CMR Header

CCMC Metadata Registry (CMR)

Menu Page

Go to:

 CMR: View Simulation Run Info

WSA/v.5.2/ROR/TEMPLATE

Run Description 

SimulationRun Metadata Template for WSA v.5.2 ROR runs

Simulation Time:

Simulation Start Time:
Simulation End Time:
Time Step in second:
Simulation Time Description:
Simulation Time Caveats:

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

Regions:

Heliosphere.Inner
Sun.Corona

Simulation Domain :

Contacts :

List of Run Input Parameter Grouping and their associated properties :

Name Description Caveats Properties
All user settings for WSA model 
All user input settings for WSA model
Name Label Description Caveats Units Default Value or Actual Value Valid Min Valid Max
OBSER OBSER 
Magnetogram source: 
The model can accept photospheric magnetograms from a range of sources. These includes 'synodic' or 'synoptic' maps from the originating observatories
(gong_z, gong_b, vsm, kpvt) and ensembles containing 12 realizations from map sequences processed through the ADAPT surface flux
evolution model (agong, ahmi, avsm, akpvt).
 gong_z
infile infile 
Input magnetogram file
 Date/CR_LONG/Magnetogram selection order of priority: If infile has a valid magnetogram file name use that, otherwise if specific_date is a valid date use the magnetogram closest to but before that date. Otherwise if CR and LONGIT are valid use these to find the appropriate magnetogram, otherwise if run_type='realtime' use the latest daily magnetogram. null
CARROT CARROT 
Carrington Rotation Number
 The data from the different sources covers different time ranges. Note some maps have know bad data issues and the ADAPT maps have not yet been backfilled to cover the full possible time ranges. kpvt : 1992/05/23 to 2003/07/27 vsm : 2003/07/28 to present gong_z : 2006/09/19 to present : CR_LONGIT 2048_323 to now. gong_b : 2006/09/19 to present : CR_LONGIT 2048_323 to now. agong : 2006/09/19 to present : CR_LONGIT 2048_323 to now. akpvt : 1992/05/23 to 2003/07/27 avsm : 2003/07/28 to present ahmi :
CARRLONG CARRLONG 
Carrington Longitude
 Should be a 3 digit integer string between 000 and 359, ie 054 or 198 or 002. 000 359
MAPTYPE MAPTYPE 
Magnetogram Type
MAPTYPE accepts 2 possible settings, ‘DU’ and ‘FR’. The default will be ‘DU’, which will be used for almost all runs DU
specific_date specific_date 
specific_date to find and use the magnetogram closest to but before that date
 Must be in format YYYYMMDDtHHMM (example: 20140212t1539) -1
run_type run_type 
run_type is set to null or 'realtime'
 run_type='realtime' use the latest daily magnetogram if infile, specific_date, and cr are not set null
object object 
Object at which to generate solution timelines and foorecasts
 List of objects includes: earth, mercury, venus, mars, stereoa, stereob, PSP, Solar Orbiter earth
RADOUT RADOUT 
Outer boundary of current sheet component
 If the model run is intended to generate a coronal field solution for use in an ENLIL model run, this must be set to 21.5 Solar radii. 5 5 21.5
GRID GRID 
resolution: 1.0 deg or 2.0deg
 2.0deg
enlil_flag enlil_flag 
To produce ENLIL input file, VEL*.fitz: 0 (false) or 1 (true)
 1
wsa_tracing wsa_tracing 
Generate and save fieldlines through objects: 0 (off) or 1 (on)
 0
wsa_bcube wsa_bcube 
Generate a datafile storing the field solutions for the coronal source surface part (ie out to 2.5 solar radii): 0 (off) or 1 (on)
 0
RADINT RADINT 
Interface radius (Rs)
 2.49
RADSS RADSS 
Source Surface radius (Rs)
 2.51
SPHHAR SPHHAR 
Number of spherical harmonics
 90
VELEQN VELEQN 
Velocity Equation
 285.0+625.0/((1.0math.exp(-(arc_ft_bd/2.0)**2.0))**3.0
MAPNAME MAPNAME 
MAPNAME
MAPDATE MAPDATE 
UT Date of this map (i.e. of last contributor)
MAPTIME MAPTIME 
UT Time of this map (i.e. of last contributor)
PROVERS PROVERS 
WSA version number
 WSA_V5.2
Output files 
Output files from the model run
Name Label Description Caveats Units Default Value or Actual Value Valid Min Valid Max
syn_filename syn_filename 
intermediate output file generated by the model run
int_filename int_filename 
intermediate output file generated by the model run
wsa_filename wsa_filename 
intermediate output file generated by the model run
vel_filename vel_filename 
intermediate output file generated by the model run

Run Access Information :

Keyword(s) :

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

spase://CCMC/SimulationModel/WSA/v.5.2

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