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BS EN 62396-1:2016

$215.11

Process management for avionics. Atmospheric radiation effects – Accommodation of atmospheric radiation effects via single event effects within avionics electronic equipment

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BSI 2016 108
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IEC 62396-1:2016(E) is available as /2 which contains the International Standard and its Redline version, showing all changes of the technical content compared to the previous edition. IEC 62396-1:2016(E) provides guidance on atmospheric radiation effects on avionics electronics used in aircraft operating at altitudes up to 60 000 ft (18,3 km). It defines the radiation environment, the effects of that environment on electronics and provides design considerations for the accommodation of those effects within avionics systems. This International Standard helps aerospace equipment manufacturers and designers to standardise their approach to single event effects in avionics by providing guidance, leading to a standard methodology. This edition includes the following significant technical changes with respect to the previous edition: – incorporation of references to some new papers and issues which have appeared since 2011; – addition of solar flares and extreme space weather reference to a proposed future Part 6; – addition of reference to a proposed new Part 7 on incorporating atmospheric radiation effects analysis into the system design process; – addition of a reference to a proposed future Part 8 on other particles including protons, pions and muons.

PDF Catalog

PDF Pages PDF Title
4 CONTENTS
8 FOREWORD
10 INTRODUCTION
11 1 Scope
2 Normative references
3 Terms and definitions
20 4 Abbreviations and acronyms
23 5 Radiation environment of the atmosphere
5.1 Radiation generation
5.2 Effect of secondary particles on avionics
5.3 Atmospheric neutrons
5.3.1 General
24 5.3.2 Atmospheric neutrons energy spectrum and SEE cross-sections
Figures
Figure 1 – Energy spectrum of atmospheric neutrons at 40 000 ft (12 160 m), latitude 45°
26 5.3.3 Altitude variation of atmospheric neutrons
27 5.3.4 Latitude variation of atmospheric neutrons
Figure 2 – Model of the atmospheric neutron flux variation with altitude (see Annex D)
28 Figure 3 – Distribution of vertical rigidity cut-offs around the world
Figure 4 – Model of atmospheric neutron flux variation with latitude
29 5.3.5 Thermal neutrons within aircraft
5.4 Secondary protons
30 5.5 Other particles
Figure 5 – Energy spectrum of protons within the atmosphere
31 5.6 Solar enhancements
5.7 High altitudes greater than 60 000 ft (18 290 m)
32 6 Effects of atmospheric radiation on avionics
6.1 Types of radiation effects
6.2 Single event effects (SEEs)
6.2.1 General
33 6.2.2 Single event upset (SEU)
6.2.3 Multiple bit upset (MBU) and multiple cell upset (MCU)
35 6.2.4 Single effect transients (SETs)
36 6.2.5 Single event latch-up (SEL)
6.2.6 Single event functional interrupt (SEFI)
6.2.7 Single event burnout (SEB)
37 6.2.8 Single event gate rupture (SEGR)
6.2.9 Single event induced hard error (SHE)
6.2.10 SEE potential risks based on future technology
38 6.3 Total ionising dose (TID)
39 6.4 Displacement damage
7 Guidance for system designs
7.1 Overview
40 Figure 6 – System safety assessment process
41 Tables
Table 1 – Nomenclature cross reference
42 7.2 System design
Figure 7 – SEE in relation to system and LRU effect
43 7.3 Hardware considerations
44 7.4 Electronic devices characterisation and control
7.4.1 Rigour and discipline
7.4.2 Level A systems
7.4.3 Level B
45 7.4.4 Level C
7.4.5 Levels D and E
8 Determination of avionics single event effects rates
8.1 Main single event effects
46 8.2 Single event effects with lower event rates
8.2.1 Single event burnout (SEB) and single event gate rupture (SEGR)
8.2.2 Single event transient (SET)
47 8.2.3 Single event hard error (SHE)
8.2.4 Single event latch-up (SEL)
8.3 Single event effects with higher event rates – Single event upset data
8.3.1 General
48 8.3.2 SEU cross-section
8.3.3 Proton and neutron beams for measuring SEU cross-sections
50 Figure 8 – Variation of RAM SEU cross-section as function of neutron/proton energy
51 Figure 9 – Neutron and proton SEU bit cross-section data
52 8.3.4 SEU per bit cross-section trends in SRAMs
53 8.3.5 SEU per bit cross-section trends and other SEE in DRAMs
Figure 10 – SEU cross-section in SRAMs as function of the manufacture date
54 Figure 11 – SEU cross-section in DRAMs as function of manufacture date
55 8.4 Calculating SEE rates in avionics
56 8.5 Calculation of availability of full redundancy
8.5.1 General
8.5.2 SEU with mitigation and SET
57 8.5.3 Firm errors and faults
9 Considerations for SEE compliance
9.1 Compliance
9.2 Confirm the radiation environment for the avionics application
9.3 Identify the system development assurance level
9.4 Assess preliminary electronic equipment design for SEE
9.4.1 Identify SEE-sensitive electronic components
9.4.2 Quantify SEE rates
9.5 Verify that the system development assurance level requirements are met for SEE
9.5.1 Combine SEE rates for the entire system
58 9.5.2 Management of electronic components control and dependability
9.6 Corrective actions
59 Annexes
Annex A (informative) Thermal neutron assessment
60 Annex B (informative) Methods for calculating SEE rates in avionics electronics
B.1 Proposed in-the-loop system test – Irradiating avionics LRU in neutron/proton beam, with output fed into aircraft simulation computer
B.2 Irradiating avionics LRU in a neutron/proton beam
61 B.3 Utilising existing SEE data for specific electronic components on LRU
B.3.1 Neutron proton data
62 B.3.2 Heavy ion data
Table B.1 – Sources of high energy proton or neutron SEU cross-section data
63 B.4 Applying generic SEE data to all electronic components on LRU
Table B.2 – Some models for the use of heavy ion SEE data to calculate proton SEE data
64 B.5 Component level laser simulation of single event effects
65 B.6 Determination of SEU rate from service monitoring
67 Annex C (informative) Review of test facility availability
C.1.1 Neutron facilities
68 C.1.2 Proton facilities
70 C.1.3 Laser facilities
71 C.2 Facilities in Europe
C.2.1 Neutron facilities
73 C.2.2 Proton facilities
74 C.2.3 Laser facilities
75 Annex D (informative) Tabular description of variation of atmospheric neutron flux with altitude and latitude
Table D.1 – Variation of 1 MeV to 10 MeV neutron flux in the atmosphere with altitude
76 Table D.2 – Variation of 1 MeV to 10 MeV neutron flux in the atmosphere with latitude
77 Annex E (informative) Consideration of effects at higher altitudes
78 Figure E.2 – Integral linear energy transfer spectra in siliconat 75 000 ft (22 860 m) for cut-off rigidities (R) from 0 to 17 GV
Figure E.1 – Integral linear energy transfer spectra in siliconat 100 000 ft (30 480 m) for cut-off rigidities (R) from 0 GV to 17 GV
79 Figure E.3 – Integral linear energy transfer spectra in siliconat 55 000 ft (16 760 m) for cut-off rigidities (R) from 0 GV to 17 GV
Figure E.4 – Influence of solar modulation on integral linear energytransfer spectra in silicon at 150 000 ft (45 720 m)for cut-off rigidities (R) of 0 GV and 8 GV
80 Figure E.5 – Influence of solar modulation on integral linear energy transferspectra in silicon at 55 000 ft (16 760 m) for cut-off rigidities (R) of 0 GV and 8 GV
81 Figure E.6 – Calculated contributions from neutrons, protons and heavy ionsto the SEU rates of the Hitachi-A 4 Mbit SRAM as a function of altitude at a cut-off rigidity (R) of 0 GV
Figure E.7 – Calculated contributions from neutrons, protons and heavy ionsto the SEU rates of the Hitachi-A 4 Mbit SRAM as a function of altitude at a cut-off rigidity (R) of 8 GV
82 Annex F (informative) Prediction of SEE rates for ions
83 Figure F.1 – Example differential LET spectrum
Figure F.2 – Example integral chord length distributionfor isotropic particle environment
85 Annex G (informative) Late news as of 2014 on SEE cross-sections applicable to the atmospheric neutron environment
G.1 SEE cross-sections key to SEE rate calculations
G.2 Limitations in compiling SEE cross-section data
86 G.3 Cross-section measurements (figures with data from public literature)
G.4 Conservative estimates of SEE cross-section data
G.4.1 General
87 G.4.2 Single event upset (SEU)
Figure G.1 – Variation of the high energy neutron SEU cross-section per bit as a function of electronic device feature size for SRAMs and SRAM arrays in microprocessors and FPGAs
88 Figure G.2 – Variation of the high energy neutron SEU cross-section per bit as a function of electronic device feature size for DRAMs
89 G.4.3 Multiple cell upset (MCU)
Figure G.3 – Variation of the high energy neutron SEU cross-section per electronic device as a function of electronic device feature size for NOR and NAND type flash memories
90 G.4.4 Single event functional interrupt (SEFI)
Figure G.4 – Variation of the MCU/SBU percentage as a function of feature size based on data from many researchers in SRAMs [43, 45]
91 G.4.5 Single event latch-up (SEL)
Figure G.5 – Variation of the high energy neutron SEFI cross-section in DRAMs as a function of electronic device feature size
92 Figure G.6 – Variation of the high energy neutron SEFI cross-sectionin microprocessors and FPGAs as a function of electronic device feature size
93 G.4.6 Single event transient (SET)
Figure G.7 – Variation of the high energy neutron single event latch-up (SEL) cross-section in CMOS devices (SRAMs, processors) as a function of electronic device feature size
94 G.4.7 Single event burnout (SEB)
Figure G.8 – Single event burnout (SEB) cross-section in power electronic devices (400 V to 1 200 V) as a function of drain-source voltage (VDS)
Table G.1 – Information relevant to neutron-induced SET
96 Annex H (informative) Calculating SEE rates from non-white (non-atmospheric like) neutron cross-sections for small geometry electronic components
H.1 Energy thresholds
H.2 Nominal neutron fluxes
Table H.1 – Approximate SEU energy thresholds for SRAM-based devices
Table H.2 – Neutron fluxes above different energy thresholds (40 000 ft, latitude 45°)
97 H.3 Calculating event rates using non-atmospheric like cross-sections for small geometry electronic devices
98 Bibliography
BS EN 62396-1:2016
$215.11