CMR Header

CCMC Metadata Registry (CMR)

Menu Page

Go to:

CMR: View Simulation Run Info

CIMI/20200203/ROR/Mitchell_Indek_032524_IM_2

Run Description

CCMC ROR run for CIMI 20200203 with RORID Mitchell_Indek_032524_IM_2

Simulation Time:

Simulation Start Time: 2015-10-07T15:00:00Z
Simulation End Time: 2015-10-07T23:00:00Z
Time Step in second: 900
Simulation Time Description:
Simulation Time Caveats:

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

Regions:

Earth.Magnetosphere.RadiationBelt
Earth.NearSurface.Plasmasphere

Simulation Domain :

Contacts :

Mitchell.Indek, ModelUser

List of Run Input Parameter Grouping and their associated properties :

Name Description Caveats Properties
Settings for the model
Settings used to run the model
Name Description Caveats Units Default Value or Actual Value Valid Min Valid Max
with_plasmasphere
Flag indicating whether to conduct the run with (1) or without (0) Plasmasphere
1
magnetic_field_model
Specifies a magnetic field model to be used for the run
TS04
KP_type
Type of Kp data (definite or provisional or realtime or user-uploaded)
provisional
type_of_F107_data
Type of F10.7 data (Kp_3h or corrected_fluxdata)
NOAA/Kp_3h
despike_solar_wind_data
Flag indicating whether to automatically de-spike solar wind (optional for automatically retrieved data only; use when solar wind data shown in next page have clusters of extreme values in plasma density, temperature or velocity).
False
despike.threshold
De-spike threshold (standard deviations)
sigmas 3 2 4
despike.number_of_samples
De-spike length (number of samples in cluster of extreme values to be eliminated)
7 3 9
b_abs
Magnitude of IMF
10.4
b_angle
IMF clock angle
150.5
ionosphere_electric_field_model
Specifies a High-Latitude Ionosphere Electric Field Model to be used for the run
Weimer-2000
sw_link
Solar wind link
plot
SW_density_floor_was_applied
Flag indicating the solar wind density has been floored with SW_density_floor value to ensure that the model will run through the requested time interval.
False
minimum_SW_Fast-Mode_mach_number
Minimum solar wind Fast-Mode mach number
4.02
SW_parameters_are_large
Flag indicating whether solar wind velocity, density or dynamic pressure are large. If they are, the run is a special request requiring attention by CCMC staff. The variables will be accepted unless they exceed certain absolute maximum values.
SW_plot
Name of solar wind plot
Mitchell_Indek_032524_IM_2_sw.gif
dipole_tilt
Dipole tilt
deg 3.63435
dipole_tilt_y
Y component of dipole tilt
deg -26.8154
with_UB_chorus_diffusion
Specifies whether to use (1) or not use (0) Upper-Band Chorus in Wave loss mechanisms (electrons only)
0
with_LB_chorus_diffusion
Specifies whether to use (1) or not use (0) Lower-Band Chorus in Wave loss mechanisms (electrons only)
1
with_hiss_diffusion
Specifies whether to use No Hiss Diffusion(0) or UCLA Hiss Diffusion (2) in Wave loss mechanisms (electrons only)
0
Dst_start
Starting value of Dst in supplied Dst index file
-74
Dst_min
Minimum value of Dst in supplied Dst index file
-124
Dst_max
Maximum value of Dst in supplied Dst index file
-74
Kp_start
Starting value of Kp in supplied Kp index file
6.33
Kp_min
Minimum value of Kp in supplied Kp index file
6
Kp_max
Maximum value of Kp in supplied Kp index file
7.33
AE_start
Starting value of AE in supplied AE index file
714.00
AE_min
Minimum value of AE in supplied AE index file
283.00
AE_max
Maximum value of AE in supplied AE index file
1839.00
AU_start
Starting value of AU in supplied AU index file
193.00
AU_min
Minimum value of AU in supplied AU index file
1.00
AU_max
Maximum value of AU in supplied AU index file
561.00
AL_start
Starting value of AL in supplied AL index file
521.00
AL_min
Minimum value of AL in supplied AL index file
172.00
AL_max
Maximum value of AL in supplied AL index file
1768.00
AO_start
Starting value of AO in supplied AO index file
164.00
AO_min
Minimum value of AO in supplied AO index file
1.00
AO_max
Maximum value of AO in supplied AO index file
897.00
dipole_time
Dipole time
2015/10/07 15:00
Solar wind inputs
Time-dependent solar wind plasma and magnetic field inputs.
Solar wind inputs are derived from a single spacecraft usually 200 R_E upstream of the sun-ward (front) simulation box boundary.
Name Description Caveats Units Default Value or Actual Value Valid Min Valid Max
solarwind
Flag indicating whether solar wind data are constant (initial values) or variable (var).
var const var
sw_source
Name of the spacecraft or data source used to generate solar wind input information. Currently one of ACE-RT ACE-L2, WIND, OMNI, DSCOVR (real time)
User-submitted data may be from any source or made-up. OMNI-1min
constant-Bx
Constant Bx value fed into the front boundary of the simulation.
nT -13.5
Bx
Sun-Earth component of solar wind magnetic field.
Bx is usually held constant (zero or average of observed values) to conserve div.B at the front boundary. Alternatively, oblique phase fronts can be assumed that update solar wind conditions along those fronts throughout the front boundary. Bx is then approximated as a linear combination of time dependent By and Bz. nT -13.5 -100 100
By
Dawn-dusk component of solar wind magnetic field.
nT 5.12 -100 100
Bz
North-south component of the solar wind magnetic field. B_z is most important magnetic field component to drive or inhibit geomagnetic activity. Other components play a role in connection with the orientation of the Earth's dipole field.
nT -9.05 -100 100
Vx
Sun-Earth component of solar wind velocity.
Low solar wind speed (less than 200 km/s in magnitude) usually indicates poor statistics in the solar wind plasma measurements. km/s -450.4 -3000 -200
Vy
Plasma velocity in dawn-dusk direction.
The orbital velocity of Earth (about 29 km/s) is usually neglected. km/s 10.177 -500 500
Vz
Solar wind plasma velocity in north-south direction.
km/s 32.754 -500 500
N
Solar wind plasma density.
Mass density described in terms of number of protons per cubic centimeter. AMU/cm^3 3.21 0.1 100
T
Solar wind plasma temperature.
Derived from observed distribution of solar wind particles. Can fluctuate widely when density N is at or below 1 AMU/cm^3. K 118266 10000 2000000
SW density floor
Lowest value of N applied during pre-processing of solar wind input data.
The density floor in the solar wind varies by magnetosphere model and it's numerical stability. A similar floor may be imposed inside the magnetotail lobes where the density may drop lower than in the solar wind. AMU/cm^3 0.01 0.1 2.5
Ionosphere conductance model
Name Description Caveats Units Default Value or Actual Value Valid Min Valid Max
iono_conductance
Parameter indicationg selection of conductance model in the ionosphere electrodynamics component of the model.
The two models offered for run-on-request are constant (user sets Pedersen Conductance and Hall Conductance) and auroral (conducances driven by f10.7 and field-aligned currents from magnetosphere part of the model). auroral constant auroral
f10.7
Solar irradiation index as represented by the flux of 10.7 cm (2800 MHz) radiation from the Sun measured in units of 10−22 W⋅m−2⋅Hz−1.
Daily index of solar radiation that affects the daytime background conductivity in the ionosphere. sfu 80.40 50 300
Magnetosphere model parameters
Name Description Caveats Units Default Value or Actual Value Valid Min Valid Max
inflow boundary
Location of sun-ward facing (front) boundary of the magnetosphere simulation box.
R_E 10 24 128

Run Access Information :

Keyword(s) :

CIR

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

spase://CCMC/SimulationModel/CIMI/20200203

List of Publications Referencing this Run :

CMR Footer

Curator: Chiu Wiegand | NASA Official: Dr. Masha Kuznetsova | Privacy and Security Notices | Accessibility | CCMC Data Collection Consent Agreement