Phys II Eng Full
Theoretical Optics
Pg 1 Spherical Grating Spectrographs Darragh O’Donoghue Southern African Large Telescope Foundation (SALT) & Chris Clemens Univ. of North Carolina The.
Optics and Telescopes Chapter Six. Telescopes The fundamental purpose of any telescope is to gather more light than the naked eye can In many cases telescopes.
Cherenkov Detectors. Index of Refraction When light passes through matter its velocity decreases. –Index of refraction n. The index depends on the medium.
CONCAVE MIRROR SUBJECT-SCIENCE CLASS-X CONCAVE MIRROR SUBJECT-SCIENCE CLASS-X CONCAVE MIRROR SUBJECT-SCIENCE CLASS-X PREPARED BY- PREPARED BY- SRADHANJALI.
Chapter 34: Mirrors 1 We will consider three varieties of mirrors Spherical Concave Mirror Plane Mirror Spherical Convex Mirror Photos from Fishbane,
Optics and Telescopes Chapter Six. Guiding Questions 1.Why is it important that telescopes be large? 2.Why do most modern telescopes use a large mirror.
Announcements No lab tonight due to Dark Sky Observing Night last night Homework: Chapter 6 # 1, 2, 3, 4, 5 & 6 First Quarter Observing Night next Wednesday.
Optical Imaging in Astronomy 1st CASSDA School for Observers Observatorio del Teide, 20 – 25 April 2015 Franz Kneer Institut für Astrophysik Göttingen.
Lecture 18 Ray Optics-4 Chapter 23 PHYSICS 270 Dennis Papadopoulos March 24, 2010.
Image Formation. The light rays coming from the leaves in the background of this scene did not form a focused image on the film of the camera that took.