2018
DOI: 10.5194/amt-11-4327-2018
|View full text |Cite
|
Sign up to set email alerts
|

Limited angle tomography of mesoscale gravity waves by the infrared limb-sounder GLORIA

Abstract: Abstract. Three-dimensional measurements of gravity waves are required in order to quantify their directionresolved momentum fluxes and obtain a better understanding of their propagation characteristics. Such 3-D measurements of gravity waves in the lowermost stratosphere have been provided by the airborne Gimballed Limb Observer for Radiance Imaging of the Atmosphere (GLORIA) using full angle tomography. Closed flight patterns of sufficient size are needed to acquire the full set of angular measurements for f… Show more

Help me understand this report
View preprint versions

Search citation statements

Order By: Relevance

Paper Sections

Select...
1
1
1

Citation Types

1
31
0

Year Published

2019
2019
2023
2023

Publication Types

Select...
7
1

Relationship

5
3

Authors

Journals

citations
Cited by 15 publications
(32 citation statements)
references
References 57 publications
1
31
0
Order By: Relevance
“…To fully constrain their directional GWMF, 3-D observations are needed. Three-dimensional stratospheric measurements are notoriously challenging and are normally limited to specialist instrumentation (Ern et al, 2004;Krisch et al, 2017Krisch et al, , 2018Krisch et al, , 2020. Combinations of instruments (e.g., Alexander, 2015;Faber et al, 2013;Wright et al, 2016), or the use of supplementary wind information (e.g., Alexander & Barnet, 2007;Alexander et al, 2009), have been used to infer 3-D GW structure, but these require limiting assumptions and are confined to colocated and/or coincident measurements.…”
Section: Introductionmentioning
confidence: 99%
“…To fully constrain their directional GWMF, 3-D observations are needed. Three-dimensional stratospheric measurements are notoriously challenging and are normally limited to specialist instrumentation (Ern et al, 2004;Krisch et al, 2017Krisch et al, , 2018Krisch et al, , 2020. Combinations of instruments (e.g., Alexander, 2015;Faber et al, 2013;Wright et al, 2016), or the use of supplementary wind information (e.g., Alexander & Barnet, 2007;Alexander et al, 2009), have been used to infer 3-D GW structure, but these require limiting assumptions and are confined to colocated and/or coincident measurements.…”
Section: Introductionmentioning
confidence: 99%
“…An important basis for MATS is the InnoSat satellite platform developed by OHB Sweden and ÅAC Microtec (Larsson et al, 2016). InnoSat has been designed as a "universal" microsatellite platform that can host a variety of different payloads for aeronomy or astronomy research in low-Earth orbit.…”
Section: Mission Developmentmentioning
confidence: 99%
“…In order to implement this technique, one needs a way to generate a random vector x with the required covariance, represented by a known, symmetric, positive definite covariance matrix S a . This can be done by generating a vector u of independent standard normal random variables and finding a square matrix L such that L L T = S a (Kroese et al, 2013). Then we can set x = Lu, and…”
Section: Monte Carlo Diagnosticsmentioning
confidence: 99%