Early measurements taken in spring 2000 showed a time dependence of
the secondary electron yield from certain surfaces. In Figure 3.10
the remarkable decrease by a factor of 4 in the yield is shown for
a MgO coated sample over a period of 1/2 hour. The investigated sample
was a candidate for a stop surface in the NPD sensor on the Mars Express
mission of ESA. Further measurements revealed this behavior to be
quiet common. Figure 3.11 shows the
decay for an Al on MgF on Si start surface also for the
NPD sensor. Run (i) was the first set of measurements taken immediately
after the 80
C/20h bake-out of the chamber. As shown
the yield started at quite high values of 0.6 but decreased within
200 minutes of beam exposure to 0.15. This decay could be reproduced
by heating the surface again to the bake-out temperature for 20h.
Later it was discovered that exposing the surface to UV radiation
(from a Xenon lamp, with wavelengths down to 145nm) could `reset'
the surface to initial conditions. In Figure 3.11
runs (ii) to (iv) were performed after run (i) without additional
heating but after exposure to UV radiation. The decay in the secondary
electron yield was well reproduced in run (ii) to (iv) although the
initial value was only 0.3. The time constants for the decay depended
on the investigated surfaces and also on the primary energy. Figure
3.12 shows the yield obtained for graphite
stop surfaces coated with 150nm Al
O
, 150nm MgO,
or 150nm MgO on 150nm Al
O
, respectively. Materials
with a tungsten top layer behaved differently. Their secondary electron
yield did not change significantly with time. Figure 3.13
shows the measured yields for two start surface with a W top layer
on MgF
on a Si substrate. The yield was dependent on the
incidence angle (see Chapter 3.3.2)
and the incidence energy but not on time.
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March 2001 - Martin Wieser, Physikalisches Institut, University of Berne, Switzerland