Universität zu Köln

Klose, Martina ORCID: 0000-0001-8190-3700, Jemmett-Smith, Bradley C., Kahanpaa, Henrik ORCID: 0000-0001-9108-186X, Kahre, Melinda, Knippertz, Peter ORCID: 0000-0001-9856-619X, Lemmon, Mark T., Lewis, Stephen R., Lorenz, Ralph D., Neakrase, Lynn D. V., Newman, Claire, Patel, Manish R., Reiss, Dennis ORCID: 0000-0002-1836-596X, Spiga, Aymeric ORCID: 0000-0002-6776-6268 and Whelley, Patrick L. (2016). Dust Devil Sediment Transport: From Lab to Field to Global Impact. Space Sci. Rev., 203 (1-4). S. 377 - 427. DORDRECHT: SPRINGER. ISSN 1572-9672

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Abstract

The impact of dust aerosols on the climate and environment of Earth and Mars is complex and forms a major area of research. A difficulty arises in estimating the contribution of small-scale dust devils to the total dust aerosol. This difficulty is due to uncertainties in the amount of dust lifted by individual dust devils, the frequency of dust devil occurrence, and the lack of statistical generality of individual experiments and observations. In this paper, we review results of observational, laboratory, and modeling studies and provide an overview of dust devil dust transport on various spatio-temporal scales as obtained with the different research approaches. Methods used for the investigation of dust devils on Earth and Mars vary. For example, while the use of imagery for the investigation of dust devil occurrence frequency is common practice for Mars, this is less so the case for Earth. Modeling approaches for Earth and Mars are similar in that they are based on the same underlying theory, but they are applied in different ways. Insights into the benefits and limitations of each approach suggest potential future research focuses, which can further reduce the uncertainty associated with dust devil dust entrainment. The potential impacts of dust devils on the climates of Earth and Mars are discussed on the basis of the presented research results.

Item Type:	Journal Article
Creators:	Creators Email ORCID ORCID Put Code Klose, Martina UNSPECIFIED orcid.org/0000-0001-8190-3700 UNSPECIFIED Jemmett-Smith, Bradley C. UNSPECIFIED UNSPECIFIED UNSPECIFIED Kahanpaa, Henrik UNSPECIFIED orcid.org/0000-0001-9108-186X UNSPECIFIED Kahre, Melinda UNSPECIFIED UNSPECIFIED UNSPECIFIED Knippertz, Peter UNSPECIFIED orcid.org/0000-0001-9856-619X UNSPECIFIED Lemmon, Mark T. UNSPECIFIED UNSPECIFIED UNSPECIFIED Lewis, Stephen R. UNSPECIFIED UNSPECIFIED UNSPECIFIED Lorenz, Ralph D. UNSPECIFIED UNSPECIFIED UNSPECIFIED Neakrase, Lynn D. V. UNSPECIFIED UNSPECIFIED UNSPECIFIED Newman, Claire UNSPECIFIED UNSPECIFIED UNSPECIFIED Patel, Manish R. UNSPECIFIED UNSPECIFIED UNSPECIFIED Reiss, Dennis UNSPECIFIED orcid.org/0000-0002-1836-596X UNSPECIFIED Spiga, Aymeric UNSPECIFIED orcid.org/0000-0002-6776-6268 UNSPECIFIED Whelley, Patrick L. UNSPECIFIED UNSPECIFIED UNSPECIFIED
URN:	urn:nbn:de:hbz:38-257998
DOI:	10.1007/s11214-016-0261-4
Journal or Publication Title:	Space Sci. Rev.
Volume:	203
Number:	1-4
Page Range:	S. 377 - 427
Date:	2016
Publisher:	SPRINGER
Place of Publication:	DORDRECHT
ISSN:	1572-9672
Language:	English
Faculty:	Unspecified
Divisions:	Unspecified
Subjects:	no entry
Uncontrolled Keywords:	Keywords Language LARGE-EDDY SIMULATION; PLANETARY BOUNDARY-LAYER; INTERANNUAL VARIABILITY; OPTICAL DEPTH; AUSTRALIAN LANDSCAPE; MODEL DESCRIPTION; WILLY-WILLIES; MARS YEARS; EMISSION; STORMS Multiple languages Astronomy & Astrophysics Multiple languages
Refereed:	Yes
URI:	http://kups.ub.uni-koeln.de/id/eprint/25799