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© Copyright University of Surrey 2013
Internal Charging: Principles, Tools and Measurements
SPENVIS Workshop, Brussels, May 2013
Keith A. Ryden
Surrey Space Centre
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© Copyright University of Surrey 2013
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Electrostatic discharge (surface charging)
A significant issue in the 1970s-80s (e.g. MARECS)
Recently again a cause of problems (e.g. solar arrays)
insulator e.g. kapton blanket
ground
iconductondaryphotoe jjjjjj sec
e
secondary
electron
photon
photoelectron
conductivity
backscatter
Aluminium plate (with oxide coating)
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0036
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Electron Energy/eV
Surf
ace p
ote
ntia
l /V
Figure 6: Test results under a surface-charging keV electron beam
Aluminium plate (with oxide coating)
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ace p
ote
ntia
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Figure 6: Test results under a surface-charging keV electron beam
© Copyright University of Surrey 2013
Internal charging and deep dielectric discharge
The plastic object has been irradiated with electrons which do not fully penetrate
the width of the material
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Plane of the Lichtenberg
figure (tubes where
plastic has vaporised)
Darkening of the plastic
where ionising dose has
caused discolouration
MeV Electrons
Electron range
Exit route of discharge –
i.e. of the vaporised
material in plasma form
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Internal charging / Deep dielectric discharge
• Generally occurs in insulating
polymers, but can occur in glass
• Energetic, penetrating electrons
(>100keV)
• Small currents <1pA cm-2
• Slow charge build up (>24 hours)
leading to ESD
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Internal charging in space
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High energy electrons from space environment
Dielectric
or
isolated
conductor
Satellite
shielding
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Outer belt electron intensity variation and effects on satellites
Anik E1 & E2,
Intelsat K disabled
DRA-Δ anomalies Note log scale – outer belt is
highly dynamic due to
buffeting by the solar wind
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GEO comsat switching anomaly
G. Wrenn, D. Rodgers, K Ryden, Annales Geophysicae (2002) 20: 953–956
Solar minimum Solar maximum
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Electrons
Electrons are light and highly
scattered within materials
Cause ionization and also deposit
charge
Can be shielded out but produce
penetrating secondary X-rays (or
Bremsstrahlung)
If electrons are stopped in insulator
they cannot easily escape
q
X-rays
Secondary
emission and
backscatter
+ - +
-
+ - +
-
+ -
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Key factors for internal charging
Space environment and space weather
Electron transport though shielding and into dielectric
Dielectric intrinsic (thermal) conductivity
Radiation induced conductivity
Charge and electric field accumulation
Breakdown strength
Breakdown propagation
Effect on circuit and component
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1-D charging equation
where:
E is electric field
t is time
x is linear position
σ is conductivity
JR is radiation current (density)
[dJ/dx is the charge deposition rate at x]
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𝜀0𝜀𝑟𝑑𝐸(𝑥, 𝑡)
𝑑𝑡+ 𝜎 𝑥, 𝑡 𝐸 𝑥, 𝑡 = −𝐽𝑅(𝑥, 𝑡)
High energy electrons from space environment
Dielectric
or
isolated
conductor
Satellite
shielding
x J
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Charging curve at given depth
At a given depth and assuming non-varying conductivity:
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𝐸 𝑡 =𝐽𝑅𝜎
1 − 𝑒−𝑡𝜏
where 𝜏 =𝜀0𝜀𝑟
𝜎
Equilibrium
field 𝐸𝑒𝑞 =
𝐽𝑅𝜎
If 𝜎 is small (leading to large equilibrium E-fields) then
time constant is long
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Thermal / intrinsic / dark conductivity
Activation of electrons across the wide ‘band gap’
Conductivity is determined by Arrhenius-type
equation
Changes rapidly with temperature
• High temperature suppresses charging effect
• Low temperature conductivity can be very small indeed
EA=1.0eV for polythene
EA=1.7eV for PMMA
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kT
EAexp
1.00E-17
1.00E-16
1.00E-15
1.00E-14
1.00E-13
1.00E-12
1.00E-11
20 30 40 50 60 70 80 90 100 110
Temperature (ºC)
Volu
me c
onductivity (
O-1m
-1)
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Illustration of temperature effects
Changes of temperature greatly affect the internal charging process
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0
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1400
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2000
0 60 120 180 240 300
Time (s)
Surf
ace p
ote
ntial (V
)
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110
115
120
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Tem
pera
ture
(ºC
)
Surface potential
Temperature
Beam interuption
Dielectric
Constant 1.1 MeVelectron beam
2pA/cm2
Surfacevoltageprobe
Temperature
controller
Vacuum
vessel
x
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Radiation induced conductivity
Ionising dose leads to generation of additional charge carriers
Can be due to primary particles or secondary (bremsstrahlung)
𝜎 = 𝜎0 + 𝑘𝑝𝐷Δ
Where 𝜎0 is the dark conductivity (Ω-1cm-1)
𝑘𝑝 is the co-efficient of prompt RIC (Ω-1cm-1 rad-1 s)
𝐷 is ionising dose (rad)
Δ is a dimensionless material dependent exponent (Δ<1)
Δ is typically in range 0.6 to 1.0
RIC not a function of temperature
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Delayed conductivity
Transient effects
Conductivity does not reduce to zero instantaneously after irradiation is stopped
Tends to decay more slowly when sample has been irradiated for a long time
Permanent effect
An increase in conductivity dependent on the ionising dose received.
Few reports
Would indicate that charging is less likely as mission proceeds
ESADDC model included this effect but was difficult to get conditions where
discharge was likely
Still a research area since some polymers receive very large doses
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Field induced conductivity
Ohmic conductivity breaks down at very high field intensities
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Dielectric breakdown
Electrical breakdown – avalanche effect caused
by high fields ( >106 V)
• Free charge carriers are accelerated
• Lichtenberg figures generated
Deep dielectric discharge produces Lichtenberg
figures in transparent materials
Inter-electrode breakdown topically at >3 x 107 Vm-
1
For internal charging, inferred that similar
thresholds apply but difficult to confirm
Threshold typically taken as 1 x 107 Vm-1 and
preferred to keep electric fields below 1 x 106
Vm-1 for safety
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Measuring polymer conductivity
Beware of typical conductivities quoted by manufacturers
Measurements of dielectric conductivity typically quoted are usually after 60s of
current flow
Current measured will decay over time due to polarisation (capacitive charging)
For internal charging, post-polarisation current is more relevant
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pA
Sourcevoltage
Sample undertest
Guardelectrode
currentTransientpolarisationcurrent
time
Steady conductioncurrent
--
+ +
-
+
pA
Fig. 2 Long-term polarisation of dielectrics
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Measuring conductivities and polymer parameters
Electron beam method (parameter selective)
• Deposit charge into material and monitor its decay
• RIC can be measured by monitoring rate of decay
under fully penetrating beam (e.g. electrons)
Realistic continuous irradiations (multi-parameter
measurements)
• Irradiate under various permutations of environmental
conditions (high flux, low flux, high temp. low temp.,
high RIC, low RIC etc..)
• Creates set of simultaneous equations to solve
• Extract parameters using fitting algorithm
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------------------------------------
Surface voltage
probe
Depositing electron beam
Penetrating electron
beam (to study RIC
etc)
------------------------------------
Surface voltage
probe
Space-like
realistic
electron beam
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Realistic Electron Environment Facility
• Sr-90 beta source, 3 GBq
• High–Vacuum
• Thermal control for sample
• Well matched to GEO spectrum and
intensity
• Long test are possible (weeks……months)
• Testing of components for major satellite
projects
− E.g. Galileo
0.1 1 10Electron energy (MeV)
Inte
gral
flu
x (
/cm
^2
/s/s
r)
Sr-90 at 3cm
Flumic, 14 April 1994
Scatha, 14 June 1980
107
106
105
104
90Sr spectrum
space spectra
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Fluence / current threshold
Unfortunately it is not always easy to obtain necessary materials parameters
0.1 pA cm-2 has been established empirically as a ‘general’ charging
threshold for safe use of dielectrics (or 2 x 1010 electrons / cm2 over 10 hours
appears to be actual threshold)
[Reduced to 0.02 pA cm-2 below room temperature in ECSS]
Based on absorbed current (often confused with incident current)
Bodeau has suggested that this level is not always safe and that 0.01 pA cm-2 is
more suitable
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In-orbit measurements of internal charging / discharging
US CRRES mission
• various materials exposed in a GTO orbit (various shielding levels etc) –
discharges detected and quantified
‘DDD’ experiment (ESA) – no discharges detected
SURF (STRV and Giove-A)
• measurement of internal charging rate behind shielding
Van Allen probes (RBSP)
• similar to SURF
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SURF charging current measurements in GTO
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Space radiation particles
Satellite telemetry system
Lid 0.6mm Al
0.5mm Al plate 1.0mm Al plate
Satellite exterior wall
Satellite ground reference
fA fA
.
• Internal charging current vs depth
measurement
• Each plate has unique energy response
curve so spectrum can be obtained
• Built and flown on STRV1d
• 300g, 0.3W
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Ch
arg
ing
cu
rre
nt
(p
A c
m-2
)
Pro
ton
flu
x /
20
00
(c
m-2
s-1
)
0
5
10
15
20
25
30
35
40
Do
se
(k
rad
(Si)
)
Internal charging (bottom plate)
Proton flux (scaled)
'6mm Al' dose
'3mm Al' dose
Merlin on Giove-A
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Orbital regimes of concern for internal charging
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NASA HDBK 40002a
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DICTAT
Dielectric Internal Charging Analysis
Tool
Developed around 1999 (ESA
funding) to provide a fast
analysis tool for engineers
Environment - FLUMIC model
(new) - analytical
Electron transport – Weber &
Sorensen formulae
Temperature effects
RIC/FEC
Cable and Flat geometries
Various grounding arrangements
Electric field calculated in ten layers
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Electron
environment
ShieldingMaterials
properties
Radiation
induced
conductivity
Field
enhanced
conductivity
Thermal
effects on
conductivity
Permittivity
Density
Electron
depositionDielectric
geometry
Electric
field
calculation
ESD event ?
Charging
current
Orbit propagator
FLUMIC
© Copyright University of Surrey 2013
FLUMIC
• Empirical model developed specifically for
internal charging (2000)
• Based mainly on data from SREM and
GOES in 1980s and 1990s
• Give ‘worst-case’ 1-day flux envelope as
function of:
− B
− L
− fraction of solar cycle
− fraction of year (seasonal)
• Latest version 3.0
with flux
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Comparison of Giove-A data with DICTAT
1.5mm Al shield, 1.0mmAl collector plate
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Merlin Giove A
0.001
0.01
0.1
1
01 Dec 2005 01 Jun 2006 01 Dec 2006 02 Jun 2007 01 Dec 2007 01 Jun 2008 01 Dec 2008 01 Jun 2009 01 Dec 2009 02 Jun 2010
Daily a
vera
ged
ch
arg
ing
cu
rren
t (p
A/c
m2)
0
25
50
75
100
Sm
oo
thed
su
nsp
ot
nu
mb
er
Charging current (1.5mm shield, 1.0mm collector) Flumic plate 3 Smoothed sunspot number
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Internal charging at Jupiter
Copious energetic electrons (up to 100
MeV?)
• Order of magnitude more intense at peak
of the belt compared to Earth
Potential for very low temperatures
in parts of spacecraft
Hard spectrum leads to increased
RIC (good)
Voyager and Galileo suffered
upsets anomalies attributed to
internal charging
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JUICE – the European mission to Jupiter
ESA L-class science
mission under Cosmic
Vision programme
JUICE - Jupiter Icy Moons
Explorer
Launch 2022, arrives at
Jupiter 2030
Will spend nearly a year in
orbit around Ganymede
making remote observations
of the surface
Also flypasts of Europa and
Callisto
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DICTATv4 beta
Higher energies
Weber range formula
replaced by Tabata (up to
30MeV)
Improved ‘straggling’
approximation
Non-Al shielding (e.g. Ta)
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Rodgers et al, IEEE RADECS, 2011
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On-going challenges
• Long term behaviour of dielectrics in space
• Some materials may have very long time constants (months, years)
− 0.01pA cm-2 rather than 0.1 pA cm-2 safe level?
• In-orbit validations still very sparse
• Extreme space weather (Carrington event)
• 3D modelling
• Discharge trigger events – e.g. cosmic rays?
• Jupiter!
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