Getting started · About 10 min

Your first solar radio spectrum

Open an observation, inspect its metadata, and find structure in the spectrum.

Before you begin: install the analyzer and have a FITS observation ready, or fetch one with the built-in e-CALLISTO downloader.

Get an observation

Open the e-CALLISTO downloader. Select a date and station, preview an available observation, then import it. You can also use File → Open with a local .fit, .fits, .fit.gz, or .fits.gz file.

Check your axes

Read the station and date in the file metadata. Identify the time axis, frequency axis, and color scale. Check whether times are UT or seconds and whether intensity is shown in digits/ADU or dB.

Your first solar radio spectrum: application example

Reveal the signal

Inspect raw data before applying background subtraction. Adjust the display thresholds gradually. In v3.1.0, choose Mean, Median, or Median (dB), then Subtract Background.

Inspect the result

Look for coherent structure across time and frequency. Persistent horizontal features may be interference; compare raw and processed views before assigning a physical interpretation.

Keep your work

Save an .efaproj project. Export a figure and record the source filename and processing settings. You now have a traceable starting point for analysis.

Continue exploring

Consult the user guide for every control and method, or ask about your workflow in GitHub Discussions.