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All Tables

- Table 1:
Observationally inferred pulsar data. Note that in
Esamdin et al. (2005) no value for
is quoted. Also, we infer
*P*_{3} from their values of *P*_{2} and using the relation for the
drift rate
,
which is a
good approximation for this system, as it is nearly aligned.
Positive and negative values are obtained due to the definition of
drift rate.
- Table 2:
The results of
*Q* and
for possible beam
configurations for PSR B0943+10 by assuming *l* = 20 and
.
The charge density
difference is found to be
.
Initial guess for
*R*_{1}/*R*_{3} and *R*_{2}/*R*_{3} is taken from Fig. 10 in DR01.