Maxwellian distribution ======================= .. toctree:: :maxdepth: 4 :hidden: Presentation ------------ This is a model for emission energy distribution of |SEs|. It does not take into account incidence angle of |PEs|. Input files ----------- You must provide an emission energy distribution at normal incidence. Currently, the fitting on several emission distribution files at different |PE| energies is not supported. +-----------------------------+---------------+-----------------------------+---------------------------+ | |Emission Yield |Emission energy distribution |Emission angle distribution| +=============================+===============+=============================+===========================+ | "True" secondaries | ❌ | ✅ | ❌ | +-----------------------------+---------------+-----------------------------+---------------------------+ | Elastically backscattered | ❌ | ❌ | ❌ | +-----------------------------+---------------+-----------------------------+---------------------------+ | Inelastically backscattered | ❌ | ❌ | ❌ | +-----------------------------+---------------+-----------------------------+---------------------------+ | Total | ❌ | ❌ | ❌ | +-----------------------------+---------------+-----------------------------+---------------------------+ Definitions ----------- Emission energy distribution is given by: .. math:: f(E_\mathrm{SE}) = 2 \sqrt{\frac{E_\mathrm{SE}}{\pi T^3}} \mathrm{e}^{-E_\mathrm{SE}/T} :math:`T` is the distribution temperature in :unit:`eV`. In order to set it's maximum to unity, we scale it by its maximum, at :math:`E_\mathrm{SE} = T/2`. Model parameters ---------------- The parameters list is dynamically created here: :py:mod:`Maxwellian API documentation<.maxwellian>`. To-do list ---------- .. todo:: - Allow fitting on several distribution files with different |PE| energy. - Consistent input files with Chung Everhart. SEs or all?