'Total emission' diaporamas de présentation

Radiation Basics - Light properties

Radiation Basics - Light properties. Remember that light is composed of photons which behave as both particles and waves. As waves, we can define the type of radiation by its wavelength, ? (?m) , or frequency, ? (hz) , which are related by:

638 views • 41 slides

Lecture 3 Radiation and Planetary Energy Balance

Lecture 3 Radiation and Planetary Energy Balance. (provide a review and add something new). Electromagnetic Radiation. Oscillating electric and magnetic field s propagate through space

461 views • 35 slides

H 3 + and the Planets

Steve Miller. H 3 + and the Planets. H 3 + - the driver of planetary atmospheres. Steve Miller. H 3 + and the Planets. Formed above the homopause - thermosphere/ionosphere N a (h) = N a0 exp[-h/H a ] H a = [kT/m a g] Pressure < 1 m bar Number density < 10 18 m -3 Temperatures:

213 views • 20 slides

Application of GIS for Emission Inventory

Application of GIS for Emission Inventory. HATHAIRATANA GARIVAIT and SIRAPONG SOOKTAWEE Environmental Research and Training Center, Thailand. xxx (Ton). xxx (Ton). xxx (Ton). xxx (Ton). emission (Ton). Assumption, Relation. Top-Down Method. SO 2 Emission plot by landuse 2003.

364 views • 15 slides

Density of active region outflows derived from Fe XIV 264/274

258 views • 15 slides

A SIMPLE MODEL FOR INTERACTION BETWEEN EQUIPMENT AT A FREQUENCY OF SOME TENS OF KHZ

272 views • 14 slides