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Electron Heating in 2D PIC Simulations of Quasi-Perpendicular Low-Beta Shocks
Authors
Lorenzo Sironi
Aaron Tran
Publication date
31 August 2023
Publisher
View
on
arXiv
Abstract
We measure the thermal electron energization in 1D and 2D particle-in-cell (PIC) simulations of quasi-perpendicular, low-beta (
Ξ²
p
=
0.25
\beta_p=0.25
Ξ²
p
β
=
0.25
) collisionless ion-electron shocks with mass ratio
m
i
/
m
e
=
200
m_i/m_e=200
m
i
β
/
m
e
β
=
200
, fast Mach number
M
m
s
=
1
\mathcal{M}_{ms}=1
M
m
s
β
=
1
-
4
4
4
, and upstream magnetic field angle
ΞΈ
B
n
=
55
\theta_{Bn} = 55
ΞΈ
B
n
β
=
55
-
8
5
β
85^\circ
8
5
β
from shock normal
n
^
\hat{\boldsymbol{n}}
n
^
. It is known that shock electron heating is described by an ambipolar,
B
\boldsymbol{B}
B
-parallel electric potential jump,
Ξ
Ο
β₯
\Delta\phi_\parallel
Ξ
Ο
β₯
β
, that scales roughly linearly with the electron temperature jump. Our simulations have
Ξ
Ο
β₯
/
(
0.5
m
i
u
s
h
2
)
βΌ
0.1
\Delta\phi_\parallel/(0.5 m_i {u_\mathrm{sh}}^2) \sim 0.1
Ξ
Ο
β₯
β
/
(
0.5
m
i
β
u
sh
β
2
)
βΌ
0.1
-
0.2
0.2
0.2
in units of the pre-shock ions' bulk kinetic energy, in agreement with prior measurements and simulations. Different ways to measure
Ο
β₯
\phi_\parallel
Ο
β₯
β
, including the use of de Hoffmann-Teller frame fields, agree to tens-of-percent accuracy. Neglecting off-diagonal electron pressure tensor terms can lead to a systematic underestimate of
Ο
β₯
\phi_\parallel
Ο
β₯
β
in our low-
Ξ²
p
\beta_p
Ξ²
p
β
shocks. We further focus on two
ΞΈ
B
n
=
6
5
β
\theta_{Bn}=65^\circ
ΞΈ
B
n
β
=
6
5
β
shocks: a
M
s
=
4
\mathcal{M}_s=4
M
s
β
=
4
(
M
A
=
1.8
\mathcal{M}_A=1.8
M
A
β
=
1.8
) case with a long,
30
d
i
30 d_i
30
d
i
β
precursor of whistler waves along
n
^
\hat{\boldsymbol{n}}
n
^
, and a
M
s
=
7
\mathcal{M}_s=7
M
s
β
=
7
(
M
A
=
3.2
\mathcal{M}_A=3.2
M
A
β
=
3.2
) case with a shorter,
5
d
i
5d_i
5
d
i
β
precursor of whistlers oblique to both
n
^
\hat{\boldsymbol{n}}
n
^
and
B
\boldsymbol{B}
B
;
d
i
d_i
d
i
β
is the ion skin depth. Within the precursors,
Ο
β₯
\phi_\parallel
Ο
β₯
β
has a secular rise towards the shock along multiple whistler wavelengths and also has localized spikes within magnetic troughs. In a 1D simulation of the
M
s
=
4
\mathcal{M}_s=4
M
s
β
=
4
,
ΞΈ
B
n
=
6
5
β
\theta_{Bn}=65^\circ
ΞΈ
B
n
β
=
6
5
β
case,
Ο
β₯
\phi_\parallel
Ο
β₯
β
shows a weak dependence on the electron plasma-to-cyclotron frequency ratio
Ο
p
e
/
Ξ©
c
e
\omega_{pe}/\Omega_{ce}
Ο
p
e
β
/
Ξ©
ce
β
, and
Ο
β₯
\phi_\parallel
Ο
β₯
β
decreases by a factor of 2 as
m
i
/
m
e
m_i/m_e
m
i
β
/
m
e
β
is raised to the true proton-electron value of 1836.Comment: 32 pages, 25 figures; submitted to Ap
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oai:arXiv.org:2308.16462
Last time updated on 10/09/2023