VLA Data Survey

This is a step-by-step tutorial for doing VLA solar data survey.

Preparatory Work

Get the visbility data

The first step of the data survey is to get the visbility data of the the event you are focusing on. Always the origrinal data should be in the the dictionary '/srg/data/evla', you can find the folders named by the date of the event.

The casa task 'listobs' can help to check the basic information of the data, to get the better understanding of each casa task, you can both type the task name followed with a question mark( for example, 'listobs?') in the server or directly google 'nrao casa listobs'.

For each casa task(take the listobs as a example), you can type 'tget listobs' and then 'inp' to get and change the input parameters.

Task listobs can tell some basic information, use the 2012 Mar 10 event as a example,

Other information of the event

Except the vla data itself, we may also need the X-ray data and EUV data to help us.

Make the dynamic spectrum

Select the appropriate baselines

Usually we use the task 'dspec' to make the dynamic spectrum, use get_dspec to create a npz file, the most important input is timerange and baseline. You can use the casa task 'viewer' to check the visbility data( remember when using the viewer, don not select too long timerange).

When coming into the window of viewer.

Better check both the longer baselines and shorter baselines.

Do the plot

Use plt_dspec to do the plot, after getting the npz file, you can do the plot. Usually we can do both LCP and RCP, also you can attach the goes figure. To get the survey of the whole timerange, we need to get a movie, select the movie as True, you can get a folder called 'dspec' which including the figures to make the movie.