========================== Get parameters from CPEMv2 ========================== Install referring to the :ref:`quickinstall`. CPEMv2 is provided in a form of module. Once installed, CPEMv2 model can be used from any python interpreters or scripts. Just start Python3. Probably, you want to use ipython, or jupyter notebook. Double-click the relevant icons, or use the command line as .. code-block:: sh % ipython Importing CPEMv2 module ======================= Once Python3 is launched, import the module. >>> from irfpy.cpem import cpemv2 Getting charge density ====================== The charge density model is available by ``cpemv2.plasma_density``. There are four models implemented under ``cpemv2.plasma_density``: - Reference model, only depending on the Jovi-center distance, :math:`R`. :meth:`cpemv2.plasma_density.reference_model <irfpy.cpem.cpemv2.CpemIonChargeDensity.reference_model>` - Mean model, depending on the Jovi-center distance and the magnetic local time, :math:`R, MLT`. :meth:`cpemv2.plasma_density.mean_model <irfpy.cpem.cpemv2.CpemIonChargeDensity.mean_model>` - Percentile model, depending on the percentile (user can specify) together with above. :meth:`cpemv2.plasma_density.percentile_model <irfpy.cpem.cpemv2.CpemIonChargeDensity.percentile_model>` - Full model, depending on the magnetic latitude, but only for Charge density. Otherwise, the return is the same as percentile model. :meth:`cpemv2.plasma_density.full_model <irfpy.cpem.cpemv2.CpemIonChargeDensity.full_model>` Charge density model -------------------- It is easy to get the CPEMv2 charge density model. >>> n = cpemv2.plasma_density.full_model(15.5, 6.0, -5.3, 0.5) This is the density modeled at R=15.5 Rj, MLT=6 hr, Mlat=-5.3 deg, and percentile of 50%. >>> print(n) 0.656950469619 Other models ------------ You can replace ``plasma_density`` to the following. - ``ion_velocity_corotation``, ``ion_velocity_polar``, and ``ion_velocity_radial`` for the corotation ion velocity vector - ``ion_temperature`` for the ion temperature - ``hot_electron_density`` and ``hot_electron_temperature`` for hot electrons.