1 Water Vapour Radiometry Bob Sault. 2 The Neutral Atmosphere H20H20 O2O2 H20H20 O2O2.

Slides:



Advertisements
Similar presentations
Ewan OConnor, Robin Hogan, Anthony Illingworth, Nicolas Gaussiat Liquid water path from microwave radiometers.
Advertisements

Radar/lidar observations of boundary layer clouds
Electro-magnetic radiation
Cloud Radar in Space: CloudSat While TRMM has been a successful precipitation radar, its dBZ minimum detectable signal does not allow views of light.
1 Ionospheres of the Terrestrial Planets Stan Solomon High Altitude Observatory National Center for Atmospheric Research
Introduction to Astrophysics Lecture 3: Light. Properties of light Light propagates as a wave, and corresponds to oscillations of electric and magnetic.
Thermal (blackbody) spectra. Recap No HW this week Project due 11/22 Light /electromagnetic energy –Wavelength, frequency, energy –Electromagnetic spectrum:
Electromagnetic Radiation Electromagnetic Spectrum Radiation Laws Atmospheric Absorption Radiation Terminology.
TRMM Tropical Rainfall Measurement (Mission). Why TRMM? n Tropical Rainfall Measuring Mission (TRMM) is a joint US-Japan study initiated in 1997 to study.
Atmospheric phase correction for ALMA Alison Stirling John Richer Richard Hills University of Cambridge Mark Holdaway NRAO Tucson.
Atmospheric Emission.
Fourth IRAM Millimeter Interferometry School 2004: The atmosphere 1 The atmosphere at mm wavelengths Jan Martin Winters IRAM, Grenoble.
Energy interactions in the atmosphere
Satellite observation systems and reference systems (ae4-e01) Signal Propagation E. Schrama.
Lecture 3: The greenhouse effect. Other concepts from Lecture 2 Temperature Scales Forms of Heat Transfer Electromagnetic Spectrum Stefan-Boltzmann Law.
Reminder of radiance quantities I λ RadianceW m -2 μm -1 sr -1 Intensity (Monochromatic) F λ Spectral IrradianceW m -2 μm -1 Monochromatic Flux F(Broadband)
CHE/ME 109 Heat Transfer in Electronics LECTURE 26 – RADIATION SURFACE DESIGN.
* Reading Assignments:
6-1 EE/Ge 157b Week 6 EE/Ae 157 a Passive Microwave Sensing.
PHYSICS 103: Lecture 17 Agenda for Today: Temperature and Heat
Chapter 3 Light and Matter
Blackbody Radiation & Atomic Spectra. “Light” – From gamma-rays to radio waves The vast majority of information we have about astronomical objects comes.
Stellar Parallax & Electromagnetic Radiation. Stellar Parallax Given p in arcseconds (”), use d=1/p to calculate the distance which will be in units “parsecs”
Page 1© Crown copyright Distribution of water vapour in the turbulent atmosphere Atmospheric phase correction for ALMA Alison Stirling John Richer & Richard.
Random Media in Radio Astronomy Atmospherepath length ~ 6 Km Ionospherepath length ~100 Km Interstellar Plasma path length ~ pc (3 x Km)
1 EE 543 Theory and Principles of Remote Sensing Derivation of the Transport Equation.
Remote Sensing Energy Interactions with Earth Systems.
ATCA synthesis workshop - May ATCA – Calibration at mm wavelengths Rick Forster University of California, Berkeley Hat Creek Radio Observatory Berkeley-Illinois-Maryland.
NATURE OF LIGHT.  The electromagnetic spectrum comprise of the following:  1. Radio waves  Electromagnetic radiation with wavelengths that range from.
Lesson 01 Atmospheric Structure n Composition, Extent & Vertical Division.
SATELLITE METEOROLOGY BASICS satellite orbits EM spectrum
Physics of the Atmosphere II
AST 443: Submm & Radio Astronomy November 18, 2003.
Wave property of light Waves can carry energy Wavelength ( ) : distance between successive crests (or troughs) Frequency (f): # of waves passing a point.
Light hits Matter: Refraction Light travels at different speeds in vacuum, air, and other substances When light hits the material at an angle, part of.
Climate Long time, Large Area. Weather short term, small area.
Language of the Energy Cycle: The Electromagnetic Spectrum
Water Vapor In The Atmosphere: An Examination For CARMA Phase Correction Y.-S. Shiao, L. W. Looney and L. E. Snyder Department of Astronomy University.
PASSIVE MICROWAVES Figure 5-2 Sensitivity of brightness temperature to geophysical parameters over ocean surface.
COST 723 Training School - Cargese October 2005 KEY 1 Radiative Transfer Bruno Carli.
Newton’s Experiments with Light. Electomagnetic Waves.
Thermodynamics. Temperature  How hot or cold something feels compared to a standard  Typically water is our standard  Function of kinetic energy 
Discussion 2 Wednesday 2/6 Quiz prep + lecture 4.
© Crown copyright Met Office Radiation scheme for Earth’s atmosphere …and what might not work for exoplanets James Manners 6/12/11.
The States Of Matter All matter is made of something, even if it looks like nothing. We make classifications according to its properties, both chemical.
Next Week: QUIZ 1 One question from each of week: –5 lectures (Weather Observation, Data Analysis, Ideal Gas Law, Energy Transfer, Satellite and Radar)
Copyright © 2010 Pearson Education, Inc. Lecture Outline Chapter 2 Light and Matter.
Electromagnetic Radiation: Interactions in the Atmosphere.
1 Microwave Interactions with the Atmosphere Microwave Interactions with the Atmosphere S. L. Cruz Pol Electrical and Computer Engineering University of.
Atmospheric phase correction at the Plateau de Bure interferometer IRAM interferometry school 2006 Aris Karastergiou.
Radiation Heat Transfer
Radiation (Ch 12 YAC) Thermal energy is emitted by matter as a result of vibrational and rotational motion of molecules, atoms and electrons. The energy.
Fourth IRAM Millimeter Interferometry School 2004: Atmospheric phase correction 1 Atmospheric phase correction Jan Martin Winters IRAM, Grenoble.
Reminder of radiance quantities I λ RadianceW m -2 μm -1 sr -1 Intensity (Monochromatic) F λ Spectral IrradianceW m -2 μm -1 Monochromatic Flux F(Broadband)
Lecture 2: Heat and radiation in the atmosphere. TEMPERATURE… is a measure of the internal heat energy of a substance. The molecules that make up all.
1 Atmospheric Radiation – Lecture 13 PHY Lecture 13 Remote sensing using emitted IR radiation.
Electromagnetic Radiation, Atomic Structure & Spectra.
WHAT MAKES OUR ATMOSPHERE DISTINCT FROM SPACE?. 1. The affected medium of atmosphere. (atmospheric composition)
Quick Review of Remote Sensing Basic Theory Paolo Antonelli SSEC University of Wisconsin-Madison Monteponi, September 2008.
Ch.22 Atmosphere. Composition 78% nitrogen 21% oxygen 0.9% argon 0.1&other gasses.
17 Chapter 17 The Atmosphere: Structure and Temperature.
Astronomy Basic Properties of Stars. Kirchhoff’s Three Kinds of Spectra.
Passive Microwave Remote Sensing
Principles of Heat and Radiation
Electromagnetic Spectrum
By Narayan Adhikari Charles Woodman
Atmospheric phase correction for ALMA
Introduction and Basic Concepts
REMOTE SENSING.
REMOTE SENSING.
Presentation transcript:

1 Water Vapour Radiometry Bob Sault

2 The Neutral Atmosphere H20H20 O2O2 H20H20 O2O2

3 Microwave Radiometry  Radiative transfer: A lossy medium will emit thermal radiation in proportion to its physical temperature and its attenuation coefficient.  For an atmosphere, the attenuation coefficient will depend on its composition, temperature and pressure. It will also be a function of frequency.  Atmospheric radiometry is the study of the radiation emitted by the atmosphere.  Microwave radiometry is extensively used to infer properties of the Earth’s atmosphere, as well as the atmospheres of other planets.

4 Water  Its dipolar structure means that its melting and boiling points are much higher than other simple molecules (e.g. CO 2, O 2, N 2 ).  Whereas CO 2, O 2 and N 2 are distributed in the lower atmosphere as ideal gases (e.g. they are distributed according to ideal gas law and gravity), water is “clumpy”.

5 Atmospheric transmission  When receiving celestial emission at radio frequencies, O 2, N 2 (the “dry”) components of the atmosphere introduce a excess path of approximately 2.2 metres over a vacuum.  Water vapour introduces cm of excess path.  Whereas the dry components are well-mixed, water vapour is clumpy.  At microwave wavelengths, water vapour fluctuations is the predominant cause of changes in the excess path lengths at different antennas.

6 Blobs of water Blobs exist on all size scales. Follow a so-called Kolmogorov spectrum of sizes. Typically the water vapour column for two sites 1 km apart are 99% the same – the so- called turbulent component consists of just 1% of the water.

7 Water vapour radiometry  Meteorologists have long used radiometry to study the water content of the atmosphere.  The use of the technique in radio interferometry has been suggested for years.  Interferometry is a very different application that meteorology. –Path lengths of interest are much smaller (~100  m). –It is a differential system (absolute path is not relevant).  Main problems: systematics!

8 Continuum vs Line systems  “Continuum” water vapour radiometers measure fluctuations far from water lines  Line systems work near either of the two water lines: 22.3 GHz or 183 GHz.  Line systems much more robust to systematics. The water line shape acts as a filter to remove systematics.

9 ATCA Water Vapour Radiometer  A radiometer near 22.3 GHz, which takes measurements at 4 bands.  Required sensitivity is to measure fluctuations of 10 mK in the sky brightness of about 30 K (and uncooled receivers with system temperatures of a 300 K). O2O2 O2O2 H2OH2O H2OH2O

10 ATCA Water Vapour Radiometer

11 Fluctuations in sky brighness

12 Compare the channels

13 Results of the WVR