PPT-Crust-atmosphere coupling and CO

2 sequestration on Mars Adrienne Macartney amacartney1researchglaacuk School of Geographical amp Earth Sciences Cold icy Mars Warm wet Mars Modern Mars What caused the loss of the Mars atmosphere and hydrosphere. Key Terms. Atmosphere. – a thin envelope of gases that encircles the earth and other particles (aerosols). Weather. – the state of the atmosphere at a specific place and time. Meteorology. – the study of the atmosphere and the processes that cause weather. Sunrise . from space over the South China Sea. An astronaut would see something like this; clearly defined bands of color through the atmosphere as the sun rises. High-peaking cumulus clouds, topping out in anvil-head cirrus can be seen as black shadows against the sunlit horizon. The brightness of the colors in the atmosphere in this photograph is due to the amount of dust in the atmosphere. More dust is found in near the equator. There are various sources for such upper level dust. Many dust storms in Africa and ash clouds from major volcanic eruptions are two reasons. . Shu. Lin. RBRC. I. . Iatrakis. , SL, Y. Yin 1405.XXXX. Outline. Axial charge in electroweak theory and QCD. Review of axial charge generation at weak coupling and strong coupling. A close look at anomaly equation. Electrical Coupling within the Earth System. Abstract. Convenors. and program committee. Objectives and Science Foci (5 science questions?). Session topics – same as science questions?. Conference format, schedule and potential speakers. of . biomolecular. and small-molecule . charge transfer reactions. Spiros. S. Skourtis. Department of Physics, University of Cyprus. Nicosia Cyprus. DPG Annual & Spring. Meeting. 2014, Symposium on . Nathalie . Degenaar. . University of Michigan. X-ray observations. Interior properties. Thermal evolution. Neutron stars . in transient X-ray binaries. Quiescence. :. No/little accretion. Faint X-ray emission. E4.p2X-A,F, I. Characteristics of the Atmosphere. Composition of the Atmosphere. Atmosphere. -mixture of gases around the Earth. 78% Nitrogen-(released from decay/eruptions). 21% Oxygen. 1% Other- (Carbon Dioxide, Argon). pg. . 115. http://www.indiana.edu/~g103/G103/week9/wk9.html. . http://www.uwgb.edu/DutchS/EarthSC202Notes/quakes.htm. . Folding. : . When . Rock Layers. . Bend. . because of STRESS. What are anticlines?. Objectives. Describe the composition of Earth’s atmosphere.. Explain why air pressure changes with altitude.. Explain how air temperature changes with atmospheric composition.. Describe the layers of the atmosphere.. Atmosphere Essential Question: How are we changing our atmosphere? Learning Goals: Be able to identify the layers of the atmosphere. Describe what molecules make up the atmosphere. Atmosphere Atmosphere ATMOSPHERE Composition of the Atmosphere The atmosphere is comprised of a variety of gases: Major Constituents (99%): Nitrogen (N): 78% Oxygen (O 2 ): 21% Trace Constituents: Other: 1% calls. CW2015. Kristian. S. . Mogensen. Marine Prediction . Section. k.mogensen@ecmwf.int. Overview of talk:. Baseline:. The focus of this talk is going to be on coupling of IFS and WAM to NEMO. Motivation. . The layer of gases surrounding Earth; composed mainly of 78% nitrogen and 21% oxygen, and other gases (water vapor, dust, pollutants, etc.). Brainpop: . Earth’s atmosphere. Layers of the Atmosphere. From the power spectral density shape a square root formula has been d. educted and used in Sweden.. Simple simulations models indicate that such formula may be true in some speed interval.. What experience is there from other markets?.