nsioulas

Pinned Repositories

Integrate-relativistic-equations-of-motion-in-EM-field
Integrate the relativistic equtions of motion for charged particles in an EM field. Four different integration schemes are available, namely: Boris, Vay, HC , Lapenta_Markidis
Language:C00
MHDTurbPy
Language:Jupyter Notebook41
SEA
Perform Superposed Epoch Analysis (SEA) using Python.
Language:Jupyter Notebook10
SwitchbackFinder
Language:Jupyter Notebook00
Charged-particle-acceleration-in-strong-MHD-turbulence
A Monte-Carlo, simulation for charged particle acceleration in strong MHD turbulence. Several acceleration mechanisms can be implemented 1) 1st order Fermi acceleration 2) 2nd order Fermi acceleration 3) Diffusive shock acceleration 4) A combinaton of the previous
Language:MATLAB22
MHDTurbPy_v2
Language:Jupyter Notebook10
3d_anisotropy
This project is still ongoing please email me before implementing it to your analysis
Language:Jupyter Notebook00
ISSI_intervals
00
MHD-course
Code related to EPSS courses
Language:Jupyter Notebook00
Orbit_plots
Scripts to create the Solar Orbiter orbit data plots
Language:Python00

nsioulas's Repositories

nsioulas/MHDTurbPy
Language:Jupyter Notebook41
nsioulas/MHDTurbPy_v2
Language:Jupyter Notebook1
nsioulas/3d_anisotropy
This project is still ongoing please email me before implementing it to your analysis
Language:Jupyter Notebook
nsioulas/Solar-Wind-Time-Series-Viewer
nsioulas/pyspedas
Python-based Space Physics Environment Data Analysis Software
Language:Python
nsioulas/SwitchbackFinder
Language:Jupyter Notebook
nsioulas/SEA
Perform Superposed Epoch Analysis (SEA) using Python.
Language:Jupyter Notebook1
nsioulas/UDWT
This file decomposes the vector magnetic field fluctuations onto the vector background magnetic field using the undecimated discrete wavelet decomposition. The scale-by-scale 'details' and 'approximations' provide the scale-by-scale fluctuations and background field, respectively. This type of anisotropy study is historically called 'variance anisotropy'. This is basically the anisotropy study of magnetic field quantities rather than the wavevector 'k_i' values that it depends upon.
Language:Jupyter Notebook
nsioulas/Integrate-relativistic-equations-of-motion-in-EM-field
Integrate the relativistic equtions of motion for charged particles in an EM field. Four different integration schemes are available, namely: Boris, Vay, HC , Lapenta_Markidis
Language:C
nsioulas/Charged-particle-acceleration-in-strong-MHD-turbulence
A Monte-Carlo, simulation for charged particle acceleration in strong MHD turbulence. Several acceleration mechanisms can be implemented 1) 1st order Fermi acceleration 2) 2nd order Fermi acceleration 3) Diffusive shock acceleration 4) A combinaton of the previous
Language:MATLAB22
nsioulas/ISSI_intervals
nsioulas/website
my website
Language:HTML
nsioulas/pfsspy
Potential Field Source Surface model package for Python
nsioulas/summer-school
nsioulas/packaging-guide
A generic Python packaging guide and template. Slightly focused more towards scientific packages.
nsioulas/MHD-course
Code related to EPSS courses
Language:Jupyter Notebook
nsioulas/Orbit_plots
Scripts to create the Solar Orbiter orbit data plots
nsioulas/PyCWT
A Python module for continuous wavelet spectral analysis. It includes a collection of routines for wavelet transform and statistical analysis via FFT algorithm. In addition, the module also includes cross-wavelet transforms, wavelet coherence tests and sample scripts.