New system in testing phase. Please wait until telescope available (ETA May 2026).
If you have any questions or run into problems, please first read the User's manual and experiment instructions below. If you still need help, contact us at salsa.onsala@gmail.com.
The user's manual describes how to operate the SALSA telescope — scheduling observations, pointing, recording spectra, and downloading data.
Step-by-step lab guides covering the scientific background, observing procedure, and data analysis for each experiment.
Observe neutral hydrogen across the Milky Way, measure Doppler-shifted 21 cm emission, derive the rotation curve, and reconstruct the positions of the spiral arms.
Receive and compare radio signals from GPS, Galileo, GLONASS, and BeiDou satellites, and see how their different modulation schemes produce distinct spectral shapes.
Use the Sun as a bright radio source to map the beam pattern of the SALSA antenna, measure its angular resolution, and compare the result to theoretical predictions for a circular aperture.
For hardware details — signal chain, rotor protocol, LNA measurements, and component references — see the Technical specifications page.