
NSF Org: |
AGS Division of Atmospheric and Geospace Sciences |
Recipient: |
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Initial Amendment Date: | January 18, 2017 |
Latest Amendment Date: | April 7, 2022 |
Award Number: | 1642644 |
Award Instrument: | Continuing Grant |
Program Manager: |
Eric DeWeaver
edeweave@nsf.gov (703)292-8527 AGS Division of Atmospheric and Geospace Sciences GEO Directorate for Geosciences |
Start Date: | February 1, 2017 |
End Date: | July 31, 2023 (Estimated) |
Total Intended Award Amount: | $372,662.00 |
Total Awarded Amount to Date: | $507,067.00 |
Funds Obligated to Date: |
FY 2018 = $105,516.00 FY 2019 = $36,231.00 FY 2020 = $135,189.00 FY 2021 = $138,568.00 FY 2022 = $59,905.00 |
History of Investigator: |
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Recipient Sponsored Research Office: |
1100 NE 45TH ST, STE 500 SEATTLE WA US 98105-4696 (206)556-8151 |
Sponsor Congressional District: |
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Primary Place of Performance: |
3380 Mitchell Lane Boulder CO US 80301-2245 |
Primary Place of
Performance Congressional District: |
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Unique Entity Identifier (UEI): |
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Parent UEI: |
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NSF Program(s): | Climate & Large-Scale Dynamics |
Primary Program Source: |
01001718DB NSF RESEARCH & RELATED ACTIVIT 01001819DB NSF RESEARCH & RELATED ACTIVIT 01001920DB NSF RESEARCH & RELATED ACTIVIT 01002021DB NSF RESEARCH & RELATED ACTIVIT 01002122DB NSF RESEARCH & RELATED ACTIVIT |
Program Reference Code(s): |
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Program Element Code(s): |
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Award Agency Code: | 4900 |
Fund Agency Code: | 4900 |
Assistance Listing Number(s): | 47.050 |
ABSTRACT
The tropical upper troposphere and lower stratosphere are home to a variety of wave motions which play key roles in weather, climate, and atmospheric circulation. Waves which are broad (horizontal wavelengths spanning several degrees latitude) but shallow (vertical wavelengths of about one to four kilometers), generated by large areas of tropical convection, are the subject of this investigation. These waves are of interest for three reasons: first, the waves can induce the formation of cirrus clouds in the tropical tropopause layer (TTL), the transition zone between the troposphere and stratosphere that extends from about 14km to 18.5km. TTL cirrus can form as rising air motions associated with the waves depress air temperatures and cause water vapor to freeze out as cirrus ice crystals. The resulting clouds may be too thin to see from the ground or from satellites, yet they have an important climatic effect as they trap outgoing infrared radiation and thus warm the atmosphere. The prevalence of such clouds is difficult to quantify, and the relative importance of wave motions as a source of TTL cirrus, in comparison to cirrus formation due to outflow of ice particles from deep cumulus clouds, is not known.
Second, the freezing out of water vapor by wave-induced temperature depression could be an important constraint on the amount of water vapor entering the stratosphere. The TTL is sometimes referred to as the "gateway to the stratosphere", as most of the water vapor in the stratosphere over the entire globe enters through the TTL. The stratosphere is extremely dry compared to the troposphere, but stratospheric water vapor is nevertheless important as it has a relatively strong greenhouse effect and can lead to the formation of the polar stratospheric clouds which are key to the formation of the ozone hole.
Third, waves can transport momentum from the troposphere to the stratosphere, and wave momentum transport is the primary driver of the stratospheric Quasi-Biennial Oscillation (QBO), an alternation between easterly and westerly winds occurring over the global tropics with a cycling time in excess of two years. While the QBO is narrowly confined to the low-latitude stratosphere, it can influence weather and climate worldwide through its effects on prominent modes of climate variability such as the North Atlantic Oscillation. While the theory of wave momentum transport is well established, uncertainties remain as to the relative importance of different wave types in driving the QBO, and current weather and climate models have difficulty in simulating it.
This project seeks to improve understanding of waves in the TTL by building and launching a balloon-borne instrument which receives positioning signals from satellites of the Global Navigation Satellite System (GNSS, which includes the GPS satellites launched by the US). The GNSS signals are refracted as they pass through the atmosphere, and the amount of refraction can be used to infer air temperature in the upper troposphere. Because the profiles are retrieved from the rising and setting, or occultation, of the GNSS satellites relative to the receiver, the balloon-borne instrument has the acronym ROC, for Radio OCcultation.
ROC is developed for use on balloons flow as part of the Strateole-2 field campaign organized by the Centre National d'Etudes Spatiales (CNES), the French Space Agency, and the Laboratoire de Meteorologie Dynamic (LMD) of the University of Paris-Saclay. Strateole-2 is a five-year campaign, with a small validation deployment in 2018 and full science deployments in 2020-2021 and 2022-2023. Balloons are launched from the Seychelles (about 5S in the Indian Ocean), with the expectation that each balloon will circle the earth for up to 90 days and observe the TTL between 20S and 15N. This award supports US participation in the validation campaign and the first full science deployment, along with post-campaign analysis. It is one of three awards made to US PIs for participation in Strateole-2, the full set being AGS-1643022, AGS-1642277/1642246, and AGS-1642650/1653644.
ROC is oriented to retrieve signals from GNSS satellites on either side of the balloon flight path, with observations taken between 8km and the flight level of about 20km and a vertical resolution between 200m and 250m. The observing geometry is such that observations at lower levels are farther away from the balloon, so that observations at 18, 15, and 12km altitude correspond to distances of roughly 100, 200, and 300km on either side of the balloon. The waves of interest have periods from hours to days and ROC can record two to three occultations per hour. Thus the three-dimensional structure of the waves is captured by the ROC measurements as the balloon advances along its trajectory.
ROC is accompanied by two other instruments which provide complementary observations. One is the Balloonborne Cloud Overshoot Observation Lidar (BeCOOL), provided by the Laboratoire Atmospheres, Milieux, Observations Spatiales (LATMOS, a laboratory of the Institut Pierre Simon Laplace) in collaboration with CNES. The lidar provides measurements of cirrus clouds which can be combined with ROC observations to examine the role of wave motions in generating cirrus clouds. The other is the Temperature SENsor (TSEN), an instrument from LMD which records atmospheric temperature and pressure at the gondola. Gondola displacements are precisely determined by ROC, and TSEN observations are used to factor out gondola movement relative to the ambient wave motion (these are super-pressure balloons which fly at a level of constant density). The displacement data are then used to estimate the wave momentum flux at flight level associated with the large-scale waves observed by ROC.
The work has scientific broader impacts due to the value of the observations for addressing a variety of questions regarding the effect of wave motions on TTL clouds, stratospheric humidity, and the QBO. Observations collected in this project will be made available to the research community from servers at the Laboratory for Atmospheric and Space Physics at the University of Colorado so that they can be freely examined by the research community. The project also engages undergraduate students through a research class, offered simultaneously at the University of California San Diego, the University of Arizona (UA), and the Autonomous University of Mexico (UNAM), in which students design a research project based on a test flight of ROC. The class is followed by undergraduate research internships at UCSD, UA, the Research Experiences in Solid Earth Sciences for Students (RESESS) program at UNAVCO (the University NAVSTAR Consortium, dedicated to applying GNSS technology to earth science), and the Significant Opportunities in Atmospheric Research and Science (SOARS) program of the University Corporation for Atmospheric Research. Beyond these broader impacts, the project supports two graduate students.
PUBLICATIONS PRODUCED AS A RESULT OF THIS RESEARCH
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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.
Through collaboration with our partners at Scripps Institution of Oceanography (see also grant #1642650), this project aimed to design and deploy next generation GPS receivers for Radio OCcultation (ROC) on board long-duration, super-pressure stratospheric balloons and to execute continuous sequences of atmospheric temperature profiles on either side of balloon trajectories in order to sample equatorial atmospheric waves in three dimensions. Characterization of equatorial waves with ROC measurements constitutes an important step toward improving tropical weather forecasts and subseasonal-to-seasonal outlooks. Improvements in tropical forecasting skill have perpetually lagged behind skill improvements at midlatitudes, primarily because of the poor characterization of tropical atmospheric waves. Tropical waves organize tropical rain patterns, and as they travel upward into the stratosphere they drive a global oscillation in the winds that switches from eastward to westward with a quasi-regular 2.3-year period. This global wind oscillation in turn feeds back onto the waves, changing their propagation, changing the altitudes where the waves drive the circulation, and affecting precipitation patterns and forecasts. A fundamental difference between the tropics and the extratropics is the existence of large-scale tropical waves that cannot be characterized by the current set of available temperature measurements that are observed globally by satellites. The tropical atmosphere is a special place in this regard because many large-scale waves exist there that are "unbalanced", which in this context means that without coincident wind observations their characterization requires unusually densely sampled temperature profiles with high vertical resolution. The ROC measurements are uniquely able to accomplish this task.
The ROC instrument flew on specially designed long-duration balloons built and controlled by the French space agency CNES. These balloons have a spherically shaped envelope that is partially filled with helium before launch. Once released, the lighter-than-air helium lifts the balloon and its gondola with instruments, rising through the increasingly rarified air above until it reaches the stratosphere where the balloon is stretched to its full spherical shape and volume. The envelope of this type of balloon does not stretch beyond this final volume, so the balloon eventually stops rising and floats at the height where the density inside the balloon equals the density of the air outside, and there it can drift passively with the wind for up to three months. The drift height of the balloons carrying ROC was approximately 66,000 ft, considerably higher than commercial flight altitudes. From this stratospheric perch, ROC scans the horizon, detecting GPS signals and following those signals as the GPS satellites appear to set behind the horizon or rise above the horizon. These GPS signals were subsequently used by our Scripps collaborators to infer changes in atmospheric temperature as a function of height at locations below the balloon and in various directions surrounding the balloon position. With measurements over weeks or months, this creates an extremely dense set of high-resolution temperature measurements, which we used to characterize tropical atmospheric waves below and surrounding the balloon.
ROC's first flight opportunity was on a balloon launched from the Seychelles in the Indian Ocean on December 5, 2019, and the flight duration was 57 days. Temperature profiles were obtained at a rate of over 40 per day. Waves observed in the ROC data during this flight include a wide variety of tropical waves with oscillation periods ranging from a few hours up to 20 days. Our analysis identified a type of wave called a Kelvin wave that had a long wavelength spanning half the entire circumference of the Earth (20,000 km = 12,500 miles), but with a vertical wavelength of only 3 km (=2 miles). The very high-resolution ROC measurements showed the strength of this wave was considerably underestimated by the best global weather forecasts. Additional measurements of 3-4-day period gravity waves showed even finer vertical wavelengths, close to 2 km, which are too short to be resolved in the forecasts. The ROC data are publicly available through the link https://strateole2.aeris-data.fr and research using these data will continue into the future.
The second flight opportunity for ROC was in October 2021, but unfortunately noise in these measurements was much larger than expected, and the noise obscured the atmospheric wave signals. Tests in the following year identified extreme cold temperatures as the cause of the noise problem and identified specific types of GPS receivers that will perform best when ROC has a next chance to fly again in 2025.
Last Modified: 12/28/2023
Modified by: M Joan Alexander
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