Light is defined conventionally by physicists as
electromagnetic emissions of any frequency and not merely the visual.
Winds are estimated by using an upward - looking Doppler radar, while temperature and moisture profiles are evaluated by using a vertically pointing radiometer that measures
electromagnetic emissions of selected wavelengths at various heights in the troposphere.
Not exact matches
In a recent experiment performed at the Radioactive Isotope Beam Factory at RIKEN, an international collaboration with scientists from eleven countries, led by scientists
of the Instituto de Estructura de la Materia, CSIC (Spain) and the RIKEN Nishina Center (Japan), made a very surprising observation: High - energy gamma rays — which are mediated by the
electromagnetic force — are emitted in the decay
of a certain excited nucleus — tin 133, in competition with neutron
emission, the decay mode mediated by the strong nuclear force.
«We control the below - threshold harmonic light
emission by using
electromagnetic fields with time - dependent ellipticity, like we have done to the above - threshold high - order harmonics,» said Chang referring to the creation
of a 67 - attosecond pulse
of extreme ultraviolet light, which earned him international recognition.
Because these
electromagnetic emissions are on the order
of an electron volt, and they probably come from a single molecule, or atom, or electron, we can now say that the energy concentration is now on the order
of one electron volt per molecule — an increase
of a factor
of 1011 or so.
Their short durations, and strong
emissions across the entire
electromagnetic spectrum, require close communication, sharing
of data, and collaborative efforts amongst astronomers.
Sky surveys and mappings
of the various wavelength bands
of electromagnetic radiation (in particular 21 - cm
emission) have yielded much information on the content and character
of the universe's structure.
So thirsty are theorists for new insights into black holes and relativistic processes that, with each LIGO detection, observational astronomers have leapt into action to target those enormous patches
of sky, hoping to see some afterglow or other
emission of electromagnetic radiation — even though by definition the resulting larger black hole should emit no light.
Depending on their size, so called near - fields (
electromagnetic fields close to the particle surface) were induced by the laser pulses, resulting in a controlled directional
emission of electrons.
The need
of the authorities to control radio
emissions has meant the development
of specific regulation on exposure to
electromagnetic fields.
The satellite data is being combined with that collected by the National Lightning Detection Network and from a network
of sensors that measure low - frequency
electromagnetic emissions, or «sferics,» and changes in the direction
of the electric field.
A powerful
electromagnetic emission from a U.S. radar in the Pacific could have caused the malfunctioning
of the Russian Phobos - Grunt probe, the Kommersant daily said on Tuesday.
The most important discovery in astronomy in 2017 was the groundbreaking discovery
of a gravitational wave event GW170817 due to the merger
of two neutron stars as well as its associated short GRB (gamma ray burst) 170817A and other
electromagnetic counterpart
emissions in multi-wavelength.
In active galaxies, a region near the center produces enormous amounts
of emission across the entire
electromagnetic spectrum.
«The game to see the light from these catastrophic mergers is on,» says Mansi Kasliwal, assistant professor
of astronomy and the leader
of the Caltech effort to search for
electromagnetic emission from gravitational waves using the intermediate Palomar Transient Factory, a robotic survey for astrophysical transients (brief, intense flashes
of light), and a network
of other telescopes.
The rest goes into pulses observed elsewhere in the
electromagnetic spectrum and into cosmic rays, with perhaps some going into the
emission of gravitational energy, or gravity waves.
Spectroscopy: The study
of the interaction between
electromagnetic radiation and matter, with absorption or
emission of radiant energy.
Another
of his recent work, on how to strategically point telescopes to find
electromagnetic counterparts to gravitational wave sources, was adapted for observations by the Very Large Array radio telescope in New Mexico, which successfully observed radio
emission from the merger.
Some, however, use a network
of antennas to collect radio
emissions (energy from a different portion
of the
electromagnetic spectrum).
Massive yet non-supergiant entities known as «Be stars» are main - sequence stars that notably have, or had at some time, one or more Balmer lines in
emission, with the hydrogen - related
electromagnetic radiation series projected out by the stars being
of particular interest.
Once the
electromagnetic environment has been significantly changed by these
emissions, then we will be in a new era
of evolution.
The resulting data connection is ultra-fast, secure and free
of harmful
electromagnetic emissions.
As a scientist, I do not understand how photons are not relevant to the
emission, transfer, and absorption
of electromagnetic energy.
Concepts
of electromagnetic and acoustic wave propagation; active and passive remote sensing techniques including radar, lidar, thermal
emission systems
[59] Science is recruited not to advance technological innovation, but to assess the potential or possible risks
of both industrialization and new technologies, from bio - and nanotechnology to pesticides,
electromagnetic waves, and greenhouse gas
emissions.
A team
of researchers at Carnegie Mellon University's Future Interfaces Group is working on the concept that could mark a huge breakthrough in the field
of NFC:
electromagnetic emissions sensing.