Abstract
We can’t measure any light until it has passed through the atmosphere, or we have risen above the atmosphere to meet it. The atmosphere blocks light, distorts it, and creates a bright background that makes it hard to see faint objects. All these problems depend strongly on wavelength (or type of particle). In this chapter we look at how these effects arise, and how to get around them. We will examine in turn transmission, sky backgrounds, refraction and seeing, and the pros and cons of working in space.
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Lawrence, A. (2014). The Atmosphere and How to Avoid it. In: Astronomical Measurement. Springer Praxis Books(). Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-39835-3_2
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DOI: https://doi.org/10.1007/978-3-642-39835-3_2
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