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Currents, Electrojets and Instabilities John D Sahr Electrical Engineering University of Washington 19 June 2016
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Page 1: Currents, Electrojets and Instabilitiescedarweb.vsp.ucar.edu/wiki/images/7/70/2016CEDAR_Sunday_Sahr.p… · John D Sahr Electrical Engineering University of Washington 19 June 2016.

Currents, Electrojets and Instabilities

John D Sahr

Electrical Engineering University of Washington

19 June 2016

Page 2: Currents, Electrojets and Instabilitiescedarweb.vsp.ucar.edu/wiki/images/7/70/2016CEDAR_Sunday_Sahr.p… · John D Sahr Electrical Engineering University of Washington 19 June 2016.

Outline• The two main sources of large scale

currents in the ionosphere:

• solar-wind/magnetosphere, and

• dynamo ( ) forces.

• wired together by the magnetic field.

• The resulting fields and currents create meter-scale plasma irregularities

~F ⇥ ~B

Page 3: Currents, Electrojets and Instabilitiescedarweb.vsp.ucar.edu/wiki/images/7/70/2016CEDAR_Sunday_Sahr.p… · John D Sahr Electrical Engineering University of Washington 19 June 2016.

Ionospheric structure!

http://www.nap.edu/read/13060/chapter/12#154

This picture is intended

to scare you.

Page 4: Currents, Electrojets and Instabilitiescedarweb.vsp.ucar.edu/wiki/images/7/70/2016CEDAR_Sunday_Sahr.p… · John D Sahr Electrical Engineering University of Washington 19 June 2016.

Let’s start slowly• The ionosphere is that part of the

atmosphere in which a significant portion of the gas is ionized; you need to include plasma physics to describe what is happening above about 90 km.

• The ionosphere is created (mostly) by UV and x-ray photons from the Sun which partially ionize the neutral atmosphere.

Page 5: Currents, Electrojets and Instabilitiescedarweb.vsp.ucar.edu/wiki/images/7/70/2016CEDAR_Sunday_Sahr.p… · John D Sahr Electrical Engineering University of Washington 19 June 2016.

Where do ionospheric currents come from?

• Distortion of the Earth’s magnetic field due to the buffeting from the solar wind.

• Dynamo situations near the Earth, caused by the neutral winds dragging ionospheric plasma through the Earth’s magnetic field.

� > 1

� < 1

� =NkBT

B2/2µ=

Plasma pressure

magnetic field energy density

Page 6: Currents, Electrojets and Instabilitiescedarweb.vsp.ucar.edu/wiki/images/7/70/2016CEDAR_Sunday_Sahr.p… · John D Sahr Electrical Engineering University of Washington 19 June 2016.

Some basics (1)• Charged particles experience force from Electric and

Magnetic Fields

• If there is an electric field component parallel to , then electrons and ions freely accelerate. An electron exposed to 1 will achieve 90 km/s after 1 second (E region electron thermal velocity).

• Earth’s Magnetic Field lines are ~superconductors

~Fs = qs⇣~E + ~vs ⇥ ~B

~BµV/m

Page 7: Currents, Electrojets and Instabilitiescedarweb.vsp.ucar.edu/wiki/images/7/70/2016CEDAR_Sunday_Sahr.p… · John D Sahr Electrical Engineering University of Washington 19 June 2016.

Some basics (2)• Charged particles experience force from

Electric and Magnetic Fields

• When the electric field is perpendicular to then the charge particles will gyrate about the magnetic field, and drift at a mean speed. 1 mV/m causes drift of 20 m/s at high latitude, 40 m/s at the equator.

~Fs = qs⇣~E + ~vs ⇥ ~B

~B

Page 8: Currents, Electrojets and Instabilitiescedarweb.vsp.ucar.edu/wiki/images/7/70/2016CEDAR_Sunday_Sahr.p… · John D Sahr Electrical Engineering University of Washington 19 June 2016.

Some basics (3)

• Charged particles experience force from Electric and Magnetic Fields

• When the ion collision frequency is higher than the gyro frequency, then the ions don’t gyrate about (much); they slowly drift parallel to the electric field .

~Fs = qs⇣~E + ~vs ⇥ ~B

~B

~E

Page 9: Currents, Electrojets and Instabilitiescedarweb.vsp.ucar.edu/wiki/images/7/70/2016CEDAR_Sunday_Sahr.p… · John D Sahr Electrical Engineering University of Washington 19 June 2016.

Ionospheric currents driven by magnetosphere-solar wind interaction

www.comet.ucar.edu www.hao.ucar.edu

Page 10: Currents, Electrojets and Instabilitiescedarweb.vsp.ucar.edu/wiki/images/7/70/2016CEDAR_Sunday_Sahr.p… · John D Sahr Electrical Engineering University of Washington 19 June 2016.

Those currents …• Field Aligned Currents are electric currents

that flow along the Earth’s magnetic field lines with very little resistance.

• Pedersen Currents are electric currents that flow parallel to the electric field but perpendicular to ,

• Hall Currents are electric currents that flow perpendicular to both and .

~B

~B~E

Page 11: Currents, Electrojets and Instabilitiescedarweb.vsp.ucar.edu/wiki/images/7/70/2016CEDAR_Sunday_Sahr.p… · John D Sahr Electrical Engineering University of Washington 19 June 2016.

Those currents …• The Earth’s nearly static natural magnetic

multipole field would induce no currents in the ionosphere because it is curl-free:

• But when the solar wind presses on the magnetosphere, currents flow to support the perturbed .

r⇥ ~B =@ ~D

@t+ ~J = 0

~B

0

Page 12: Currents, Electrojets and Instabilitiescedarweb.vsp.ucar.edu/wiki/images/7/70/2016CEDAR_Sunday_Sahr.p… · John D Sahr Electrical Engineering University of Washington 19 June 2016.

Magnetospheric currents

https://ww

w.researchgate.net/publication/24014482_TIPO

_Tesla_Interferometric_Planetary_O

bserver

… are not the topic of this talk; the point is that the solar-wind

interacts with the magnetosphere,

and drive currents along the Earth’s magnetic field into

the ionosphere.

Page 13: Currents, Electrojets and Instabilitiescedarweb.vsp.ucar.edu/wiki/images/7/70/2016CEDAR_Sunday_Sahr.p… · John D Sahr Electrical Engineering University of Washington 19 June 2016.

Ohm’s Law

• In simple media, a simple Ohm’s Law:

• In partially ionized plasmas, we need a more complicated Ohm’s Law:

~J = � ~E

2

4Jx

Jy

Jz

3

5 =

2

4�p

�h

0��

h

�p

00 0 �0

3

5

2

4E

x

Ey

Ez

3

5

Page 14: Currents, Electrojets and Instabilitiescedarweb.vsp.ucar.edu/wiki/images/7/70/2016CEDAR_Sunday_Sahr.p… · John D Sahr Electrical Engineering University of Washington 19 June 2016.

What does that mean?

Altitude pedersen hall specific

h < 80 km small:no plasma

small:no plasma

small:no plasma

80 < h < 150 modest:ion collisions

large:magnetized e

unmagnetized i

large:plenty of plasma

150 < hsmall:

magnetized emagnetized i

small:magnetized emagnetized i

large:plenty of plasma

�p �h �0

Page 15: Currents, Electrojets and Instabilitiescedarweb.vsp.ucar.edu/wiki/images/7/70/2016CEDAR_Sunday_Sahr.p… · John D Sahr Electrical Engineering University of Washington 19 June 2016.

Ohm’s Law, again• If you think of those magnetospheric currents

being forced through the lower ionosphere, they will produce an electric field due to the finite resistivity in the ionosphere:

• These electric fields can generate meter scale plasma waves if they are large enough.

2

4E

x

Ey

Ez

3

5 =

$⌃

��12

4Jx

Jy

Jz

3

5

Page 16: Currents, Electrojets and Instabilitiescedarweb.vsp.ucar.edu/wiki/images/7/70/2016CEDAR_Sunday_Sahr.p… · John D Sahr Electrical Engineering University of Washington 19 June 2016.

Ohm’s Law, again• That Ohm’s law is correct in frame drifting

with the neutral gas, but viewed in an Earth-fixed system we need a (relativistic) coordinate change:

• These electric fields can generate meter scale plasma waves if they are large enough.

~E + ~U ⇥ ~B =$⌃ · ~J

Page 17: Currents, Electrojets and Instabilitiescedarweb.vsp.ucar.edu/wiki/images/7/70/2016CEDAR_Sunday_Sahr.p… · John D Sahr Electrical Engineering University of Washington 19 June 2016.

How about the equator?

• The magnetosphere can only (directly) drive ionospheric currents at high latitudes, since the field lines connect the ionosphere to the magnetosphere.

• …Yet there is a large ionospheric current at the magnetic equator; what causes this?

Page 18: Currents, Electrojets and Instabilitiescedarweb.vsp.ucar.edu/wiki/images/7/70/2016CEDAR_Sunday_Sahr.p… · John D Sahr Electrical Engineering University of Washington 19 June 2016.

Neutral Atmosphere vs. the Ionosphere; or

Superman vs. Batman

• The neutral atmosphere has greater mass and number density than the ionosphere below about 2000 km.

• The neutral atmosphere is massive compared to the ionosphere below about 500 km; where the neutral atmosphere goes (perp to B), that’s where the ionosphere goes.

Page 19: Currents, Electrojets and Instabilitiescedarweb.vsp.ucar.edu/wiki/images/7/70/2016CEDAR_Sunday_Sahr.p… · John D Sahr Electrical Engineering University of Washington 19 June 2016.

Tides and Winds

• When you heat a gas, it expands; when you heat the atmosphere, it expands in the only direction that it can: up. And it drags the ionosphere along with it (especially the ions).

• Of course, the Earth is also spinning, and once you put gas in motion around the Earth, Coriolis forces will push it around.

• You’ll hear a lot about tides and (thermospheric) winds at CEDAR.

Page 20: Currents, Electrojets and Instabilitiescedarweb.vsp.ucar.edu/wiki/images/7/70/2016CEDAR_Sunday_Sahr.p… · John D Sahr Electrical Engineering University of Washington 19 June 2016.

E region dynamo

• If you just think about the Earth getting heated on the dayside, and cooled on the night side, you can figure out the basic equatorial current (the Equatorial Electrojet).

B

day night

U Ueastward E, J westward E, J

heating cooling

Page 21: Currents, Electrojets and Instabilitiescedarweb.vsp.ucar.edu/wiki/images/7/70/2016CEDAR_Sunday_Sahr.p… · John D Sahr Electrical Engineering University of Washington 19 June 2016.

Tides (2)

• The daytime eastward electric field creates an upward E x B drift, but the ions are collisional; only the electrons E x B drift, separating the charges in the E-region slab.

B

day timenight time

EE

+++

��� +++

���

Page 22: Currents, Electrojets and Instabilitiescedarweb.vsp.ucar.edu/wiki/images/7/70/2016CEDAR_Sunday_Sahr.p… · John D Sahr Electrical Engineering University of Washington 19 June 2016.

Tides (3)• This secondary Electric field induces its own E x B

drift; westward during the day, eastward during the night.

• Again, the current is carried mostly by electrons, eastward during the day, westward at night.

B

day timenight time

EE

Ve VeJ J

Page 23: Currents, Electrojets and Instabilitiescedarweb.vsp.ucar.edu/wiki/images/7/70/2016CEDAR_Sunday_Sahr.p… · John D Sahr Electrical Engineering University of Washington 19 June 2016.

a little differently• a small Ex (East) is created by neutral wind/tide

• it generates a Pederson Current and a Hall current (down, Jy)

• … but the Jy current runs out of conductivity, charging the top and bottom of the electrojet, and Jy goes to zero.

Jx

Jy

�=

�p

�h

��h

�p

� E

x

Ey

�h

Ex

= �p

Ey

Jx

= �p

Ex

+ �h

Ey

=

✓�p

+�2

h

�p

| {z }Cowling conductivity, �c

Ex

�c � �h

Page 24: Currents, Electrojets and Instabilitiescedarweb.vsp.ucar.edu/wiki/images/7/70/2016CEDAR_Sunday_Sahr.p… · John D Sahr Electrical Engineering University of Washington 19 June 2016.

Equatorial Electrojet

• When you fold in other details — such as the descent of field lines to lower altitudes — you find that this large current is restricted to flow within a few degrees of the magnetic equator, peaking at about 105 km altitude.

• When the electrojet velocity exceeds C_s, then meter-scale, field aligned, plasma sounds waves are generated.

Page 25: Currents, Electrojets and Instabilitiescedarweb.vsp.ucar.edu/wiki/images/7/70/2016CEDAR_Sunday_Sahr.p… · John D Sahr Electrical Engineering University of Washington 19 June 2016.

Equatorial Electrojet

http://geomag.org/info/equatorial_electrojet.html

Page 26: Currents, Electrojets and Instabilitiescedarweb.vsp.ucar.edu/wiki/images/7/70/2016CEDAR_Sunday_Sahr.p… · John D Sahr Electrical Engineering University of Washington 19 June 2016.

F region dynamo

• At higher altitudes the Hall conductivity is quite small because both electrons and ions ExB drift (low collisions).

• The neutral atmosphere, although still dense, begins to exchange momentum with the F-region plasma.

Page 27: Currents, Electrojets and Instabilitiescedarweb.vsp.ucar.edu/wiki/images/7/70/2016CEDAR_Sunday_Sahr.p… · John D Sahr Electrical Engineering University of Washington 19 June 2016.

F region dynamo

• The equatorial F region field lines descend into the E-region at mid latitudes: the F-region dynamo is connected to the E region dynamo at mid latitudes.

• The E region Dynamo can enhance or suppress the F region Dynamo, depending upon which way the winds are blowing.

• In the upper F region, the ions can start to exert noticeable force on the neutrals.

Page 28: Currents, Electrojets and Instabilitiescedarweb.vsp.ucar.edu/wiki/images/7/70/2016CEDAR_Sunday_Sahr.p… · John D Sahr Electrical Engineering University of Washington 19 June 2016.

F region dynamo, seasonal effects

• At equinoxes, both E-region “footprints” of the equatorial F region are “on” or “off” together.

• In January, the southern footprint is on longer

• in June, the northern foot print is on longer

Page 29: Currents, Electrojets and Instabilitiescedarweb.vsp.ucar.edu/wiki/images/7/70/2016CEDAR_Sunday_Sahr.p… · John D Sahr Electrical Engineering University of Washington 19 June 2016.

Field Aligned Irregularities

• E and F region irregularities are highly field aligned, because high electron mobility (large ) along B “shorts out” any parallel E fields that could form.

• Thus, the density irregularities look like long columns of high and low density that are aligned with B.

�0

Page 30: Currents, Electrojets and Instabilitiescedarweb.vsp.ucar.edu/wiki/images/7/70/2016CEDAR_Sunday_Sahr.p… · John D Sahr Electrical Engineering University of Washington 19 June 2016.

What causes E region irregularities?

• In the E region, electrons drift in the ExB direction, while the ions barely move.

• When the electron drift exceeds the plasma sound speed, it creates a plasma “sonic boom”, strong perturbations in the plane perpendicular to B, and strongest in the ExB direction

Page 31: Currents, Electrojets and Instabilitiescedarweb.vsp.ucar.edu/wiki/images/7/70/2016CEDAR_Sunday_Sahr.p… · John D Sahr Electrical Engineering University of Washington 19 June 2016.

numerical simulation:

E di

rect

ion

Oppenheim, Otani, Ronchi “Saturation of Farley-

Buneman …” JGR v101 N A8, August 1996

B

Page 32: Currents, Electrojets and Instabilitiescedarweb.vsp.ucar.edu/wiki/images/7/70/2016CEDAR_Sunday_Sahr.p… · John D Sahr Electrical Engineering University of Washington 19 June 2016.

Halloween Storm, 2003

Cascades E region turbulence

Range, km150 300 600 900 1200

+1200

+300

-300

-1200

Dop

pler

Vel

ocity

, m/s

96.5 MHz radio waves (3 meter wavelength) scattering from 1.5 meter ion sound waves

Doppler upshift

Doppler up and downshift

Page 33: Currents, Electrojets and Instabilitiescedarweb.vsp.ucar.edu/wiki/images/7/70/2016CEDAR_Sunday_Sahr.p… · John D Sahr Electrical Engineering University of Washington 19 June 2016.

Other E region things …

• Quasi-Periodic Echoes

• Sporadic E

• 150 km echoes (at the equator) closely track the day time vertical E field.

Page 34: Currents, Electrojets and Instabilitiescedarweb.vsp.ucar.edu/wiki/images/7/70/2016CEDAR_Sunday_Sahr.p… · John D Sahr Electrical Engineering University of Washington 19 June 2016.

What causes F region irregularities?

• In the F region, the whole plasma moves in the ExB direction. However the Rayleigh-Taylor instability works.

• In the F region the peak density is around 350 km, with less density below. Thus, there’s a heavy fluid above a light fluid — the heavy fluid tries to fall down, and the light fluid should try to bubble up.

Page 35: Currents, Electrojets and Instabilitiescedarweb.vsp.ucar.edu/wiki/images/7/70/2016CEDAR_Sunday_Sahr.p… · John D Sahr Electrical Engineering University of Washington 19 June 2016.

F x B drifts

• In studying plasmas E x B drifts are a special case of F x B (Force x B) drifts.

• Pressure gradient produces a force in the same direction for electrons and ions, so they drift in opposite directions, thus producing a non zero current.

Page 36: Currents, Electrojets and Instabilitiescedarweb.vsp.ucar.edu/wiki/images/7/70/2016CEDAR_Sunday_Sahr.p… · John D Sahr Electrical Engineering University of Washington 19 June 2016.

F x B drifts

more plasma

less plasma

B

ionelectronrP

Page 37: Currents, Electrojets and Instabilitiescedarweb.vsp.ucar.edu/wiki/images/7/70/2016CEDAR_Sunday_Sahr.p… · John D Sahr Electrical Engineering University of Washington 19 June 2016.

F x B drifts with perturbation

more plasma

less plasma

B

ionelectron E

E x B

downward perturbation

Page 38: Currents, Electrojets and Instabilitiescedarweb.vsp.ucar.edu/wiki/images/7/70/2016CEDAR_Sunday_Sahr.p… · John D Sahr Electrical Engineering University of Washington 19 June 2016.

Find JRO plumes

From Jorge Chau: https://en.wikipedia.org/wiki/Jicamarca_Radio_Observatory#/media/File:Esf.jpg

Page 39: Currents, Electrojets and Instabilitiescedarweb.vsp.ucar.edu/wiki/images/7/70/2016CEDAR_Sunday_Sahr.p… · John D Sahr Electrical Engineering University of Washington 19 June 2016.

Air glow plumes

Page 40: Currents, Electrojets and Instabilitiescedarweb.vsp.ucar.edu/wiki/images/7/70/2016CEDAR_Sunday_Sahr.p… · John D Sahr Electrical Engineering University of Washington 19 June 2016.

summary

• Two main sources of ionospheric currents:

• neutral winds (low latitude), and

• magnetosphere currents (high latitude)

• sufficiently strong currents cause E region irregularities

• sufficiently strong gradients cause F region irregularities

Page 41: Currents, Electrojets and Instabilitiescedarweb.vsp.ucar.edu/wiki/images/7/70/2016CEDAR_Sunday_Sahr.p… · John D Sahr Electrical Engineering University of Washington 19 June 2016.

Questions?

Big thanks

To my students: Weiwei Sun, Marcos Iñonan

To my past students/present colleagues: Frank Lind, Melissa Meyer, Andy Morabito, Cliff Zhou, Laura Vertatschitsch

To my advisors and mentors: Don Farley, Sunanda Basu, Wes Swartz, Bela Fejer, Jason Providakes

Mike Kelly, and his book!

To my sponsors NSF, AFOSR, NATO, Boeing, Xilinx, Washington Research Foundation


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