Abstract
The fundamental data of asteroseismology are pulsation frequencies and mode identifications (see Chapters 5, 6, and 7). There are two main observational techniques for obtaining these data: 1) photometric observations of variability in the stellar flux, and 2) spectroscopic observations of velocity variations caused by the motion of surface elements. Of course, the observations are always the sum of the effects of all of the pulsation modes simultaneously, hence the need for frequency analysis techniques (explained in detail in Chapter 5) to extract the individual frequencies of the pulsation modes. For very large amplitude pulsating stars it is becoming possible to use interferometry to study the radial cross-section changes in a few stars, but this technique is in its infancy and will not be discussed further here. The relationship between asteroseismology and interferometry – primarily using the latter to provide precise fundamental stellar data – is discussed in detail in Cunha et al. (2007).
We discuss the two techniques of photometry and spectroscopy separately. They require different instrumentation and observing conditions, sources of noise are different for them, and they sample the physics of the pulsation differently. For example, in the Sun – and by implication in all solar-like stars – granulation generates much higher noise in photometric measurements than in spectroscopic measurements at the frequencies of interest, as is illustrated in Fig. 4.1 with observations from the GOLF (Global Oscillations at Low Frequencies)GOLF and VIRGO (Variability of Solar Irradiance and Gravity Oscillations)VIRGO instruments onboard the SOHO (Solar and Heliospheric Observatory) satellite.
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Notes
- 1.
http://www.physics.udel.edu/darc/wet; http://wet.physics.iastate.edu.
- 2.
astro.phys.au.dk/SONG.
- 3.
tycho.usno.navy.mil/systime.html.
- 4.
http://www.aavso.org.
- 5.
iraf.noao.edu/iraf/ftp/iraf/docs/apuser.ps.Z.
- 6.
http://www.shef.ac.uk/physics/people/vdhillon/ultracam/.
- 7.
http://exoplanet.eu/.
- 8.
several examples are available from http://www.eso.org.
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Aerts, C., Christensen-Dalsgaard, J., Kurtz, D.W. (2010). Observational Techniques for Asteroseismology. In: Asteroseismology. Astronomy and Astrophysics Library. Springer, Dordrecht. https://doi.org/10.1007/978-1-4020-5803-5_4
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