Noise (electronics)

Noise temperature (antenna)

In radio frequency (RF) applications such as radio, radar and telecommunications, noise temperature of an antenna is a measure of the noise power density contributed by the antenna to the overall RF receiver system. It is defined as "The temperature of a resistor having an available thermal noise power per unit bandwidth equal to that at the antenna’s output at a specified frequency." In other words, antenna noise temperature is a parameter that describes how much noise an antenna produces in a given environment. This temperature is not the physical temperature of the antenna. Moreover, an antenna does not have an intrinsic "antenna temperature" associated with it; rather the temperature depends on its gain pattern, pointing direction, and the thermal environment that it is placed in. (Wikipedia).

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Sound waves interference!

In this video i demonstrate sound waves interference and standing waves from loudspeaker used sound sensor. The frequency on loudspeaker is about 5500Hz. Enjoy!!!

From playlist WAVES

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Astronomy - Ch. 5: Light & E&M Radiation (6 of 30) Difference of E&M Frequence

Visit http://ilectureonline.com for more math and science lectures! In this video I will explain the different frequencies of electromagnetic radiation.

From playlist ASTRONOMY 5 LIGHT AND RADIATION

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Waves 3_4 Interference

Intensity and sound levels.

From playlist Physics - Waves

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Waves 3_5 Interference

Intensity and sound levels.

From playlist Physics - Waves

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thermo-acoustics

skip to 3:50 if you are impatient.

From playlist NightHawkInLight Community Video Responses!

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Physics 50 E&M Radiation (4 of 33) Frequency of E&M Radiation and Temperature

Visit http://ilectureonline.com for more math and science lectures! In this video I will explain the relationship of an object (and it's temperature) and the kinds of E&M radiation emitted from the object. Next video in series: http://youtu.be/SCMK0UJH1p4

From playlist PHYSICS 50 ELECTROMAGNETIC RADIATION

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Waves 3_6 Intensity and Sound Level

Intensity and sound levels.

From playlist Physics - Waves

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Waves 3_7 Intensity and Sound Level

Intensity and sound levels.

From playlist Physics - Waves

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Physics 20 Sound and Sound Waves (3 of 53) Velocity of Sound in Air

Visit http://ilectureonline.com for more math and science lectures! In this video I will show you how to find v=? of sound (in air) at various temperatures.

From playlist PHYSICS MECHANICS 5: WAVES, SOUND

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What is the Cosmic Microwave Background Radiation? And what does it mean?

This video provides an overview of the accidental discovery and explanation of the cosmic microwave background radiation, the afterglow of the big bang. After reviewing the initial experimental work of Penzias and Wilson, a detailed account of the theoretical interpretation is presented, i

From playlist Cosmology

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GRCon19 - RF System Synchronization - LO's by Dan Baker

RF System Synchronization - LO's by Dan Baker, Brian Avenell Multi-channel applications including MIMO, phased array RADAR, and direction finding require channel-to-channel phase and time synchronization. Phase synchronization implies having deterministic relative phase between all of the

From playlist GRCon 2019

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25c3: RF fingerprinting of RFID

Speakers: cryptocrat, Boris Danev In the lecture portion of this workshop we will present an overview of existing and our own novel methods for hacking electronic passports and driver's licenses including novel radio frequency fingerprinting techniques. In the the hands-on section we wi

From playlist 25C3: Nothing to hide

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GRCon20 - Software defined radio based Synthetic Aperture noise and OFDM (WiFi) RADAR mapping

Presented by Jean-Michel Friedt, and Weike Feng at GNU Radio Conference 2020 https://gnuradio.org/grcon20 Software defined radio based Synthetic Aperture noise and OFDM (WiFi) RADAR mapping (Main Track) [application] Session Chair: Jean-Michel Friedt, FEMTO-ST/Time & Frequency We demonst

From playlist GRCon 2020

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MagLab User Summer School: The Physics of Noise and Musings of Experimental Errors

This video was recorded in 2016 at the National MagLab’s annual User Summer School, where early-career scientists learn from lab experts best practices for conducting experiments at the lab. For more information, please visit https://nationalmaglab.org/user-summer-school

From playlist User Summer School Talks

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Observing Cosmic Dawn Through 21-cm Signal by Saurabh singh

PROGRAM LESS TRAVELLED PATH TO THE DARK UNIVERSE ORGANIZERS: Arka Banerjee (IISER Pune), Subinoy Das (IIA, Bangalore), Koushik Dutta (IISER, Kolkata), Raghavan Rangarajan (Ahmedabad University) and Vikram Rentala (IIT Bombay) DATE & TIME: 13 March 2023 to 24 March 2023 VENUE: Ramanujan

From playlist LESS TRAVELLED PATH TO THE DARK UNIVERSE

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GRCon19 - Multichannel phase coherent transceiver system with GNU Radio... by Michael Hennerich

Multichannel phase coherent transceiver system with GNU Radio interface by Michael Hennerich Many applications need multiple channels of phase and frequency synchronization and coherency. Applications like Direction of Arrival (DOA) accuracy are directly related to the number of channels

From playlist GRCon 2019

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Detection of B-mode Polarization at Degree Scales Using BICEP2 - J. Bock - March 20, 2014

Jamie Bock, Professor of Physics at Caltech and Senior Research Scientist at the Jet Propulsion Laboratory, presents results from the BICEP2 team on the first direct evidence of inflation and primordial gravitational waves. The team measured a B-mode polarization signal in the cosmic micr

From playlist Research & Science

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This thing is -270°C and is EVERYWHERE

Download the PBS Video App: https://www.pbs.org/pbs-video-app/ The universe is microwaving itself. A mystery signal discovered in the 1960s led to a Nobel prize. In this video, Dianna explores one of the most mysterious discoveries in physics - a constant microwave signal that seemed to

From playlist Unique Astrophysics #BackToSchool

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Reflections on BICEP2 - J. Bock - 5/17/2014

Workshop on Primordial Gravitational Waves and Cosmology (May 16 - 17, 2014) Learn more about this workshop: http://burkeinstitute.caltech.edu/workshops Produced in association with Caltech Academic Media Technologies. © 2014 California Institute of Technology

From playlist Walter Burke Institute for Theoretical Physics - Workshop on Primordial Gravitational Waves and Cosmology (May 16 - 17, 2014)

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SAT math Q13 calculator allowed #shorts

The speed of a sound wave in air depends on the air temperature. The formula above shows the relationship between a, the speed of a sound wave, in feet per second, and t, the air temperature, in degrees Fahrenheit (ºF). Which of the following air temperatures will the speed of a sound wav

From playlist #shorts mathematicsonline

Related pages

Johnson–Nyquist noise | Noise power | Noise temperature