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This course is designed for technical and management personnel who wish to gain an understanding of the fundamentals and the effects of space radiation on space systems and astronauts. The radiation environment imposes strict design requirements on many space systems and is the primary limitation to human exploration outside of the Earth’s magnetosphere. The course specifically addresses issues of relevance and concern for participants who expect to plan, design, build, integrate, test, launch, operate or manage spacecraft and spacecraft subsystems for robotic or crewed missions. The primary goal is to assist attendees in attainment of their professional potential by providing them with a basic understanding of the interaction of radiation with non-biological and biological materials, the radiation environment, and the tools available to simulate and evaluate the effects of radiation on materials, circuits, and humans.
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Single Particle Motion
©VLPisacane,2012 Space Radiation and its Effects on Space Systems and Astronauts 1 5 ─
SPACE RADIATION AND ITS EFFECTS ON SPACE SYSTEMS AND ASTRONAUTS
Single Particle Motion
by V. L. Pisacane
Single Particle Motion
©VLPisacane,2012 Space Radiation and its Effects on Space Systems and Astronauts 2 5 ─
TOPICS
Introduction Equation of Motion
Gyration Motion
Guiding Center Motion
Mirror Points
Summary
Single Particle Motion
©VLPisacane,2012 Space Radiation and its Effects on Space Systems and Astronauts 3 5 ─
INTRODUCTION Background
Trapping of particles by magnetic fields was first studied by Kristian Birkeland in Norway in ~1895 – He aimed beams of electrons at a magnet inside a
vacuum chamber and noted that they seemed to be channeled towards its near magnetic pole
Birkeland interested Poincaré who analyzed the motion of charged particles in a magnetic field and showed that they spiraled around field lines and were repelled from regions of strong field
Birkeland also interested Carl Stormer who carried out more detailed analyzes
Existence of trapped radiation was confirmed by the Explorer 1 and Explorer 3 missions in early 1958, under Dr. James Van Allen at the University of Iowa
As a consequence, the trapped radiation are often called the Van Allen radiation belts
http://www.centennialofflight.gov/essay/Dictionary/RADIATION_BELTS/DI160.htm
Single Particle Motion
©VLPisacane,2012 Space Radiation and its Effects on Space Systems and Astronauts 4 5 ─
5– 4
INTRODUCTION Summary Motion
Motion of the trapped radiation as illustrated in Figure 6.4 consists of three primary components: – Gyration ~ milliseconds
• Particles rotating around field lines – Mirroring ~0.1 ─ 1.0 s
• Particles traveling from one hemisphere to the other and back – Longitudinal drift ~ 1 ─ 10 min
• Particles driting east or west
Figure 6.4 Motion of charged
particles trapped in the Earth’s
magnetic field,
Single Particle Motion
©VLPisacane,2012 Space Radiation and its Effects on Space Systems and Astronauts 5 5 ─
EQUATION OF MOTION Introduction
Force on a particle in a magnetic and av electric field with charge q is given by the Lorentz force
where B = magnetic flux density or magnetic field vector, T E = electric field, V m-1
FL = Lorentz force, N q = charge, C v = velocity, m s-1 F = applied force
Equation of motion with the addition of an applied force F is then
BvEF qL
)(qdt
dm BvEF
v
Single Particle Motion
©VLPisacane,2012 Space Radiation and its Effects on Space Systems and Astronauts 6 5 ─
GYRATION MOTION Introduction
For a uniform magnetic flux density and no electric field, the force will be constant and perpendicular to the motion resulting in circular motion
Speed will remain constant
Positive particles will rotate clockwise around an out of plane field line
Negative particles will rotate counterclockwise around an out of plane field line
g
g
Positive charge Negative charge
Single Particle Motion
©VLPisacane,2012 Space Radiation and its Effects on Space Systems and Astronauts 7 5 ─
GYRATION MOTION Gyro-Frequency and Larmor Radius
Gyro-frequency or relativistic cyclotron frequency wc and Larmor radius rc follow from the gyration equation of motion
where
F = force, N m = gm0, relativistic mass, kg m0 = rest mass, kg a = acceleration, m s-2
q = charge, C v = magnitude of particle velocity, m s-1
vg = magnitude of gyration velocity, m s-1
R
cB
q
q
R
vcB
q
qvcB
pc
q
mvc
vcqB
m
qB
c
v1
m
qB
m
qB
m
qB
mrBrq
mrBqv
qdt
dm
2
g
2
2
00
g
2
clgl
2
clg
g
g
w
g
w
ww
w
Bvv
g
g
g
w
w
cB
R
cB
1
q
pc
qB
p
qB
mvr
qB
cm
qB
mc
qB
mvr
vr
vr
0g
l
00g
l
g
g
l
gcl
rl = Larmor radius, m R = magnetic rigidity, V g ≡ (1-v2/c2)─1/2
wg = gyrofrequency, s-1
fc = wc/ 2p, gyrofrequency, Hz B = magnetic flux density perpendicular to plane of
motion, T
Single Particle Motion
©VLPisacane,2012 Space Radiation and its Effects on Space Systems and Astronauts 8 5 ─
GYRATION MOTION Gyro-Frequency for Electrons and Protons
For electrons
For protons
Ratio of gyro-frequencies for the electron and proton is
where me= 9.11 x 10-31 kg qe = ─ e = ─1.60 x 10-19 C mp= 1.67 x 10-27 kg qp = e = 1.60 x 10-19 C
Hz B
1080.22
f
s rad B
1076.11011.9
B1060.1
m
qB
m
qB
10cg
1-11
31
19
0
g
g
p
w
g
g
gw
Hz B
1052.12
f
s rad B
1058.91067.1
B1060.1
m
qB
m
qB
7cg
1-7
27
19
0
g
g
p
w
g
g
gw
18331011.9
1067.1
m
m
f
f31
27
electron,0
proton,0
proton,g
electron,g
Single Particle Motion
©VLPisacane,2012 Space Radiation and its Effects on Space Systems and Astronauts 9 5 ─
GYRATION MOTION Larmor Radii for Electrons and Protons
For electrons
For protons
Ratio Larmor radii for the electron and proton is
where me= 9.11 x 10-31 kg qe = ─ e = ─1.60 x 10-19 C mp= 1.67 x 10-27 kg qp = e = 1.60 x 10-19 C
18331011.9
1067.1
m
m
r
r31
27
electron,0
proton,0
electron,l
proton,l
g
g
g
B
c1068.5
B
c
1060.1
1011.9
qB
cmr 12
19
31
0electron,l
g
g
g
B
c1004.1
B
c
1060.1
1067.1
qB
cmr 8
19
27
0protons,l
Single Particle Motion
©VLPisacane,2012 Space Radiation and its Effects on Space Systems and Astronauts 10 5 ─
Magnetic Rigidity
Kinetic Energy
Speed [% of c]
Gyro-frequency
Corona (10 mT)
Interplanetary 1 AU (5 nT)
Earth Surface (30 μT)
1 GV 0.43 GeV 73% 105.6 kHz 0.053 Hz 316.9 Hz
5 GV 4.1 GeV 98% 28.4 kHz 0.142 Hz 85.1 Hz
20 GV 19.1 GeV 99.8% 7.2 kHz 0.004 Hz 21.7 Hz
GYRATION MOTION Larmor Radii and Gyro-frequency in Terms of Magnetic rigidity
Magnetic Rigidity
Kinetic Energy
Speed [% of c]
Larmor Radius, Re = Earth radii
Corona (10 mT)
Interplanetary 1 AU (5 nT)
Earth Surface (30 μT)
1 GV 0.43 GeV 73% 330 m 6.6x108 m ≈ 100 Re 1.1x105 m ≈ 0.017 Re
5 GV 4.1 GeV 98% 1.65 km 3.3x109 m ≈ 520 Re 5.5x105 m ≈ 0.086 Re
20 GV 19.1 GeV 99.8% 6.60 km 1.3x1010 m ≈ 2100 Re 2.2x106 m ≈ 0.340 Re
Examples of Larmor radii and gyro-frequency for any charged particle with a given rigidity at
Sun near Earth surface of the Earth
Single Particle Motion
©VLPisacane,2012 Space Radiation and its Effects on Space Systems and Astronauts 11 5 ─
GYRATION MOTION Summary Motion in Uniform Magnetic Field
Orbit of a charged particle in a uniform, static magnetic field is a spiral trajectory
Particle gyrates in plane perpendicular to magnetic field in a circular orbit
Radius of orbit is the Larmor radius, rl
Sense of gyration depends on sign of the particle’s charge
Positive and negative charged particles will rotate in opposite directions
Gyro-frequency is given by wg or fg
Gyro-period given by 1/fg or 2p/ wg
Tangential velocity is constant
Particle’s energy is conserved
Single Particle Motion
©VLPisacane,2012 Space Radiation and its Effects on Space Systems and Astronauts 12 5 ─
GUIDING CENTER MOTION Introduction
When geomagnetic field in not constant and uniform and electric field is not zero, motion is more complicated
However, when the variation in the forces over distances comparable to the Larmor radius is small, these effects can be treated as perturbations
Partitioning the motion into gyro motion and motion of the guiding center where – Gyration motion – circular motion of the particle around the magnetic field in the
plane perpendicular to the magnetic field, vg
– Guiding center motion – motion of the center of the gyrating particle (all motion but gyration motion), vgc
Let
so that the equation of motion
can be approximated by
Bv
v g
g qdt
dmBvEF
v gc
gc qqdt
dm
gcg vvv
BvEFv
qqdt
dm
Single Particle Motion
©VLPisacane,2012 Space Radiation and its Effects on Space Systems and Astronauts 13 5 ─
GUIDING CENTER MOTION Guiding Center Equations
Equation of motion of the guiding center is
Partitioning the velocity and force into components parallel and normal to the magnetic field
gives
If for E|| and F|| are constant, guiding center motion parallel to the magnetic field is
Forces parallel to magnetic field accelerates particle along the field line with direction depending on sign of the force or charge of the particle
Forces perpendicular to the magnetic field will accelerate the particle orthogonal to the magnetic field line
||||
||gc qEFdt
dvm
gc||||gcv vεv
BvEFv
gc
gc qqdt
dm
FεF ||||F
)0(vtm
qEFv ||gc
||||
||gc
EεE ||||E
BvEFv
gc
gc qqdt
dm
Single Particle Motion
©VLPisacane,2012 Space Radiation and its Effects on Space Systems and Astronauts 14 5 ─
GUIDING CENTER MOTION Motion in Uniform Magnetic Field
General motion of proton and electron in a constant magnetic field with an initial velocity along the field line results in the direction of the magnetic field results in helical motion
g
g
Single Particle Motion
©VLPisacane,2012 Space Radiation and its Effects on Space Systems and Astronauts 15 5 ─
GUIDING CENTER MOTION Orthogonal Drift Velocities of the Guiding Center 1/2
Gyration without perturbations (see A)
General Force Drift (see C) – Drift due to presence of general force F
Electric Field Drift (see B) – Drift due to presence of electric field E
Gradient Drift (see D) – Drift due to gradient in t magnetic field ∇B – Dominates for the Earth
http://en.wikipedia.org/wiki/File:Charged-particle-drifts.svg
B
2E,gcB
BEv
2F,gcqB
BFv
EF q
BBv
3
2
BgcqB2
mv
Single Particle Motion
©VLPisacane,2012 Space Radiation and its Effects on Space Systems and Astronauts 16 5 ─
GUIDING CENTER MOTION Orthogonal Drift Velocities of the Guiding Center 2/2
Gravitational drift – Drifts due to presence of gravity vector g
Magnetic Curvature Drift – Drift due to Rc radius of curvature of magnetic field
Polarization Drift – Drifts due time derivative of the electric field dE/dt
2gcgqB
m Bgv
BBBBRv2
4
2
||
c
c
2
2
||
gcRqB
vm
RqB
vm
dt
d
qB
m
dt
d
B
12
g
gc
EEv
p
w
|| B
Drift out for positive charge Drift into for negative charge
dt
dE
Single Particle Motion
©VLPisacane,2012 Space Radiation and its Effects on Space Systems and Astronauts 17 5 ─
MIRRORS POINTS Introduction
If the electromagnetic fields do not vary in time, the energy of the particle is constant so that
The energy can be expressed as
in regions where charged particles can drift in either direction along magnetic field-lines
However, particles are excluded from regions where v|| is imaginary
Charged particles must reverse direction at those points on magnetic field-lines, these points are termed bounce points or mirror points
E = Energy
t = time m = particle mass
v|| = velocity parallel to field line vd = drift velocity
0dt
d
E
qBvvm2
1 2
D
2
||E
2/1
2
D||v)qB(
m
2v
E
qBmv2
1 2
DE
qBmv2
1 2
DE
= electric field potential, E = ─
Vm = magnetic field potential q = charge = orbital dipole moment of particle
=IA = 2riwc/2, I = current, A = area
Single Particle Motion
©VLPisacane,2012 Space Radiation and its Effects on Space Systems and Astronauts 18 5 ─
MIRRORS POINTS Mirror Points in Dipole Field
Distance a particle travels from the equator before mirroring is determined by its pitch angle at the equator
Equatorial pitch angle for a particle that mirrors at a given magnetic latitude in a dipole field is
where lm = magnetic latitude of mirror point aeq = pitch angle at the equator
6 – 18
From: http://www.altfuels.org/sampex/losscone/index.html
Pitch Angle 60o
Pitch Angle 40o
0 10 20 30 40 50 60 70 80 90
-80
-60
-40
-20
0
20
40
60
80
Equatorial Pitch Angle, degs
Mirro
r Latitu
e,
degs
Mirror magnetic latitude as function of magnetic equatorial
pitch angle
2/1
m
2
m
6
eq
2
sin31
cossin
l
la
Single Particle Motion
©VLPisacane,2012 Space Radiation and its Effects on Space Systems and Astronauts 19 5 ─
MIRRORS POINTS Mirror Points in Dipole Field
Mirror points occur at same field strength on each bounce, i.e., at same magnetic latitude and drift equatorially
If pitch angle close to 0 or 180 degrees (nearly aligned with magnetic field), mirror point will fall below planet surface
Particle with equatorial pitch angle 90 degrees, will mirror at equator and remain in magnetic equatorial plane
How far the particle travels from magnetic equator before "mirroring" is determined by pitch angle at the equator
Single Particle Motion
©VLPisacane,2012 Space Radiation and its Effects on Space Systems and Astronauts 20 5 ─
MIRRORS POINTS Equatorial Loss Cone
Equatorial Loss Cone is a cone of velocities of charged particle whose apex is on the equator and axis along a magnetic field line that represents the charged particles that will be lost due to interaction with the atmosphere or the surface in a dipole field
Loss-cone angle for intersection with the Earth depends solely on L-shell value and not on particle mass, charge or energy where
lca
Loss -one geometry
http://www-spof.gsfc.nasa.gov/Education/wtrap2.html
4/156
lcL3L4sin
a
Single Particle Motion
©VLPisacane,2012 Space Radiation and its Effects on Space Systems and Astronauts 21 5 ─
MIRRORS POINTS Mirror Points of Trapped Radiation 1/2
Spenvis simulation Initial Conditions
– L-shell: 2 Re – Equatorial pitch
angle: 30o
6 – 21
3D view of L shell
Altitude of mirror points
Cylindrical projection of the shell Footprints in Northern and Southern hemisphere
Single Particle Motion
©VLPisacane,2012 Space Radiation and its Effects on Space Systems and Astronauts 22 5 ─
MIRRORS POINTS Mirror Points of Trapped Radiation 2/2
3D view of L shell Altitude of mirror points
Cylindrical projection of the shell Footprints in Northern and Southern hemisphere
Spinvis simulation Initial Conditions
– L-shell: 2 Re – Equatorial pitch
angle: 15o
Mirror Points – Some mirror
points subsurface
Single Particle Motion
©VLPisacane,2012 Space Radiation and its Effects on Space Systems and Astronauts 23 5 ─
6 – 23
SUMMARY Typical Particle Characteristics
Table 6.5 Characteristics of typical radiation belt charged particles
Single Particle Motion
©VLPisacane,2012 Space Radiation and its Effects on Space Systems and Astronauts 24 5 ─
SUMMARY Summary Single Particle Motion
Motion along uniform magnetic field – Uniform B, no E: constant speed along B – Uniform B, E parallel to B: charge dependent acceleration along B
Gyration motion – Circular orbit in plane perpendicular to B – Sense of gyration depends on charge sign – Larmor radius rl and gyration frequency fg
Drift motion orthogonal to magnetic flux density B from force F – Drift perpendicular to B and F according to may depend on charge sign – If F proportional to q then drift motion independent of charge – If F not proportional to q then drift motion dependent on charge sign
Non-uniform and time-varying magnetic field – Gradient drift perpendicular to B and ∇B depends on charge sign – Converging/diverging B: deceleration/acceleration along B with mirroring
In a dipole field – Charged particles will mirror at a latitude depending on the equatorial pitch angle – Particles will intersect Earth if equatorial pitch angle is within equatiorial loss cone
6 – 24
2
FqBBFv
Single Particle Motion
©VLPisacane,2012 Space Radiation and its Effects on Space Systems and Astronauts 25 5 ─
DISCUSSION