2006
DOI: 10.5194/acp-6-3343-2006
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Imaging gravity waves in lower stratospheric AMSU-A radiances, Part 2: Validation case study

Abstract: Abstract. Two-dimensional radiance maps from Channel 9 (∼60-90 hPa) of the Advanced Microwave Sounding Unit (AMSU-A), acquired over southern Scandinavia on 14 January 2003, show plane-wave-like oscillations with a wavelength λ h of ∼400-500 km and peak brightness temperature amplitudes of up to 0.9 K. The wave-like pattern is observed in AMSU-A radiances from 8 overpasses of this region by 4 different satellites, revealing a growth in the disturbance amplitude from 00:00 UTC to 12:00 UTC and a change in its ho… Show more

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Cited by 54 publications
(77 citation statements)
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“…Background signals are caused not only by large-scale temperature gradients and planetary waves, but also by the limbbrightening effect. A standard detrending technique for AIRS is to remove the background defined by means of a polynomial fit to the brightness temperature measurements of each across-track scan (Wu, 2004;Eckermann et al, 2006;Alexander and Barnet, 2007;Hoffmann et al, 2014). Usually, a fourth-order polynomial is applied for this purpose.…”
Section: Introductionmentioning
confidence: 99%
“…Background signals are caused not only by large-scale temperature gradients and planetary waves, but also by the limbbrightening effect. A standard detrending technique for AIRS is to remove the background defined by means of a polynomial fit to the brightness temperature measurements of each across-track scan (Wu, 2004;Eckermann et al, 2006;Alexander and Barnet, 2007;Hoffmann et al, 2014). Usually, a fourth-order polynomial is applied for this purpose.…”
Section: Introductionmentioning
confidence: 99%
“…Both methods are standard methods that have been optimized for each instrument. The removal of background signals in AIRS temperature measurements follows the detrending method described by Wu and Zhang (2004), Eckermann et al (2006), and Alexander and Teitelbaum (2007). A fourth-order polynomial fit in the across-track direction is used in this method for defining the background.…”
Section: Removal Of Background Signals To Extract Gravity Wave Informmentioning
confidence: 99%
“…The observed brightness temperatures are mainly composed of three contributions: (i) gravity wave signals, (ii) slowly varying background signals, and (iii) measurement noise. Background signals associated with large-scale temperature gradients or planetary waves are removed with the detrending procedure of Wu (2004), Eckermann et al (2006), and Alexander and Barnet (2007), i.e., brightness temperature perturbations are calculated as dif- Table 1 for details).…”
Section: Airs Observations Of Stratospheric Gravity Wavesmentioning
confidence: 99%
“…The analysis is based on a 12-year record (January 2003-December 2014) of 4.3 µm radiance observations of AIRS/Aqua. Stratospheric gravity wave signals in terms of brightness temperature perturbations and variances are extracted by applying a number of standard techniques developed for nadir sounders (Wu, 2004;Eckermann et al, 2006;Alexander and Barnet, 2007;Hoffmann et al, 2014). We introduce a simple and effective new method to detect orographic gravity wave signals from infrared nadir sounder measurements.…”
Section: Introductionmentioning
confidence: 99%