physics 5150 sol'n to hw #7 due: tues, april 25, 2017 1 5150 sol'n to hw #7 due: tues,...

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Physics 5150 Sol'n to HW #7 Due: Tues, April 25, 2017 1 1. Certain linear quasilongitudinal waves propagating at an arbitrary angle θ to B0 can be shown using common approximations to satisfy, ω 2 = ωi 2 + ωe 2 cos 2 θ, where ωe,i are the electron and ion plasma frequencies. Note that as θ -> 90 degrees, ω goes to the lower hybrid frequency, while at θ = 0 the waves become electron plasma (Langmuir) waves. For θ close to 90 degrees these waves are sometimes called electrostatic whistlers. a) Beginning with cold 2-fluid eqns. and assuming infinitely magnetized electrons and unmagnetized ions (Ωι = 0 and Ω e ), derive this frequency for these longitudinal waves propagating at an arbitrary angle θ. b) Beginning with the Maxwell matrix eqns. at arbitrary angle θ and making the same approximations, derive this same frequency from the condition that det M = 0. c) Explain physically why it is sometimes stated that the electrons have an effective mass m e /cos 2 θ in this approximation. Solution on next three pages:

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Physics 5150 Sol'n to HW #7 Due: Tues, April 25, 2017

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1. Certainlinearquasilongitudinalwavespropagatingatanarbitraryangleθ

toB0canbeshownusingcommonapproximationstosatisfy,ω2=ωi2+ωe2cos2θ,whereωe,iaretheelectronandionplasmafrequencies.Notethatasθ->90degrees,ωgoestothelowerhybridfrequency,whileatθ=0thewavesbecomeelectronplasma(Langmuir)waves.Forθcloseto90degreesthesewavesaresometimescalledelectrostaticwhistlers.

a) Beginning with cold 2-fluid eqns. and assuming infinitely magnetized electrons

and unmagnetized ions (Ωι = 0 and Ωe → ∞ ), derive this frequency for these longitudinal waves propagating at an arbitrary angle θ.

b) Beginning with the Maxwell matrix eqns. at arbitrary angle θ and making the

same approximations, derive this same frequency from the condition that det M = 0. c) Explain physically why it is sometimes stated that the electrons have an effective

mass me/cos2θ in this approximation. Solution on next three pages:

Physics 5150 Sol'n to HW #7 Due: Tues, April 25, 2017

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Physics 5150 Sol'n to HW #7 Due: Tues, April 25, 2017

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Physics 5150 Sol'n to HW #7 Due: Tues, April 25, 2017

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Physics 5150 Sol'n to HW #7 Due: Tues, April 25, 2017

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2. Morewavestoanalyze

a. Findthemagnitude(relativetoE)andsketchthemotion(relativetoEandBo)ofthewavemagneticfield,B,forthefollowingwavesinthecoldplasmaapproximation:

• Parallel propagating (torsional) Alfven waves • Parallel propagating low frequency whistler waves • Perpendicular propagating lower hybrid waves

b. Findthedirectionandmagnitudeofthefirst-orderwaveelectronandionfluidvelocitiesandthefirst-orderwavedensity(ifitisnon-zero)foreachofthewavesintheaboveproblem.Interpretyourresultsasmuchaspossible.

Part (a) solution on next pages:

Physics 5150 Sol'n to HW #7 Due: Tues, April 25, 2017

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Physics 5150 Sol'n to HW #7 Due: Tues, April 25, 2017

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Part (b) solution on next pages:

Physics 5150 Sol'n to HW #7 Due: Tues, April 25, 2017

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Physics 5150 Sol'n to HW #7 Due: Tues, April 25, 2017

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Physics 5150 Sol'n to HW #7 Due: Tues, April 25, 2017

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Physics 5150 Sol'n to HW #7 Due: Tues, April 25, 2017

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3. Assume the magnetic field above a sunspot varies (only in the vertical z-direction) as

B (z) = B0 z

1 + z/a , B0 = 200 G , a = 104 km Assume the density in the region is uniform, with n = 107 cm-3. A left-

circularly-polarized wave is launched vertically upwards from z = 0, with frequency f = 10 kHz.

a) What kind of wave is it? b) What is the wavenumber at z = 0? At z = 105 km? What is the zero-order

WKB wave form at altitudes z in between these? Prove WKB is valid in these regions.

c) What happens at high altitudes, as the local ion cyclotron frequency

decreases and approaches the wave frequency?

Physics 5150 Sol'n to HW #7 Due: Tues, April 25, 2017

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Physics 5150 Sol'n to HW #7 Due: Tues, April 25, 2017

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