Weather and Climate Jim Keller & Paul Belanger. Classroom assistant: Fritz Ihrig. Week 2: January 22 nd, Announcements

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Weather and Climate Jim Keller & Paul Belanger Classroom assistant: Fritz Ihrig Week 2: January 22 nd, 2019 1 Announcements Fritz Ihrig; classroom assistant, liaison to OLLI: fgihrig@msn.com ; h. 303-526-1750 Announcements: Paul Belanger: PEBelanger@glassdesignresources.com c. 303-249-7966; h 303-526-7996 Jim Keller: kellerjb10@aol.com H 303-526-0867 c 303-503-9711 2 1

WEEK 2 3 2 nd Session links/references Links: Disk 4 References: https://www.space.com/17683-earthatmosphere.html https://en.wikipedia.org/wiki/electromagnetic_spectrum ; https://en.wikipedia.org/wiki/thermal_radiation; https://www.acs.org/content/acs/en/climatescience/greenhousegase s/properties.html Links: Disk 5 References: http://hyperphysics.phyastr.gsu.edu/hbase/thermo/heatra.html Link Disk 6: References: https://en.wikipedia.org/wiki/santa_ana_winds ; https://en.wikipedia.org/wiki/chinook_wind 4 2

5 Radiation: https://en.wikipedia.org/wiki/electromagnetic_spectrum Solar radiation Earth radiation High Energy High Frequency 6 3

Radiation 7 Where the energy of the sun is distributed 44% 7% 37% 11% 8 High Energy High Frequency 4

Sun vs. Earth Energy in = energy out No overlap Short waves from Sun Long waves emitted from the entire Earth s surface SUN = EARTH ~290 K High Energy High Frequency 9 Reflection & Absorption A color of something indicates the color that is NOT absorbed Which gases absorb Infrared: carbon dioxide (CO 2 ), water (H 2 O), Nitrous Oxide (N 2 O), methane (CH 4 ), etc. Absorption vs. emission video talks about: Black body absorption, plus specific affinity for infrared due to greenhouse gases molecular vibrations: https://www.acs.org/content/acs/en/climatescience/greenhousegases/properties.html Black body emission depends on temperature of emitter: https://en.wikipedia.org/wiki/thermal_radiation But greenhouse Gases also emit infrared at specific frequencies 10 5

The Atmosphere absorbs BEST what the Sun makes the LEAST of SUN 11 A progression of captures from video EARTH 12 6

13 14 7

How GHGs Blanket the Earth Blanket Earth: NASA Global Climate Change Cause: http://climate.nasa.gov/causes/ Denial 101x Video: Global warming: https://www.youtube.com/watch?v=aqkgocglp_u&feature=youtu.be Denial 101x Video: Increasing Greenhouse Effect: https://www.youtube.com/watch?v=we8vxwa83fq 15 16 8

Greenhouse Warming 17 Lecture 5: Conduction vs. convection 18 9

19 The Sun High Energy High Frequency 20 10

21 Unequal heating: Sun s energy is spread out towards poles 22 11

Obliquity 41,000 year 23 The Earth s Elliptical Orbit CHANGES EVERY 100,000 YEARS 24 12

Radiation, conduction, convection Radiation does not need mass to transfer energy Conduction needs mass solid or fluid (gas or liquid) Convection needs mass and it needs to be a fluid (gas or liquid) What is heat? = a property (internal energy heat transfer temperature is the means to measure ; something that s hot -flow of energy Heat transfer = Heat capacity of substances 25 Conduction and rotation 26 13

Transfer of Energy Warm to cold Objects differ in conductive properties Air poor conductor - poor in transfer of heat Water conducts 26x better 650 times worse than copper Air = good insulation 27 Thermal Inertia (Heat Capacity) Thermal Heat conductivity, inertia convection (Heat Capacity) & thermal inertia Heat Transfer (Q) = Cp (T2 T1) Cp = heat capacity Water has high heat capacity solids typically have much lower heat capacity 28 14

Convection Wind as the means 29 Convection of Fluids Hot fluid becomes less dense and rises; cold fluid descends to replace it and is heated in turn. 30 15

FROST 31 Lecture 6: Sea Breezes and Santa Anas In Colorado Chinook winds 32 16

1/21/2019 Temperature differences Varying locations Varying amounts of sun (due to clouds, latitude (incident angle), time of year, time of day Surface color: albedo, heat capacity/thermal inertia (water vs. land) Radiation, conduction, convection Winds to equalize Hot to cold vs cold to warm expressions 33 Pressure Decreases with height Isobars = pressure Temperature differences make pressure differences NEW thickness of parcel of air Starting thickness of parcel of air NEW thickness of parcel of air Starting thickness of parcel of air 34 17

1/21/2019 From a certain height: when I look toward colder area, both 500 and 1000 mb below; but when I look toward warmer 1000 mb still below but 500 mb above. Cold dense air lowers 500 mb level. 35 This makes wind From high to low adds mass and then creates a circulation l 36 18

1/21/2019 Sea Breezes Ocean absorbs more heat than land But land heats faster (lower thermal inertia /heat capacity) so less dense air rises, moves out over ocean, cools and descends; cool air from ocean moves to land replacing rising hot air and is heated in turn 37 Typical weather stations Temperature measured at 2.5 m above surface Wind at 10 m above surface And free of buildings 38 19

1/21/2019 39 The breeze reverses at night when the land cools faster 40 20

1/21/2019 Wind chill 41 How to change air temperature Mix, but parcels of air of different densities don t easily mix. Thermally direct: Change pressure i.e. change parcel s elevation (in absence of heat input) Chinook & Santa Ana winds compress and heat up when losing altitude Thermally indirect forcing air to descend over warm ground Or forcing cold air to rise over cold air 42 21

1/21/2019 Katabatic winds Cp = heat capacity https://en.wikipedia.org/wiki/katabatic_wind https://en.wikipedia.org/wiki/anabatic_wind 43 End of week 2 lessons 4, 5 6 44 22