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Assimilation of N2O in the U
| Title |
Assimilation of N2O in the Upper Atmosphere Using a Kalman Filter: N2O Mixing Ratio |
| Abstract |
This series of animations shows assimilation of N2O in the upper atmosphere using observations from the Cryogenic Limb Etalon Spectrometer (CLAES) on the Upper Atmosphere Research Satellite (UARS). Winds were provided by the Goddard EOS Data Assimilation System (GEOS-DAS). Flow is at the 850K isentropic level. N2O mixing ratio is expressed in parts per billion volume (ppbv). |
| Completed |
1996-03-22 |
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Energetic Particle Flux over
| Title |
Energetic Particle Flux over the Arctic from PEM (11/9/91) |
| Abstract |
UARS measures the flux of energetic particles from space using the Particle Environment Monitor, PEM. These high energy particles cause ozone depletion at high altitudes by producing nitrogen and hydrogen radicals. |
| Completed |
1999-04-09 |
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Graph Showing Antarctic Ozon
| Title |
Graph Showing Antarctic Ozone Decreasing by 60% from the 1950s to the 1980s |
| Abstract |
During the spring of 1985, British researchers using ground-based instruments measured dramatic changes in the ozone layer. As much as sixty percent of the ozone over Antarctica was rapidly disappearing each spring. |
| Completed |
1999-04-09 |
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MLS Looking at the Limb
| Title |
MLS Looking at the Limb |
| Abstract |
The chemistry of ozone destruction involves very small quantities of stratospheric gases which change rapidly with altitude. UARS is able to determine the altitude variation of these gases by looking at the atmosphere edge on. This is called limb sounding. The Microwave Limb Sounder (MLS) measures microwave emission from ozone and chlorine monoxide, a major ozone destroying radical. |
| Completed |
1999-04-09 |
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Viewing the ISAMS and CLAES
| Title |
Viewing the ISAMS and CLAES Instruments on UARS |
| Abstract |
Key to understanding the chlorine chemistry in the polar stratosphere is the measurement of polar stratospheric clouds, chlorine monoxide, and the reservoir gas chlorine nitrate. Polar stratospheric clouds are seen by the Improved Stratospheric and Mesospheric Sounder, ISAMS, and chlorine nitrate has been measured by the Cryogen Limb Array Etalon Spectrometer, CLAES. Both ISAMS and CLAES make measurements by looking at infrared emission from cloud particles and trace gases. |
| Completed |
1999-04-09 |
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Viewing the ISAMS and CLAES
| Title |
Viewing the ISAMS and CLAES Instruments on UARS |
| Abstract |
Key to understanding the chlorine chemistry in the polar stratosphere is the measurement of polar stratospheric clouds, chlorine monoxide, and the reservoir gas chlorine nitrate. Polar stratospheric clouds are seen by the Improved Stratospheric and Mesospheric Sounder, ISAMS, and chlorine nitrate has been measured by the Cryogen Limb Array Etalon Spectrometer, CLAES. Both ISAMS and CLAES make measurements by looking at infrared emission from cloud particles and trace gases. |
| Completed |
1999-04-09 |
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Viewing the ISAMS and CLAES
| Title |
Viewing the ISAMS and CLAES Instruments on UARS |
| Abstract |
Key to understanding the chlorine chemistry in the polar stratosphere is the measurement of polar stratospheric clouds, chlorine monoxide, and the reservoir gas chlorine nitrate. Polar stratospheric clouds are seen by the Improved Stratospheric and Mesospheric Sounder, ISAMS, and chlorine nitrate has been measured by the Cryogen Limb Array Etalon Spectrometer, CLAES. Both ISAMS and CLAES make measurements by looking at infrared emission from cloud particles and trace gases. |
| Completed |
1999-04-09 |
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Viewing the SUSIM and SOLSTI
| Title |
Viewing the SUSIM and SOLSTICE Instruments on UARS |
| Abstract |
The Solar Ultraviolet Spectral Irradiance Monitor, SUSIM, and the Solar/Stellar Irradiance Comparison Experiment, SOLSTICE, measure the sun's ultraviolet radiation. |
| Completed |
1999-04-09 |
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Viewing the SUSIM and SOLSTI
| Title |
Viewing the SUSIM and SOLSTICE Instruments on UARS |
| Abstract |
The Solar Ultraviolet Spectral Irradiance Monitor, SUSIM, and the Solar/Stellar Irradiance Comparison Experiment, SOLSTICE, measure the sun's ultraviolet radiation. |
| Completed |
1999-04-09 |
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Viewing the SUSIM and SOLSTI
| Title |
Viewing the SUSIM and SOLSTICE Instruments on UARS |
| Abstract |
The Solar Ultraviolet Spectral Irradiance Monitor, SUSIM, and the Solar/Stellar Irradiance Comparison Experiment, SOLSTICE, measure the sun's ultraviolet radiation. |
| Completed |
1999-04-09 |
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The Microwave Limb Sounder O
| Title |
The Microwave Limb Sounder Observes the Lower Stratosphere and Upper Troposphere |
| Abstract |
MLS measures lower stratospheric temperature and concentrations of H2O, O3, ClO, BrO, HCl, OH, HO2, HNO3, HCN, and N2O, for their effects on (and diagnoses of) ozone depletion, transformations of greenhouse gases, and radiative forcing of climate change. |
| Completed |
2004-12-14 |
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Chemical Model Animation of
| Title |
Chemical Model Animation of O3 Absorbing Low-energy UV |
| Abstract |
Ozone is a strong absorber of lower energy ultraviolet radiation which can kill living organisms. This radiation is absorbed by the ozone layer when it breaks the ozone bonds. An oxygen atom is released, but the atom quickly re-combines with another oxygen molecule to regenerate ozone. |
| Completed |
1999-04-09 |
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Chemical Model Animation of
| Title |
Chemical Model Animation of Chlorine Release from Reservoir Gases over Antarctica |
| Abstract |
Over the Antarctic continent, ice clouds form in the cold winter darkness. On the surface of the cloud particles, chlorine nitrate and hydrogen chloride react and release chlorine. The chlorine then reacts with ozone forming chlorine monoxide and starting the catalytic ozone destruction cycle. The massive ozone loss results in the development of the Antarctic ozone hole. |
| Completed |
1999-04-09 |
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Water Vapor Measurements fro
| Title |
Water Vapor Measurements from HALOE (1992-1997) |
| Abstract |
An animated graph showing HALOE measurements of the water vapor amounts in the upper stratosphere, illustrating that it takes about 5 years for CFCs to reach the upper atmosphere. Tropical water vapor changes slowly with seasonal cycles. These changes, shown here as thick bands, were found to slowly ascend. These measurements tell us how fast the CFCs and other pollutants rise into the stratosphere. |
| Completed |
1999-04-09 |
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HALOE Measurements of HCl in
| Title |
HALOE Measurements of HCl in the Stratosphere (1992 - 1998) |
| Abstract |
HALOE was designed to carefully monitor hydrogen fluoride and hydrogen chloride, byproducts of CFC destruction in the stratosphere. HALOE operates by observing the absorption of infrared radiation by these molecules against the rising and setting sun. When UARS was first launched, measurements by HALOE showed that CFC byproducts were still increasing in the stratosphere. But the newest HALOE measurements now show that CFC by-products are no longer increasing. UARS has shown that the stratosphere is starting to respond to the international ban on CFC manufacture. |
| Completed |
1999-04-09 |
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Viewing the WINDII Instrumen
| Title |
Viewing the WINDII Instrument on UARS |
| Abstract |
The Wind Imaging Interferometer, WINDII, measures the winds in the mesosphere, using air glow. |
| Completed |
1999-04-09 |
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Viewing the WINDII Instrumen
| Title |
Viewing the WINDII Instrument on UARS |
| Abstract |
The Wind Imaging Interferometer, WINDII, measures the winds in the mesosphere, using air glow. |
| Completed |
1999-04-09 |
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Nine Datasets on a Single Gl
| Title |
Nine Datasets on a Single Globe with Wipe Between Different Datasets Run as a Continuous Two Minute Loop |
| Abstract |
Single globe with wipe between different datasets run as a continuous 2 minute loop. Sequence: Galileo, radiant energy (Globe), vegetation index anomalies, temperature (globe), fires, aerosols (TOMS), clouds (GOES 9 & 10, Meteosat, and GMS-5), methane (UARS), water vapor (GOES 9 & 10, Meteosat, and GMS-5), biosphere (SeaStar/SeaWiFS), Galileo |
| Completed |
1999-11-10 |
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Nine Datasets on a Single Gl
| Title |
Nine Datasets on a Single Globe with Wipe Between Different Datasets |
| Abstract |
Single globe with wipe between different datasets. Sequence: Galileo, radiant energy, vegetation index anomalies, temperature, fires, aerosols, clouds, methane, water vapor, biosphere, Galileo |
| Completed |
1999-11-10 |
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Tropical Winds in the Strato
| Title |
Tropical Winds in the Stratosphere from HRDI (1991-1996) |
| Abstract |
The High Resolution Doppler Interferometer (HRDI) measures winds in both the stratosphere and mesosphere. The tropical winds in the stratosphere undergo a slow two year variation called the quasibianunual oscillation. This oscillation controls mixing throughout the stratosphere and HRDI has given us much detail on wind changes associated with this oscillation. The animation indicates the line of zero wind speed in the zonal tropical winds, the height at which the winds change from eastward to westward. |
| Completed |
1999-04-09 |
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Sun Spot Number Compared wit
| Title |
Sun Spot Number Compared with Solar UV from SUSIM (1991-1997) |
| Abstract |
An animated graph showing the eleven-year sun spot cycle, as shown by measurements of sun spot number. Following this graph, an animation compares sun spot number measurements for the 1990s with direct measurements of the change in solar ultraviolet irradiance from SUSIM. |
| Completed |
1999-04-09 |
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HALOE Looking at the Sun
| Title |
HALOE Looking at the Sun |
| Abstract |
The Halogen Occultation Experiment, HALOE, was designed to carefully monitor hydrogen fluoride and hydrogen chloride, byproducts of CFC destruction in the stratosphere. HALOE operates by observing the absorption of infrared radiation by these molecules against the rising and setting sun. |
| Completed |
1999-04-09 |
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Viewing the HALOE Instrument
| Title |
Viewing the HALOE Instrument on UARS |
| Abstract |
The Halogen Occultation Experiment, HALOE, was designed to carefully monitor hydrogen fluoride and hydrogen chloride, byproducts of CFC destruction in the stratosphere. |
| Completed |
1999-04-09 |
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Viewing the HALOE Instrument
| Title |
Viewing the HALOE Instrument on UARS |
| Abstract |
The Halogen Occultation Experiment, HALOE, was designed to carefully monitor hydrogen fluoride and hydrogen chloride, byproducts of CFC destruction in the stratosphere. |
| Completed |
1999-04-09 |
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Viewing the HRDI Instrument
| Title |
Viewing the HRDI Instrument on UARS |
| Abstract |
The High Resolution Doppler Interferometer, HRDI, measures winds in both the stratosphere and mesosphere. |
| Completed |
1999-04-09 |
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Viewing the HRDI Instrument
| Title |
Viewing the HRDI Instrument on UARS |
| Abstract |
The High Resolution Doppler Interferometer, HRDI, measures winds in both the stratosphere and mesosphere. |
| Completed |
1999-04-09 |
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Viewing the ACRIM Instrument
| Title |
Viewing the ACRIM Instrument on UARS |
| Abstract |
To understand the solar effects on the ozone layer, UARS was equiped with three instruments to measure the sun. One of them, the Active Cavity Radiometer Irradiance Monitor, ACRIM, measures the total energy output from the sun. |
| Completed |
1999-04-09 |
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Viewing the ACRIM Instrument
| Title |
Viewing the ACRIM Instrument on UARS |
| Abstract |
To understand the solar effects on the ozone layer, UARS was equiped with three instruments to measure the sun. One of them, the Active Cavity Radiometer Irradiance Monitor, ACRIM, measures the total energy output from the sun. |
| Completed |
1999-04-09 |
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Chemical Model Animation of
| Title |
Chemical Model Animation of O3 Losing an Oxygen Atom to a Radical |
| Abstract |
Ozone is very reactive. It easily loses the third oxygen atom in the presence of other highly reactive compounds called radicals, which contain chlorine, hydrogen, nitrogen, or bromine. Minute quantities of these radicals can cause large decreases in ozone because they are not consumed in the reaction. This is called a catalytic cycle. |
| Completed |
1999-04-09 |
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Chemical Model Animation of
| Title |
Chemical Model Animation of O2 being Broken Up and Reforming as O3 |
| Abstract |
Ozone is formed when high energy ultra-violet radiation from the sun breaks apart molecular oxygen. An oxygen atom then combines with an oxygen molecule producing a new molecule with three atoms of oxygen, ozone. |
| Completed |
1999-04-09 |
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UARS Flyover Fading to CHEM
| Title |
UARS Flyover Fading to CHEM |
| Completed |
1999-04-09 |
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UARS 3D Wireframe
| Title |
UARS 3D Wireframe |
| Completed |
1999-04-09 |
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Earth Probe TOMS Orbiting th
| Title |
Earth Probe TOMS Orbiting the Earth |
| Abstract |
A composite image of the Earth from SeaWIFS is used as the background of this beauty shot of Earth Probe TOMS. |
| Completed |
1999-04-09 |
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UARS Title Sequence
| Title |
UARS Title Sequence |
| Abstract |
Title sequence for the UARS video, both with and without words. |
| Completed |
1999-04-09 |
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UARS Title Sequence
| Title |
UARS Title Sequence |
| Abstract |
Title sequence for the UARS video, both with and without words. |
| Completed |
1999-04-09 |
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UARS Title Sequence
| Title |
UARS Title Sequence |
| Abstract |
Title sequence for the UARS video, both with and without words. |
| Completed |
1999-04-09 |
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Ozone Layer Shielding Our Pl
| Title |
Ozone Layer Shielding Our Planet |
| Abstract |
An animation showing the ozone layer shielding our planet from the sun's intense ultraviolet radiation. Ozone absorbs nearly all of the biologically damaging UV radiation from the sun. |
| Completed |
1999-04-09 |
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TOMS Data Showing the Ozone
| Title |
TOMS Data Showing the Ozone Hole over Antarctica (8/20/92 - 10/19/92) |
| Completed |
1999-04-09 |
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Stratospheric Ozone Transpor
| Title |
Stratospheric Ozone Transport in the Northern Hemisphere (2/19/92 - 3/19/92) |
| Abstract |
This animation, derived from both remote sensing measurements of ozone and a computational ozone transport model, illustrates the complexity of ozone transport in the stratosphere. |
| Completed |
1999-04-09 |
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