Title: Michael A.H. Hedlin
1Studies in Atmospheric Acoustics at UCSD
- Michael A.H. Hedlin
- Laboratory for Atmospheric Acoustics
- Scripps Institution of Oceanography
- University of California, San Diego
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5Overview of presentation
- Sources
- Clear-air turbulence
- Solid Earth/Atmosphere interaction
- Large-scale storms
- Bolides
- Atmosphere structure
- Use an encoded acoustic signal?
- Sensor technology
- OFIS
- Sensor grids
6Morning Glory
- Long, narrow, white
- Travel at 40-60 km/hr
- 150 -300 m above Earths surface
- Common in the Gulf of Carpenteria
- Seen elsewhere - e.g. Sable Island, Canada
- Seen in spring near dawn
- Formed by a solitary wave in lower
- atmosphere
- Thought to occur in the presence of a
- temperature inversion -gt a wave guide
- Perhaps due to collision of opposing ocean
- breeze fronts or during thunderstorm activity
- If they occur in a dry area (e.g. over land),
- generally there is no visible cloud
Leading edge
Trailing edge
7NOAA satellite image
8Study of the Solid Earth/ Atmosphere Interaction
9Solid Earth/Atmosphere Interaction
Modified from Calais and Minster, 1995
10Ionospheric perturbations
- Due to
- Coupling between gravity waves and ionosphere
- Caused by (partial list)
- Mining blasts
- Large earthquakes
- Rocket launches
- Can be investigated using dual-frequency GPS
- Radio frequencies broadcast at 1.58 GHz and 1.23
GHz are dispersively delayed by interaction with
electrons in ionosphere - Delay proportional to electron content along
line-of-sight between receiver and satellite - Give us measure of ionospheric electron density
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12From Calais, Minster, Hofton and Hedlin, 1998
13SCIGN
Continuously recording Operated by SCEC with
NASA/JPL, USGS, UCSD Funded by WM Keck
foundation, NSF, USGS, NASA
14From Calais et al, 2003
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16Study of Storms
- Using the soon to-be-built IMS infrasound station
in Cape Verde - Can we use sound waves to learn about the
embryonic stage of hurricanes?
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18North Atlantic Hurricanes, 1931-1980
4
197
2029
2139
2217
233
24IMS Infrasound Network
25Bolides
- Can we pin down the power law using larger
bolides? - Small numerous but not readily recorded
- Largest can be studied using ground- or
space-based observing systems. - Do the large bolides hold the key to the
distribution of the largest and smallest
earth-crossing asteroids?
26The structure of the atmosphere
- Possible to characterize atmosphere using an
ATOC-style encoded acoustic signal? - Any advantage over simple explosions?
- Might improve SNR from peak-power limited sources
such as loudspeakers
27Sensor technology
28Daniels Filter
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31OFIS
32Sensor grid
33L2As Portable Instrumentation
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35L2As Portable Instrumentation
- IMS stations not necessarily tuned for natural
events - Have portable instrumentation we can use to
supplement existing facilities if necessary - Can be used to instrument new locations
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37HPWRENHigh Performance Wireless Research and
Education Network
38HPWren
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