a. Calculation of the ion contribution to SEE rates shall be performed as follows:
1.
By using the LET
spectra for
cosmic rays and heavy ions from solar particle events given by the radiation
environmental specification, obtain the cross section experimental curve giving
at least LET threshold and saturation cross-section, or the Weibull parameters.
(a) Assume that the sensitive volume is a parallelepiped of the same volume as the sensitive one.
(b) Calculate the error rate using one of the following formulae:
-
![]()
with ![]()
-
Blandford and Adams formula: ![]()
where:
A = total surface area of the SV;
l, w and h = length, width and height of the SV;
dΦ/d(LET
) = differential ion
flux spectrum expressed as a function of LET
(shortened to “differential LET
spectrum”);
PCL(>D(LET
)) = integral chord length distribution, i.e. the probability of particles
travelling through the sensitive region with a pathlength greater than D;
LET
Min = minimum LET
to upset the cell (also referred
to as the LET threshold);
LET
Max = maximum LET
of the incident distribution
(~105 MeV×cm2/g).

Figure 9‑1: Procedure flowchart for hardness assurance for single event effects.
(a) Use the real sensitive volume for the integration.
(b) Calculate the error rate using the following formula:
![]()
with ![]()
where:
dF/d(LET
) = differential LET
spectrum;
PCL(>D(LET
)) = integral
chord length distribution;
dsion/d(LET
) = differential upset cross section;
A = total surface area of the sensitive volume;
S = surface area of the sensitive volume in the plane of the semiconductor die;
l, w and h = length, width and height of the sensitive volume;
DMax = maximum length that can be encountered in the SV;
LET
Max = maximum LET
of the LET spectrum;
LET
i,Min = lower bin limit in the differential upset
cross section dsion/d(LET
);
LET
i,Max = upper bin limit in the differential upset
cross section dsion/d(LET
).
NOTE For a detailed discussion of the RPP and IRPP approaches, see ECSS-E-HB-10-12 Sections 8.5.2 to 8.5.4. References can be found in [6], [7], [8], [9] and [10].