'Solar flux' presentation slideshows

Part II Remote Sensing using Reflected Visible and Infrared Radiation

1.34k views • 118 slides

Climate Change A simple climate model

Climate Change A simple climate model. Dudley Shallcross and Tim Harrison, Bristol University. Simple climate model. A simple climate model Students can use an excel spreadsheet to run it Simple factors to change Can look at feedbacks on climate

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Selected Topics in Propagation

511 views • 36 slides

Lesson 2

Lesson 2. AOSC 621. Radiative equilibrium. Where S is the solar constant. The earth reflects some of this radiation . Let the albedo be ? , then the energy absorbed by the earth is (1- ? ) F s . The thermal energy emitted by the earth is ? B T e 4. Hence we get . Radiative equilibrium.

474 views • 32 slides

Lesson 2

Lesson 2. AOSC 621. Radiative equilibrium. Where S is the solar constant. The earth reflects some of this radiation . Let the albedo be ? , then the energy absorbed by the earth is (1- ? ) F s. The thermal energy emitted by the earth is ? B T e 4. Hence we get. Radiative equilibrium.

395 views • 32 slides

Conversations with the Earth Tom Burbine tburbine@framingham

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GOES-R Calibration Working Group: Progress and Status

GOES-R Calibration Working Group: Progress and Status. Jared Clarke CWG/GOES-R Program Liaison. GOES-R Program Overview. Objective: Provide the next generation in US geosynchronous meteorological products Flight Project: NASA-led effort to develop and procure spacecraft and instruments

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LYRA Tests and Calibration

LYRA Tests and Calibration. LYRA Meeting Davos 05/06 Oct 2006. Contents. I. From Model to Configuration II. BESSY Campaigns a. Flux Linearity b. Stability, Drift c. LEDs, Dark Current d. Spectral Responsivity e. Homogeneity, Flatfield f. Cadence, Response Time

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LYRA Tests and Selections

LYRA Tests and Selections. SCSL Meeting Bern 29 Nov - 01 Dec 2006. Contents. I. From Model to Configuration II. BESSY Campaigns a. Flux Linearity b. Stability, Drift c. LEDs, Dark Current d. Spectral Responsivity e. Homogeneity, Flatfield III. Summary.

381 views • 23 slides

The Weekend Effect

The Weekend Effect. Does it really exist in surface temperature and if so, what is the cause?. David Ridley (Ken Carslaw and Martyn Chipperfield). The Weekend Effect. > Why look at the weekend effect? > Aerosol & Cloud - Direct Effects - Indirect Effects

392 views • 22 slides

DEBUNKING NEUTRINO DETECTION EXPERIMENTS

DEBUNKING NEUTRINO DETECTION EXPERIMENTS. THE GHOSTLY NEUTRINOS. Hate them or love them, neutrinos do exist. Vector Particle Physics (VPP) automatically gives the correct structures and characteristics for the neutrinos.

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Statistical Analysis of Solar Geomagnetic Storm Occurrences

Statistical Analysis of Solar Geomagnetic Storm Occurrences. By: Seth Sivak. Why We Study Geomagnetic Storms. Blackouts Cell Phone Disruption Global Positioning Satellite Failure Danger to Satellites Danger to Astronauts Possible Danger to Airline Passengers.

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Term 8 Senior Design Project

Term 8 Senior Design Project. Sustainable Water Desalination Tuesday February 7, 2012. Project Team. Team Members: Mission Statement:

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Cassini UVIS Update: He 584 ?? Dayglow at Saturn

Cassini UVIS Update: He 584 ?? Dayglow at Saturn. Christopher Parkinson Ian Stewart and Yuk Yung January 05, 2006. Before. Voyager 1 and 2 epoch UVS He 584 A measurements showed brightness at disk center to be 3.1 +/- 0.4 and 4.2 +/- 0.5 R, respectively (Sandel et al., 1982)

328 views • 16 slides

Global Change: Class Exercise

Global Change: Class Exercise. Global Energy Balance & Planetary Temperature. Mteor/Agron/Envsci/Envst 404/504. Zero-Dimensional, Global Energy Balance Model. Zero-dimensional: steady, time-average averaged over all spatial directions Global: average is over the entire planet

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Paul Withers and Michael Mendillo Spring AGU talk SA24A-05 Tuesday May 18th, 2004, Montreal

Testing Simple Parameterizations for the Basic Characteristics of the Martian Ionosphere (How does the martian ionosphere respond to changes in solar flux?). Paul Withers and Michael Mendillo Spring AGU talk SA24A-05 Tuesday May 18th, 2004, Montreal.

251 views • 12 slides

VCE Unit 2

VCE Unit 2. At PLC. Time allotments Total time 65 periods. Movement: 25 periods Electricity: 15 periods Alternative sources of energy:15-20 periods Revision: 5-10 periods Total: 65 periods. Assessment tasks. 3 major assessment tasks as set in study guide Tests Exams

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Space weather effects on the Mars ionosphere due to solar flares and meteors

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Astronomy 340 Fall 2005

Astronomy 340 Fall 2005. Class #4 18 September 2007. Announcements. HW #1 due Thursday A little out of order Last time ? radiation (notes available today) This time ? tides. Solar Heating and Transport. Why? Astrophysics is all about how energy gets from point A to point B

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Full Solar Spectrum Photovoltaic Materials Identified

Full Solar Spectrum Photovoltaic Materials Identified. Perfect matching of band gap of In 1-x Ga x N to solar spectrum. LBNL, 2002. Literature. Energy (eV). Energy (eV). GaInP. GaAs. Ge. Solar Flux (10 21 photons/sec/m 2 / m m). Ga content in In 1-x Ga x N alloy. m.

134 views • 1 slides