'Circular aperture' presentation slideshows

Exoplanet Detection Techniques II GUASA 12/10/2013 Prof. Sara Seager MIT

Exoplanet Detection Techniques II GUASA 12/10/2013 Prof. Sara Seager MIT. Exoplanet Detection Techniques II. Planet Detection Techniques in More Detail Direct Imaging Microlensing Astrometry. Direct Imaging Lecture Contents. Direct Imaging Planet and Star Spatial Separation

1.15k views • 90 slides

FLIR Concept

FLIR Concept. Prepared by Ernest Grimberg - Opgal chief scientist. General background. Physical Constants. Basic radiometric concepts. Black body radiation. Optics - introduction. IR Detectors. Spatial resolution and thermal resolution. Signal processing block diagram. Table of contain.

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Interference

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1446 Introductory Astronomy II

1446 Introductory Astronomy II. Chapter 3 Light, EM Radiation & Telescopes R. S. Rubins Fall 2011. Dispersion of White Light by a Prism. The upper picture shows the variation of wavelength with color.

566 views • 47 slides

Lecture 16 Diffraction Chp. 36

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PC20312 Wave Optics

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Chapter 38 Serway & Beichner 6 th Ed.

Chapter 38 Serway & Beichner 6 th Ed. Diffraction. Fig 38-4a, p.1207. wave front. P. D = a. Phasor Model. Where we assume:. Note: ? = ? and E R = E ?. These produces the same interference patterns!. b. a. Diffraction from Circular Aperture. Diffraction and Interference. a.

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3671 Multi-Wavelength Astronomy

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11: Wave Phenomena

11: Wave Phenomena. 11.3 Single slit diffraction. Single Slit Diffraction We have already established that diffraction will occur at an aperture of width b if ? ? b

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Fraunhofer Diffraction: Circular aperture

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When Texture takes precedence over Motion

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Announcements

Announcements . Project Medley Outlines due Tuesday! 1 page typed and double-spaced What do you plan to do for your project? On-Campus Observing Moved (likely July 15, depending on weather forecasts). Photometry of the Pleiades. Tiffany Pewett pewett@chara.gsu.edu. The Pleiades.

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A: Wave Phenomena

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The Resolution Of A Telescope

The Resolution Of A Telescope. ?. The resolving power of a telescope is the ability of the device to measure the angular separation ( ? ) of the points in an object. Light From A Star.

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