Physics & Astronomy
accretion disks
72%
simulation
52%
magnetohydrodynamics
51%
turbulence
47%
hydrodynamics
43%
protoplanetary disks
39%
magnetic fields
38%
shock
33%
astrophysics
30%
radiation
27%
shearing
26%
angular momentum
26%
magnetohydrodynamic simulation
26%
Godunov method
21%
boxes
21%
gases
18%
magnetohydrodynamic turbulence
17%
planets
17%
ambipolar diffusion
14%
Taylor instability
14%
stars
14%
galaxies
13%
saturation
13%
dissipation
13%
molecular clouds
13%
cooling
12%
magnetic flux
11%
scale height
11%
gas pressure
10%
dust
10%
field strength
10%
barred galaxies
10%
stellar winds
10%
radii
9%
viscosity
9%
x rays
9%
active galactic nuclei
8%
protoplanets
8%
kinematics
8%
grids
8%
energy
7%
radiation pressure
7%
vortices
7%
interactions
7%
gravitation
7%
high resolution
6%
coronas
6%
Mach number
6%
collisionless plasmas
6%
bubbles
6%
torque
6%
filaments
6%
luminosity
6%
orbits
6%
fluids
6%
heating
6%
approximation
6%
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%
mesh
5%
acoustics
5%
integrators
5%
bows
5%
coalescing
5%
buoyancy
5%
ejecta
5%
opacity
5%
Earth & Environmental Sciences
accretion
100%
magnetohydrodynamics
93%
simulation
65%
magnetic field
63%
turbulence
47%
hydrodynamics
42%
angular momentum
40%
radiation
35%
gas
29%
code
26%
outflow
22%
planet
20%
dissipation
17%
energy
13%
saturation
13%
cooling
13%
rate
13%
effect
10%
luminosity
10%
plasma
10%
particle
10%
viscosity
9%
inflow
9%
dust
9%
merger
9%
vortex
8%
kinematics
8%
heating
8%
corona
8%
torque
7%
shell
7%
electrical resistivity
7%
planetesimal
7%
astrophysics
7%
geometry
7%
test
6%
temperature
6%
bubble
6%
method
6%
timescale
6%
young
6%
calculation
6%
cold
6%
speed
5%
gravity
5%
Kelvin-Helmholtz instability
5%
fluid
5%
coalescence
5%
outburst
5%
amplification
5%
buoyancy
5%
radio
5%
