Digital Signal Processing Reference
In-Depth Information
diagonal
˙
n
. This is recognized as a “rank-1 factor analysis” model in multivariate
˙
n
in several ways
on
g
and is rank 1. This allows direct estimation of
g
. This property is related to
the gain and phase closure relations often used in the radio astronomy literature for
calibration (in particular, these relations express that the determinant of any 2
2
submatrix away from the main diagonal will be zero, which is the same as saying
that this submatrix is rank 1).
In general, there are more calibrator sources (
Q
) in the field of view, and we have
×
would be
known, then we can correct
R
for it, so that we have precisely the same problem as
˙
and
˙
n
using the techniques
˙
known, we can say we know a reference
A
H
, and the problem is to identify the element gains
model
R
0
=
A
˙
=
diag
(
g
)
from a model of the form
H
R
=
R
0
+ ˙
n
or, after applying the vec
(
·
)
-operation,
vec
(
R
)=
diag
(
vec
(
R
0
))(
g
⊗
g
)+
vec
(˙
n
)
.
This leads to the Least Squares problem
R
2
g
=
arg mi
g
vec
(
−
˙
n
)
−
diag
(
vec
(
R
0
))(
g
⊗
g
)
.
This problem cannot be solved in
c
losed form. Alternatively, we can first solve an
unstructured problem: define
x
=
g
⊗
g
and solve
R
0
))
−
1
vec
R
x
=
diag
(
vec
(
(
−
˙
n
)
gg
H
,
or equivalently, if we define
X
=
X
R
=(
−
˙
n
)
R
0
.
where
denotes an entrywise matrix division. After estimating the unstructured
X
, we enforce the rank-1 structure
X
gg
H
, via a rank-1 approximation, and find
an estimate for
g
. The pointwise division can lead to noise enhancement; this is
remediated by only using the result as an initial estimate for a Gauss-Newton
With
g
known, we can again estimate
=
n
, and make an iteration. Overall
we then obtain an alternating least squares solution. A more optimal solution can
asymptotically unbiased and statistically efficient solution.
˙
and
˙