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ENLIL/2.8f-beta/ROR/Dan_Aksim_122319_SH_8

Run Description 

CCMC ROR run for ENLIL 2.8f-beta with RORID Dan_Aksim_122319_SH_8

Simulation Time:

Simulation Start Time: 2019-12-23T12:28:51Z
Simulation End Time: 2019-12-23T12:28:51Z
Time Step in second:
Simulation Time Description:
Simulation Time Caveats:

Temporal Dependence (whether the outputs of the simulation code are time-dependent?): true

Regions:

Heliosphere
Sun

Simulation Domain :

Contacts :

Dan.Aksim, ModelUser

List of Run Input Parameter Grouping and their associated properties :

Name Description Caveats Properties
Region and Grid Parameters 
Region and Grid Parameters
Name Description Caveats Units Default Value or Actual Value Valid Min Valid Max
reg 
Computational region
 AU 2 1 10
res 
Numerical grid resolution (options: low, med, high)
 res is related to nx (resolution factor), res=low set nx=1, res=med set nx=2, res=high set nx=4 medium
nblk 
Number of computational blocks
 1
x1l 
Inner boundary
 AU null
x1r 
Outer boundary
 AU 1.7 1 11
x2l 
Minimum co-latitude
 latitude grid settings: -60 to -60 degrees set x2l=30 x2r=150 n2=30 (default); -66 to 66 degrees set x2l=24 x2r=156 n2=33; -70 to 70 degrees set x2l=20 x2r=160 n2=35; -70 to 70 degrees set x2l=14 x2r=166 n2=38; degree 70
x2r 
Maximum co-latitude
 latitude grid settings: -60 to -60 degrees set x2l=30 x2r=150 n2=30 (default); -66 to 66 degrees set x2l=24 x2r=156 n2=33; -70 to 70 degrees set x2l=20 x2r=160 n2=35; -70 to 70 degrees set x2l=14 x2r=166 n2=38; degree 110
nx 
Grid resolution factor
 res is related to nx (resolution factor), res=low set nx=1, res=med set nx=2, res=high set nx=4 1
n1 
No. of basic X1-grid points
 n1, n2, n3 should not be changed via interface, we can change on our end. We must also change x1l,x1r,x2l,x2r,x3l,x3r in order to preserve the same grid resolution size (4 deg, 2 deg, 1 deg) in delta(theta) and delta(phi). 256
n2 
No. of basic X2-grid points
 n1, n2, n3 should not be changed via interface, we can change on our end. We must also change x1l,x1r,x2l,x2r,x3l,x3r in order to preserve the same grid resolution size (4 deg, 2 deg, 1 deg) in delta(theta) and delta(phi) 10
n3 
No. of basic X3-grid points
 n1, n2, n3 should not be changed via interface, we can change on our end. We must also change x1l,x1r,x2l,x2r,x3l,x3r in order to preserve the same grid resolution size (4 deg, 2 deg, 1 deg) in delta(theta) and delta(phi) null
numo 
Numerical model setting (options: mcp1umn1cd, mcp1van2cd)
 mcp1van2cd
x3l 
Minimum longitude
 deg 0 0
x3r 
Maximum longitude
 deg 360 360
CME parameters 
CME parameters
Name Description Caveats Units Default Value or Actual Value Valid Min Valid Max
cmefile 
Transient data file
 null
cld 
Hydrodynamic cloud conditions setting
 d4t1x1
ncmes 
Number of simulated CMEs; ncmes=-1 (use cmefile); ncmes>=1 (explicitly list); ncmes=0 (ambient run)
 0
vcldmin 
Minimum cloud velocity
 km/s 0 0
dcld 
Cloud density / fast stream density
 null 0.5 10
tcld 
Cloud temperature / fast stream temperature
 null
xcld 
Cloud trailing elongation over spherical shape
 null 0.5 10
radcav 
Cavity radius / cloud radius
 null 0 0.9
dcav 
Cavity density / fast stream density
 null 0.5 8
tcav 
Cavity temperature / fast stream temperature
 null 0.25 8
ncld 
Cloud geometric shape (1=piston,2=spheroid,3=sphere)
 2 1 3
Ambient wind conditions parameters 
Ambient wind conditions parameters
Name Description Caveats Units Default Value or Actual Value Valid Min Valid Max
cordata 
Coronal data subdirectory
 wsadu_all
corfile 
Coronal data file (custom or full rotation file)
 null
amb 
Ambient wind conditions setting (options: a4b1, a3b1, a3b2)
 a6b1
corobs 
Observatory name (options: gongb, gongz, mdi, mwo, nso)
 gongb
cr 
Carrington Rotation number
 null
obsdate 
Use observations of this date (yyyy-mm-ddThh)
 null
vfast 
Radial flow velocity of fast stream
 km/s null 200 700
vslow 
Radial flow velocity of slow stream
 km/s null
vrfast 
Reduction of the maximum flow velocity
 km/s null
vrslow 
Reduction of the minimum flow velocity (km/s)
 km/s null
bfast 
Radial magnetic field of fast stream
 nT null 0 350
dfast 
Number density at the inner boundary
 cm-3 null 125 1000
tfast 
Mean temperature at the inner boundary
 MK null 0.2 1.5
xalpha 
Fraction of alpha particles (rel. to protons)
 null
bndrot 
Rotation of the inner boundary (sidereal | synodic)
 null
runpar 
Gamma and heating parameters (options: g53q5, g15q0, g53q0)
 g53q5
bscl 
Magnetic field scaling factor
 default=2 except GONG default=4 null 1 6
Restart Parameters 
Restart Parameters
Name Description Caveats Units Default Value or Actual Value Valid Min Valid Max
resdate 
Restart computation from this date (null | yyyy-mm-ddThh)
 2011-01-01T00
resgrd 
Restart computation from this grid
 null
resbnd 
Restart computation from this boundary
 null
Simulation Time Parameters 
Simulation Time Parameters
Name Description Caveats Units Default Value or Actual Value Valid Min Valid Max
tstop 
Stop computation at this time
 vutime 8784
tstep 
3D output timestep
 vutime 12
vutime 
Time unit scale factor
 second null
tstart 
Start computation at this time
 For run setup, tstart is set for reg=1 (default=-240 hours). This is then multiplied by the actual region used to compute the final tstart. vutime null

Run Access Information :

Keyword(s) :

2012 amb (from restart)

Linked to Parent Spase Resource(s) (example: SimulationModel) :

spase://CCMC/SimulationModel/ENLIL/2.8f

List of Publications Referencing this Run :

  • Dan Aksim, Dmitry Pavlov, Improving the solar wind density model used in processing of spacecraft ranging observations, Monthly Notices of the Royal Astronomical Society, Volume 514, Issue 3, August 2022, Pages 3191–3201, https://doi.org/10.1093/mnras/stac1229
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