Spectral slope

In astrophysics and planetary science, spectral slope, also called spectral gradient, is a measure of dependence of the reflectance on the wavelength.

In digital signal processing, it is a measure of how quickly the spectrum of an audio sound tails off towards the high frequencies, calculated using a linear regression.[1]

Illustration of the spectral slope

Spectral slope in Astrophysics / Planetary Science

The visible and infrared spectrum of the reflected sunlight is used to infer physical and chemical properties of the surface of a body. Some objects are brighter (reflect more) in longer wavelengths (red). Consequently, in visible light they will appear redder than objects showing no dependence of reflectance on the wavelength.

The diagram illustrates three slopes:

The slope (spectral gradient) is defined as:

where is the reflectance measured with filters F0, F1 having the central wavelengths λ0 and λ1, respectively.[2]

The slope is typically expressed in percentage increase of reflectance (i.e. reflexivity) per unit of wavelength: %/100 nm (or % /1000 Å)

The slope is mostly used in near infrared part of the spectrum while colour indices are commonly used in the visible part of the spectrum.

The trans-Neptunian object Sedna is a typical example of a body showing a steep red slope (20%/100 nm) while Orcus' spectrum appears flat in near infra-red.

Spectral slope in audio

The spectral "slope" of many natural audio signals (their tendency to have less energy at high frequencies) has been known for many years,[3] and the fact that this slope is related to the nature of the sound source. One way to quantify this is by applying linear regression to the Fourier magnitude spectrum of the signal, which produces a single number indicating the slope of the line-of-best-fit through the spectral data.[1]

Alternative ways to characterise a sound signal's distribution of energy vs. frequency include spectral rolloff, spectral centroid.[1]

See also

References

  1. 1 2 3 G. Peeters, A large set of audio features for sound description, tech. rep., IRCAM, 2004.
  2. ↑ A. Deressoundiram; H. Boehnhardt; S. Tegler & C. Truillo (2008). "Color Properties and Trends of the Transneptunian Objects". in The Solar System Beyond Neptune. ISBN 978-0-8165-2755-7.
  3. ↑ D. B. Fry, The Physics of Speech, Cambridge Textbooks in Linguistics, Cambridge University Press, 1996.
This article is issued from Wikipedia - version of the 6/29/2016. The text is available under the Creative Commons Attribution/Share Alike but additional terms may apply for the media files.