Award Abstract # 1242943
CEDAR: Numerical Investigation of Observed Multiscale Dynamics in the Middle Atmosphere

NSF Org: AGS
Division of Atmospheric and Geospace Sciences
Recipient: GLOBAL ATMOSPHERIC TECHNOLOGIES AND SCIENCES, INC.
Initial Amendment Date: July 12, 2012
Latest Amendment Date: January 16, 2014
Award Number: 1242943
Award Instrument: Continuing Grant
Program Manager: Therese Moretto Jorgensen
AGS
 Division of Atmospheric and Geospace Sciences
GEO
 Directorate for Geosciences
Start Date: July 1, 2012
End Date: December 31, 2015 (Estimated)
Total Intended Award Amount: $244,022.00
Total Awarded Amount to Date: $244,022.00
Funds Obligated to Date: FY 2012 = $79,478.00
FY 2013 = $81,310.00

FY 2014 = $83,234.00
History of Investigator:
  • Brian Laughman (Principal Investigator)
    b.laughman@gats-inc.com
Recipient Sponsored Research Office: GLOBAL ATMOSPHERIC TECHNOLOGIES AND SCIENCES, INC.
11828 CANON BLVD STE D
NEWPORT NEWS
VA  US  23606-2554
(757)873-5920
Sponsor Congressional District: 03
Primary Place of Performance: G & A Technical Software, Inc.
3360 Mitchell Lane
Boulder
CO  US  80301-2775
Primary Place of Performance
Congressional District:
02
Unique Entity Identifier (UEI): FNZFG585K6U3
Parent UEI:
NSF Program(s): AERONOMY
Primary Program Source: 01001213DB NSF RESEARCH & RELATED ACTIVIT
01001314DB NSF RESEARCH & RELATED ACTIVIT

01001415DB NSF RESEARCH & RELATED ACTIVIT
Program Reference Code(s): 1323, EGCH
Program Element Code(s): 152100
Award Agency Code: 4900
Fund Agency Code: 4900
Assistance Listing Number(s): 47.050

ABSTRACT

This is a 3-year modeling effort to be undertaken as part of the Coupling, Energetics and Dynamics of Atmospheric Regions program. Atmospheric gravity waves are believed to play a vital role in the transport of energy and momentum between atmospheric layers. This transport is enabled by the propagation of these waves vertically through the background atmosphere and dissipation of these occurs via the growth of instabilities (both convective and shear instabilities). This project utilizes two advanced numerical simulations to investigate gravity wave and instability processes in the Mesosphere-Lower Thermosphere (MLT) region. Previous simulations have been performed in idealized environments and small periodic domains. Here, the simulations will be extended to deep domain studies, which will examine these wave and instability processes in more realistic flows inspired by detailed observations.

Gravity waves are a significant forcing source on MLT dynamics and their effects strongly impact general circulation and climate models. In addition, numerical weather prediction models, despite their tropospheric focus, have been shown to make better predictions when the upper-atmospheric dynamics are more accurately modeled. Specifically, improved understanding of when / where gravity waves become unstable in realistic flows that would result from this effort is a vital step towards improving parametrization of these waves in global-scale models.

PUBLICATIONS PRODUCED AS A RESULT OF THIS RESEARCH

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David C. Fritts and Ling Wang "Gravity Wave?Fine Structure Interactions. Part II: Energy Dissipation Evolutions, Statistics, and Implications." J. Atmos. Sci. , 2013 http://dx.doi.org/10.1175/JAS-D-13-059.1
David C. Fritts, Ling Wang, and Joseph A. Werne "Gravity Wave?Fine Structure Interactions. Part I: Influences of Fine Structure Form and Orientation on Flow Evolution and Instability" J. Atmos. Sci. , 2013 http://dx.doi.org/10.1175/JAS-D-13-055.1
Fritts, D. C., and L. Wang "Gravity wave - fine structure interactions, Part 2: Energy dissipation evolutions, statistics, and implications" Journal of the Atmospheric Sciences , v.70 , 2013 , p.3735 http://dx.doi.org/10.1175/JAS-D-13-059.1
Fritts, D. C., B. Laughman, T. S. Lund, and J. B. Snively "Self-acceleration and instability of gravity wave packets: 1. Effects of temporal localization" J. Geophys. Res. Atmos. , 2015 10.1002/2015JD023363
Fritts, D. C., K. Wan, J. Werne, T. Lund, and J. H. Hecht "Modeling Influences of Kelvin-Helmholtz Instability Dynamics on Airglow" J. Geophys. Res. , 2014 10.1002/2014JD021737
Fritts, D. C., L. Wang, and J. Werne "Gravity wave - fine structure interactions, Part 1: Influences of fine-structure form and orientation on flow evolution and instability" Journal of the Atmospheric Sciences , v.70 , 2013 , p.3710 http://dx.doi.org/10.1175/JAS-D-13-055.1
Miller, A. D., D. C. Fritts, D. Chapman, G. Jones, M. Limon, D. Araujo, J. Didier, S. Hillbrand, C. B. Kjellstrand, A. Korotkov, G. Tucker, Y. Vinokurov, K. Wan, L. Wang "Stratospheric imaging of polar mesospheric clouds: A new window on small-scale atmospheric dynamics" GRL , 2015 10.1002/2015GL064758

PROJECT OUTCOMES REPORT

Disclaimer

This Project Outcomes Report for the General Public is displayed verbatim as submitted by the Principal Investigator (PI) for this award. Any opinions, findings, and conclusions or recommendations expressed in this Report are those of the PI and do not necessarily reflect the views of the National Science Foundation; NSF has not approved or endorsed its content.

The flow of air in the atmosphere affects our lives in many ways. It drives weather systems across land and sea. It can affect the quality of the air we breathe. It can make a plane ride turbulent and bumpy. The study of how air moves in the atmosphere is called atmospheric dynamics. Atmospheric dynamics studies all altitudes – from the troposphere where we live, though the stratosphere where we fly, and above that into the mesosphere, thermosphere, ionosphere, and to the very edge of space. These layers of the atmosphere are linked; as air moves in these layers, energy can be transferred between them. Better understanding of the movement of energy and air in the upper layers of the atmosphere helps us better understand the dynamics throughout the whole atmosphere.

One way air and energy flow through the atmosphere is in the form of waves. Although we can't observe them as easily as waves on a body of water, similar waves occur in the atmosphere. Like water waves, atmospheric waves can be gentle, like when the wind is slow and only small, smooth waves form. Or atmospheric waves can be turbulent, like whitecaps that form when fast moving air flows over the water. And like waves in the water, atmospheric waves can move great distances, both horizontally and vertically. Atmospheric waves and their energy transfer are the focus of this research. We report three interesting findings from this research project.

Large water waves called tsunamis can follow large earthquakes. Tsunami prediction and tracking helps alert vulnerable communities to danger from these potentially devastating waves. Tsunamis are difficult to track on the open ocean, in part because they have exceedingly large length scales (over 100 miles) and very small wave heights, or amplitudes (shorter than 2 ft). Nevertheless, these small amplitude disturbances create waves in the air. These newly formed atmospheric waves also have very small amplitudes, and they move vertically through the atmosphere. As the waves move vertically, their amplitudes grow. The waves carry energy into upper layers of the atmosphere. If these waves reach high enough into the ionosphere, scientists who monitor this region may be able to detect them and issue tsunami warnings faster and more reliably than current methods. However, wind between the Earth's surface and the ionosphere could change the amount of energy that reaches those upper layers; they may not reach the altitude where they can be detected. Our research explores the propagation of these waves under a variety of wind conditions. Our models confirm that these waves can reach the ionosphere under many wind conditions. Our next step is to collaborate with scientists who model electrons in the ionosphere, so that we can then work with with scientists who monitor this region of the atmosphere. This research has been an important step in developing real-time tsunami monitoring.

A second part of this research explores other ways in which vertically propagating waves interact with the atmosphere. When atmospheric waves break, like whitecaps on the water, their energy and momentum are deposited to flow in the surrounding atmosphere. This is one specific way that energy can be transported between parts of the atmosphere. Predicting how waves will travel through the atmosphere, when they will break, and how that energy affects the surrounding atmosphere depends on atmospheric conditions such as wind and temperature profiles, atmospheric stabili...

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