1. The Earth and its Atmosphere

2. Temperature and the Seasons Why?

4. Solar Radiation Solar Constant Atmospheric Effects Angle of the Sun Length of the day

5. Solar Angle = angle above the horizon

6. Earth orbits the Sun once every 365 1/4 days as if it were riding along a flat plane. We refer to this imaginary surface as the ecliptic plane and to Earth’s annual trip about the plane as its revolution. Earth is nearest the Sun (perihelion) on or about January 3 (147,000,000 km). Earth is farthest from the Sun (aphelion) on or about July 3 (152,000,000 km).

13. The latitudinal position of the subsolar point is the solar declination, which can be visualized as the latitude at which the noontime Sun appears directly overhead.

14. What date is this?

23. Daily Insolation - top of the atmospere. 75º N in June gets more sun than the Equator Compare meridional gradient of insolation by seasons Very little tropical seasonality

25. Controls - Temperature Latitude Land and Water Ocean Currents Elevation

26. Mean July Temp (F.)

27. Mean January Temp (F.)

28. One of the most immediate and obvious outcomes of radiation gain or loss is a change in the air temperature. The map depicts differences between mean temperatures in January and July through the use of isotherms, which are lines that connect points of equal temperature.

35. Certain geographical factors combine to influence temperature patterns across the globe. These factors include latitude, altitude, atmospheric circulation patterns, local conditions, continentality, (the effect of an inland location that favors greater temperature extremes) and ocean current characteristics along coastal locations.

36. Data Air Temperature

39. Local Variations microclimates