Archaeology, Formality & the CIDOC CRM Leif Isaksen, Kirk Martinez & Graeme Earl ECS/Archaeology University of Southampton.
Stars Dr Katy Lancaster. Overview Introduction to stars –What they are –What we can measure The Hertzsprung-Russell Diagram Star life cycles –Evolution.
Boating Course Weather Canadian Power & Sail Squadrons.
Topic 4 : I/O Devices & Networks I/O Devices and Techniques Reference : G & L pp 169-170 (note that most of the material isnt in G & L)
Magnetic Fields in T Tauri Disks A. Meredith Hughes Wesleyan University What Millimeter Polarimetry Can Tell Us Chat Hull, David Wilner, Sean Andrews,
Characterisation of Aerosols over Indo- Gangetic Basin during Winter Season By Hiren Jethva Ph.D. Student Centre for Atmospheric & Oceanic Sciences Indian.
Lunar Eclipse Chapter 3 from book. Objectives To be able to describe the phenomenon of how a lunar eclipse occurs. To be able to apply what they already.
Chapter 3 Photophysics. Emission and loss processes: Several of pathways for loss of electronic excitation shown in Fig. as a emission of light as luminescence.
MAP TAP 2003-2004The Electromagnetic Spectrum1 Wavelength/frequency/energy.
Presented By: Usama Ashraf ID: 110101001 Terminal Doppler Weather Radar (TDWR): TDWR is a doppler weather radar system used primarily for the detection.
Electromagnetic waves are transverse wave, made up of continually changing electic and magnetic fields. Like mechanical waves, electromagnetic waves.
Could Planets orbiting Red Dwarf Stars support Oxygenic Photosynthesis and hence Complex Life? - A reappraisal and update. Joe Gale Institute of Life Sciences.