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Compound List

Here are the classes, structs, unions and interfaces with brief descriptions:

• AlbedoPSpectrum (Calculate the earth albedo proton spectrum in low earth orbit. Uses data produced by AMS detector, preliminary graphs from web page. No angular or geographic dependence included)
• AlbedoSpectrum (Simulate the Earth albedo neutron and photon spectra. Choose origins uniformly in a plane, and isotropic angles)
• CHIMEAvg (No description available)
• CHIMEMax (No description available)
• CHIMEMin (No description available)
• CHIMESpectrum (Calculate the cosmic ray proton spectrum in low earth orbit. Uses data produced by CHIME, assuming 600 km circular orbit at solar minimum (worst case))
• CompositeSource (Holds multiple Eventsource objects ; acts as a container for them)
• GPS::Coords (No description available)
• CrElectron (The class that calls each cosmic-ray electron components based on their flux)
• CrElectronPrimary (The primary cosmic-ray electron spectrum (and incident angle) source)
• CrElectronReentrant (No description available)
• CrElectronSplash (No description available)
• CrProton (No description available)
• CrProtonPrimary (CrProtonPrimary: The primary cosmic-ray electron spectrum (and incident angle) source)
• CrProtonReentrant (CrProtonReentrant: The reentrant cosmic-ray electron spectrum (and incident angle) source)
• CrProtonSplash (CrProtonSplash: The splash cosmic-ray electron spectrum (and incident angle) source)
• CrSpectrum (No description available)
• EventSource (Interface to the EventSource class. Provides a generic interface to what Glastsim uses as a data source. This can constitute GISMO based event generation, reading in from a file, etc..)
• ExtraGalacticDiffuse (No description available)
• FILESpectrum (Spectrum that reads its differential spectrum from a table)
• FluxMgr (The point of entry for interfacing with the flux package)
• FluxSource (FluxSource: class which manages to compute flux from various particle source configurations)
• GalElSpectrum (A quick and dirty implementation of the high-energy (galactic) cosmic ray spectrum)
• GPS (Represents the Global Positioning System on-board the spacecraft. An Orbit)
• HeSpectrum (Calculate the cosmic ray 4He spectrum in low earth orbit. Uses data produced by CHIME, assuming 600 km circular orbit at solar minimum (worst case). Patrick Nolan, Stanford University, 1998)
• HeSpectrum::InterpVec (A vector with methods added to do searches and linear interpolation)
• CHIMESpectrum::InterpVec (A vector with methods added to do searches and linear interpolation)
• ISpectrumFactory (This is an abstract base class for the SpectrumFactory template classes)
• std::map (No description available)
• Orbit (Calculates the position of a satellite in a low, circular orbit. The path is assumed to go to the east, with the rotation of the earth, as is the case for most satellite orbits. All angles are expressed in degrees. Longitude increases to the east)
• ProtonSpectrum (This is the cosmic ray proton spectrum appropriate for low inclination Earth orbit)
• rootAngleHist (This class stores the the flux vs. incident angle information for creating a graph)
• rootEnergyHist (This class stores and graphs the flux vs. energy)
• rootHist (This class serves as an array that checks for invalid indexing)
• SimpleSpectrum (A convenient Spectrum : a single particle at a particular energy, or a power-law spectrum)
• Spectrum (Class for holding function definitions of Spectrums - i.e. HeSpectrum, SimpleSpectrum, etc... Basically an abstract base class for these classes)
• SpectrumFactory (Template class designed to hold method by which to polymorphically instantiate new Spectrum objects)
• SpectrumFactoryTable (Singleton table holding references to all the spectrum classes. serves to instantiate new classes based on a name)
• StaticOrbit (Child-class of the Orbit class which defines a static - specifiable orbit designed for situations in which the orbit is specified by some external data source)
• tbl (No description available)
• TrappedProtonSpectrum (Purpose: Simulate the flux and spectrum of protons trapped in the earth's magnetic field. Implemented only for a 600 km circular orbit, so only the South Atlantic Anomaly (SAA) is seen)
• HeSpectrum::std::vector (No description available)
• CHIMESpectrum::std::vector (No description available)

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