Simplified model of
atmospheric neutron flux variation with altitude. Data is from Dr.
Eugene Normand, Boeing Radiation Effects Lab.
Atmospheric radiation is an issue for avionics
designers today, with every indication of becoming a greater issue in
the future. Atmospheric radiation causes single event effects (SEE) in
electronics, resulting in various system failure conditions, including
hazardous misleading information.
Cosmic radiation, including high energy
neutrons, is constantly showering the earth. Galactic cosmic rays and
solar rays hit the earth's atmosphere, interact with oxygen and nitrogen
atoms, and produce particle cascades of secondary radiation. This
secondary radiation leads to a high flux of energetic particles,
including protons, neutrons, and pions.
Of the possible secondary particles,
neutrons have been shown to be mainly responsible for causing single
event upsets in memories and other devices in aircraft since the early
1990s. Neutrons interact with the silicon structures of a component and
release energy that can change the state of a bit.
While the flux density varies with
global position, altitude, and solar activity, all surface locations are
exposed to this radiation, including ground level. Typical commercial
airliners operate up to 40,000 ft, where the flux density is in the
range of 300 to 450 times greater than at sea level, resulting in
greater incidences of SEEs for avionics equipment compared to
ground-based equipment.
Altitude variation of atmospheric
neutrons derives from competition between various production and removal
processes that affect how the neutrons and the initiating cosmic rays
interact with the atmosphere. The result is a maximum in the flux at
about 60,000 ft, called the Pfotzer maximum.
Although altitude is the largest single
factor driving atmospheric neutron flux, latitude is also very
important. The variation with latitude is due to the bending of primary
particles' trajectory by the earth's geomagnetic field, increasing by a
factor of six between equatorial latitude and the high latitude polar
regions.
The energy variation of atmospheric
neutrons is usually presented by plotting the differential flux (flux
per unit energy interval) as a function of energy, which is often called
the spectrum. Neutron spectrum measurements at altitude are more
complex than the neutron flux measurements at altitude and latitude, but
they have been made and are in good agreement with detailed and
elaborate neutron transport calculations.
The level of atmospheric radiation is
also dependent on the sun. During a typical 11-year sunspot cycle, the
sun produces about 100 severe coronal mass ejections (CMEs) or solar
flares and about four extreme CMEs into the solar system—only a fraction
of which usually hit the earth.
Particles from these solar flares
“typically” have energies much lower than particles produced by galactic
cosmic rays from outside the solar system. During periods of low solar
activity, the surface of the sun is comparatively stable and the
particles produced “normally” contribute very little (<2%) to the
resulting secondary neutron particle creation in the atmosphere.
But during times of high activity, large
solar flares occur. These can produce large numbers of high energy
solar energetic particles over a period of a few hours, creating SEE
rates from 30 to 300 times normal. Documented occurrences have been rare
over the last 60 years, and therefore this should be considered a
specific risk.
During the solar maximum period, the
sun's magnetic field pushes out away from the sun shielding the earth
from galactic particles; the atmospheric neutron flux decreases.
Conversely, during the solar minimum, the magnetic field collapses and
is not effective at deflecting galactic particles, and the atmospheric
neutron flux increases.
SEEs are caused by a single particle,
most likely a neutron, and can take on various forms. The definition of a
single event is the disturbance of an active electronic device, such as
a transistor, caused by the energy deposited in a device by a single
energetic particle. The effect is caused when a radiation-generated
ionization charge exceeds the device's critical charge. There are
various types of these events, but they all are the result of a single
particle depositing sufficient energy to cause a disturbance in an
electronic device.
When charged particles lose energy by
ionizing the medium through which they pass, they create a path of
electron-hole pairs. These electron-hole pairs collect at the source and
drain of a transistor and produce a current pulse. While the majority
of the neutrons passing through a microelectronic device will have no
impact, if the particle deposits enough charge, a malfunction of the
device results; the state of a node can change from logic 1 to logic 0
and vice versa.
Various failure modes in electronic
systems can occur, such as data corruption or unplanned events.
Additional types of undesirable effects may include the following:
• Damage to hardware
• Corrupted software residing in volatile memory
• Corrupted data in memory
• Microprocessor halts and interrupts
• Writing over critical data tables
The industry trend is for continued
decreases in component feature size and operating voltages, while the
number of gates on a given device continues to increase. As this trend
continues to deep submicron gate lengths, the expected critical charge
decreases and the expected sensitivity to radiation increases. Note that
extrapolating the level of susceptibility and resulting behavior of
future IC technologies from older devices cannot be guaranteed without
measurement.
There are various types of SEEs which
result in different types of failure modes. These include single and
multiple event upsets, latch-up, transients, single event functional
interrupts, and burnout. Hardware can be damaged, as in the case of a
burnout or gate rupture, but most often the failures are nondestructive.
Single event upsets are the most common type of event. Under current IC
technology conditions, many devices are being fabricated with feature
sizes of 90 nm, 65 nm, and below. At this technology point, many SRAMs
are experiencing multiple cell upsets in which a single neutron
interaction leads to two or more physically adjacent cell upsets.
Single event latch-up is another area of
concern. Latch-up is caused by a charged particle creating a localized
short circuit across the device. When the condition occurs, there is a
loss of device functionality due to a single event induced high current
state. Often the device is not permanently damaged, but power cycling is
required to resume normal device operation.
The development of highly reliable and
available systems requires consideration of both the occurrence of SEEs
and the impact they have on system performance. An addition to the
System Safety Assessment Guidelines would provide instruction and an
analysis methodology for performing a system assessment of atmospheric
radiation susceptibility.
The addition proposed here would provide
a process for assessing each component in the design, incorporating IC
effect rates, determining mitigation requirements, and finally
summarizing the total SEE faults for the system. Also provided would be
SEE analysis preparation steps, instructions on determining neutron
cross-section data for each sensitive IC, and the calculation of the SEE
effect rates. That data would then be utilized to complete the analysis
with the cumulative results and impact to the system.
While many factors go into determining a
hardware design, the level of susceptibility to SEEs needs to play a
role in device selection and play a role in hardware and software
architecture. This radiation susceptibility assessment could be a part
of a component selection phase of a system design process, and it would
begin with a review of available test and analysis data for each
selected component. The data could be analyzed and an impact analysis on
system operation performed. With this information, the need for and
degree of mitigation can be determined. Finally, an on-going program to
monitor the design could be used to verify that the system continues to
meet requirements through the life of the product.
Because susceptibility to atmospheric
radiation impacts the safety and reliability of a system, the system
designer needs to address SEE as a formal part of the system development
process. Having the guidelines and SEE analysis method to aid in the
radiation susceptibility evaluation of ICs and system impact will result
in a more complete and accurate system safety assessment.
More information on this technical paper can be found at http://papers.sae.org/2011-01-2497.
This article is based on SAE technical paper 2011-01-2497 by Mike Dion, Rockwell Collins, and Laura Dominik, Honeywell
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