Slide 1 First direct image of extrasolar planets Slide 2 Slide 3 10.7 billion miles Slide 4 Fomalhaut A is 16 times brighter than the Sun and is 200 million years old. The…

Slide 1 Slide 2 Coronal hard X-rays prior to RHESSI H. S. Hudson Space Sciences Lab, UC Berkeley Slide 3 Coronal hard X-rays prior to RHESSI H. S. Hudson Space Sciences Lab,…

Slide 1 Slide 2 PHY134 Introductory Astronomy Tides and Matter 1 Slide 3 Leftovers Earth is in free fall under gravity of Sun, so Sun’s gravity has no effect on Earth!…

Slide 1 Optical flow (motion vector) computation Course: Computer Graphics and Image Processing Semester:Fall 2002 Presenter:Nilesh Ghubade ([email protected]) Advisor:…

Slide 1 Properties and Detection of Sound The human ear is a detector that receives pressure waves and converts them into electrical impulses. Sound waves entering the auditory…

Slide 1 Slide 2 1 Waves and Vibrations Slide 3 2 Common Wave Characteristics: Waves come in many types: water, sound, radio, light, etc. Slide 4 3 Wave Parts: T = 1/f Frequency:…

Slide 1 ***Doppler effect … Slide 2 What is the Doppler effect? Slide 3 NEXRAD Slide 4 Stationary observers hear the frequency of the source. Slide 5 Can you estimate how…

Waves transfer energy without transferring mass. Figure 6-1 You can use a domino to knock over other dominoes in two different ways: (a) you can throw a domino, or (b) you…

AGATA: Status and Perspectives E.Farnea INFN Sezione di Padova, Italy on behalf of the AGATA Collaboration Outline Basic concepts: pulse shape analysis and gamma-ray tracking…

3. Seismic Sources and Source Parameters 3.3 Determination of fault-plane solutions (M. Baumbach, H. Grosser) 3.4.1 Introduction The direction (polarity) and amplitude of…