Multipactor in Low Pressure Gas and in ... - of Richard Udiljak
Multipactor in Low Pressure Gas and in ... - of Richard Udiljak
Multipactor in Low Pressure Gas and in ... - of Richard Udiljak
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are assumed to have a Maxwellian distribution, i.e.<br />
f(vx,vy,vz) ∝ vn<br />
v exp<br />
�<br />
− 1 v<br />
( )<br />
2 vT<br />
2<br />
�<br />
(5.21)<br />
where v is the absolute value <strong>of</strong> the <strong>in</strong>itial velocity, vn its normal component<br />
with respect to the surface <strong>of</strong> emission, <strong>and</strong> vT is the thermal<br />
<strong>in</strong>itial velocity spread. Another <strong>of</strong> the used parameters related to this<br />
is the normalised spread <strong>of</strong> <strong>in</strong>itial electron velocity def<strong>in</strong>ed as vT/vmax,<br />
where vmax is the impact velocity for maximum SEY.<br />
Calculations were performed for 2-D arrays <strong>of</strong> different sets <strong>of</strong> the<br />
normalised parameters (e.g. ρ = Vω/vmax vs. λ with the other parameters<br />
fixed) <strong>and</strong> each run corresponds to one particular po<strong>in</strong>t <strong>in</strong> one <strong>of</strong><br />
these arrays. Each run was primed with 200 seed electrons, uniformly<br />
distributed over <strong>in</strong>itial phase, <strong>and</strong> the run was term<strong>in</strong>ated when either<br />
the number <strong>of</strong> particles exceeded 4500 or when 200 RF-periods had<br />
elapsed. The run was also term<strong>in</strong>ated <strong>in</strong> case the number <strong>of</strong> electrons<br />
dropped below 10 before 200 RF-cycles had passed. At the end <strong>of</strong> each<br />
run, the follow<strong>in</strong>g parameters were recorded:<br />
• Number <strong>of</strong> RF-periods needed to exceed 4500 particles. If 4500<br />
particles were not atta<strong>in</strong>ed with<strong>in</strong> 200 RF-cycles, this parameter<br />
was set to 200.<br />
• Number <strong>of</strong> electrons at the end <strong>of</strong> each run.<br />
• Heat<strong>in</strong>g asymmetry, i.e. the ratio between the average power deposited<br />
on the <strong>in</strong>ner conductor <strong>and</strong> the average power deposited<br />
on the outer conductor.<br />
• Average electron growth rate (over the 10 last RF-periods), normalised<br />
with respect to the RF-period.<br />
5.2.2 Simulations<br />
To facilitate comparison between the theoretical result presented <strong>in</strong><br />
Fig. 5.7 a simulation was made <strong>in</strong> the same parameter space. Figure 5.8<br />
shows the number <strong>of</strong> electrons obta<strong>in</strong>ed after 200 RF-cycles. As expected,<br />
the lower order resonances (i.e. at lower <strong>and</strong> leftmost G-values)<br />
<strong>in</strong>dicate high electron numbers, s<strong>in</strong>ce more impacts with the conductors<br />
will occur dur<strong>in</strong>g the same number <strong>of</strong> RF-periods. Due to this fact, a<br />
parameter space was chosen, which did not <strong>in</strong>clude any po<strong>in</strong>ts <strong>in</strong> the<br />
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