23 Titles Match Your Query 
Showing 1 through 23 of 23

1.
CORHEL (MAS/WSA/ENLIL) [CORHEL]
CORHEL is a software package that: (1) obtains and processes photospheric magnetograms; (2) runs the coronal model (either MAS or WSA); (3) processes the results to generate boundary conditions for ...

2.
SAMI2 LowtomidLatitude Ionosphere Model [SAMI3]
The SAMI2 model calculates the evolution of the low to midlatitude ionosphere. SAMI2 treats the dynamic plasma and chemical evolution of seven ion species (H+, He+, N+, O+, N2+, NO+, and O2+) in ...

3.
Solar Corona and Inner Heliosphere Model [SWMF]
The AlfvenWave driven SOlar wind Model (AWSOM) is part of the Space Weather Modeling Framework (SWMF). The SWMF has been developed by the Center for Space Environment Modeling (CSEM) team led by ...

4.
HOMER: Hybrid Optimization Modeling Software [HOMER]
The HOMER Hybrid Optimization Modeling Software is used for designing and analyzing hybrid power systems, which contain a mix of conventional generators, cogeneration, wind turbines, solar photovoltaics, ...

5.
CISM_DX  A data and model explorer [CISM_DX]
CISM_DX is a communitydeveloped suite of integrated data, models, and data and model explorers, for research and education. The data and model explorers are based on code written for OpenDX and Octave. ...

6.
Potential Field Source Surface Models [PFSS]
Potential Field Source Surface Models provide an approximate description of the solar coronal magnetic field based on observed photospheric fields (magnetograms). They were initially developed by ...

7.
International Geomagnetic Reference Field (IGRF) [IAGA_IGRF]
The International Geomagnetic Reference Field (IGRF) is a mathematical description of the Earth's main magnetic field used widely in studies of the Earth's deep interior, the crust and the ionosphere ...

8.
Gravity Profile Forward Modeling Tool [Talwani]
The Talwani software is a gravity profile forward modeling program based on the technique of Talwani et al. (1959) and Cady (1980). This version of the program runs on a PC using the Windows operating ...

9.
MHD Model of Solar Corona. Model [MAS]
This is a model of the solar corona.
Input at Photosphere:
Coronal base plasma temperature and density
Radial magnetic field Br from synoptic magnetogram (Kitt ...

10.
Solar Model [solarmodel]
The Solar Model is real time modeling of solar system. It allows user to navigate in space, to control time counting (speedup time flow) and estimate movement of space bodies, bind camera to space ...

11.
ABBY NORMAL Model [abbyNormal]
The ABsorption BY the D and E Region of HF Signals with NORMAL Incidence or
the ABBYNORMAL Model calculates the D and E region (60150 km) ionization
sources and ionneutral chemistry to obtain an ...

12.
BlockAdaptiveTreeSolarwindRoeUpwindScheme [BATSRUS]
BATSRUS, the BlockAdaptiveTreeSolarwindRoeUpwindScheme, was developed
by the Computational Magnetohydrodynamics (MHD) Group at the University of
Michigan, now Center for Space Environment ...

13.
Coupled Thermosphere/Ionosphere Plasmasphere (CTIP) Model [ION_THERMO_FULLER_ROLLELL]
The coupled thermosphereionosphereplasmasphere (CTIP) model consists of three
distinct components:
A global thermosphere model;
A high latitude ionosphere model;
A mid and lowlatitude ionosphere/plasmasphere ...

14.
ENLIL: TimeDependent 3D MHD Model of the Heliosphere [ENLIL]
ENLIL is a timedependent 3D MHD model of the heliosphere. It solves for plasma
mass, momentum and energy density, and magnetic field, using a
FluxCorrectedTransport (FCT) algorithm. Its inner radial ...

15.
Exospheric Solar Wind Model [Exospheric]
This is an exospheric model of the solar wind with only protons and electrons
(we defer the inclusion of heavy ions to upcoming versions of the code), with a
nonmonotonic total potential for the ...

16.
Heliospheric Tomography Model [HelTomo]
Heliospheric Tomography Model makes use of interplanetary scintillation (IPS)
to tomographically reconstract the global structure of the solar wind.
Model Input:
Remote sensing data of the solar ...

17.
Open Geospace General Circulation Model [MagUCLA_GGCM]
The Open Geospace General Circulation Model (Open GGCM) was originally
developed as a magnetohydrodynamic (MHD) model of Earth's magnetosphere at UCLA
in the early 1990's by J. Raeder. Besides solving ...

18.
University Partnering for Operational Support Radiation Belt UPOS RB Forecasting Model [UPOS]
Satellites in space are instrumental in providing surveillance, communication,
and navigation capability. Geomagnetic disturbances, which are related to
enhancements of MeV electron intensity at geostationary ...

19.
Utah State University Global Assimilation of Ionospheric
Measurements (USUGAIM) Model [GAIM]
Physicsbased data assimilation models of the ionosphere were developed at
Utah State University as part of a DoD Multidisciplinary University Research
Initiative (MURI) program. The USU effort ...

20.
Weimer Ionosphere Models [ION_WEIMER]
Weimer models are statistical electric potential models for the highlatitude
ionosphere, developed by Daniel Weimer of Mission Research Corporation. Past
satellite measurements of ionospheric electric ...

21.
Fok Ring Current Model (FRC) [RADIATION_BELT]
The Fok Ring Current Model (FRC) is a bounceaveraged kinetic model of the ring
current. This model calculates the temporal and spatial variation of the phase
space density of ring current species, ...

22.
Solar and Heliospheric Forecasts [SolarHelio_Weather_Model]
The forecast of solar and heliospheric information is based on assimilation (by
direct insertion) of SOHO/MDI observations or, if not available, NSO/KPVT
observations (weather permitting) within 52 ...

23.
World Magnetic Model [WMM]
The World Magnetic Model is the standard model of the US Department of Defense,
the UK Ministry of Defence, the North Atlantic Treaty Organization (NATO), and
the World Hydrographic Office (WHO) navigation ...

Showing 1 through 23 of 23
