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Cross-helicity conservation law
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Branch of physics
Fluid mechanics
Astrophysical fluid dynamics
Magnetohydrodynamics
Ideal magnetohydrodynamics
Cross-helicity
2026-09-28
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In
ideal magnetohydrodynamics
,
∂
t
h
c
+
∇
⋅
[
u
h
c
+
B
(
h
+
Φ
−
2
u
2
)
]
=
T
B
⋅
∇
s
.
(1)
The source vanishes in
a
homentropic flow
.
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(8)
Cross-helicity
Ideal magnetohydrodynamics
Magnetohydrodynamics
Astrophysical fluid dynamics
Fluid mechanics
Branch of physics
Physics
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(1)
Past exam of the mathematics course of the University of Cambridge
/
2022
/
iii
/
Paper 314
/
4
/
a
/
Solution
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