High Speed Streams & Earth’s Quadrupole Cusp: Implications for ORBE R. B. Sheldon, NASA/MSFC/NSSTC...

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High Speed Streams & Earth’s Quadrupole Cusp: Implications for ORBE R. B. Sheldon, NASA/MSFC/NSSTC T. Fritz & J.-S. Chen, CSP/BU Manaus, Brazil Feb 10, 2005

Transcript of High Speed Streams & Earth’s Quadrupole Cusp: Implications for ORBE R. B. Sheldon, NASA/MSFC/NSSTC...

Page 1: High Speed Streams & Earth’s Quadrupole Cusp: Implications for ORBE R. B. Sheldon, NASA/MSFC/NSSTC T. Fritz & J.-S. Chen, CSP/BU Manaus, Brazil Feb 10,

High Speed Streams & Earth’s Quadrupole Cusp:

Implications for ORBE

R. B. Sheldon, NASA/MSFC/NSSTC

T. Fritz & J.-S. Chen, CSP/BU

Manaus, Brazil

Feb 10, 2005

Page 2: High Speed Streams & Earth’s Quadrupole Cusp: Implications for ORBE R. B. Sheldon, NASA/MSFC/NSSTC T. Fritz & J.-S. Chen, CSP/BU Manaus, Brazil Feb 10,

The Oldest Physics Problem• How does point A influence point B?

– Aristotle: mind, “spooky action at a distance”– Democritus to Descartes: particles– Newton: gravity (e.g. tides)– Huygens: waves– Faraday: fields

• How does the Sun transfer energy to Earth?1. Photons & protons (DC equilibrium): pressure, heat2. Waves & impulsive events (AC mechanical): Alfvenic,

compressional, shocks3. Electric & Magnetic fields (AC/DC): currents

Page 3: High Speed Streams & Earth’s Quadrupole Cusp: Implications for ORBE R. B. Sheldon, NASA/MSFC/NSSTC T. Fritz & J.-S. Chen, CSP/BU Manaus, Brazil Feb 10,

Sun-Earth Transducers

• Proton pressure Bow shock, hot plasma (100eV electron, 1 kev/nuc ion), thermalized ram energy “Frictional” or “viscous” (V5/2)

• Impulsive SSC, shock acceleration, Fermi, radial diffusion, Kp, “mechanical” (V2)

• Fields Polar cap potential, convection, ring current, Dst, AE, “electrical” (V*Bz) [ICME]

• What transducer is CIR ORBE? Poor correlation of ORBE with all of the above! Best with Vsw.

Page 4: High Speed Streams & Earth’s Quadrupole Cusp: Implications for ORBE R. B. Sheldon, NASA/MSFC/NSSTC T. Fritz & J.-S. Chen, CSP/BU Manaus, Brazil Feb 10,

Springs & Shock Absorbers• Why does a car have BOTH springs & shocks?

– Springs are “reversible”, adiabatic, they “bounce back” (and ruin the tire tread).

– Shock absorbers are “irreversible”, non-adiabatic, they convert the energy to heat.

– Ex: manual dynamo with lightbulb or with 1F capacitor.

• Vsw energy transducer must be irreversible.– Cannot be too “stiff”, ideally it is “critically damped”

• Magnetic fields are “springy”, what are “shocks”?– Something responding to Vsw, yet not stiff…

Page 5: High Speed Streams & Earth’s Quadrupole Cusp: Implications for ORBE R. B. Sheldon, NASA/MSFC/NSSTC T. Fritz & J.-S. Chen, CSP/BU Manaus, Brazil Feb 10,

The Quadrupole Cusp -- Static Equilibrium

Page 6: High Speed Streams & Earth’s Quadrupole Cusp: Implications for ORBE R. B. Sheldon, NASA/MSFC/NSSTC T. Fritz & J.-S. Chen, CSP/BU Manaus, Brazil Feb 10,

The Dipole Trap

• Great Trap

• Poor accelerator

• ENA of E >1 keV

particles outside trap.

Page 7: High Speed Streams & Earth’s Quadrupole Cusp: Implications for ORBE R. B. Sheldon, NASA/MSFC/NSSTC T. Fritz & J.-S. Chen, CSP/BU Manaus, Brazil Feb 10,

Quadrupole Trap in the Laboratory

(Two 1-T magnets, -400V, 50mTorr)

Page 8: High Speed Streams & Earth’s Quadrupole Cusp: Implications for ORBE R. B. Sheldon, NASA/MSFC/NSSTC T. Fritz & J.-S. Chen, CSP/BU Manaus, Brazil Feb 10,

Maxwell 1880 Chapman 1930

Page 9: High Speed Streams & Earth’s Quadrupole Cusp: Implications for ORBE R. B. Sheldon, NASA/MSFC/NSSTC T. Fritz & J.-S. Chen, CSP/BU Manaus, Brazil Feb 10,

QuadrupolarT87 Magnetosphere

• All modern B-models have high latitude cusps.

• Since Chapman & Ferraro 1937, we’ve known the magnetosphere is a quadrupole, yet all the trapping models to the present have assumed a dipole.

Page 10: High Speed Streams & Earth’s Quadrupole Cusp: Implications for ORBE R. B. Sheldon, NASA/MSFC/NSSTC T. Fritz & J.-S. Chen, CSP/BU Manaus, Brazil Feb 10,

Cusp Equator

B-field lines

|B|

C=2

C=1

C=1.5

Page 11: High Speed Streams & Earth’s Quadrupole Cusp: Implications for ORBE R. B. Sheldon, NASA/MSFC/NSSTC T. Fritz & J.-S. Chen, CSP/BU Manaus, Brazil Feb 10,

The Simulated T96 Quadrupole Trap

• Lousy Trap

• Great Accelerator

• Can be made to trap better though.

Page 12: High Speed Streams & Earth’s Quadrupole Cusp: Implications for ORBE R. B. Sheldon, NASA/MSFC/NSSTC T. Fritz & J.-S. Chen, CSP/BU Manaus, Brazil Feb 10,

Chaotic, nearly trapped

Page 13: High Speed Streams & Earth’s Quadrupole Cusp: Implications for ORBE R. B. Sheldon, NASA/MSFC/NSSTC T. Fritz & J.-S. Chen, CSP/BU Manaus, Brazil Feb 10,

H+ Trapping in T96 Cusp

Page 14: High Speed Streams & Earth’s Quadrupole Cusp: Implications for ORBE R. B. Sheldon, NASA/MSFC/NSSTC T. Fritz & J.-S. Chen, CSP/BU Manaus, Brazil Feb 10,

e- Trapping of T96 Cusp

Page 15: High Speed Streams & Earth’s Quadrupole Cusp: Implications for ORBE R. B. Sheldon, NASA/MSFC/NSSTC T. Fritz & J.-S. Chen, CSP/BU Manaus, Brazil Feb 10,

Cusp Provisional Invariants• Minimum energy, Emin, is defined by “separatrix”

energy (ExB = B) ~ 30 keV

• Max energy, Emax, defined by rigidity.~ 3 MeV e-

• Mapping cusp Energy limits to the rad belts, give ~ 0-100 keV for protons, and 1-5 MeV for electrons.

• Mapping C-shell limits to the dipole give ~4<L<∞. very close to the PSD “bump”

• Mapping pitchangles 50o < < 90o at dipole eq.

• Cusp particles have all the right properties ORBE

Page 16: High Speed Streams & Earth’s Quadrupole Cusp: Implications for ORBE R. B. Sheldon, NASA/MSFC/NSSTC T. Fritz & J.-S. Chen, CSP/BU Manaus, Brazil Feb 10,

The Outer Radiation Belt Electrons (ORBE)

Page 17: High Speed Streams & Earth’s Quadrupole Cusp: Implications for ORBE R. B. Sheldon, NASA/MSFC/NSSTC T. Fritz & J.-S. Chen, CSP/BU Manaus, Brazil Feb 10,

McIlwain, 1966

Page 18: High Speed Streams & Earth’s Quadrupole Cusp: Implications for ORBE R. B. Sheldon, NASA/MSFC/NSSTC T. Fritz & J.-S. Chen, CSP/BU Manaus, Brazil Feb 10,

ORBE (McIlwain 1966)

Page 19: High Speed Streams & Earth’s Quadrupole Cusp: Implications for ORBE R. B. Sheldon, NASA/MSFC/NSSTC T. Fritz & J.-S. Chen, CSP/BU Manaus, Brazil Feb 10,

McIlwain 1966

Page 20: High Speed Streams & Earth’s Quadrupole Cusp: Implications for ORBE R. B. Sheldon, NASA/MSFC/NSSTC T. Fritz & J.-S. Chen, CSP/BU Manaus, Brazil Feb 10,

Empirical Prediction

• McIlwain 1966: Geo MeV e increases

• Paulikas & Blake 1979: Vsw best external

• Nagai 1988: Kp best internal predictor

• Baker 90 LPF, Koons&Gorney 90 NN

• Dmitriev&Chao03 Log-Linear

• Ukhorskiy et al., 04 NonLinear

Page 21: High Speed Streams & Earth’s Quadrupole Cusp: Implications for ORBE R. B. Sheldon, NASA/MSFC/NSSTC T. Fritz & J.-S. Chen, CSP/BU Manaus, Brazil Feb 10,

Correlations• Highest SW correlation for energetic particles in the

radiation belts is: velocity. R=.7-.8 during high-speed streams)

• V is NOT an energy. Not a density. Nor a Force(mv)• Multiplying by density ram or mechanical

energy, makes the correlation worse.• Multiplying by Bz Electrical energy, makes the

correlation worse.• Whatever the mechanism, it is not energy-starved

(2nd moment) or density starved (0th moment).

Page 22: High Speed Streams & Earth’s Quadrupole Cusp: Implications for ORBE R. B. Sheldon, NASA/MSFC/NSSTC T. Fritz & J.-S. Chen, CSP/BU Manaus, Brazil Feb 10,

1996

Page 23: High Speed Streams & Earth’s Quadrupole Cusp: Implications for ORBE R. B. Sheldon, NASA/MSFC/NSSTC T. Fritz & J.-S. Chen, CSP/BU Manaus, Brazil Feb 10,

The Discovery of Cusp MeV Electrons

Page 24: High Speed Streams & Earth’s Quadrupole Cusp: Implications for ORBE R. B. Sheldon, NASA/MSFC/NSSTC T. Fritz & J.-S. Chen, CSP/BU Manaus, Brazil Feb 10,

POLAR: Oct 12-16, 1996

Page 25: High Speed Streams & Earth’s Quadrupole Cusp: Implications for ORBE R. B. Sheldon, NASA/MSFC/NSSTC T. Fritz & J.-S. Chen, CSP/BU Manaus, Brazil Feb 10,

Sheldon et al., GRL 1998

POLAR/ CAMMICE data

1 MeV electron

PSD in outer cusp

Page 26: High Speed Streams & Earth’s Quadrupole Cusp: Implications for ORBE R. B. Sheldon, NASA/MSFC/NSSTC T. Fritz & J.-S. Chen, CSP/BU Manaus, Brazil Feb 10,

POLAR 4/1/97 Cusp Traversal

Page 27: High Speed Streams & Earth’s Quadrupole Cusp: Implications for ORBE R. B. Sheldon, NASA/MSFC/NSSTC T. Fritz & J.-S. Chen, CSP/BU Manaus, Brazil Feb 10,

Accelerator Efficiency

Why would the cusp accelerate at all? Why not just use standard well-

known accelerators?

Page 28: High Speed Streams & Earth’s Quadrupole Cusp: Implications for ORBE R. B. Sheldon, NASA/MSFC/NSSTC T. Fritz & J.-S. Chen, CSP/BU Manaus, Brazil Feb 10,

The Dipole Trap “Accelerator”

• The dipole trap has a positive B-gradient that causes particles to trap, by B-drift in the equatorial plane.

Three symmetries to the Dipole each with its own “constant of the motion”1)Gyromotion around B-field Magnetic moment, “”; 2) Reflection symmetry about equator Bounce invariant “J”; 3) Cylindrical symmetry about z-axis Drift invariant “L”

Betatron acceleration by E┴ compression, violation of 3rd invariant, L-shell

Page 29: High Speed Streams & Earth’s Quadrupole Cusp: Implications for ORBE R. B. Sheldon, NASA/MSFC/NSSTC T. Fritz & J.-S. Chen, CSP/BU Manaus, Brazil Feb 10,

The 1-D Fermi-Trap Accelerator

Waves convecting withthe solar wind, compresstrapped ions between the local |B| enhancementand the planetary bow shock, resulting in 1-Dcompression, or E// enhancement. Pitchangle diffusion keeps it in.

Page 30: High Speed Streams & Earth’s Quadrupole Cusp: Implications for ORBE R. B. Sheldon, NASA/MSFC/NSSTC T. Fritz & J.-S. Chen, CSP/BU Manaus, Brazil Feb 10,

The 2-D Quadrupole Trap

• A quadrupole is simply the sum of two dipoles. • Quadrupoles have “null-points” which stably trap

charged particles (eg. Paul trap)• Motion of the dipoles results in a 2D constriction of

the volume. This is just a generalization of 1D Fermi-acceleration to 2D.

• 1D Fermi acceleration increases E//, violating the 2nd invariant.

• 2D betatron acceleration increases E┴ , violating the 1st & 3rd invariants

Page 31: High Speed Streams & Earth’s Quadrupole Cusp: Implications for ORBE R. B. Sheldon, NASA/MSFC/NSSTC T. Fritz & J.-S. Chen, CSP/BU Manaus, Brazil Feb 10,

PROPERTY DIPOLE FERMI QUADRUPOLE

Stochasticity .001:1:1000 s .001:>103:>104 s 0.1:1:10 s

Process Flow rim>ctr>blocked end>side>diffus ctr>rim>open

Wave Coupling hi E weak all E same hi E best

Accel. in trap Traps Detraps Trap/Release

Diffusion Essential Helpful Neutral

Adiabatic Heat 2D pancake 1D cigar 2D pancake

Energy Source SW compress SW Alfven SW+internal

e- Max Energy 900MeV@10Re 1.8 [email protected] 280 MeV@3Re

e- Min Energy 45 keV 2.5 keV 30 keV

Trap Volume 1024 m3 1020 m3 1022 m3

Trap Lifetime > 1013s 104s 109:105s

Accel. Time > 300,000s 8,000s 25,000s

Trap Power < 5x108W 106W 5x107W

Page 32: High Speed Streams & Earth’s Quadrupole Cusp: Implications for ORBE R. B. Sheldon, NASA/MSFC/NSSTC T. Fritz & J.-S. Chen, CSP/BU Manaus, Brazil Feb 10,

Model1. Fast solar wind is trapped in the cusp

– 27 day recurrence, non-linear with Vsw

2. High Alfvenic turbulence of fast SW heats the trap– Low Q-value, compressional, BEN

3. 2nd Order “Fermi” accelerates electrons– Low energy appear first, then high w/rigidity cutoff.

4. Trap empties into rad belts simultaneous L=4-10 – “gentle” evaporation, or “rapid” topology change – Initially “butterfly” around 70-deg equatorial

Page 33: High Speed Streams & Earth’s Quadrupole Cusp: Implications for ORBE R. B. Sheldon, NASA/MSFC/NSSTC T. Fritz & J.-S. Chen, CSP/BU Manaus, Brazil Feb 10,

1. Non-Linear Vsw Dependence

E

Flux

EFlux

30keV100eV 1keV 10keV

Vsw

seed trap seed trap

The Reason that Vsw interacts non-linearly is that it does several things at once. It heats the seed population,while also making the trap deeper.

Page 34: High Speed Streams & Earth’s Quadrupole Cusp: Implications for ORBE R. B. Sheldon, NASA/MSFC/NSSTC T. Fritz & J.-S. Chen, CSP/BU Manaus, Brazil Feb 10,

Kolmogorov, Arnol’d, Moser (applied to Jupiter perturbation of

Earth)………Earth orbit as Perturbed byJupiter.

Earth orbit if Jupiter were 50k Earth masses.

Poincaré slicex vs. vX takenalong the E-J

line.

Page 35: High Speed Streams & Earth’s Quadrupole Cusp: Implications for ORBE R. B. Sheldon, NASA/MSFC/NSSTC T. Fritz & J.-S. Chen, CSP/BU Manaus, Brazil Feb 10,

T96 Cusp Topology

Solstice16UT

Solstice4UT

Equinox16UT Equinox

16UT,-Bz

Page 36: High Speed Streams & Earth’s Quadrupole Cusp: Implications for ORBE R. B. Sheldon, NASA/MSFC/NSSTC T. Fritz & J.-S. Chen, CSP/BU Manaus, Brazil Feb 10,

Cusp Feedback

But the cusp is turbulent! How can the REAL cusp trap anything for 2 days!?

It doesn’t.

Usually.

Page 37: High Speed Streams & Earth’s Quadrupole Cusp: Implications for ORBE R. B. Sheldon, NASA/MSFC/NSSTC T. Fritz & J.-S. Chen, CSP/BU Manaus, Brazil Feb 10,

Cusp Diamagnetic Cavitiesa.k.a Magnetic Bubbles

Page 38: High Speed Streams & Earth’s Quadrupole Cusp: Implications for ORBE R. B. Sheldon, NASA/MSFC/NSSTC T. Fritz & J.-S. Chen, CSP/BU Manaus, Brazil Feb 10,

Diamagnetic Effect of Cold Plasma

Page 39: High Speed Streams & Earth’s Quadrupole Cusp: Implications for ORBE R. B. Sheldon, NASA/MSFC/NSSTC T. Fritz & J.-S. Chen, CSP/BU Manaus, Brazil Feb 10,

An Interplanetary Test

Page 40: High Speed Streams & Earth’s Quadrupole Cusp: Implications for ORBE R. B. Sheldon, NASA/MSFC/NSSTC T. Fritz & J.-S. Chen, CSP/BU Manaus, Brazil Feb 10,

Cusp Scaling Laws

• Maximum energy from rigidity cutoffs, scaled by distance of planetary cusp to surface of planet.

• Assuming:– Brad ~ Bsurface= B0

– Bcusp ~ B0/Rstag3

– Erad= 5 MeV for Earth

– Ecusp ~ v2perp~ (Bcusp)2 ~ [(B0/Rstag

3)Rstag]

• E/B is constant

Erad-planet~(Rstag-Earth/Rstag-planet)(B0-planet/B0-Earth)2Erad-Earth

Page 41: High Speed Streams & Earth’s Quadrupole Cusp: Implications for ORBE R. B. Sheldon, NASA/MSFC/NSSTC T. Fritz & J.-S. Chen, CSP/BU Manaus, Brazil Feb 10,

Scaled Planetary ORBE

Planet

Mercury

Earth

Mars

Jupiter

Saturn

Uranus

Neptune

ERAD

4 keV

5 MeV

< 1.5 eV

150 MeV

1.2 MeV

1.4 MeV

0.42 MeV

R STAG

1.4

10.4

1.25

65

20

20

25

B0 (nT)

330

31,000

< 6

430,000

21,000

23,000

14,000

Page 42: High Speed Streams & Earth’s Quadrupole Cusp: Implications for ORBE R. B. Sheldon, NASA/MSFC/NSSTC T. Fritz & J.-S. Chen, CSP/BU Manaus, Brazil Feb 10,

Conclusions• The quadrupole is a nearly universal trap and cosmic

accelerator more efficient than Fermi (and shocks).

• The quadrupole cusp has ideal properties to couple AC mechanical energy from SW into the magnetosphere.

• The peculiar correlations of ORBE with SW can be explained by requiring an intermediate stage of the non-linear cusp.

• A test of the mechanism using comparative magnetospheres shows the correct energy scaling.

Soli Deo Gloria