This is the main program. The RAPID (IES or IIMS), FGM,
and EFLOW or IFLOW CDF files are loaded and synchro-
nized. Additionally, pitch angle calculations such as pitch an-
gle and averaging are performed here. All data is stored in a
python dictionary, which is extended to include the relevant
variables for each spacecraft.
This program calculates the average flux (3D distribution) for each energy bin
across all times and viewing directions. The resulting energy
spectrum is then plotted on a double-logarithmic graph.
Generates a Mollweide diagram for a selected channel of a
spacecraft including color-coded fluxes, which can be compared
on the color bar with the corresponding counts per sector.
Generates a time series, which displays the PADs as a heat map
for all channels of a spacecraft. It also provides the components
and magnitude of the magnetic field, as well as the coordinates
and radial distance from Earth.
This is the main program. The RAPID (IES or IIMS), FGM,
and EFLOW or IFLOW CDF files are loaded and synchro-
nized. Additionally, pitch angle calculations such as pitch an-
gle and averaging are performed here. All data is stored in a
python dictionary, which is extended to include the relevant
variables for each spacecraft.
This code generates a plot of electron flux, ion flux, trajectory, and radial distance from Earth for ONE spacecraft over a specified time interval. To do this, it reads in an .npy file and accepts the desired time interval as input.
This code allows you to visualize the position, trajectory of all spacecraft, and Key Science Regions of PMO in 3D.
One .npy file is loaded per spacecraft. To plot the trajectory over a time interval, the variables start and end must correspond to the desired time interval. To plot a discrete point in time, set start=None and end=None, and only target_time receives the desired timestamp.
