PPT-The Influence of Solar Variability on the Atmosphere and Oc

Speaker PeiYu Chueh Adviser YuHeng Tseng Date 20100916 Review Observation Solar variability The amplitude of the solar cycle is relatively small about 02 Wm 2. APES. Ms. . Tooker. 2015. Composition. Earth’s atmosphere is composed of seven primary compounds:. Nitrogen. . (N. 2. ) 78%. Oxygen (O. 2. ) 21%. Water vapor (H. 2. O) 0-4%. Carbon dioxide (CO. the Earth on solar EUV observations from LEO satellites . V. Slemzin. 1. , A. Ulyanov. 1. , S. Kuzin. 1. , K. Gaikovitch. 2. , D. Berghmans. 3. , M. Dominique. 3. , B. Nicula. 3. , F. Hourrier. atmosphere . to the upper atmosphere and ionosphere is through the generation and propagation of waves.. . Wave Coupling in the Atmosphere-Ionosphere System . 1. Jeff Forbes, Aerospace Engineering Sciences . Ch 27. Questions??. What are some theories about how our solar system began?. The Nebular Hypothesis. solar nebular. a rotating cloud of gas and dust from which the sun and planets formed. In 1796, French mathematician . Terra-forming. ASTR 1420. Lecture . 2. 6. Not . in the Textbook. Space Colonization. Space colonization in this lecture is a narrow sense : colonization by human and in the Solar System only (say within next few . Chapter 23. 23.1 The Solar System. 99.85%. of the mass of our solar system is in the Sun, planets make up the rest.. Gravity holds planets in orbit.. Overview of the Planets. . Terrestrial planets. The . Milky Way Galaxy. , one of billions of other galaxies in the universe, contains about 400 billion stars and countless other objects.. Why is it called . the “Milky Way?”. Welcome to your Solar System, how well do you know your neighbors?. Stars, solar systems form within giant molecular clouds. Requires . high density. , . dust, and low temperatures. to initiate gravitational . collapse. Most material is hydrogen and helium; only a few percent is other elements. Characteristics/Composition /Position . Planets of the Solar System . The Solar System Song . Terrestrial Planets . These planets are solid and rocky . There are four terrestrial planets Mercury, Venus, Earth and Mars . from PROBA2/LYRA/SWAP. R. . Kariyappa. (guest investigator), . S. T. Kumar, M. Dominique, . D. . Berghmans. , L. Dame, C.L. . Pradeep. Objectives. Analyze the source of variability of. . Lyra. channels 3 and 4 . in this class.. You will be compensated $$$ for your note-taking.. To . apply to be a note-taker please visit. http://sds.umbc.edu/becoming-a-note-taker/. Composition and Structure of the Atmosphere. The atmosphere APES Ms. Tooker 2015 Composition Earth’s atmosphere is composed of seven primary compounds: Nitrogen (N 2 ) 78% Oxygen (O 2 ) 21% Water vapor (H 2 O) 0-4% Carbon dioxide (CO 2 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% Matthew DeLand. 1. 1. Science Systems and Applications, Inc. (SSAI). Impacts of Intermediate Time Scale SSI Variability Workshop. 9 December 2018, Columbia, MD. Definition of “Short-Term SSI Variability”.