The rate of electromagnetic
radiation emitted at a given frequency is proportional to the amount of absorption that it would experience by the source.
But, just as the absorption from the surface is saturated, so is
the radiation emitted at the top of the atmosphere.
(Note, by the way, that what is true for a radiating object is that the amount of
radiation emitted AT ANY PARTICULAR WAVELENGTH is an increasing function of the temperature, a fact that is not always obvious because people often tend to normalize the emission curves when showing emission curves for different temperatures on the same graph.)
Within the X-ray glow, Reeves and his colleagues discerned
radiation emitted at energy levels associated with several specific elements, including magnesium, silicon, sulfur, argon, and calcium — a mix of ingredients similar to that cast out from a supernova explosion.
Not exact matches
«The older an organism's remains are, the less beta
radiation it
emits because its C - 14 is steadily dwindling
at a predictable rate.»
«I think most physicists would agree that Hawking's greatest contribution is the prediction that black holes
emit radiation,» says Sean Carroll, a theoretical physicist
at the California Institute of Technology.
At a conference, another astronomer asked him if the center could archive a terabyte of data that had been collected from the MACHO sky survey, a project designed to study mysterious cosmic bodies that
emit very little light or other
radiation.
Upon Hawking's death on March 14
at age 76, his most famous discovery — that black holes aren't entirely black, but
emit faint
radiation — was still fueling debate.
In 1903 French scientist René Blondlot added to the frenzy with his announcement of N - rays, a strangely democratic form of
radiation emitted by wood, iron, living organisms — just about anything
at all.
Dead stars known as pulsars (one illustrated above)
emit beams of
radiation that sweep past Earth
at regular intervals.
The parallel sheets of incoming and outgoing current force the electrons to
emit coherent, laserlike
radiation at radio wavelengths as they spiral along the planet's magnetic field lines, Ergun says.
«And if you did, wouldn't that mean my phone isn't
emitting radiation at all?»
Some black holes do this conspicuously, releasing outbursts of gamma rays and X-rays every time they feed, while others are «closet eaters» that
emit very little
radiation at feeding time.
The actual data did not look like much, mostly line graphs showing the intensity of
radiation emitted by the stars
at various wavelengths, but the meaning hidden behind those numbers had us talking all
at once, lost in the fever of discovery.
Early in their lives, the
radiation they
emitted was largely blocked by the thick veil of their host nebula, visible only to telescopes
at infrared and radio wavelengths.
Physicists fired polarized laser pulses
at a block of glass, creating distortions that
emitted Hawking
radiation out the sides of the block (inset).
They then took a closer look
at the spectrum of
radiation emitted by each of these objects, using optical telescopes in Arizona and the world's largest radio telescope, the 305 - metre dish
at Arecibo in Puerto Rico.
At the same time the surface and the atmosphere
emit infrared
radiation back to space, which produces cooling.
At that time, the Universe became transparent to
radiation, and light -
emitting objects became visible.
The telescope — based
at the US National Radio Astronomy Observatory (NRAO) in West Virginia — was tuned to a frequency of 1420 megahertz, the wavelength of
radiation naturally
emitted by hydrogen in space.
Known as pulsars, the dead stars
emit beams of
radiation that sweep past Earth
at regular intervals, like the rotating beams from a lighthouse.
The Unruh effect is closely related to Hawking
radiation, extremely faint
radiation emitted by a black hole
at a temperature determined by its mass.
In computer simulations, the researchers show that a black hole can rapidly grow
at the center of its host galaxy if a nearby galaxy
emits enough
radiation to switch off its capacity to form stars.
In 2009, the Spitzer Space Telescope discovered infrared
radiation from a ring far beyond all the others encircling Saturn; sunlight heats the ring's dust, which
emits its heat
at infrared wavelengths.
Researchers looked
at seven of these worlds — distant planets whose mass lies between one and 10 times ours — including 55 Cancri e (
at right, compared to Earth) and GJ1214b, evaluating how the x-ray and extreme ultraviolet
radiation emitted by their parent stars might affect their atmospheres over their remaining lifetimes.
The discovery could potentially provide a way to test Stephen Hawking's prediction that a real black hole should slowly evaporate as it
emits radiation generated in the quantum turmoil
at its event horizon.
They then looked
at another source of data: that of the Clouds» and Earth's Radiant Energy System (CERES) satellite instruments which measure fluxes of reflected and
emitted radiation from Earth to space, to help scientists understand how the climate varies over time.
So we said, «Why not look
at the
radiation [electrons]
emit directly?»»
As some of this matter falls toward the black hole, it heats up and
emits synchrotron
radiation, which is characteristic of electrons whirling
at nearly the speed of light around a magnetic field.
They found that HD 98800, which is an orange star,
emits 10 per cent of its
radiation in the far - infrared —
at wavelengths between 10 and 100 micrometres.
In fact, a typical coal - fired power plant exposes local residents to as many as 18 millirems of
radiation yearly, whereas a nuclear power plant
emits less than six millirems per annum, according to researchers
at Oak Ridge National Laboratory.
While observing
at the frequency that hydrogen atoms
emit radiation, it will be able to image a circle on the sky as wide as about five Full Moons.
Until now, XFELs have normally
emitted one
radiation pulse
at a single wavelength like conventional visible lasers.
The electrons in strontium atoms
emit radiation at 429,500 giga - hertz.
In the new study, Charles Hailey, an astrophysicist
at Columbia University, and his colleagues scrutinized the past dozen years of data gathered by the Chandra X-ray Observatory, an orbiting craft whose instruments are designed to detect high - energy
radiation emitted by the immensely hot material surrounding exploded stars and near black holes.
Clouds of dust and gas in the famIliar constellation
emit radiation at infrared and radio wa velengths.
Neutral hydrogen
emits radiation at a frequency of 1,420 MHz, but thanks to the ongoing expansion of the Universe and the Doppler Effect, that
radiation shifts to a lower frequency.
When gas falls toward the black hole
at the center of the galaxy NGC 4151, the gas heats up and
emits ultraviolet
radiation, which in turn heats the ring - shaped dust cloud orbiting the black hole
at a distance.
X-ray source, in astronomy, any of a class of cosmic objects that
emit radiation at X-ray wavelength.
Radio telescopes can detect neutral hydrogen because it
emits radiation at a wavelength of 21 cm.
Many such objects contain detectable amounts of molecules that
emit radio
radiation at wavelengths that allow them to be identified and analyzed.
That the nebula is so much brighter than the star shows that the star
emits primarily highly energetic
radiation of the non-visible part of the electro - magnetic spectrum, which is absorbed by exciting the nebula's gas, and re-emitted by the nebula,
at last to a good part in the visible light.
What is unique is that
at the dawn of radio astronomy, a scientist predicted hydrogen would
emit this
radiation at detectable radio wavelengths, and this prediction offered astronomers a new tool for studying the universe.
Numerous molecules
emit radiation at these wavelengths and thus can be detected by the 12 - Meter telescope.
It has been suggested by some vitamin D researchers, for example, that approximately 5 — 30 minutes of sun exposure between 10 AM and 3 PM
at least twice a week to the face, arms, legs, or back without sunscreen usually lead to sufficient vitamin D synthesis and that the moderate use of commercial tanning beds that
emit 2 % — 6 % UVB
radiation is also effective [6,20].
Most infrared saunas
emit electromagnetic
radiation at base levels.
Further, electromagnetic
radiation (such as that
emitted by Wi - Fi, cell phones, cell towers and «smart» meters) may affect the body like light does
at night — and inhibit melatonin production.
For me, the
radiation emitted by these devices was so intense (even
at lower brightness settings) that my eyes watered and burned to the point where I was forced to quit.
Radiative transfer in the earth's atmosphere is not particularly amenable to simple formulas because the atmosphere is semi-transparent to differing degree
at different wavelengths, which allows
radiation emitted locally to interact with the entire atmosphere.
Absorption of thermal
radiation cools the thermal spectra of the earth as seen from space,
radiation emitted by de-excitation is what results in the further warming of the surface, and the surface continues to warm until the rate
at which energy is radiated from the earth's climate system (given the increased opacity of the atmosphere to longwave
radiation) is equal to the rate
at which energy enters it.