Solar Luminosity Oscillation Telescope (SLOT)

Details Solar Luminosity Oscillation Telescope (SLOT) Solar Luminosity Oscillation Telescope (SLOT)

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988esasp.286..175a&link_type=abstract

In its Seismology of the Sun and Sun-Like Stars p 175-176 (SEE N89-25819 19-92)

Physics

4

P Waves, Solar Observatories, Solar Oscillations, Solar Radiation, Telescopes, Data Acquisition, Signal To Noise Ratios, Spectrophotometers, Systems Engineering

Scientific paper

Low degree l=0-2 solar p-modes were detected with the SLOT instruments at Izana and Baja California. The main source of noise for these ground based observations is in the terrestrial atmosphere. However, the data acquisition system still has to have very low intrinsic noise. It is shown how this is achieved in the SLOT instruments. Design and operating principles of the photometers and data acquisition system are outlined.

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