Profile#
- class pydrad.parse.Profile(hydrad_root, time: Unit('s'), **kwargs)[source]#
Bases:
objectContainer for HYDRAD results at a given timestep. Typically accessed through pydrad.parse.Strand
- Parameters:
hydrad_root (str) – Path to HYDRAD directory
time (~astropy.units.Quantity) – Timestep corresponding to the profile of interest
Attributes Summary
Coordinate as a function of \(s\)
Electron conduction as a function of \(s\)
Electron density as a function of \(s\)
Electron pressure as a function of \(s\)
Electron temperature as a function of \(s\)
Spatial location of the grid centers
Spatial location of the edges of each grid cell, including the rightmost edge
Spatial location of the left edge of each grid cell
Spatial location of the right edge of each grid cell
Spatial width of each grid cell
Ion conduction as a function of \(s\)
Ion density as a function of \(s\)
Ion pressure as a function of \(s\)
Ion temperature as a function of \(s\)
Level population hydrogen 1 as a function of \(s\)
Level population hydrogen 2 as a function of \(s\)
Level population hydrogen 3 as a function of \(s\)
Level population hydrogen 4 as a function of \(s\)
Level population hydrogen 5 as a function of \(s\)
Level population hydrogen 6 as a function of \(s\)
Sound speed as a function of \(s\)
Velocity as a function of \(s\)
Methods Summary
column_emission_measure([bins, bounds])Computes the column emission measure, where it is assumed that the loop is confined to a single pixel and oriented along the line of sight.
peek(**kwargs)Quick look at profiles at a given timestep.
peek_emission_measure(**kwargs)Quick look at the column emission measure.
spatial_average(quantity[, bounds])Compute a spatial average of a specific quantity
Attributes Documentation
- coordinate#
Coordinate as a function of \(s\)
- electron_conduction#
Electron conduction as a function of \(s\)
- electron_density#
Electron density as a function of \(s\)
- electron_pressure#
Electron pressure as a function of \(s\)
- electron_temperature#
Electron temperature as a function of \(s\)
- grid_centers#
Spatial location of the grid centers
- grid_edges#
Spatial location of the edges of each grid cell, including the rightmost edge
- grid_edges_left#
Spatial location of the left edge of each grid cell
- grid_edges_right#
Spatial location of the right edge of each grid cell
- grid_widths#
Spatial width of each grid cell
- ion_conduction#
Ion conduction as a function of \(s\)
- ion_density#
Ion density as a function of \(s\)
- ion_pressure#
Ion pressure as a function of \(s\)
- ion_temperature#
Ion temperature as a function of \(s\)
- level_population_hydrogen_1#
Level population hydrogen 1 as a function of \(s\)
- level_population_hydrogen_2#
Level population hydrogen 2 as a function of \(s\)
- level_population_hydrogen_3#
Level population hydrogen 3 as a function of \(s\)
- level_population_hydrogen_4#
Level population hydrogen 4 as a function of \(s\)
- level_population_hydrogen_5#
Level population hydrogen 5 as a function of \(s\)
- level_population_hydrogen_6#
Level population hydrogen 6 as a function of \(s\)
- sound_speed#
Sound speed as a function of \(s\)
- velocity#
Velocity as a function of \(s\)
Methods Documentation
- column_emission_measure(bins: Unit('K') = None, bounds: Unit('cm') = None)[source]#
Computes the column emission measure, where it is assumed that the loop is confined to a single pixel and oriented along the line of sight.
- Parameters:
bins (~astropy.units.Quantity, optional) – Temperature bin edges, including rightmost edge. If None (default), the bins will be equally-spaced in \(\log{T}\), with a left edge at \(\log{T}=3\), a right edge at \(\log{T}=8\), and a bin width of \(0.05\).
- Returns:
em (~astropy.units.Quantity) – The column emission measure in each bin
bins (~astropy.units.Quantity) – Temperature bin edges. Note that
len(bins)=len(em)+1.
- peek(**kwargs)[source]#
Quick look at profiles at a given timestep.
Takes the same keyword arguments as ~pydrad.visualize.plot_profile.