Lecture 11: Passive Microwave Remote Sensing

Total Page:16

File Type:pdf, Size:1020Kb

Lecture 11: Passive Microwave Remote Sensing Passive Microwave Radiometry Satellite Remote Sensing • Microwave region: 1-200 GHz (0.15-30cm) SIO 135/SIO 236 • Uses the same principles as thermal remote sensing • Multi-frequency/multi-polarization sensing • Weak energy source so need large IFOV and wide Lecture 11: Passive Microwave bands Remote Sensing • Related more closely to classical optical and IR sensors than to radar (its companion active Helen Amanda Fricker microwave sensor) Passive Microwave Radiometry Passive Microwave Radiometry microwave microwave • Recall the "windows" of low opacity, which allow the transmission of only certain EMR (caused by the absorption spectra of the gasses in the • The microwave portion of the electromagnetic spectrum includes atmosphere) wavelengths from 0.1 mm to > 1 m. It is more common to refer to microwave radiation in terms of frequency, f, rather than wavelength, λ. • Atmospheric attenuation of microwave radiation is primarily through • The microwave range is approx. 300 GHz to 0.3 GHz. absorption by H 0 & O - absorption is strongest at the shortest wavelength. 2 2 Most radiometers operate in the range 0.4-35 GHz (0.8-75 cm). Attenuation is very low for λ > 3 cm (f < 10 GHz). In general µwave radiation • is not greatly influenced by cloud or fog, especially for λ > 3 cm. 1 Thermal Radiation Rayleigh-Jeans approximation • Thermal radiation is emitted by all objects above absolute zero Convenient and accurate description for spectral radiance for • In many cases the spectrum of this wavelengths much greater than the wavelength of the peak in radiation (i.e. intensity vs wavelength) the black body radiation formula i.e. λ >> λmax follows the idealized black-body radiation curve Stefan-Boltzmann law: Total energy emitted Approximation is better than 1% when hc/λkT << 1 over time by a black body is proportional to T4 or λT > 0.77 m K. For example, for a body at 300˚K, the approximation is valid Wiens displacement law: The wavelength when λ > 2.57 mm; in other words this approximation is good -1 of the spectral peak is proportional to T when viewing thermal emissions from the Earth over the microwave band. Planck’s law Rayleigh-Jeans Approximation Describes the amplitude of radiation emitted (i.e., spectral radiance) from a black body. It is generally provided in one of two forms; Lλ(λ) is the a constant radiance per unit wavelength as a function of wavelength λ and L ν(ν) is 2kcT spectral radiance is the radiance per unit frequency as a function of frequency ν. L = # a linear function of The first form is: " "4 kinetic temperature • k is Planck’s constant, c is the speed of light, ε is emissivity, T is kinetic temperature • This approximation only holds for λ >> λmax • (e.g. λ > 2.57mm @300 K) ! 2 Planck’s law Microwave Brightness Temperature To relate the two forms and establish L ν(ν), we take the derivative of L with respect to ν using the chain rule: • Microwave radiometers can measure the emitted spectral radiance received (Lλ) • This is called the brightness temperature and is linearly related to the kinetic temperature of the surface Since λ = c/ν, so that • The Rayleigh-Jeans approximation provides a simple linear relationship between measured spectral which gives: radiance temperature and emissivity Microwave Brightness Temperature At the long wavelengths, of the microwave region, the relationship between εT is also called the “brightness spectral emittance and temperature” typically shown as T wavelength can be B approximated by a straight line. "4 T = L B 2kc " ! 3 e r Snow Emissivity Example u t a Microwave Brightness Temperature r e p m Brightness temperature can be related to kinetic • e t Dry temperature through the emissivity of the material, i.e. its s s e Snow ability to emit radiation. n t h g i r dry snow (2) Soil T = "T b b kin snow water equivalent • So passive microwave brightness temperatures can be used to monitor temperature as well as properties related to Wet emissivity Snow • In the microwave region, materials have large variations in (1) Soil (3) Soil emissivity Wet snow is a strong ! absorber/emitter Microwave Radiometers • Advanced Microwave Sounding Unit (AMSU) 1978-present • Scanning Multichannel Microwave Radiometer (SMMR) 1981- 1987 • Special Sensor Microwave/Imager (SSM/I) 1987-present • Tropical Rainfall Measuring Mission (TRMM) 1997-present • Advanced Microwave Scanning Radiometer (AMSR-E) 2002-present 4 Comparative Operating Characteristics of SMMR, SSM/I, and AMSR Passive Microwave Radiometry Parameter (Nimbus-7) (DMSP-F08,F10, (Aqua) SMMR F11,F13) SSM/I AMSR-E • Passive microwave sensors use an antenna (“horn”) to Time Period 1978 to 1987 1987 to Present 2002 to Present detect photons at microwave frequencies which are then converted to voltages in a circuit Frequencies 6.6, 10.7, 18, 21, 37 19.3, 22.3, 36.5, 85.5 6.9, 10.7, 18.7, (GHz) 23.8, 36.5, 89.0 Sample 148 x 95 (6.6 GHz) 37 x 28 (37 GHz) 74 x 43 (6.9 GHz) • Scanning microwave radiometers Footprint 27 x 18 (37 GHz) 15 x 13 (85.5 GHz) 14 x 8 (36.5 GHz) Sizes (km): 6 x 4 (89.0 GHz) – mechanical rotation of mirror focuses microwave energy onto horns Passive Microwave Applications Example radiometer • Soil moisture sin φ = λ/D • Snow water equivalent r D • Sea-ice extent, concentration and type (and lake ice) R = 2 H λ /D • Sea surface temperature Atmospheric water vapor • H = 800 km H • Surface wind speed only over the oceans Φr • Cloud liquid water λ = 1cm • Rainfall rate D = 1m R ==> R = 16 km 5 Monitoring Temperatures with Passive Microwave Passive Microwave Sensing of Land Surface • Sea surface • Land surface Emissivity Differences temperature temperature • Microwave emissivity is a function of the “dielectric constant” • Most earth materials have a dielectric constant in the range of 1 to 4 (air=1, vegetation=3, ice=3.2) • Dielectric constant of liquid water is 80 • Thus, moisture content strongly affects emissivity (and therefore brightness temperature) • Surface roughness also influences emissivity Passive Microwave Sensing of Land Surface SSM/I Emissivity Differences Northern Hemisphere snow water equivalent (mm of water) 6 Atmospheric Effects Atmospheric Mapping • Mapping global water vapor • 85 GHz • At frequencies less than 50 GHz there is little effect of clouds and fog on EMR (it “sees through” clouds) • So PM can be used to monitor the land surface under cloudy conditions • In atmospheric absorption bands, PM is used to map water vapour, rain rates, clouds etc. Passive Microwave Sensing of Rain Rainfall from passive microwave sensors: • Over the ocean: Accumulated – Microwave emissivity of rain (liquid water) is about 0.9 precipitation from – Emissivity of the ocean is much lower (0.5) the Tropical – Changes in emissivity (as seen by the measured brightness Rainfall Measuring temperature) provide and estimate of surface rain rate Mission (TRMM) Similar to SSM/I • Over the land surface: – Microwave scattering by frozen hydrometeors is used as a measure of rain rate – Physical or empirical models relate the scattering signature to surface rain rates 7 Passive Microwave Remote Sensing from Space Sea-ice Sea ice is frozen seawater floating on the ocean surface Advantages Disadvantages • • Penetration through non- • Larger field of views (10- • Sea-ice has an insulating effect on the ocean (traps heat) & precipitating clouds 50 km) compared to affects the Earth’s albedo • Radiance is linearly related VIS/IR sensors Some sea ice is semi-permanent, persisting from year to year, to temperature (i.e. the Variable emissivity over • • and some is seasonal, melting and refreezing from season to retrieval is nearly linear) land season. • Highly stable instrument • Polar orbiting satellites calibration provide discontinuous • The sea ice cover reaches its minimum extent at the end of • Global coverage and wide temporal coverage at each summer and the remaining ice is called the perennial ice swath low latitudes (need to cover. create weekly composites) • Passive microwave data have shown that the spatial extent of the Arctic sea-ice cover is shrinking Passive Microwave Remote Sensing from Space Sea-ice monitoring Measures thermal emissions - as for Thermal IR, but at longer wavelengths. Rayleigh-Jeans approximation: TB = Ts ε (λ, θ) Large contrast in ε of open ocean (~0.4 @18 GHz) & sea ice (~0.9 @ 18 GHz) Sea Ice Extent Combine 19 & 37GHz data Sea Ice Concentration Lubin & Massom (2007), after Comiso (1985) 8 Emissivities of sea-ice types and open water at Sea-ice monitoring microwave frequencies Suppose we measure the thermal emissions at 10 GHz in a polar ocean which has a mixture of open seawater, young sea ice, and old sea ice. It is a warm day so both the ice and water are at the melting point. At 10 GHz (~3 cm), the EMR waves penetrate ~1 mm into the seawater and ~1 m into the ice. Tb Emissivities: seawater = 0.4 young ice = 0.95 old ice = 0.85 Brightness temperature observed by the radiometer aboard the spacecraft will reflect the variations in the emissivity of the surface. This is an excellent way to monitor the ice cover of the polar oceans and discriminate first-year ice from multi-year ice. Massom (in press) after Svendsen et al. (1993) The Passive Microwave Radiometer is the “Bread and Butter” Sensor Sea-ice monitoring for Measuring Sea-Ice Concentration and Extent DMSP SSM/I Monthly Means Including the February annual growth March and decay cycle April May & its variability. June July ~3 million km2 ~19 million km2 August September October In Operation Since 1973 November Poor Spatial Resolution (25km) December January But Penetrates Cloud and Darkness, + Complete Daily Coverage Courtesy Leanne Armand 9 First views of seasonal waxing and waning in 1973.
Recommended publications
  • Radiant Heating with Infrared
    W A T L O W RADIANT HEATING WITH INFRARED A TECHNICAL GUIDE TO UNDERSTANDING AND APPLYING INFRARED HEATERS Bleed Contents Topic Page The Advantages of Radiant Heat . 1 The Theory of Radiant Heat Transfer . 2 Problem Solving . 14 Controlling Radiant Heaters . 25 Tips On Oven Design . 29 Watlow RAYMAX® Heater Specifications . 34 The purpose of this technical guide is to assist customers in their oven design process, not to put Watlow in the position of designing (and guaranteeing) radiant ovens. The final responsibility for an oven design must remain with the equipment builder. This technical guide will provide you with an understanding of infrared radiant heating theory and application principles. It also contains examples and formulas used in determining specifications for a radiant heating application. To further understand electric heating principles, thermal system dynamics, infrared temperature sensing, temperature control and power control, the following information is also available from Watlow: • Watlow Product Catalog • Watlow Application Guide • Watlow Infrared Technical Guide to Understanding and Applying Infrared Temperature Sensors • Infrared Technical Letter #5-Emissivity Table • Radiant Technical Letter #11-Energy Uniformity of a Radiant Panel © Watlow Electric Manufacturing Company, 1997 The Advantages of Radiant Heat Electric radiant heat has many benefits over the alternative heating methods of conduction and convection: • Non-Contact Heating Radiant heaters have the ability to heat a product without physically contacting it. This can be advantageous when the product must be heated while in motion or when physical contact would contaminate or mar the product’s surface finish. • Fast Response Low thermal inertia of an infrared radiation heating system eliminates the need for long pre-heat cycles.
    [Show full text]
  • A Compilation of Data on the Radiant Emissivity of Some Materials at High Temperatures
    This is a repository copy of A compilation of data on the radiant emissivity of some materials at high temperatures. White Rose Research Online URL for this paper: http://eprints.whiterose.ac.uk/133266/ Version: Accepted Version Article: Jones, JM orcid.org/0000-0001-8687-9869, Mason, PE and Williams, A (2019) A compilation of data on the radiant emissivity of some materials at high temperatures. Journal of the Energy Institute, 92 (3). pp. 523-534. ISSN 1743-9671 https://doi.org/10.1016/j.joei.2018.04.006 © 2018 Energy Institute. Published by Elsevier Ltd. This is an author produced version of a paper published in Journal of the Energy Institute. Uploaded in accordance with the publisher's self-archiving policy. This manuscript version is made available under the Creative Commons CC-BY-NC-ND 4.0 license http://creativecommons.org/licenses/by-nc-nd/4.0/ Reuse This article is distributed under the terms of the Creative Commons Attribution-NonCommercial-NoDerivs (CC BY-NC-ND) licence. This licence only allows you to download this work and share it with others as long as you credit the authors, but you can’t change the article in any way or use it commercially. More information and the full terms of the licence here: https://creativecommons.org/licenses/ Takedown If you consider content in White Rose Research Online to be in breach of UK law, please notify us by emailing [email protected] including the URL of the record and the reason for the withdrawal request. [email protected] https://eprints.whiterose.ac.uk/ A COMPILATION OF DATA ON THE RADIANT EMISSIVITY OF SOME MATERIALS AT HIGH TEMPERATURES J.M Jones, P E Mason and A.
    [Show full text]
  • Passive Microwave Radiometer Channel Selection Based on Cloud and Precipitation Information Content Estimation
    475 Passive Microwave Radiometer Channel Selection Based on Cloud and Precipitation Information Content Estimation Sabatino Di Michele and Peter Bauer Research Department Submitted to Q. J. Royal Meteor. Soc. July 2005 Series: ECMWF Technical Memoranda A full list of ECMWF Publications can be found on our web site under: http://www.ecmwf.int/publications/ Contact: [email protected] c Copyright 2005 European Centre for Medium-Range Weather Forecasts Shinfield Park, Reading, RG2 9AX, England Literary and scientific copyrights belong to ECMWF and are reserved in all countries. This publication is not to be reprinted or translated in whole or in part without the written permission of the Director. Appropriate non-commercial use will normally be granted under the condition that reference is made to ECMWF. The information within this publication is given in good faith and considered to be true, but ECMWF accepts no liability for error, omission and for loss or damage arising from its use. Microwave Channel Selection from Precipitation Information Content Abstract The information content of microwave frequencies between 5 and 200 GHz for rain, snow and cloud wa- ter retrievals over ocean and land surfaces was evaluated using optimal estimation theory. The study was based on large datasets representative of summer and winter meteorological conditions over North Amer- ica, Europe, Central Africa, South America and the Atlantic obtained from short-range forecasts with the operational ECMWF model. The information content was traded off against noise that is mainly produced by geophysical variables such as surface emissivity, land surface skin temperature, atmospheric temperature and moisture. The estimation of the required error statistics was based on ECMWF model forecast error statistics.
    [Show full text]
  • Fundametals of Rendering - Radiometry / Photometry
    Fundametals of Rendering - Radiometry / Photometry “Physically Based Rendering” by Pharr & Humphreys •Chapter 5: Color and Radiometry •Chapter 6: Camera Models - we won’t cover this in class 782 Realistic Rendering • Determination of Intensity • Mechanisms – Emittance (+) – Absorption (-) – Scattering (+) (single vs. multiple) • Cameras or retinas record quantity of light 782 Pertinent Questions • Nature of light and how it is: – Measured – Characterized / recorded • (local) reflection of light • (global) spatial distribution of light 782 Electromagnetic spectrum 782 Spectral Power Distributions e.g., Fluorescent Lamps 782 Tristimulus Theory of Color Metamers: SPDs that appear the same visually Color matching functions of standard human observer International Commision on Illumination, or CIE, of 1931 “These color matching functions are the amounts of three standard monochromatic primaries needed to match the monochromatic test primary at the wavelength shown on the horizontal scale.” from Wikipedia “CIE 1931 Color Space” 782 Optics Three views •Geometrical or ray – Traditional graphics – Reflection, refraction – Optical system design •Physical or wave – Dispersion, interference – Interaction of objects of size comparable to wavelength •Quantum or photon optics – Interaction of light with atoms and molecules 782 What Is Light ? • Light - particle model (Newton) – Light travels in straight lines – Light can travel through a vacuum (waves need a medium to travel in) – Quantum amount of energy • Light – wave model (Huygens): electromagnetic radiation: sinusiodal wave formed coupled electric (E) and magnetic (H) fields 782 Nature of Light • Wave-particle duality – Light has some wave properties: frequency, phase, orientation – Light has some quantum particle properties: quantum packets (photons). • Dimensions of light – Amplitude or Intensity – Frequency – Phase – Polarization 782 Nature of Light • Coherence - Refers to frequencies of waves • Laser light waves have uniform frequency • Natural light is incoherent- waves are multiple frequencies, and random in phase.
    [Show full text]
  • Black Body Radiation and Radiometric Parameters
    Black Body Radiation and Radiometric Parameters: All materials absorb and emit radiation to some extent. A blackbody is an idealization of how materials emit and absorb radiation. It can be used as a reference for real source properties. An ideal blackbody absorbs all incident radiation and does not reflect. This is true at all wavelengths and angles of incidence. Thermodynamic principals dictates that the BB must also radiate at all ’s and angles. The basic properties of a BB can be summarized as: 1. Perfect absorber/emitter at all ’s and angles of emission/incidence. Cavity BB 2. The total radiant energy emitted is only a function of the BB temperature. 3. Emits the maximum possible radiant energy from a body at a given temperature. 4. The BB radiation field does not depend on the shape of the cavity. The radiation field must be homogeneous and isotropic. T If the radiation going from a BB of one shape to another (both at the same T) were different it would cause a cooling or heating of one or the other cavity. This would violate the 1st Law of Thermodynamics. T T A B Radiometric Parameters: 1. Solid Angle dA d r 2 where dA is the surface area of a segment of a sphere surrounding a point. r d A r is the distance from the point on the source to the sphere. The solid angle looks like a cone with a spherical cap. z r d r r sind y r sin x An element of area of a sphere 2 dA rsin d d Therefore dd sin d The full solid angle surrounding a point source is: 2 dd sind 00 2cos 0 4 Or integrating to other angles < : 21cos The unit of solid angle is steradian.
    [Show full text]
  • CNT-Based Solar Thermal Coatings: Absorptance Vs. Emittance
    coatings Article CNT-Based Solar Thermal Coatings: Absorptance vs. Emittance Yelena Vinetsky, Jyothi Jambu, Daniel Mandler * and Shlomo Magdassi * Institute of Chemistry, The Hebrew University of Jerusalem, Jerusalem 9190401, Israel; [email protected] (Y.V.); [email protected] (J.J.) * Correspondence: [email protected] (D.M.); [email protected] (S.M.) Received: 15 October 2020; Accepted: 13 November 2020; Published: 17 November 2020 Abstract: A novel approach for fabricating selective absorbing coatings based on carbon nanotubes (CNTs) for mid-temperature solar–thermal application is presented. The developed formulations are dispersions of CNTs in water or solvents. Being coated on stainless steel (SS) by spraying, these formulations provide good characteristics of solar absorptance. The effect of CNT concentration and the type of the binder and its ratios to the CNT were investigated. Coatings based on water dispersions give higher adsorption, but solvent-based coatings enable achieving lower emittance. Interestingly, the binder was found to be responsible for the high emittance, yet, it is essential for obtaining good adhesion to the SS substrate. The best performance of the coatings requires adjusting the concentration of the CNTs and their ratio to the binder to obtain the highest absorptance with excellent adhesion; high absorptance is obtained at high CNT concentration, while good adhesion requires a minimum ratio between the binder/CNT; however, increasing the binder concentration increases the emissivity. The best coatings have an absorptance of ca. 90% with an emittance of ca. 0.3 and excellent adhesion to stainless steel. Keywords: carbon nanotubes (CNTs); binder; dispersion; solar thermal coating; absorptance; emittance; adhesion; selectivity 1.
    [Show full text]
  • Instruments for Earth Science Measurements
    NASA SBIR 2004 Phase I Solicitation E1 Instruments for Earth Science Measurements NASA's Earth Science Enterprise (ESE) is studying how our global environment is changing. Using the unique perspective available from space and airborne platforms, NASA is observing, documenting, and assessing large- scale environmental processes with emphasis on atmospheric composition, climate, carbon cycle and ecosystems, the Earth’s surface and interior, the water and energy cycles, and weather. A major objective of the ESE instrument development programs is to implement science measurement capabilities with small or more affordable spacecraft so development programs can meet multiple mission needs and therefore, make the best use of limited resources. The rapid development of small, low cost remote sensing and in situ instruments is essential to achieving this objective. Consequently, the objective of the Instruments for Earth Science Measurements SBIR topic is to develop and demonstrate instrument component and subsystem technologies that reduce the risk, cost, size, and development time of Earth observing instruments, and enable new Earth observation measurements. The following subtopics are concomitant with this objective and are organized by measurement technique. Subtopics E1.01 Passive Optics Lead Center: LaRC Participating Center(s): ARC, GSFC The following technologies are of interest to NASA in the remote sensing subtopic “passive optics.” Passive optical remote sensing generally requires that deployed devices have large apertures and large throughput. NASA is interested primarily in instrument technologies suitable for aircraft or space flight platforms, and these inherently also prefer low mass, low power, fast measurement times, and a high degree of robustness to survive vibrations in flight or at launch.
    [Show full text]
  • Radiation Exchange Between Surfaces
    Chapter 1 Radiation Exchange Between Surfaces 1.1 Motivation and Objectives Thermal radiation, as you know, constitutes one of the three basic modes (or mechanisms) of heat transfer, i.e., conduction, convection, and radiation. Actually, on a physical basis, there are only two mechanisms of heat transfer; diffusion (the transfer of heat via molecular interactions) and radiation (the transfer of heat via photons/electomagnetic waves). Convection, being the bulk transport of a fluid, is not precisely a heat transfer mechanism. The physics of radiation transport are distinctly different than diffusion transport. The latter is a local phenomena, meaning that the rate of diffusion heat transfer, at a point in space, precisely depends only on the local nature about the point, i.e., the temperature gradient and thermal conductivity at the point. Of course, the temperature field will depend on the boundary and initial conditions imposed on the system. However, the diffusion heat flux at, say, one point in the system does not directly effect the diffusion flux at some distant point. Radiation, on the other hand, is not local; the flux of radiation at a point will, in general, be directly and instantaneously dependent on the radiation flux at all points in a system. Unlike diffusion, radiation can act over a distance. Accordingly, the mathematical description of radiation transport will employ an integral equation for the radiation field, as opposed to the differential equation for heat diffusion. Our objectives in studying radiation in the short amount of time left in the course will be to 1. Develop a basic physical understanding of electromagnetic radiation, with emphasis on the properties of radiation that are relevant to heat transfer.
    [Show full text]
  • N€WS 'RELEASE NATIONAL AERONAUTICS and SPACE Admln ISTRATION 400 MARYLAND AVENUE, SW, WASHINGTON 25, D.C
    https://ntrs.nasa.gov/search.jsp?R=19630002483 2020-03-11T16:50:02+00:00Z b " N€WS 'RELEASE NATIONAL AERONAUTICS AND SPACE ADMlN ISTRATION 400 MARYLAND AVENUE, SW, WASHINGTON 25, D.C. TELEPHONES WORTH 2-4155-WORTH. 3-1110 RELEASE NO. 62-182 MARINER SPACECRAFT Mariner 2, the second of a series of spacecraft designed for planetary exploration,- will be launched within a few days (no earlier than August 17) from the Atlantic Missile Range, Cape Canaveral, Florida, by the National Aeronautics and Space Administration. Mariner 1, launched at 4:21 a.m. (EST) on July 22, 1962 from AMR, was destroyed by the Range Safety Officer after about 290 seconds of flight because of a deviation from the planned flight path. Measures have been taken to correct the difficulties experienced in the Mariner 1 launch. These measures include a more rigorous checkout of the Atlas rate beacon and revision of the data editing equation. The data editing equation Is designed as a guard against acceptance of faulty databy the ground guidance equipment. The Mariner 2 spacecraft and its mission are identical to the first Mariner. Mariner 2 will carry six experiments. Two of these instruments, infrared and microwave radiometers, will make measurements at close range as Mariner 2 flys by Venus and communicate this in€ormation over an interplanetary distance of 36 million miles, Four other experiments on the spacecraft -- a magnetometer, ion chamber and particle flux detector, cosmic dust detector and solar plasma spectrometer -- will gather Information on interplantetary phenomena during the trip to Venus and in the vicinity of the planet.
    [Show full text]
  • An Assessment of Rain “Contamination” in ARM Two
    An assessment of rain “contamination” in ARM two-channel microwave radiometer measurements Roger Marchand1, Casey Wall1*, Wei Zhao1 and Maria Cadeddu2 1University of Washington, 2Argonne National Laboratory, *Presenting Author Case 1 Case 3 Motivation! ? !! ✔ ? � ✔ 5000 wet-window flag (open/covered) ! Microwave radiometers (MWRs) are the most commonly used and wet-window flag (open/covered) 1500 3000 accurate instruments ARM has to retrieve cloud liquid water path. open MWR open MWR Unfortunately, MWR data are not easily used in precipitating conditions. 1000 500 There are two reasons for this:" 5000 ) ) 2 1500 " 2 1. The measurements are “contaminated” by water on the MWR radome." 3000 covered! covered! MWR MWR 2. Precipitating particles can scatter microwave radiation, yet traditional 1000 500 MWR retrievals neglect scattering." 5000 " 1500 "We designed an experiment that alleviates the “wet radome” problem. 3000 1000 500 5000 The Experiment! 1500 !! 3000 500 ! Two MWRs were operated side by side in a “scanning” or tip-cal mode. Path (g/m Water Liquid 1000 Liquid Water Path (g/m Path Water Liquid One MWR was placed under a cover that kept the radome dry while still 5000 permitting measurements away from zenith (photograph below). The 1500 other MWR was operated normally, with the radome exposed to the sky. 3000 We refer to these as the “covered” and “open” MWRs, respectively. 1000 500 Coincident measurements from the 17.8 18.2 18.6 19 19.4 19.8 covered and open MWRs are 17.5 18 18.5 19 compared to estimate contamination Hours (UTC) Hours (UTC) Case 2 due to a wet radome.
    [Show full text]
  • Evidence of Diurnal Variations of Titan's Near-Surface Temperature
    EPSC Abstracts Vol. 14, EPSC2020-618, 2020 https://doi.org/10.5194/epsc2020-618 Europlanet Science Congress 2020 © Author(s) 2021. This work is distributed under the Creative Commons Attribution 4.0 License. Evidence of diurnal variations of Titan’s near-surface temperature and of a cooling effect of the northern seas from the Cassini radar/radiometer Alice Le Gall1,2, Léa Bonnefoy1,3, Robin Sultana4, Michael Janssen5, Ralph Lorenz6, and Tetsuya Tokano7 1LATMOS/IPSL, UVSQ, Université Paris-Saclay, CNRS, Sorbonne Université 2Institut Universitaire de France (IUF), Paris, France 3LESIA, Observatoire de Paris/Université PSL, CNRS, Sorbonne Université, Université Paris-Diderot, Meudon, France 4IPAG, Université Grenoble Alpes, CNRS, Grenoble, France 5Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA 6Johns Hopkins Applied Physics Laboratory, 11100 Johns Hopkins Road, Laurel, MD, USA 7Institut für Geophysik und Meteorologie, Universität zu Köln, Cologne, Germany At first order, the physical temperature of Titan’s surface can be regarded as nearly constant and predictable. Due to the low incident solar flux reaching its surface (1/1000 of what Earth receives) and the high thermal inertia of its atmosphere, diurnal, seasonal (including latitudinal) and altitudinal variations of temperature are limited as well as the effect of surface albedo (Lorenz et al., 1999). Voyager 1 radio-occultation measurements indeed show no diurnal effect and point to lapse rates in the lower atmosphere smaller than 1.5 K/km (McKay et al 1997). Voyager infrared observations indicate a pole-to-equator temperature contrast of 2-3 K (Flasar et al., 1981; 1998). The Cassini mission (2004-2017) somewhat confirmed these predictions and first measurements.
    [Show full text]
  • Technological Advances to Maximize Solar Collector Energy Output
    Swapnil S. Salvi School of Mechanical, Materials and Energy Engineering, Indian Institute of Technology Ropar, Rupnagar 140001, Punjab, India Technological Advances to Vishal Bhalla1 School of Mechanical, Maximize Solar Collector Energy Materials and Energy Engineering, Indian Institute of Technology Ropar, Rupnagar 140001, Punjab, India Output: A Review Robert A. Taylor Since it is highly correlated with quality of life, the demand for energy continues to School of Mechanical and increase as the global population grows and modernizes. Although there has been signifi- Manufacturing Engineering; cant impetus to move away from reliance on fossil fuels for decades (e.g., localized pollu- School of Photovoltaics and tion and climate change), solar energy has only recently taken on a non-negligible role Renewable Energy Engineering, in the global production of energy. The photovoltaics (PV) industry has many of the same The University of New South Wales, electronics packaging challenges as the semiconductor industry, because in both cases, Sydney 2052, Australia high temperatures lead to lowering of the system performance. Also, there are several technologies, which can harvest solar energy solely as heat. Advances in these technolo- Vikrant Khullar gies (e.g., solar selective coatings, design optimizations, and improvement in materials) Mechanical Engineering Department, have also kept the solar thermal market growing in recent years (albeit not nearly as rap- Thapar University, idly as PV). This paper presents a review on how heat is managed in solar thermal and Patiala 147004, Punjab, India PV systems, with a focus on the recent developments for technologies, which can harvest heat to meet global energy demands. It also briefs about possible ways to resolve the Todd P.
    [Show full text]