nrl sami2/3 ionosphere model at ccmcnrl sami2/3 ionosphere model at ccmc j. krall and j.d. huba...
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NRL SAMI2/3 IONOSPHERE MODEL ATCCMC
J. Krall and J.D. HubaPlasma Physics DivisionNaval Research LaboratoryWashington, DC
CCMC WorkshopJanuary 2012Key Largo, FL
Acknowledge: G. Joyce (deceased) and M. Swisdak
Research supported by ONR
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SAMI2 VERSION AT CCMCsami2-0.98
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SAMI2 AT CCMCsami2-0.98
Magnetic field: IGRF-like
Interhemispheric
Nonorthogonal, nonuniform fixed grid
Seven (7) ion species (all ions are equal):H+, He+, N+, O+, N+
2 , NO+, and O+2
Solve continuity and momentum for all 7 speciesSolve temperature for H+, He+, O+, and e−
Plasma motion
E×B drift perpendicular to BIon inertia included parallel to B
Neutral species: NRLMSISE00 and HWM93
Chemistry: 21 reactions + recombination
Photoionization: Daytime (EUVAC) and nighttime
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PLASMA DYNAMICSModeling the earth’s ionosphere
Ion Continuity∂ni
∂t+∇ · (niVi) = Pi − Lini
Ion Velocity
∂Vi
∂t+Vi · ∇Vi) = −
1
ρi∇Pi +
e
miE+
e
micVi ×B+ g
−νin(Vi −Vn −∑j
νij (Vi −Vj)
Ion Temperature
∂Ti
∂t+Vi · ∇Ti +
2
3Ti∇ ·Vi +
2
3
1
nik∇ ·Qi = Qin +Qij +Qie
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PLASMA DYNAMICSModeling the earth’s ionosphere
Electron Momentum
0 = −1
nemebs∂Pe
∂s−
e
meEs
Electron Temperature
∂Te
∂t−
2
3
1
nekb2s∂
∂sκe∂Te
∂s= Qen +Qei +Qphe
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MAGNETIC FIELDModeling the earth’s ionosphere
Low- to mid-latitude:closed field lines
Appropriate field: IGRF
Modeled as IGRF-like:a dipole field is fit to the IGRFfor the longitude of thesimulation (vary offset and tilt)
Important assumption:field lines are equipotentials
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EMPIRICAL MODELSInputs
NRLMSISE-00 (Picone et al)
Neutral composition H, He, O, N, N2, O2
Neutral temperature Tn
HWM (Hedin)
Neutral wind Vn (meridional/zonal)
Electric field (Fejer/Scherliess)
E ×B drift VE (vertical at magnetic equator)
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NONORTHOGONAL EULERIAN GRIDPresent grid: ‘1 zone’
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CCMC OUTPUTSElectron and ion densities
2D color contour plot
1D line plot(altitude/latitude)
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UPGRADE GRAPHICS AT CCMCAnimations
Example: ion dynamics as a function of time
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NEW UPGRADE AT CCMC: SAMI3Modeling the near-earth space environment
Global low- to mid-latitudeionosphere model
IGRF-like magnetic field
Zonal drifts
Parallelized with MPI:Requires Beowulf cluster
Nominal longitudinal resolution:2◦ − 4◦
Outputs: TEC, nmf2, hmf2
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GRAPHICS AT CCMCAnimations
Example: global/temporal change in TEC
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SAMI2 Te MODELComparison to Millstone Hill data (Swisdak et al., GRL, 2005)
Qphe based on simple modeldeveloped by Bailey (e.g.,SUPIM)
SAMI2 had an adjustableparameter ‘cqe’ that affectsQphe
Other comparisons to datasuggest another parameter beincluded, e.g., αQphe
Major upgrade by Varney- physics based photoelectronphysics model- computationally expensive
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IMPROVE SAMI2 Te MODELPhotoelectron heating term had to be modified: α = 0.2
Jicamarca data
SAMI2
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NEXT SAMI3 UPGRADE AT CCMC
global SAMI3 (±89◦ magnetic latitude)
electrostatic potential
self-consistent low-latitude dynamo potentialHWM07 to provide neutral windhigh-latitude potential: Weimer
ETA: late spring/early summer