Efficient kinetic simulations in the Z inner MITL
POSTER
Abstract
The Z inner magnetically insulated transmission line (MITL)
is subjected to extreme fields, of the order of 100s of Tesla
and 100s of MV/m. Kinetic simulations, preferred in MITL numerical design,
can be very computationally expensive. The challenge comes from
two main constraints on the time step, the small Larmor period of electrons
and the Courant condition. To lift these restrictions, we utilize the
operational parameters on Z, namely, the time scale of the current pulse
on Z (~100ns) and the dimensions of the inner MITL (~10cm).
For such parameters, one could use an electrostatic and magnetostatic
fields model to remove the Courant limit. In the strong magnetic fields, we show
that a drift kinetic guiding center model for electrons can be used
as an approximation, removing the need to resolve the Larmor period.
As a test problem we model space charge limited emission (SCL) from the
cathode due to field stress. We show that typically observed vortex
formation and evolution can be well reproduced by using only drift kinetic
particles. We also discuss the possibility of a hybrid full kinetic and
drift kinetic approach.
is subjected to extreme fields, of the order of 100s of Tesla
and 100s of MV/m. Kinetic simulations, preferred in MITL numerical design,
can be very computationally expensive. The challenge comes from
two main constraints on the time step, the small Larmor period of electrons
and the Courant condition. To lift these restrictions, we utilize the
operational parameters on Z, namely, the time scale of the current pulse
on Z (~100ns) and the dimensions of the inner MITL (~10cm).
For such parameters, one could use an electrostatic and magnetostatic
fields model to remove the Courant limit. In the strong magnetic fields, we show
that a drift kinetic guiding center model for electrons can be used
as an approximation, removing the need to resolve the Larmor period.
As a test problem we model space charge limited emission (SCL) from the
cathode due to field stress. We show that typically observed vortex
formation and evolution can be well reproduced by using only drift kinetic
particles. We also discuss the possibility of a hybrid full kinetic and
drift kinetic approach.
Presenters
-
Evstati G Evstatiev
Sandia National Laboratories
Authors
-
Evstati G Evstatiev
Sandia National Laboratories
-
Mark H Hess
Sandia National Laboratories