and solar wind. Jasper S. Halekas Space Sciences Laboratory University of California, Berkeley. The Lunar Space Plasma Environment: Pre-ARTEMIS. Precursor Effects in the Terrestrial Magnetosphere. All Electrons. Upgoing e - (0-15°). - PowerPoint PPT Presentation

Transcript of Lunar precursor effects in the Terrestrial magnetosphere and solar wind

Page 1: Lunar precursor effects in the Terrestrial magnetosphere and solar wind

ARTEMIS Science Working Team Meeting 9/14-16/2011

LUNAR PRECURSOR EFFECTS IN THE TERRESTRIAL MAGNETOSPHERE AND SOLAR WINDJasper S. HalekasSpace Sciences LaboratoryUniversity of California, Berkeley

Page 2: Lunar precursor effects in the Terrestrial magnetosphere and solar wind

The Lunar Space Plasma Environment: Pre-ARTEMIS

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Precursor Effects in the Terrestrial Magnetosphere

All Electrons

Upgoing e- (0-15°)

Downgoing e- (165-180°)

EFI FFTSCM FFT

B Wavelets

B Field

fpfce

fci

fpfce

Spin Tone

EFI Background

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Free Energy Sources: Reflected Electrons in Magnetosphere

Loss Cone

Beam

Beam + Loss Cone:Produced By CombinedMagnetic & ElectrostaticEffects Near Surface

DownwardElectric Field

Plasma Electrons Follow Magnetic Field Linesand Reflect from E & B

Secondary ElectronsAccelerated Upward

E = - UΔConverging Magnetic Field Lines above Crustal Magnetic Fields

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Polarization Properties

Coherent

Parallel-Propagating

Right-Handed

• Wave properties all consistent with parallel-propagating whistlers coming down the magnetic field line towards the Moon

NarrowbandWaves propagating anti-parallel to field

EXB

EB

B0

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Instability Conditions

EFI

SCW

Reduced DistributionFunctionWhistler Mode: ω/k, (ωce-ω)/k

Streaming instabilities where df/dv|| positive

Whistlers correlate with edges of loss cone: i.e. df/dvperp positive

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Ions in the Mix?• Waves near fci modulate both the electron beam and the whistlers• Possible sources: Electron beam, shadowed ion distributions, bi-ion streaming

FGM Wavelets

Loss Cone Modulated

Electron Beam Modulated

Whistlers ModulatedProton & HeliumCyclotron Frequencies

ICWs?

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Precursor Effects in the Solar Wind

IonsUpgoing e- (0-15°)

Downgoing e- (165-180°)

EFI FFT

SCM FFTB Wavelets

B Field

SZA of SurfaceConnection

Page 9: Lunar precursor effects in the Terrestrial magnetosphere and solar wind

Fitzenreiter et al., 1990

Solar

Wind

Free Energy Sources: Reflected Electrons in Solar Wind

Generalized obstacle with magnetic fieldgradient and/or electrostatic potential gradient

MagneticField

ConvectionElectric Field

Electron Trajectory

Adiabatic Reflection in dHT Frame Gives you “Ears” in Solar Wind Frame

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Whistler Cyclotron Resonance Conditions

EFI

SCW

Reduced DistributionFunction(ωce-ω)/k : ω, k on whistler branch

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Ion Observations

P2 Ions

P1 Ions

P1 Reduced Dist. Funct.

P1 Power Spectrum

P1 Propagation

P1 Ellipticity

Parallel-Propagating

RH, LH

Foreshock Ions

Reflected Protons

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Free Energy Sources: Reflection From Crustal Magnetic Fields

Reflected Proton FluxesLue et al., 2010

Reflected ProtonsFollow PickupIon Trajectories

Solar

Wind

GyratingProtons

Distribution Near Cycloid “Cusp”

IMF

SW

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Pickup Ion Trajectories

Surface Crustal Magnetic Field

ConnectedUnconnected

ReconstructedIon Trajectories

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Ion Reflection Source Map

26 Event Periods, June 29 – August 31

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Lunar Precursor Effects