Welcome to the new CCMC website!

Please note that some pages may have moved during the migration. If you experience any issues with the new website, please reach out to gsfc-ccmc-support@lists.hq.nasa.gov.

Last Updated: 05/26/2022

RAM-SCB

Version: v.2.x

The RAM‐SCB model includes two fully coupled modules: a kinetic ring current‐atmosphere interaction model (RAM) [Jordanova et al., 1994, 2006, 2010] self‐consistently coupled with a 3‐D equilibrium magnetic field (B) code [Zaharia et al., 2004, 2006, 2010]. It has been validated via a variety of spaceborne observations and geomagnetic indices [Yu et al., 2012]. The model determines the magnetic field configuration in three dimensions and the particle distribution functions Ql(R,ϕ,E,α) from bounce‐averaged Fokker‐Planck equations for both ring current ions and electrons in the equatorial plane: where Ql (l represents different species) is a function of radial distance R from 2 to 6.5 Re with spatial resolution of 0.25 Re, geomagnetic east longitude ϕ with resolution of 15°, energy E between 0.15 and 400 keV, and pitch angle α from 0 to 90°.

Inputs

Initial fluxes - usually taken from measurements at quiet times, such as from Van Allen Probes SCB's magnetic field boundary is usually taken from a magnetic field model or global MHD simulations

Outputs

ion and electron fluxes (0.15 - 400 keV) as a function of radial distance, local time, energy, pitch angle; also time dependent 3-D magnetic field configurations

Model is time-dependant.

Domains

  • Magnetosphere / Inner Magnetosphere / RingCurrent

Space Weather Impacts

  • Near-earth radiation and plasma environment (aerospace assets functionality)

Publications

Code

Code Languages: Fortran

Contacts

Publication Policy

In addition to any model-specific policy, please refer to the General Publication Policy.