Publications by Fred Taylor

Remote sensing of planetary atmospheres: Venus

ADV SPACE RES 21 (1998) 409-418

FW Taylor

More than any other planet except the Earth, Venus has been the subject of a variety of remote sensing investigations over a wide range of wavelengths. Since Venus has complete cloud cover, with a complex composition and layering, the retrieval of the information from these measurements is particularly challenging. The problem is further complicated by the high temperatures and pressures found in the deep atmosphere, resulting in a novel and interesting radiative transfer problem even before scattering and absorption by cloud particles is taken into account. This paper reviews the achievements so far of remote sensing of Venus and future challenges and opportunities. (C) 1998 COSPAR. Published by Elsevier Science Ltd.

The solar reflected component in Jupiter's 5-μm spectra from NIMS/Galileo observations

Journal of Geophysical Research E: Planets 103 (1998) 23043-23049

P Drossart, M Roos-Serote, T Encrenaz, E Lellouch, KH Baines, RW Carlson, LW Kamp, GS Orton, S Calcutt, P Irwin, FW Taylor, A Weir

A comparison between low-flux dayside and nightside spectra of Jupiter recorded by the Galileo near-infrared mapping spectrometer (NIMS) experiment gives the first accurate estimate of the solar reflected component at 5 μm, in the equatorial zone of Jupiter. A minimum flux level of about 0.6 μW cm-2sr-1V/μm is found on the dayside, compared with 0.1 /μW cm-2sr-1/μm on the nightside. These fluxes are 100-800 times lower respectively than the bright 5-μm thermal emission in the north equatorial belt (NEB) hot spots. The day/night difference can be interpreted as a solar reflected component from a cloud, presumably the ammonia cloud, with an albedo of the order of 15%, located at a pressure level of 0.79 bar or at higher altitudes (corresponding to cloud temperature of 160 K or lower). Compared to the measurements in hot spots made at other wavelengths from ground-based observations and from NIMS real time spectra, they imply a high cloud opacity in cold regions at atmospheric levels where the cloud optical depth in the hot spots is very low. The residual flux on the nightside arises from (1) a very small cloud transparency giving some access to deeper thermal emission or (2) as high-resolution solid-state imaging (SSI) images of Galileo suggest, to cloud inhomogeneities, with clearer regions of medium brightness temperatures, mixed with dark regions of much lower thermal emission. If the former have the same brightness as a typical hot spot, a filling factor of a few percent is sufficient to explain the observed flux level on the nightside cold regions. Copyright 1998 by the American Geophysical Union.

Non local thermodynamic equilibrium (LTE) atmospheric limb emission at 4.6 mu m - 2. An analysis of the daytime wideband radiances as measured by UARS improved stratospheric and mesospheric sounder


M Lopez-Puertas, G Zaragoza, MA Lopez-Valverde, FW Taylor

Global evolution of the Mt Pinatubo volcanic aerosols observed by the infrared limb-sounding instruments CLAES and ISAMS on the Upper Atmosphere Research Satellite

J GEOPHYS RES-ATMOS 102 (1997) 1495-1512

A Lambert, RG Grainger, CD Rodgers, FW Taylor, JL Mergenthaler, JB Kumer, ST Massie

The cryogenic limb array etalon spectrometer (CLAES) and the improved stratospheric and mesospheric sounder (ISAMS) instruments on board the Upper Atmosphere Research Satellite (UARS) have been used to produce global information on the Mt. Pinatubo volcanic aerosol for the period from October 1991 to April 1993, The Satellite infrared extinction measurements near 12 mu m are converted into the aerosol-related parameters necessary for modelling the effects of the volcanic aerosol on the aeronomy of the stratosphere and are presented as zonal mean distributions for 80 degrees S to 80 degrees N averaged over similar to 35-day periods. The aerosol composition is derived from the CLAES and ISAMS temperature measurements and the water vapour abundances are obtained from the microwave limb sounder (MLS). The aerosol volume density is obtained from the extinction measurements from which the Surface area density and the effective particle radius are estimated. The maximum aerosol surface area density has a value of about 50 mu m(2) cm(-3) at a height of 24 km at the equator in October 1991, before decaying exponentially with a time constant of 443 +/- 10 days. The surface area density remained well above preeruption values in April 1993. The effective particle radius in the tropics decays monotonically from 0.65 mu m in October 1991 to 0.4 mu m in April 1993. The global aerosol sulphate mass loading is 19.5 Mt in October 1991 and decays exponentially with a time constant of 342 +/- 8 days to a value of 4.3 Mt by April 1993. Four months after the eruption the calculated optical thickness at 1.02 mu m was similar to 0.25 in the tropics. Rate constants are derived for the heterogeneous reactions of N2O5 and ClONO2 on the sulphate aerosols. The application of the aerosol parameters to the investigation of tracer transport, heterogeneous chemistry, and radiative transfer is discussed.

Radiative transfer models for Galileo NIMS studies of the atmosphere of Jupiter

ADV SPACE RES 19 (1997) 1149-1158

PGJ Irwin, SB Calcutt, FW Taylor

Scientific results from NIMS observations of Venus have been extensively reported in the literature, while those of Jupiter have, at the time of writing, just barely commenced. The planning and interpretation of studies of these planets, with their massive atmospheres and exotic compositions (by terrestrial standards), requires a comprehensive treatment of radiative transfer in both. This paper describes work done at Oxford to develop the underlying theory and practical radiative transfer schemes, with particular reference to the NIMS wavelength range, spectral resolution, and scientific objectives for Jupiter. Equivalent work for Venus has already been reported in the literature (e.g. Kamp and Taylor, 1990) and will not be covered in detail here. (C) 1997 COSPAR. Published by Elsevier Science Ltd.

UARS first global N<inf>2</inf>O<inf>5</inf> data sets: Application to a stratospheric warming event in January 1992

Journal of Geophysical Research Atmospheres 102 (1997) 3575-3582

JB Kumer, SR Kawa, AE Roche, JL Mergenthaler, SE Smith, FW Taylor, PS Connell, AR Douglass

For the first time, global measurements of N<inf>2</inf>O<inf>5</inf> are available for study. N<inf>2</inf>O<inf>5</inf> has long been a missing link in large-scale observations of stratospheric nitrogen species, the chemical family that comprises the major global loss cycle for ozone above about 25 km [McElroy et al., 1992]. N<inf>2</inf>O<inf>5</inf> is also an important intermediate in conversion of NO<inf>x</inf> to HNO<inf>3</inf>, thus limiting the effect of nitrogen-catalyzed ozone destruction below about 25 km [Fahey et al., 1993]. The new N<inf>2</inf>O<inf>5</inf> observations come from both the Cryogenic Limb Array Etalon Spectrometer (CLAES) and Improved Stratospheric and Mesospheric Sounder (ISAMS) instruments on the Upper Atmosphere Research Satellite (UARS), providing near-global coverage at high spatial and temporal resolution for almost 20 months. Here we focus on data obtained near 40 km during a stratospheric warming in January 1992. The N<inf>2</inf>O<inf>5</inf> fields show globally coherent structures with large variation in response to global transport coupled with highly temperature dependent chemistry. Comparison of the data with chemistry and transport models indicates that our understanding of processes controlling N<inf>2</inf>O<inf>5</inf> amounts and the interaction with other reactive nitrogen species is largely accurate under most conditions; however, an exceptional disagreement is found in the prolonged polar dark. This example demonstrates the utility of global data to understand the combined effects of chemistry and transport on N<inf>2</inf>O<inf>5</inf> under a wide range of conditions.

A GCM climate database for Mars: For mission planning and for scientific studies

ADV SPACE RES 19 (1997) 1213-1222

PL Read, M Collins, F Forget, R Fournier, F Hourdin, SR Lewis, O Talagrand, FW Taylor, NPJ Thomas

The construction of a new database of statistics on the climate and environment of the Martian atmosphere is currently under way, with the support of the European Space Agency. The primary objectives of this database are to provide information for mission design specialists on the mean state and variability of the Martian environment in unprecedented detail, through the execution of a set of carefully validated simulations of the Martian atmospheric circulation using comprehensive numerical general circulation models. The formulation of the models used are outlined herein, noting especially new improvements in various schemes to parametrize important physical processes, and the scope of the database to be constructed is described. A novel approach towards the representation of large-scale variability in the output of the database using empirical eigenfunctions derived from statistical analyses of the numerical simulations, is also discussed. It is hoped that the resulting database will be of value for both scientific and engineering studies of Mars' atmosphere and near-surface environment. (C) 1997 COSPAR. Published by Elsevier Science Ltd.

Pathfinder on Mars

ASTRONOMY & GEOPHYSICS 38 (1997) 15-16

FW Taylor

Reference Model for Methane and Nitrous Oxide

Advances in Space Research 18 (1996) 91-124

FW Taylor, A Dudhia, CD Rodgers

Data from the Stratospheric and Mesospheric Sounder (SAMS) on Nimbus 7 have been used as the basis for a model of the abundances of nitrous oxide and methane in the stratosphere. The model is presented in tabular form on seventeen pressure surfaces from 20 to 0.1-mb, in 10° latitude bins from 50°S to 70°N, and for each month of the year. Some details of the acquisition of the data which went into the model, its limitations, and the general behaviour of methane and nitrous oxide in the middle atmosphere are given. Formal errors in the data and other uncertainties, interannual variability, and systematic trends are discussed. As expected, no trends which exceed the estimated error in the data are found in either methane or nitrous oxide over the five-year period of SAMS observations.

Semidiurnal and diurnal temperature tides (30-55 km): Climatology and effect on UARS-LIDAR data comparisons


P Keckhut, ME Gelman, JD Wild, F Tissot, AJ Miller, A Hauchecorne, ML Chanin, EF Fishbein, J Gille, JM Russell, FW Taylor

Remote sounding of the Martian atmosphere in the context of the InterMarsNet mission: General circulation and meteorology

PLANET SPACE SCI 44 (1996) 1347-1360

FW Taylor, SB Calcutt, PGJ Irwin, DJ McCleese, JT Schofield, DO Muhleman, RT Clancy, CB Leovy

A concept has been developed for a remote sensing experiment to investigate the physics of the Martian atmosphere from a spin-stabilized orbiter, like that planned for the InterMarsNet mission. Using coincident infrared and microwave channels and limb-to-limb scanning, it can map the planet much more extensively than previously in temperature atmospheric dust loading, and humidity. When combined with one or more surface stations measuring the same variables, the sounder experiment can contribute to major progress in understanding the general circulation and dust and water cycles of the atmosphere of Mars, and the characterization of medium-scale meteorological systems. Copyright (C) 1996 Elsevier Science Ltd

Stratospheric methane distributions: Comparisons of a CIRA reference model and recent observational data


SL Ruth, JJ Remedios, FW Taylor, AE Roche, JB Kumer

Dinitrogen pentoxide measurements from the improved stratospheric and mesospheric sounder: Validation of preliminary results


SE Smith, A Dudhia, PE Morris, JJ Remedios, CD Rodgers, FW Taylor, BJ Kerridge, MP Chipperfield, JB Kumer, AE Roche, MR Gunson

Ozone in the middle atmosphere as measured by the improved stratospheric and mesospheric sounder


BJ Connor, CJ Scheuer, DA Chu, JJ Remedios, RG Grainger, CD Rodgers, FW Taylor

Comparison of CLAES preliminary N2O5 data with correlative data and a model


JB Kumer, JL Mergenthaler, AE Roche, RW Nightingale, F Zele, JC Gille, ST Massie, PL Bailey, PS Connell, MR Gunson, MC Abrams, GC Toon, B Sen, JF Blavier, SE Smith, FW Taylor

Validation of measurements of carbon monoxide from the improved stratospheric and mesospheric sounder


MA LopezValverde, M LopezPuertas, JJ Remedios, CD Rodgers, FW Taylor, EC Zipf, PW Erdman

Calculated k distribution coefficients for hydrogen- And self-broadened methane in the range 2000-9500 cm<sup>-1</sup>from exponential sum fitting to band-modelled spectra

Journal of Geophysical Research E: Planets 101 (1996) 26137-26154

PGJ Irwin, SB Calcutt, FW Taylor, AL Weir

The spectral band data derived by Strong et al. [1993] for laboratory-measured transmission spectra of hydrogen-broadened methane at 10 cm-1resolution have been fitted with k coefficients over a wide range of pressures and temperatures representing those likely to be encountered in the atmosphere of Jupiter. The mean fitting error is found to be only 2.0×10-3in transmission. These data are essential for the scattering calculations likely to be necessary for analysis of the data from the Near Infrared Mapping Spectrometer aboard the NASA Galileo spacecraft. The new data have significant advantages over those previously derived by Baines et al. [1993] in that they cover a wider spectral range, are applicable to longer paths, and also apply to the hydrogen-broadened case, which is the dominant broadening mechanism in this atmosphere. A similar table has also been calculated for the self-broadening case for comparison. Copyright 1996 by the American Geophysical Union.

The H<inf>2</inf>so<inf>4</inf> component of stratospheric aerosols derived from satellite infrared extinction measurements: Application to stratospheric transport studies

Geophysical Research Letters 23 (1996) 2219-2222

A Lambert, RG Grainger, HL Rogers, WA Norton, CD Rodgers, FW Taylor

The ambient water vapour and temperature conditions of stratospheric sulphate aerosol particles govern their composition and thereby influence their infrared extinction properties. This causes problems in the use of the infrared aerosol extinction as a tracer because variations in the aerosol composition modify the changes in extinction that may arise from the transport of aerosols. An improved tracer which can be derived from measurements of the infrared aerosol extinction, temperature and water vapour abundance, is the H2SO4 component of aerosols. The application of this tracer to studies of stratospheric transport is demonstrated using data from instruments on the Upper Atmosphere Research Satellite and the results are compared to a contour advection calculation. Copyright 1996 by the American Geophysical Union.

Validation of nitrogen dioxide measurements from the improved stratospheric and mesospheric sounder


WJ Reburn, JJ Remedios, PE Morris, CD Rodgers, FW Taylor, BJ Kerridge, RJ Knight, J Ballard, JB Kumer, ST Massie

Validation studies using multiwavelength cryogenic limb array etalon spectrometer (CLAES) observations of stratospheric aerosol


ST Massie, JC Gille, DP Edwards, PL Bailey, LV Lyjak, CA Craig, CP Cavanaugh, JL Mergenthaler, AE Roche, JB Kumer, A Lambert, RG Grainger, CD Rodgers, FW Taylor, JM Russell, JH Park, T Deshler, ME Hervig, EF Fishbein, JW Waters, WA Lahoz