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PHaRLAP (4.7)Provision of High-frequency Raytracing LAboratory for Propagation studiesModel DescriptionPHaRLAP is a MATLAB toolbox for the study and modelling of the propagation of High Frequency (HF) radio waves in the Earth's ionosphere. It provides 2D and fully magneto-ionic 3D numerical ray tracing (NRT) engines, analytical ray tracing (ART) routines and the necessary supporting routines. Model Figure(s) :Model Inputs DescriptionUT date and time, frequency, elevation, and azimuth angles of the wave’s starting point, and latitude and longitude of the source location, number of hops, background ionosphere, collision frequency and geomagnetic field. Model Outputs DescriptionProperties of the wave along its path such as group range, phase, attenuation, coordinates of potential reflection from the ionosphere, coordinates of arrival to ground, etc. Model CaveatsThe numerical ray trace routines require gridded profiles of the Earth's ionosphere and magnetic field. Users supply their own models or employ the International Reference Ionophere and International Geomagnetic Reference Field models supplied with PHaRLAP. Change LogReleases are accessible at: https://www.dst.defence.gov.au/our-technologies/pharlap-provision-high-frequency-raytracing-laboratory-propagation-studies Changelog is accessible from within the release Model Acknowledgement/Publication Policy (if any)Please add the following acknowledgement to any published material which contains results obtained using this toolbox: "The results published in this paper were obtained using the HF propagation toolbox, PHaRLAP, created by Dr Manuel Cervera, Defence Science and Technology Group, Australia (manuel.cervera@dsto.defence.gov.au). This toolbox is available by request from its author." Model Domains:Global_IonosphereSpace Weather Impacts:Ionosphere variability (navigation, communications)Phenomena :Variablility_of_Plasma_DensityEquatorial_Anomaly Traveling_Ionospheric_Disturbances HF_Signal_Absorption Simulation Type(s):Physics-basedPhysics-based.Kinetic Physics-based.MHD Temporal Dependence Possible? (whether the code results depend on physical time?)trueModel is available at?CCMCSource code of the model is publicly available?falseCCMC Model Status (e.g. onboarding, use in production, retired, only hosting output, only source is available):productionCode Language:FORTRAN 2008, MATLAB, and CRegions (this is automatically mapped based on model domain):Contacts :Manuel.Cervera, ModelDeveloperReza.Janalizadeh Choobbasti, ModelHostContact Jia.Yue, ModelHostContact Acknowledgement/Institution :Australian Department of Defence, Defence Science and Technology GroupRelevant Links :Model Website at the Australian Department of Defence, Defence Science and Technology Group: https://www.dst.defence.gov.au/our-technologies/pharlap-provision-high-frequency-raytracing-laboratory-propagation-studiesPublications :Model Access Information :Access URL: https://kauai.ccmc.gsfc.nasa.gov/instantrun/pharlap/Access URL Name: Instant Run Repository ID: spase://CCMC/Repository/NASA/GSFC/CCMC Availability: online AccessRights: OPEN Format: HTML Encoding: None Linked to Other Spase Resource(s) (example: another SimulationModel) : |
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Curator: Chiu Wiegand | NASA Official: Dr. Masha Kuznetsova | Privacy and Security Notices | Accessibility | CCMC Data Collection Consent Agreement |
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