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Interplanetary shocks generated by expanding magnetic loops
T. V. Stepanova,
A. G. Kosovichev
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peer-review
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Engineering & Materials Science
Shock waves
79%
Electrons
47%
Piles
44%
Plasmas
43%
Ions
43%
Ion exchange
32%
Heat conduction
24%
Navier Stokes equations
23%
Relaxation
21%
Turbulence
21%
Magnetic fields
20%
Numerical models
19%
Viscosity
19%
Heating
16%
Fluids
15%
Earth & Environmental Sciences
shock wave
83%
plasma
36%
electron
32%
ion
29%
coronal mass ejection
28%
Navier-Stokes equations
24%
ion exchange
21%
magnetic field
20%
perturbation
18%
viscosity
18%
turbulence
18%
heating
16%
cold
16%
fluid
13%
loss
12%
energy
11%
material
9%
parameter
8%
Physics & Astronomy
interplanetary shock waves
100%
heliosphere
43%
shock
36%
shock waves
30%
magnetohydrostatics
19%
magnetic clouds
17%
ions
16%
coronal mass ejection
14%
conductive heat transfer
11%
Navier-Stokes equation
11%
field strength
10%
electrons
9%
energy transfer
9%
turbulence
8%
viscosity
8%
perturbation
7%
heating
7%
fluids
6%
coefficients
6%
magnetic fields
5%