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The top documents tagged [radio astronomy slide]

Wind Power and Radio Astronomy A. Jessner, MPIfR Effelsberg April 2010
Wind Power and Radio Astronomy A. Jessner, MPIfR Effelsberg April 2010
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23/01/2009 1 ITU-R Study Group Activities Kevin Hughes Radiocommunication Bureau ITU Kevin Hughes Radiocommunication Bureau ITU
23/01/2009 1 ITU-R Study Group Activities Kevin Hughes Radiocommunication Bureau ITU Kevin Hughes Radiocommunication Bureau ITU
217 views
Padova 03 3D Spectrography 3D Spectrography: II - The tracers Morphology: distribution of each component Dynamics: kinematics via the emission or absorption
Padova 03 3D Spectrography 3D Spectrography: II - The tracers Morphology: distribution of each component Dynamics: kinematics via the emission or absorption
217 views
Receiver Systems Alex Dunning. The Basic Structure of a typical Radio Telescope CSIRO. Receiver Systems for Radio Astronomy ReceiverConversionDigitiser
Receiver Systems Alex Dunning. The Basic Structure of a typical Radio Telescope CSIRO. Receiver Systems for Radio Astronomy ReceiverConversionDigitiser
218 views
National Science Foundation 1 Andrew CLEGG U.S. National Science Foundation aclegg@nsf.gov Third Summer School on Spectrum Management for Radio Astronomy
National Science Foundation 1 Andrew CLEGG U.S. National Science Foundation [email protected] Third Summer School on Spectrum Management for Radio Astronomy
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On-line collaboration with SURFnet. Outline SURFnet organisation Lightpaths for science Goup Communication -SURFgroepen -Videoconferencing and webconferencing
On-line collaboration with SURFnet. Outline SURFnet organisation Lightpaths for science Goup Communication -SURFgroepen -Videoconferencing and webconferencing
218 views
Weather Forecasting for Radio Astronomy Part I: The Mechanics and Physics Ronald J Maddalena August 1, 2008
Weather Forecasting for Radio Astronomy Part I: The Mechanics and Physics Ronald J Maddalena August 1, 2008
214 views
Chapter 3: Telescopes. Images can be formed through reflection or refraction. Reflecting mirror 3.1 Optical Telescopes
Chapter 3: Telescopes. Images can be formed through reflection or refraction. Reflecting mirror 3.1 Optical Telescopes
229 views
HELIX ANTENNAS REAL WORLD COMPARISON MEASUREMENTS Clare - VE3NPC QCWA Dinner Nov. 21, 2006
HELIX ANTENNAS REAL WORLD COMPARISON MEASUREMENTS Clare - VE3NPC QCWA Dinner Nov. 21, 2006
221 views
The Electromagnetic Spectrum. Optics and Photonics is an enabling technology and science It enables advances in many different disciplines of science,
The Electromagnetic Spectrum. Optics and Photonics is an enabling technology and science It enables advances in many different disciplines of science,
216 views
Electromagnetic Wave Propagation High School Science Demonstration Melanie Leong June 25, 2003
Electromagnetic Wave Propagation High School Science Demonstration Melanie Leong June 25, 2003
217 views
Electron Scattering Length - Mean Free Path – le - Avg. distance between scattering Si - ~ 5nm; GaAs - ~ 100 nm Electrical Resistance is closely related
Electron Scattering Length - Mean Free Path – le - Avg. distance between scattering Si - ~ 5nm; GaAs - ~ 100 nm Electrical Resistance is closely related
219 views