Physics & Astronomy
accretion disks
68%
magnetohydrodynamics
51%
simulation
50%
turbulence
44%
hydrodynamics
41%
protoplanetary disks
36%
magnetic fields
36%
shock
31%
astrophysics
29%
radiation
27%
magnetohydrodynamic simulation
26%
angular momentum
25%
shearing
25%
Godunov method
20%
boxes
19%
gases
18%
magnetohydrodynamic turbulence
16%
planets
16%
ambipolar diffusion
13%
stars
13%
Taylor instability
13%
galaxies
13%
saturation
12%
dissipation
12%
molecular clouds
12%
cooling
11%
magnetic flux
10%
scale height
10%
stellar winds
10%
gas pressure
10%
dust
10%
field strength
9%
radii
9%
barred galaxies
9%
viscosity
8%
x rays
8%
grids
8%
active galactic nuclei
8%
gravitation
8%
protoplanets
7%
kinematics
7%
energy
7%
radiation pressure
7%
interactions
6%
vortices
6%
high resolution
6%
luminosity
6%
coronas
6%
Mach number
6%
collisionless plasmas
6%
bubbles
6%
torque
6%
heating
6%
filaments
5%
orbits
5%
fluids
5%
approximation
5%
mesh
5%
Reynolds stress
5%
signatures
5%
geometry
5%
divergence
5%
radiative transfer
5%
shear
5%
orbitals
5%
gas dynamics
5%
conduction
5%
electrical resistivity
5%
kinetics
5%
Earth & Environmental Sciences
accretion
100%
magnetohydrodynamics
93%
simulation
64%
magnetic field
60%
turbulence
44%
hydrodynamics
40%
angular momentum
38%
radiation
36%
gas
29%
code
25%
outflow
21%
planet
19%
dissipation
16%
rate
13%
energy
12%
saturation
12%
cooling
12%
luminosity
10%
effect
10%
plasma
9%
particle
9%
inflow
9%
viscosity
9%
dust
9%
merger
8%
vortex
8%
heating
7%
kinematics
7%
corona
7%
torque
7%
shell
7%
electrical resistivity
7%
test
7%
gravity
6%
planetesimal
6%
astrophysics
6%
geometry
6%
timescale
6%
method
6%
cold
6%
temperature
6%
calculation
6%
bubble
6%
young
5%
speed
5%
gas flow
5%
Kelvin-Helmholtz instability
5%
fluid
5%
coalescence
5%
outburst
5%
amplification
5%
