Photochemistry can be dramatically different from “ordinary” chemistry See example below.

Slides:



Advertisements
Similar presentations
Atmospheric chemistry
Advertisements

Applications of UV-Vis Spectroscopy
5-2. OZONE LAYER Formation of Ozone Layer  Ozone layer: A part of stratosphere (ca. 20km high) in which ozone concentration is relatively high.
1 Microwave Interactions with the Atmosphere S. L. Cruz Pol Electrical and Computer Engineering University of Puerto Rico.
Climate-Greenhouse Effect. Greenhouse Glass, the material that greenhouse is made of, 1) transmit short-wavelength visible light, 2) absorbs and redirects.
Chemistry in the Atmosphere Chapter 17 Copyright © The McGraw-Hill Companies, Inc. Permission required for reproduction or display.
Chapter 12 Alkanes 12.4 Haloalkanes.
The Stratospheric Chemistry and The Ozone Layer
MALDI-TOF:
Chemical Kinetics Chapter 12
Balancing Chemical Equations
Atmospheric Chemistry Global Warming. GasMole Percent N O Ar0.934 CO O3O3 1.0 x Composition of Atmosphere:
IR absorption Greenhouse gases vary in their ability to trap IR radiation, One molecule of Methane is 26 times more effective at IR absorption than one.
Meto 637 Lesson 11. The Ozone Hole Antarctic total ozone.
Atmospheric Chemistry Global Warming. GasMole Percent N O Ar0.934 CO O3O3 1.0 x Composition of Atmosphere:
Pat Arnott, ATMS 749, UNR, 2008 Chapter 9: Absorption by Atmospheric Gases Visible and UV Absorption: due to electronic transitions. Monatomic - polyatomic.
Refrigeration and Cryogenics Maciej Chorowski Faculty of Mechanical and Power Engineering.
Electron Dot and Structual Diagrams for Covalent Compounds.
Earth’s Atmosphere. Atmosphere Envelope of gases that surround the Earth Envelope of gases that surround the Earth Protects the Earth Protects the Earth.
Greenhouse Effect - Natural Heating of Earth’s surface by certain atmospheric gases.
The Atmosphere Chapter 18. The atmosphere supports life  Living things occupy only a relative thin layer of the Earth’s crust. –The ocean and the atmosphere.
MwpntspeciesMwcalc 191H+1, C+11, CH+13, CH2+13, CH3+15, C2+24, C2H+24, C2H2+25,94874.
Symmetry Edward A. Mottel Department of Chemistry Rose-Hulman Institute of Technology.
Chapter 4 and 6 Foldable notes
Spectrometry and Photochemistry Theodore S. Dibble Chemistry Department SUNY-Environmental Science and Forestry Syracuse, NY.
The Greenhouse Effect *The earth is similar to a greenhouse. The earth atmosphere acts like the glass in a greenhouse. *Sunlight streams through the.
Greenhouse Gases and Energy Budget LP 3 1. What are greenhouse gases? Where do they come from? How do they work? 2.
1974 Sherwood Rowland & Mario Molina Calculated that CFCs were lowering the average concentration of Ozone in the stratosphere. Chemical Time Bomb: Spray.
Space Science: Atmosphere Part -2 Thermal Structure Stability of an Air Mass Absorption of Radiation Chapman Layer Ozone.
TROPOSPHERIC OZONE AND OXIDANT CHEMISTRY Troposphere Stratosphere: 90% of total The many faces of atmospheric ozone: In stratosphere: UV shield In middle/upper.
The Earth’s Atmosphere. Temperature Temperature is a measure of the average speed of the molecules, faster motion = higher temperature. Temperature is.
Essential Questions: 1) What role have humans played in the destruction of the Ozone Layer? 2) Why should humans be concerned about the destruction of.
Ozone O3O3 Ozone Depletion Ozone (O 3 ) –Absorbs harmful UV radiation from sun ozone is produced during lightning storms Chlorofluorocarbons (CFC’s)
Atmosphere. Space Ice The original stellar nebula included water. –Icy grains in protoplanets Half of Earth’s water from came from before the Sun. Bill.
Solving the Ozone Puzzle. Troposphere Layer where our weather takes place. Layer closest to the earth’s surface. Layer we breathe. Ozone is created here.
Ozone Depletion O3O3. Ozone Factoids Good in the stratosphere, bad in the troposphere Produced at a height of ~50 km, settles to a height of 23 km Filters.
Response of the Earth’s environment to solar radiative forcing
12 34  ozone (O 3 ) is both created and destroyed in the atmosphere  UV from the sun splits molecular oxygen (O 2 ) into single atoms (O) that then.
1 Microwave Interactions with the Atmosphere Microwave Interactions with the Atmosphere S. L. Cruz Pol Electrical and Computer Engineering University of.
© Oxford University Press, All rights reserved. 1 Chapter 3 CHAPTER 3 THE GLOBAL ENERGY SYSTEM.
Arthur N. Samel Chair, Department of Geography Bowling Green State University & Chief Reader, Advanced Placement Environmental Science Program.
Atmospheric Chemistry. Objectives Know the components of the atmosphere. Discuss the different forms of electromagnetic radiation emitted by the sun.
The Atmosphere The atmosphere is the layer of gases that surrounds the Earth. Earth’s atmosphere is a mixture of nitrogen, oxygen, water vapor, and many.
The Dynamic EarthSection 2 Objective #9 Describe the layers of the Earth’s atmosphere.
Atmosphere Students know the origin/effects of temperature inversions.
Green Chemistry This lesson we will...
EÐL620M / Life in the Universe
Temperature Changes With Earth’s Atmosphere
Temperature Changes With Earth’s Atmosphere
OZONE DEPLETION Ayşe Melis AYGAR 12/D 1261.
9. Reaction dynamics /.
TROPOSPHERIC OZONE AND OXIDANT CHEMISTRY
Chemistry in the Atmosphere
GLOBAL ENERGY BUDGET - 3 Atmosphere Basics.
Section 2 The Ozone Shield
The Structure of the Atmosphere
CH 3: The Electromagnetic Spectrum
Photochemistry Ljósefnafræði, hefur áhuga á efnafræðilegum áhrifum ljóss Efni örvað með ljóseindum (e.photons) úr grunnástandi í örvað ástand Efni aförvast.
Chemistry and Contrails
Intercontinental Transport, Hemispheric Pollution,
Points for discussion Have human activities changed the composition of Earth’s atmosphere? Has Earth’s temperature changed in the past 150 years? In the.
Atmospheric Layering.
Air Pollution contamination of the atmosphere
Climate Change.
Atmosphere and Climate Change
Atmospheric Layering.
Photochemistry can be dramatically
Chlorofluorocarbons (CFCs) and their impact on Environment
What is ozone? An ozone molecule is a temporary association of three oxygen atoms. Energy from lightning or ultraviolet radiation from the sun breaks.
Presentation transcript:

Photochemistry can be dramatically different from “ordinary” chemistry See example below

Ar Cl

Ar Cl...

Ar

Cl Ar + -

Cl Ar

O3 O3O3 Cl Hvernig er efnafræði ósoneyðingar- innar?/ Ozon depletion?

( ) 20 km ( )

Heildarloftstyrkur og ósonstyrkur yfir jörðu. / Concentration profiles for air and ozone in the Earth´s atmosphere.

20 km

Gleypni ósons á nær-útfjólubláa litrófssviðinu. Gleypnistuðull er í réttu hlutfalli við gleypni efnisins fyrir fastann efnisstyrk. Absorption cross section of ozone in the near UV spectral region.

20 km

20 km O 3 + O -> O 2 +O 2

Chemistry and spectroscopy of the greenhouse effect/ Global warming effects(?)

Gegnskin og gleypni andrúmsloftsins ÚF SÝNSÝN IR

Bylgjulengd (  m) Gleypni O=C=OO=C=O

UltravioletVisibleNear-IRInfraredFar-InfraredMicrowave

Organic photochemistry: photoisomerization

Stilben e(1)

Stilbene(2)

Astrochemistry

C2H2C2H2 Big organic molecules : Life(?) ???

C2H2C2H2 Big organic molecules : Life(?) ???

C2H2C2H2 Big organic molecules : Life(?) ??? C2C2 C CH 2

H+H+ CH + CH 2 + C+C+ C2+C2+ C2H+C2H+ C2H2+C2H2+ Magn jóna Ion yield LASER radiation of C 2 H 2 Mw Time of flight

Orka HCCH: HCCH*:

Orka C2C2 H2H2 HCCH*: C2C2 + +

Orka HCCH*:

Orka HCCH*: CH 2 C

A + M ??? M 1 + M 2 ??? A + B C + D Reaction cross section:

A + M ??? M 1 + M 2 ??? A + B C + D Cross section =  = 2  d But ions: Reaction cross section:

A + + B C + D But ions: F  1/r 2 Reaction cross section:

+ A + + B C + D But Ions: Reaction cross section:

A + + B C + D But ions: ++ Collision frequency much larger Reaction cross section:

A + M ??? M 1 + M 2 ??? A + B C + D d + Ions: Collision cross section =  >> 2  Reaction cross section: