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7.3 Accuracy in the Measurement of the Coordinate 261
proportional to
σ
2
(cf. (7.81)) hides the complications in the symbol N
. Although it
is true that in the limiting cases of (7.17) and (7.18) N
is exactly equal to N, the total
number of electrons on the track segment delimited by the cell width, N
changes
as a function of
θ
,
σ
and b so as to make the variance
σ
2
X
AV
larger. The physical
cause of this is the rare larger clusters outside the cell that send some electrons via
diffusion to the edge of the cell, and more so when
θ
is large. We have two reasons
not to go into these details here. When we omit the primes in (7.19) the omissions
amount to less than 25% in the quantity
σ
X
AV
(except in extreme cases). The omitted
parts, which pull measurements to one side in our cell, have a tendency to pull the
corresponding measurement in the neighbouring cell to the opposite side. Therefore
it is better to leave them out when combining several cells. The contributions of
several wires are discussed in Sects. 7.3 and 7.4.
In conclusion we simplify (7.19) to read
σ
2
X
AV
=
1
N
σ
2
cos
2
θ
+
1
N
eff
b
2
12
tan
2
θ
. (7.22)
It represents the square of the accuracy with which a track coordinate X
AV
(7.10)
can be measured along a single wire in the absence of a magnetic field.
7.3 Accuracy in the Measurement of the Coordinate
in or near the Wire Direction
7.3.1 Inclusion of a Magnetic Field Perpendicular to the Wire
Direction: the Wire E ×
×
× B Effect
Drift chambers with precise measurements of the track coordinates along the wire
direction are often operated with a magnetic field perpendicular to the direction of
the wires. With this configuration one can obtain a precise determination of the cur-
vature induced on the particle trajectory by the magnetic field, and the momentum
of the particle can be determined (see Chap. 8 for details).
The presence of a magnetic field perpendicular to the wire direction modifies the
angular wire term of the variance of the arrival position of the electrons (7.5). It
becomes asymmetric and, on average, larger because the track segment is projected
onto the wire in a more complicated way. The electrons that after their drift are
collected in the cylindrical field of the wire have to move transverse to the magnetic
field (Fig. 7.4). This produces an E ×B force according to (2.6) and causes the
electrons to drift under an effective angle
ψ
toward the wire. The angle
ψ
is such
that tan
ψ
=
ωτ
, where
ω
is the cyclotron frequency and
τ
is the time between two
electron collisions suitably averaged. Details have been treated in Sect. 2.1.
The arrival position x
w
of an electron entering the region close to the wire
with coordinates x and y is x
w
= x −ytan
ψ
; the variance of x
w
on the frequency
distribution (7.3) is