Climate and Radiation Projects

Project Icon   ARMAtmospheric Radiation Measurements
  Project Homepagehttp://www.arm.gov
  Project Science Contact — Warren Wiscombe

The Department of Energy's Atmospheric Radiation Measurements Program (ARM) complements NASA's satellite observations of the Earth. ARM employs sophisticated arrays of surface-based sensors to study shortwave and longwave radiation and cloud physics and dynamics. The first of fie projected ARM sites was installed in Oklahoma in July, 1992. One of the most vexing and difficult problems ARM will face is the interpretation of high-temporal-resolution radiation data in terms of properties of the cloud field overhead. Under a grant from ARM, our Branch is engaged in modeling the fractal-statistical character of cloud fields, using observed data from cloud field programs, with Monte Carlo computations of radiation emerging from simulated fractal cloud fields. This work has ramifications for satellite as well as surface radiation measurements.

An issue addressed by the ARM Enhanced Shortwave Experiment (ARESE) in Sept-Oct 1995 is the atmospheric absorption of solar radiation, estimated by some to be as much as 10 % greater than plane-parallel computations seem to indicate. Daily status reports on the ARESE field measurements are at: ARESE daily status. The Spring 1996 UAV deployment featured the first coordinated flights with the Multispectral Pushbroom Imaging Radiometer (MPIR) being developed at DoE's Sandia Lab for mapping cloud properties, and the Microwave Radiometer being developed here at Goddard by Paul Racette and Jim Weinman, for mapping cloud liquid water. Some of the flights will focus on manmade contrails, in coordination with the SUCCESS field program. The main focus, though, is on how cloud structure is related to cloud albedo, transmission, and especially cloud absorption.


    There are no links for this project right now.
 


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Project Icon   CLAMSChesapeake Lighthouse & Aircraft Measurements for Satellites
  Project Homepagehttp://www-clams.larc.nasa.gov/clams/index.html
  Project Science Contact — Lorraine Remer

The Chesapeake Lighthouse and Aircraft Measurements for Satellites (CLAMS) field campaign is a shortwave closure experiment designed to make a detailed characterization of atmospheric aerosols while simultaneously characterizing the lower boundary condition with measurements of ocean optical properties and radiative fluxes under cloud-free conditions, and coincident with satellite overpasses (e.g. NASAÕs Terra satellite). The experiment, based from NASA Wallops Flight Facility, was successfully carried out over the middle Atlantic eastern seaboard of the U.S. from 10 JulyÐ2 August, 2001.

Central to CLAMS measurement objectives is to validate and to improve Terra satellite data products derived from three sensors, namely, radiative fluxes from CERES (Clouds and the EarthÕs Radiant Energy System), and aerosol properties from MISR (Multiangle Imaging SpectroRadiometer) and MODIS (Moderate Resolution Imaging Spectroradiometer). Of significance to CLAMS objectives is the Chesapeake Lighthouse, a stable sea platform located in the Atlantic Ocean, 13 miles east of Virginia Beach and the site of an ongoing CERES Ocean Validation Experiment (COVE) where long-term measurements of radiative fluxes, aerosol properties, ocean optics, sea state and meteorology are obtained. During CLAMS, a micropulse lidar was deployed at COVE. Aerosol chemistry measurements were made from aircraft and at two surface sites (COVE site and a site at Wallops Island). Numerous coordinated aircraft experiments were conducted under a variety of aerosol conditions over the coastal and deep ocean areas.

The dataset from CLAMS consisting of coincident observations of the atmosphere and lower boundary condition is being archived at the NASA Langley Atmospheric Sciences Data Center.

CLAMS is jointly sponsored by the CERES, MISR and MODIS science teams.


  • MODIS Airborne Simulator - An airborne scanning spectrometer that acquires high spatial resolution imagery of cloud and surface features from its vantage point on-board a NASA ER-2 high-altitude research aircraft.
  • Cloud Absorption Radiometer - An airborne multispectral scanning radiometer that can determine single scattering albedo of clouds at selected wavelengths in the visible and near-infrared and can measure the bidirectional reflectance of various terrestrial surfaces
  • Cloud Absorption Radiometer CLAMS - Cloud Absorption Radiometer (CAR) documentation and quicklook imagery from the CLAMS campaign.
 


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Project Icon   CRYSTAL-FACECirrus Regional Study of Tropical Anvils and Cirrus Layers-Florida Area Cirrus Experiment
  Project Homepagehttp://cloud1.arc.nasa.gov/crystalface
  Project Science Contact — Si-Chee Tsay

CRYSTAL-FACE, Cirrus Regional Study of Tropical Anvils and Cirrus Layers-Florida Area Cirrus Experiment, is a measurement campaign designed to investigate tropical cirrus cloud physical properties and formation processes. Understanding the production of upper tropospheric cirrus clouds is essential for the successful modeling of the EarthÕs climate. The CRYSTAL-FACE mission took place during the month of July 2002 in the south Florida region. Measurements from ground sites, aircraft, and satellites were conducted, and the vast majority of aircraft flights were coordinated with NASA's Terra, Aqua, and/or TRMM satellites.


 


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Project Icon   CARCloud Absorption Radiometer
  Project Homepagehttp://car.gsfc.nasa.gov
  Project Science Contact — Michael King

The Cloud Absorption Radiometer (CAR) was conceived and developed at NASA Goddard Space Flight Center to study cloud radiative properties at selected wavelengths in the visible and near-infrared, and to acquire imagery of cloud and Earth surface features. In the early years the focus was on measurements of the angular distribution of scattered radiation deep within a cloud layer. In later years, the focus shifted to the bidirectional reflectance properties of various surfaces (ocean, sea ice, vegetation, etc.).

The CAR is a 14-channel scanning radiometer that was designed to operate from various aircraft platforms. It was first operated from the tail gunner's position of the University of Washington Douglas B-23 (1983-1984), later in a special nose cone on the UW Convair C-131A (1985-1997), then in the improved nose cone of the UW Convair CV-580 (1998-2001), and most recently on the South African Weather Service Aerocommander 690A (2005) and Sky Research Jetstream J31 (2006).

The instrument scans in a vertical plane on the right hand side of the aircraft from 5° before zenith to 5° past nadir (190° aperture). This permits observations of both the zenith and nadir radiance with as much as a 5° aircraft roll, an angle that was measured simultaneously aboard the aircraft. In addition to its traditional starboard viewing mode, the CAR instrument can be operated in zenith viewing, nadir viewing, and bidirectional reflectance distribution function (BRDF) mode; and can be switched between each of these four modes during flight.

The CAR has been deployed on a regular basis in field campaigns around the world including deployments to Portugal (Azores), Brazil, Kuwait, Mexico, the continental U.S., Alaska, and various countries in southern Africa. During typical field campaigns, the CAR is flown in concert with an array of cloud microphysics, aerosol, atmospheric chemistry, and general meteorological instruments in collaboration with the Department of Atmospheric Sciences at the University of Washington or, more recently, with other solar radiation instrumentation.

The CAR instrument was developed by Dr. Michael King and is the most frequently used airborne instrument ever built in-house at Goddard.


    There are no links for this project right now.
 


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Project Icon   Earth Observatory
  Project Homepagehttp://earthobservatory.nasa.gov
  Project Science Contact Unkonwn

NASA's Earth Observatory is an interactive Web-based magazine where the science-attentive public can obtain new satellite imagery and scientific information about our home planet. The focus is on Earth's climatic and environmental change. The site is also designed to be useful to public media and educators. Any and all materials published on the Earth Observatory are freely available for re-publication, re-use, or re-broadcast (except in rare cases where copyright is indicated).


  • NASA Visible Earth - NASAÕs Visible Earth is a digital repository of images, animations, and data visualizations produced by personnel from across the agencyÕs Earth Science Enterprise. Currently, there are more than 6,200 records available in the Visible Earth.
  • Image Composite Editor - The Image Composite Editor is designed to be an easy first step for teachers & students into the realm of Earth system science, image processing, data analysis, and satellite remote sensing via their Web browser.
 


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Project Icon   IDS-AeroSysIDS - The Global Aerosol System
  Project HomepageUnknown
  Project Science Contact Unkonwn

The project seeks to characterize the Global Aerosol System using a combination of satellite observations and chemical transport models. The end goal is to understand and quantify aerosol effects and aerosol forcing on global and regional climate. This will include:
1) estimating aerosol source strength
2) estimating the anthropogenic fraction of the aerosol from satellite
3) estimating the direct effect and direct forcing of aerosols in the Earth's energy balance
4) understanding aerosol-cloud interaction, including aerosol effects on cloud microphysics, cloud coverage, lifetime and precipitation processes.


  • AeroCenter web page - AeroCenter is the community of researchers at GSFC and nearby facilities who are interested in a wide range of aerosol topics, one of which is the Global Aerosol System. AeroCenter sponsors a popular informal seminar series.
 


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Project Icon   I3RCIntercomparison of 3D Radiation Codes
  Project Homepagehttp://i3rc.gsfc.nasa.gov
  Project Science Contact — Robert Cahalan

Whenever a scattering medium, such as clouds or sea ice, is highly inhomogeneous and optically thick, then 3-dimensional radiative transfer (3DRT) techniques are required. These can be based on Monte Carlo, discrete ordinates, and/or finite volume methodologies. I3RC has defined various baseline cloud cases and coordinated the application of a wide variety of codes to these cases, as a means of certifying the accuracy of codes, and enhancing the ability of codes to handle a variety of cases, and produce the variety of outputs needed for the modeling and remote sensing of clouds and other inhomogeneous scattering media. I3RC is one activity of the 3DRT Working Group of the International Radiation Commission (IRC), and is jointly funded by the NASA Radiation Sciences Program and the DoE Atmospheric Radiation Measurement Program.


  • I3RC-3 Workshop - Third I3RC Workshop, October 10-14, 2005, at University of Kiel, FRG.
 


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Project Icon   EOS-MODISModerate Resolution Imaging Spectroradiometer
  Project Homepagehttp://modis-atmos.gsfc.nasa.gov
  Project Science Contact — Michael King

The Moderate Resolution Imaging Spectroradiometer (MODIS) is an earth-viewing sensor that flies on the Earth Observing System (EOS) Terra and Aqua satellites, launched in 1999 and 2002, respectively. MODIS scans a swath width of 2330 km that is sufficiently wide to provide nearly complete global coverage every two days from a polar-orbiting, sun-synchronous, platform at an altitude of 705 km. MODIS provides images in 36 spectral channels between 0.414 and 14.235 µm with spatial resolutions of 250 m (two bands), 500 m (five bands) and 1000 m (29 bands). These bands have been carefully selected to enable advanced studies of land, ocean, and atmospheric properties, including state-of-the-art global measurements of precipitable water, aerosol particles, and clouds. Branch scientists participate as members of the MODIS science team, both in algorithm development and in science investigations, including validation. An aircraft spectrometer—the MODIS Airborne Simulator—was developed in collaboration with NASA Ames Research Center.


  • MODIS Airborne Simulator - An airborne scanning spectrometer that acquires high spatial resolution imagery of cloud and surface features from its vantage point on-board a NASA ER-2 high-altitude research aircraft.
  • MODIS - MODIS website contains data documentation, including Algorithm Theoretical Basis Documents (ATBDs), product descriptions, and data tutorials on ordering MODIS data from the various DAACs. It also contains images of the day, instrument details such as spe
 


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Project Icon   PRiDEPuerto Rico Dust Experiment
  Project Homepagehttp://modis-atmos.gsfc.nasa.gov/PRIDE/index.html
  Project Science Contact — Lorraine Remer

The Puerto Rico Dust Experiment (PRiDE) took place out of Roosevelt Roads Naval Base, Puerto Rico, from 26 June to 24 July 2000. A group of Navy, NASA, and university scientists came together to study the radiative, microphyiscal, chemical and transport properties of Saharan Dust transported into the region. This unique campaign combined measurements from surface, airborne and satellite platforms, that increased knowledge of dust transport and distribution. Results from PRiDE were published in a JGR special issue, published 16 October 2003.

Two groups within the Climate and Radiation Branch attended PRiDE. For the MODIS aerosol group, led by Lorraine Remer, PRiDE was the first opportunity for intensive comparison of MODIS aerosol products with sunphotometer and in-situ measurements from both surface and airborne platforms. Results from PRiDE led to an effort to account for nonspericity of dust within the MODIS algorithm. The second group, led by Si-Chee Tsay, measured a multitude of radiation measurements from a platform, now known as SMART. Results from their measurements led to estimates of aerosol direct radiative forcing.


    There are no links for this project right now.
 


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Project Icon   SORCESolar Radiation and Climate Experiment
  Project Homepagehttp://lasp.colorado.edu/sorce
  Project Science Contact — Robert Cahalan

SORCE, the SOlar Radiation and Climate Experiment, was launched January 25, 2003 from Kennedy Space Center, onboard an Orbital Sciences Pegasus, and has a 5 year design lifetime. SORCE orbits Earth about every 90 minutes, and when on the sunlit side observes the Sun with 4 instruments: TIM, that measures the Total Solar Irradiance (TSI); SIM, that measures the Spectral Solar Irradiance (SSI) from 200 nanometers to 2000 nanometers (2 microns); SOLSTICE, that measures the SSI from 115 to 320 nanometers (overlapping SIM's coverage); and XPS, that measures SSI from 1 to 34 nanometers, as well as the important Lyman alpha spectral emission line at 121 nanometers, due to transitions between the hydrogen atom's ground state and the first excited state. When on the dark side of Earth, SOLSTICE monitors the SSI from 18 stable early-type blue stars, as a way of determining its varying transmission. SIM measures its own transmission internally. Data from any of these instruments can be obtained from the Goddard DAAC. SORCE observed several of the largest sunspots ever recorded, that appeared and moved across the solar disk during the week of October 27, 2004.


  • Sun-Climate Center - The Goddard Sun-Climate Center is an integrated program of observational systems and research to improve the understanding and prediction of the response of Earth's climate to solar forcing from monthly to multi-centennial time scales.
  • Total Solar Irradiance Plot - Greg Kopp's latest Total Solar Irradiance Plot.
 


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Project Icon   SAFARI 2000Southern African Regional Science Initiative 2000
  Project Homepagehttp://www.daac.ornl.gov/S2K/safari.html
  Project Science Contact — Steven Platnick

The Southern African Regional Science Initiative (SAFARI 2000) was a major surface, airborne and spaceborne field campaign carried out in southern Africa in 2000 and 2001, that addressed a broad range of phenomena, related to land-atmosphere interactions and the biogeochemical functioning of the southern African system. The integrating themes of this experiment deal with surface emissions characterization, airborne characterization of aerosols and trace gases, regional haze and trace gas characterization, and radiant measurements by surface, aircraft and remote sensing platforms. Enhanced regional fuel loads associated with the moist La Niña phase of the ENSO cycle produced above average biomass burning emissions, which consequently dominated all other aerosol and trace gas emissions during the dry season. The overall conclusion is that SAFARI 2000, as an integrating theme, has been able to give significant new insights into the regional scale biogeochemical cycling of southern Africa, and contributed in important ways to the validation of remote sensing instruments on board the NASA Terra spacecraft.


  • MODIS Airborne Simulator - An airborne scanning spectrometer that acquires high spatial resolution imagery of cloud and surface features from its vantage point on-board a NASA ER-2 high-altitude research aircraft.
  • Cloud Absorption Radiometer - An airborne multispectral scanning radiometer that can determine single scattering albedo of clouds at selected wavelengths in the visible and near-infrared and can measure the bidirectional reflectance of various terrestrial surfaces
  • MODIS Airborne Simulator SAFARI 2000 - MODIS Airborne Simulator (MAS) documentation and quicklook imagery from the SAFARI 2000 campaign.
  • Cloud Absorption Radiometer SAFARI 2000 - Cloud Absorption Radiometer (CAR) documentation and quicklook imagery from the SAFARI 2000 campaign.
 


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Project Icon   SMART-COMMITSurface-sensing Measurements for Atmospheric Radiative Transfer/Chemical, Optical, & Microphysical Measurements of In-situ Troposphere
  Project Homepagehttp://smart-commit.gsfc.nasa.gov
  Project Science Contact — Si-Chee Tsay

Surface-sensing Measurements for Atmospheric Radiative Transfer (SMART)-Chemical, Optical, & Microphysical Measurements of In-situ Troposphere (COMMIT) is a suite of instruments that take measurements (both in-situ and by remote sensing) to characterize, as completely as possible, the atmosphere at a given location. SMART and COMMIT are both mobile, which allows them to be sent to locations that exhibit interesting atmospheric phenomena and to participate in coordinated measurement campaigns.


    There are no links for this project right now.
 


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Project Icon   THORTHickness from Offbeam Returns
  Project Homepagehttp://climate.gsfc.nasa.gov/thor/
  Project Science Contact — Robert Cahalan

THOR, THickness from Offbeam Returns, is a laser system with 10 multiple fields-of-view (FoVs) photon counting detector channels. Channel 1 FoV is seen by a single 200 micron optical fiber, which has the usual narrow field-of-view of most lidar systems, typically dominated by single-scattering backscatter from the cloud, water, or ice target. Each succeeding FoV for channels 2, 3, .., 8 is 2 X wider, so that Channel 8 sees 128 X the central (Ch 1) FoV. To get 10 channels instead of 8, the Channel 8 FoV is subdivided into 3 equal sectors, Channels 8, 9, and 10, each of which sees a 120¡ azimuthal sector of the outermost annulus. The outer FoVs are seen by bundles of 50 micron optical fibers, and the 3 outermost channels each consist of about 50,000 such fibers, entering a single photon counting detector. These outer channels are dominated by multiple scattering, and are typically not sensitive to single scattering properties, but only to the macroproperties such as layer thickness. A "THOR Validation Campaign" over the DOE/ARM/CART site in Oklahoma, with THOR flying on the NASA P-3B at an altitude of 8.5 km, showed that THOR can "see through" a thick low-level cloud, more than 750 meters thick, with optical thickness exceeding 20, and determine not only cloud top height (as can most lidars) but also cloud base height, to an accuracy of 5% and better. The THOR team includes not only members of the Climate and Radiation Branch, but also the Mesoscale Atmospheric Processes Branch (Dr. Matthew McGill) and the Electrical Systems Branch (Mr. John KolasinskI) as well as non-NASA colleagues (A. Davis and S. Love, LANL). [Example THOR Cloud Retrieval]


    There are no links for this project right now.
 


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Project Icon   TRMM/GPMTropical Rainfall Measuring Mission/Global Precipitation Measurement
  Project Homepagehttp://trmm.gsfc.nasa.gov/
  Project Science Contact — Thomas Bell

The Tropical Rainfall Measuring Mission (TRMM) is jointly managed by the United States and Japanese space agencies. Its primary objective is to measure precipitation and related quantities between latitudes 35N and 35S. The orbit altitude is low enough to ensure unusually good instrument resolution, and the orbit inclination (35¡) causes the satellite's observation times to cover all hours of the day over a period of about a month and a half. The satellite is special in that it carries the only precipitation radar in orbit, as well as a multichannel microwave radiometer, a visible-infrared scanner, a lightning imager, and an instrument designed to monitor the earth's "radiative energy budget". The satellite was launched in November 1997 and has been providing data virtually flawlessly since then.

The Global Precipitation Mission (GPM) is now being planned. Building on the success of TRMM, it will involve multiple satellites to provide better coverage and a core satellite with much improved instrumentation.

Branch activities funded by the TRMM/GPM project focus on extracting climatological information about rain using TRMM and other satellite data, as well as data collected from surface observations. Developing methods of estimating the accuracy of rainfall maps produced from satellites is of particular interest.


  • TRMM Satellite Validation - The function of the TRMM GV program at the NASA/Goddard Space Flight Center is to provide support for Tropical Rainfall Measuring Mission (TRMM), in connection with the ground based validation of the TRMM satellite observations.
 


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Updated:
September 15, 2008 in Personnel
Site Maintained By: Dr. William Ridgway
Responsible NASA Official: Dr. Robert Cahalan
 
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