Validation of atmospheric temperature profiles derived from CHAMP radio occultation measurements - PowerPoint PPT Presentation

1 / 21
About This Presentation
Title:

Validation of atmospheric temperature profiles derived from CHAMP radio occultation measurements

Description:

1 Deutscher Wetterdienst, Offenbach. 2 Institute for Meteorology, ... Assumptions: Dry atmosphere, ideal gas, adiabatic conditions. Temperature perturbation ... – PowerPoint PPT presentation

Number of Views:52
Avg rating:3.0/5.0
Slides: 22
Provided by: mla62
Category:

less

Transcript and Presenter's Notes

Title: Validation of atmospheric temperature profiles derived from CHAMP radio occultation measurements


1
Validation of atmospheric temperature profiles
derived from CHAMP radio occultation
measurements
  • M. Lange1, Ch. Jacobi2
  • 1 Deutscher Wetterdienst, Offenbach
  • 2 Institute for Meteorology, University of
    Leipzig
  • email martin.lange_at_dwd.de

2
Outline
  • Motivation for the campaign
  • GPS Radio Occultation principle
  • The problem of detecting gravity waves by radio
    occultation measurements
  • Experimental setup
  • Results from the campaign
  • Conclusions

3
Motivation
  • Gravity waves transport energy from the
    troposphere into the middle atmosphere
    influencing the large scale circulation.
  • Champ provides temperature profiles in the range
    5-50 km on a global scale aiming to derive
    gw-characteristics from the perturbations.
  • Validation of these measurements is necessary to
    assess the quality of the temperature profiles
    for that purpose.

4
Radio Occultation measurement
GPS Sat.
LEO
5
Temperature retrieval for small perturbations
Assumptions Dry atmosphere, ideal gas, adiabatic
conditions
Refractive index
Refractivity
?N106 ?n k1 R ??
Density
??-p0 /(RT0) ?T/T0 ? p/(RT0).
Temperature perturbation
?T 1/k1 ? 106? 2/5 ?n T02 / p0.
6
Phase shift from GWs
7
The problem of detecting gravity waves by RO
measurements
8
Increased phase lag for short ?x
9
Good resolution of wave amplitudes
10
Good phase resolution for ?xgt200 km
11
Experimental setup
  • Three radiosondes are released consecutively
    around occultation events to detect vertical
    propagating gw structures.
  • During Champ occultation The 2. balloon is
    centered at a height of 15 km.
  • The time delay between balloon releases is set to
    2.5 hours corresponding to the shortest release
    timedifference including the preparation phase.

12
Deviation about 1-2 K from average
13
Periodic perturbations due to gws ?
14
2. Balloon doesnt fit Champ patterns
15
Correspondence for ?z6 km (3 km)
16
Partial correspondence in amplitude
17
Stationary phase, Amplitude damping
18
No distinct GW behaviour
19
Unrealistic Champ retrieval
20
Conclusions
  • Comparison of Temperature sounding by radiosonde
    and RO measurements at 8-20 km show mean
    deviation around 1-2 K overlayed with small scale
    perturbations of about 1-2 K. This approves the
    quality of concept and the ability to detect long
    term trends on a global scale.
  • As no gravity wave event could be clearly
    identified from the measurements no conclusion
    could be drawn if Champ is able to reproduce
    realistic phase and amplitudes as assumed from
    theoretical considerations.
  • To derive 3D wave parameter from RO measurements
    additional information is necessary. Future
    satellite missions may provide this by higher
    measurement density.

21
Acknowledgement
  • Thanks to all the Alomar people who provided very
    good support for the realisation of the project.
  • Especially to the technical staff who carried out
    the balloon measurements remotely even during
    nighttimes.
Write a Comment
User Comments (0)
About PowerShow.com