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Climatology of Superrefraction Observed by GPS Radio Occultation

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Title: Climatology of Superrefraction Observed by GPS Radio Occultation


1
Climatology of Superrefraction Observed by GPS
Radio Occultation
  • Dione (Dee) Lee Rossiter
  • University of California, Berkeley
  • COSMIC-UCAR

2
Outline
  • Background
  • GPS Radio Occultation
  • The Problem Superrefraction
  • Motivation
  • GPS Radio Occultation
  • Current Research
  • Proposed Questions
  • Procedure
  • Generating Plots
  • Finding Reoccurring Features
  • Conclusions

3
Background Global Positioning System (GPS)
Satellites
Low-Earth Orbit (LEO) Satellites
  • Equipped with a GPS receiver, a LEO can track GPS
    radio signals
  • These GPS signals are required to pass through
    the atmosphere where they are refracted

GPS Satellite
LEO Orbit
Atmosphere
Radio Signal
LEO Satellite
4
Background Radio Occultation (RO)
  • GPS signals are refracted by the Earths
    atmosphere as they travel to a receiver in LEO.
  • Refractivity is a function of
  • - electron density in the
    ionosphere
  • - temperature, pressure, and water
    vapor in the stratosphere and
    troposphere

5
Background Radio Occultation (RO)
From Anthes et al., 2003
  • Phase and amplitude
  • ?Doppler shift
  • positions and velocities
  • ?Bending angles, a, as a function of impact
    parameter, a

?Profiles of refractivity vs. altitude
?Profiles of atmospheric properties vs.
altitude
6
Motivation GPS RO
Meteorology
  • Provide global coverage in time and space
  • Provide fundamentally unbiased atmospheric
    measurements
  • The technique is mission independent
  • Provide advancements in space weather research
  • GPS RO will provide high quality soundings at a
    low cost!

Climate
Ionosphere
7
The Problem Superrefraction
  • Caused by a sharp decrease in refractivity with
    an increase of altitude
  • The radius of curvature, rc, becomes smaller than
    the radius of the atmosphere, ra
  • Ray remains trapped in the atmosphere and results
    in a temporary extinction of the radio signal
    reaching the LEO
  • Commonly occurs at the top of the Planetary
    Boundary Layer (PBL) at 2 km

8
BackgroundRadio Occultation (RO)
From Anthes et al., 2003
  • Phase and amplitude
  • ?Doppler shift
  • positions and velocities
  • ? Bending angles a as a function of a

?Profiles of refractivity vs. altitude
9
Abel Transform
  • The Abel inversion integrates from the top of the
    atmosphere to the surface
  • The Abel inversion works great up until the
    superrefraction layer

10
The Problem Superrefraction
True Retrieved
True Retrieved
True Retrieved
From Sokolovskiy, 2003
Below the superrefraction layer the function
  • Results in a negative N bias
  • Becomes multi-valued and therefore invalid

11
Motivation Current Research
  • GPS RO will soon be utilized in an array of
    atmospheric models (weather, climate,
    ionospheric composition)
  • Attaining the highest level of accuracy is
    essential!
  • Problem Superrefraction causes errors!
  • Understand ? Predict ? Remove Errors

12
Proposed Questions
  • What are the reoccurring features of
    superrefractions?
  • Annual?
  • Seasonal?
  • Where does it occur?
  • Geographically?
  • Topographically?
  • Can we predict where or when it might occur or
    recognize when it is occurring in order to
    truncate the sounding or to remove the negative
    bias altogether?
  • (Understand ? Predict ? Remove Errors)

13
Generating Plots
  • Divide the globe by 15 latitudinally

14
Generating Plots
  • Divide the globe by 15 latitudinally
  • Take latitude band and divide up by 19 lon.
    bins
  • Combine Challenging Mini-Satellite Payload for
    Geophysical Research and Application (CHAMP)
    occultations within bin

15
Generating Plots
  • Divide the globe by 15 latitudinally
  • Take latitude band and divide up by 19 lon
    bins
  • Combine Challenging Mini-Satellite Payload for
    Geophysical Research and Application (CHAMP)
    occultations within bin
  • Create refractivity vs. altitude stats for
    each lat lon grid against European Center for
    Medium Range Weather Forecast (ECMWF) model
  • Color code the different mean bias
    interpolate across entire latitude band

16
June-Aug/75º to 90º lat
-90
17
June-Aug/0º to 15º lat
2003
18
Dec-Feb/-75º to -60º lat
2003
19
Dec-Feb/-30º to -15º lat
2003
20
Finding Reoccurring Features
Dec-Feb/-30º to -15º lat
2001
2002
2003
Altitude (km)
Altitude (km)
Altitude (km)
Longitude
Longitude
Longitude
21
Scatter Plot
  • Measures individual occultations bias at 0.5 km
    that did not agree within 4 of ECMWF model
  • Color codes the different bias

22
Scatter Plots
  • Midlatitude mostly effected
  • Land vs. ocean
  • High occurrence in some areas

Dec-Feb 2003
  • Greater neg. bias in some areas
  • Less positive bias

23
Soden Bretherton (1994)
  • Compare ECMWF with Special Sensor
    Microwave/Imager (SSM/I)
  • Conclude the model had problems in predicting the
    dry subtropical ridges off the west coast of
    continents where marine stratocumulus clouds
    often occur
  • This is where dry air sinks from above and
    creates a sharp vertical gradient in water vapor
    near the top of the PBL
  • conditions needed for superrefraction to occur!!!

24
Finding Trends
Latitude
CHAMP-ECMWF June-Aug 2003
(10)-2
Longitude
25
Finding Trends
Latitude
(10)-2
CHAMP-ECMWF Dec-Jan 2003
Longitude
26
Conclusions
  • There are seasonal and geographic features
    associated with superrefraction
  • Geographically, superrefraction occurs off the
    west coast of continents
  • We can possibly use the superrefraction
    climatology found in this research to predict
    where and when to truncate soundings or correct
    or negative bias
  • Future Research Diurnal cycles in the PBL

27
Acknowledgements
  • Research Mentors
  • Bill Kuo
  • Bill Schreiner
  • Chris Rocken
  • Writing Mentor
  • Chris Halvorson
  • Doug Hunt
  • Karl Hudnut
  • Kim Prinzi-Kimbro
  • All of the COSMIC project office
  • All of the SOARS staff and protégés

28
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