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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 ([email protected]) 1

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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

([email protected])

1

© Copyright University of Surrey 2013

2

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)

0

500

1000

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2000

2500

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060

012

0018

0024

0030

0036

0042

0048

00

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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500

1000

1500

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012

0018

0024

0030

0036

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Electron Energy/eV

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ace p

ote

ntia

l /V

Figure 6: Test results under a surface-charging keV electron beam

© Copyright University of Surrey 2013

BBC Dara O’Briain’s Science Club Deep dielectric discharge!

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© 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

4

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

© Copyright University of Surrey 2013

5

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

© Copyright University of Surrey 2013

Internal charging in space

6

High energy electrons from space environment

Dielectric

or

isolated

conductor

Satellite

shielding

© Copyright University of Surrey 2013

7

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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8

GEO comsat switching anomaly

G. Wrenn, D. Rodgers, K Ryden, Annales Geophysicae (2002) 20: 953–956

Solar minimum Solar maximum

© Copyright University of Surrey 2013

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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

+ - +

-

+ - +

-

+ -

© Copyright University of Surrey 2013

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

10

© Copyright University of Surrey 2013

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

© Copyright University of Surrey 2013

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

© Copyright University of Surrey 2013

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)

© Copyright University of Surrey 2013

Illustration of temperature effects

Changes of temperature greatly affect the internal charging process

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0

200

400

600

800

1000

1200

1400

1600

1800

2000

0 60 120 180 240 300

Time (s)

Surf

ace p

ote

ntial (V

)

105

110

115

120

125

Tem

pera

ture

(ºC

)

Surface potential

Temperature

Beam interuption

Dielectric

Constant 1.1 MeVelectron beam

2pA/cm2

Surfacevoltageprobe

Temperature

controller

Vacuum

vessel

x

© Copyright University of Surrey 2013

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

15

© Copyright University of Surrey 2013

RIC measurements

16

© Copyright University of Surrey 2013

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

17

© Copyright University of Surrey 2013

Field induced conductivity

Ohmic conductivity breaks down at very high field intensities

18

© Copyright University of Surrey 2013

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

19

© Copyright University of Surrey 2013

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

20

pA

Sourcevoltage

Sample undertest

Guardelectrode

currentTransientpolarisationcurrent

time

Steady conductioncurrent

--

+ +

-

+

pA

Fig. 2 Long-term polarisation of dielectrics

© Copyright University of Surrey 2013

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

© Copyright University of Surrey 2013

22

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

© Copyright University of Surrey 2013

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

23

© Copyright University of Surrey 2013

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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© Copyright University of Surrey 2013

IDM sample configurations

25

© Copyright University of Surrey 2013

IDM results

26

© Copyright University of Surrey 2013

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

© Copyright University of Surrey 2013

28

SURF results

• GTO orbit

• 500 x 36,000 km

© Copyright University of Surrey 2013

0.001

0.01

0.1

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4/20

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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

29

© Copyright University of Surrey 2013

Orbital regimes of concern for internal charging

30

NASA HDBK 40002a

© Copyright University of Surrey 2013

Earth, Jupiter and Saturn electron belts

31

© Copyright University of Surrey 2013

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

33

© Copyright University of Surrey 2013

FLUMIC 3 for outer belt

34

© Copyright University of Surrey 2013

Comparison of Giove-A data with DICTAT

1.5mm Al shield, 1.0mmAl collector plate

35

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

© Copyright University of Surrey 2013

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

36

© Copyright University of Surrey 2013

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

37

© Copyright University of Surrey 2013

DICTATv4 beta

Higher energies

Weber range formula

replaced by Tabata (up to

30MeV)

Improved ‘straggling’

approximation

Non-Al shielding (e.g. Ta)

38

Rodgers et al, IEEE RADECS, 2011

© Copyright University of Surrey 2013

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!

39

© Copyright University of Surrey 2013

Key references

Standards:

• NASA HDBK 4002A Mitigating In-Space Charging Effects

• ECSS-E-ST-20-06C Spacecraft Charging Standard

Book:

• Guide to Mitigating Spacecraft Charging Effects, H. Garrett and A.

Whittlesey, Wiley, 2012

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