The Effects of Turbulence in an Absorbing Atmosphere on the Propagation of Microwave Signals Used in an Active Sounding System

Proper and precise interpretation of radio occultation soundings of planetary atmospheres requires understanding the signal amplitude and phase variations caused by random perturbations in the complex index of refraction caused by atmospheric turbulence. This research focuses on understanding the turbulence and its impact on these soundings.From aircraft temperature, pressure and humidity measurements we obtained a parametric model for estimating the strength of the atmospheric turbulence in the troposphere. We used high-resolution balloon measurements to understand the spatial spectrum of turbulence in the vertical dimension.We also review and extend electromagnetic scintillation theory to include a complex index of refraction of the propagating medium. In contrast to when the fluctuations in only the real component of the index of refraction are considered, this work quantifies how atmospheric turbulent eddies contribute to the signal amplitude and phase fluctuations and the amplitude frequency correlation function when the index of refraction is complex. The generalized expressions developed for determining the signal's amplitude and phase fluctuations can be solved for planar, spherical or beam electromagnetic wave propagation.We then apply our mathematical model to the case of a plane wave propagating through a homogenous turbulence medium and estimate the amplitude variance for signals at various frequencies near the 22 GHz and 183 GHz water vapor absorption features. The theoretical results predict the impact of random fluctuations in the absorption coefficient along the signal propagation path on the signal's amplitude fluctuations. These results indicate that amplitude fluctuations arising from perturbations of the absorption field can be comparable to those when the medium has a purely real index of refraction. This clearly indicates that the differential optical depth approach devised by Kursinski et al. (2002) to ratio out the effects of turbulence on signals passing through a medium of a purely real index of refraction must be modified to include the effects of turbulent variations in the imaginary part of the refractivity.

[1]  R. A. Silverman,et al.  Wave Propagation in a Turbulent Medium , 1961 .

[2]  Gottfried Kirchengast,et al.  The ACE+ Mission: An Atmosphere and Climate Explorer based on GPS, GALILEO, and LEO-LEO Radio Occultation , 2004 .

[3]  V. Eshleman,et al.  The Atmosphere of Jupiter: An Analysis of Voyager Radio Occultation Measurements. , 1981 .

[4]  A. Kliore,et al.  The neutral atmosphere of Venus as studied with the Mariner V radio occultation experiments , 1971 .

[5]  T. VanZandt,et al.  A model for gravity wave spectra observed by Doppler sounding systems , 1985 .

[6]  Jean M. Rüeger,et al.  Refractive Index Formulae for Radio Waves , 2002 .

[7]  D. Anderson,et al.  On the radio occultation method for studying planetary atmospheres , 1968 .

[8]  Fluctuations of radio occultation signals in X/K band in the presence of anisotropic turbulence and differential transmission retrieval performance , 2007 .

[9]  G. D. Nastrom,et al.  A Climatology of Atmospheric Wavenumber Spectra of Wind and Temperature Observed by Commercial Aircraft , 1985 .

[10]  D. Gautier,et al.  The helium abundance of Saturn from Voyager measurements , 1984 .

[11]  A. Kolmogorov A refinement of previous hypotheses concerning the local structure of turbulence in a viscous incompressible fluid at high Reynolds number , 1962, Journal of Fluid Mechanics.

[12]  J. Jenkins,et al.  Radio Occultation Studies of the Venus Atmosphere with the Magellan Spacecraft: 2. Results from the October 1991 Experiments , 1994 .

[13]  G S Levy,et al.  Occultation Experiment: Results of the First Direct Measurement of Mars's Atmosphere and Ionosphere , 1965, Science.

[14]  P. Webster,et al.  TOGA COARE: The Coupled Ocean-Atmosphere Response Experiment. , 1992 .

[15]  John L. Lumley,et al.  A Century of Turbulence , 2001 .

[16]  A. von Engeln,et al.  Retrieval of temperature and water vapor profiles from radio occultation refractivity and bending angle measurements using an Optimal Estimation approach: A simulation study , 2005 .

[17]  A. Engeln A first test of climate monitoring with radio occultation instruments: Comparing two processing centers , 2006 .

[18]  Corinne S. Morse,et al.  Real-time estimation of atmospheric turbulence severity from in-situ aircraft measurements , 1995 .

[19]  J. Wyngaard,et al.  Structure–Function Parameters in the Convective Boundary Layer from Large-Eddy Simulation , 1995 .

[20]  G. Fjeldbo,et al.  The atmosphere of mars analyzed by integral inversion of the Mariner IV occultation data , 1968 .

[21]  Christopher D. Barnet,et al.  Chemical behavior of the tropopause observed during the Stratosphere-Troposphere Analyses of Regional Transport experiment , 2006 .

[22]  A. Ishimaru,et al.  Radio scintillations during occultations by turbulent planetary atmospheres. [remote sensing via flyby spacecraft] , 1980 .

[23]  R. Hodges,et al.  GENERATION OF TURBULENCE IN THE UPPER ATMOSPHERE BY INTERNAL GRAVITY WAVES. , 1967 .

[24]  Fabrizio Cuccoli,et al.  Impact of tropospheric scintillation in the Ku/K bands on the communications between two LEO satellites in a radio occultation geometry , 2006, IEEE Transactions on Geoscience and Remote Sensing.

[25]  Benjamin M. Herman,et al.  A Microwave Occultation Observing System Optimized to Characterize Atmospheric Water, Temperature, and Geopotential via Absorption , 2002 .

[26]  Benjamin M. Herman,et al.  Deriving atmospheric water vapor and ozone profiles from active microwave occultation measurements , 2001, SPIE Remote Sensing.

[27]  L. C. Andrews,et al.  An Analytical Model for the Refractive Index Power Spectrum and Its Application to Optical Scintillations in the Atmosphere , 1992 .

[28]  David P. Hinson,et al.  Initial results from radio occultation measurements with Mars Global Surveyor , 1999 .

[29]  B. Herman,et al.  An overview of the University of Arizona ATOMS project , 2004 .

[30]  Rolf König,et al.  Atmosphere sounding by GPS radio occultation: First results from CHAMP , 2001 .

[31]  O. I. Yakovlev,et al.  Scintillations of centimeter waves and the atmospheric irregularities from radio occultation data , 2003 .

[32]  W. G. Melbourne,et al.  Initial Results of Radio Occultation Observations of Earth's Atmosphere Using the Global Positioning System , 1996, Science.

[33]  O. I. Yakovlev,et al.  Attenuation and scintillation of radio waves in the Earth's atmosphere from radio occultation experiments on satellite-to- , 1995 .

[34]  W. Noble Diffraction of light by ultrasonic waves , 2019, Principles of Optics.

[35]  Sandra E. Yuter,et al.  TOGA COARE Aircraft Mission Summary Images: An Electronic Atlas , 1995 .

[36]  S. Asmar,et al.  Possible Detection of Titan's Ionosphere from Voyager 1 Radio Occultation Observations , 1995 .

[37]  R. Frehlich,et al.  Estimates of Turbulence from Numerical Weather Prediction Model Output with Applications to Turbulence Diagnosis and Data Assimilation , 2004 .

[38]  A. Kliore,et al.  Preliminary Results on the Atmospheres of Io and Jupiter from the Pioneer 10 S-Band Occultation Experiment , 1974, Science.

[39]  G R Ochs,et al.  Effects of saturation on the optical scintillometer. , 1990, Applied optics.

[40]  Steven Businger,et al.  GPS Sounding of the Atmosphere from Low Earth Orbit: Preliminary Results , 1996 .

[41]  D. Fritts Shear Excitation of Atmospheric Gravity Waves , 1982 .

[42]  J. Wyngaard,et al.  The Budgets of Turbulent Kinetic Energy and Temperature Variance in the Atmospheric Surface Layer , 1971 .

[43]  Donald H. Lenschow,et al.  The Temperature-Humidity Covariance Budget in the Convective Boundary Layer , 1978 .

[44]  A. Kolmogorov The local structure of turbulence in incompressible viscous fluid for very large Reynolds numbers , 1991, Proceedings of the Royal Society of London. Series A: Mathematical and Physical Sciences.

[45]  G. Fjeldbo,et al.  The bistatic radar‐occultation method for the study of planetary atmospheres , 1965 .

[46]  M. Sprenger,et al.  A Northern Hemispheric climatology of indices for clear air turbulence in the tropopause region derived from ERA40 reanalysis data , 2007 .

[47]  S. Asmar,et al.  First results from the Cassini radio occultations of the Titan ionosphere , 2008 .

[48]  Janet G. Luhmann,et al.  An observational study of the nightside ionospheres of Mars and Venus with radio occultation methods , 1990 .

[49]  A. D. Sarma,et al.  Effect of meteorological conditions on scintillation fading in the oxygen absorption region. , 1988, Applied optics.

[50]  A S Monin,et al.  BASIC LAWS OF TURBULENT MIXING IN THE GROUND LAYER OF ATMOSPHERE , 1954 .

[51]  U. Frisch Turbulence: The Legacy of A. N. Kolmogorov , 1996 .

[52]  Kaoru Sato,et al.  Vertical structure of atmospheric gravity waves revealed by the wavelet analysis , 1994 .

[53]  B. Wheelwright,et al.  A Single 30 cm Aperture Antenna Design for The Operation of 2 Widely Separated Frequency Bands for the Active Temperature, Ozone and Moisture Microwave Spectrometer (ATOMMS) , 2009 .

[54]  J. Lunine,et al.  Ethane Ocean on Titan , 1983, Science.

[55]  G. D. Nastrom,et al.  Theoretical Interpretation of Atmospheric Wavenumber Spectra of Wind and Temperature Observed by Commercial Aircraft During GASP , 1986 .

[56]  T. P. Yunck,et al.  AMORE: An autonomous constellation concept for atmospheric and ocean observation , 2000 .

[57]  Christian Rocken,et al.  The COSMIC/FORMOSAT-3 Mission: Early Results , 2008 .

[58]  E. Dewan,et al.  Saturation and the “universal” spectrum for vertical profiles of horizontal scalar winds in the atmosphere , 1986 .

[59]  Yu. A. Kravtsov,et al.  Principles of statistical radiophysics. 4. Wave propagation through random media. , 1989 .

[60]  K. Tung,et al.  The k−3 and k−5/3 Energy Spectrum of Atmospheric Turbulence: Quasigeostrophic Two-Level Model Simulation , 2001 .

[61]  Anthony J. Mannucci,et al.  CHAMP and SAC-C atmospheric occultation results and intercomparisons , 2004 .

[62]  J. Schofield,et al.  Observing Earth's atmosphere with radio occultation measurements using the Global Positioning System , 1997 .

[63]  S. Ungar,et al.  Sensing the earth's atmosphere with occultation satellites , 1969 .

[64]  D. Halpern Visiting TOGA's Past , 1996 .

[65]  Thomas P. Yunck,et al.  A History of GPS Sounding , 2000 .

[66]  T. P. Yunck,et al.  The role of GPS in precise Earth observation , 1988, IEEE PLANS '88.,Position Location and Navigation Symposium, Record. 'Navigation into the 21st Century'..

[67]  Geoffrey Ingram Taylor,et al.  Eddy Motion in the Atmosphere , 1915 .

[68]  K. Bowman,et al.  Observations of fine‐scale transport structure in the upper troposphere from the High‐performance Instrumented Airborne Platform for Environmental Research , 2007 .

[69]  T. Tsuda,et al.  Spectral analysis of temperature and Brunt-Väisälä frequency fluctuations observed by radiosondes , 1991 .

[70]  G. E. Wood,et al.  Radio science investigations of the saturn system with voyager 1: preliminary results. , 1981, Science.