Fig. 3

Integrand function in Eq. (3) for an
O atom on the orbit whose perihelion is at the location of the Earth at the time
corresponding to IBEX Orbit 16 in 2009 (λE = 130°). The
red line is the
from Eq. (1), taken along the orbit
of the atom. The model used in
is
time dependent and has a component of electron impact rate, which does not follow
the 1/r2 dependence. The dark-blue
line is the integrand function calculated for
, i.e., assuming
that the ionization rate is equal to the ionization rate from our model calculated
for the instant of detection t0. The history of the
radial distance of the atom from the Sun is shown in the lower right inset and is
identical for the red and dark-blue lines. The upper-left inset presents the ratio
of the actual ionization rate for atoms following this trajectory and the rate used
in the analytical model
. To obtain
the survival probability, one must calculate the exponent of the time integral of
the function drawn in red, see Eqs. (2) and (3). The analytic
approximation is equivalent to taking the exponent of the integral of the function
drawn with the blue line, i.e., to evaluating the exponent of the expression from
Eqs. (2) and (4).
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