FORM¶
The First Order Reliability Method is used under the following
context: let  be a random input vector with
joint density probability  
,
let  
 be the
limit state function of the model and let 
 be
an event whose probability 
 is defined as:
(1)¶
The objective of FORM is to evaluate . The method proceeds in three steps:
Step 1: Map the probabilistic model in terms of  thanks to an
isoprobabilistic transformation 
 which is a diffeomorphism from
 into 
, such that the distribution of the random vector
 has
the following properties: 
 and 
 have the same
distribution for all rotations 
.
The usual Isoprobabilistic transformations are the Generalized
Nataf transformation and the Rosenblatt one.
The mapping of the limit state function is
.
Then, the event probability 
 can be written as:
(2)¶
where  is the density function of the distribution in the standard space:
that distribution is spherical (invariant by rotation by definition). That property implies
that 
 is a function of 
 only.
Furthermore, we suppose that outside the sphere  tangent to the limit state surface in the standard space,
 is decreasing.
Step 2: Find the design point  which is the point
verifying the event of maximum likelihood : the decreasing hypothesis of the standard
distribution 
 outside the sphere tangent to the limit state surface in
the standard space implies that the design point is the point on the limit state boundary that is closest
to the origin of the standard space. Thus, 
 is the result of a constrained
optimization problem.
Step 3: In the standard space, approximate the limit state surface by a linear surface at the design
point . Then, the probability
 (2) where the limit state surface has been approximated by a linear surface (hyperplane)
can be obtained exactly, thanks to the rotation invariance of the standard distribution 
:
(3)¶
where  is the Hasofer-Lind reliability index, defined as the distance of the design point
 to the origin of the standard space and 
 the marginal cumulative distribution function
along any direction of
the spherical distribution in the standard space (refer to Generalized Nataf Transformation and
Rosenblatt Transformation).
Let us recall here that in the Rosenblatt standard space, random vectors follow the standard
normal
distribution (with zero mean, unit variance and unit correlation matrix), which implies that
 where 
 is the CDF of the normal distribution with zero mean and unit variance.
In the Generalized Nataf standard space, random vectors follow a spherical
distribution, with zero mean, unit variance, unit correlation matrix and whose type 
 is the type of the
copula of the physical random vector 
: in that case, 
 is the 1D cumulative  distribution
function with zero mean, unit variance and with type 
.
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