Solar Luminosity Oscillation Telescope (SLOT)

Bibcode
1988ESASP.286..175A
Andersen, Bo Nyborg; Domingo, V.; Jones, A. R.; Korzennik, Sylvain G.; Jimenez, A.; Palle, Pere L.; Regulo, C.; Roca Cortés, Teodoro
Bibliographical reference

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

Advertised on:
12
1988
Number of authors
8
IAC number of authors
0
Citations
6
Refereed citations
6
Description
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.
Type
Non-refereed
Solar observatories
Solar oscillations
Solar radiation
Telescopes

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