1 / 12

METEO 3 Lab 1

METEO 3 Lab 1. 9/4/19. TA: Rachel Gutierrez Office: 412 Walker Office Hour: Thursdays 10am – 11am or by appointment Email: rachel.tstorm@gmail.com Labs are due on Fridays at the beginning of class. Tips for Labs. Bring a hard copy of the lab Come ready with questions

mindys
Download Presentation

METEO 3 Lab 1

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. METEO 3 Lab 1 9/4/19

  2. TA: Rachel Gutierrez Office: 412 Walker Office Hour: Thursdays 10am – 11am or by appointment Email: rachel.tstorm@gmail.com Labs are due on Fridays at the beginning of class

  3. Tips for Labs • Bring a hard copy of the lab • Come ready with questions • Bring the textbook • Show all work for problems (and all units!) • Work with other students to solve problems but don’t copy each other • Don’t wait until the last minute • Come to office hours

  4. Problem 1.4: Temperature Conversions • What is absolute zero? • In K? • Convert to oC • Convert to oF • Use C  F and F  C conversions to find out what’s special about -40oF

  5. Problem 1.7: Isoplething

  6. Problem 1.7: Isoplething • What’s an isopleth? • Line of constant __________ • Isobar: line of constant pressure • Isotherm: line of constant temperature • Isodrosotherm: line of constant dewpoint • Isoplething is like connecting the dots • To check your isopleths: does your line fit between the surrounding numbers correctly? • Don’t isopleth where you don’t have data • Don’t cross your isopleths • Label your isopleths • Isopleths can form closed loops

  7. Problem 2.1: Radiation • Stefan-Boltzmann Law: • E = σT4 • E: energy emitted per unit area (W m-2) • σ: 5.67 x 10-8 W m-2 K-4 • T: temperature (K) • a) E sun / E earth • b) Find E for both Venus and Mars • c) Thought question – why do you think Venus has a high temperature? What is unique about the atmosphere?

  8. Problem 2.2 and 2.6: Radiation • Wien’s Law: • Wavelength of Maximum Emission = • 2.2: Find wavelength of max emission for: • Sun • Earth • Human body • 2.6: This problem discusses energy … so use Stefan-Boltzmann Law! • What happens when you emit more than you absorb? • What happens when you absorb more than you emit?

More Related