Sentences with phrase «ultraviolet wavelengths from»

In the past, researchers have focused on studying the corona at ultraviolet wavelengths from space, and at visible wavelengths from the ground.

Not exact matches

Exposure of the skin to ultraviolet B wavelengths from sunlight is the usual mechanism for production of vitamin D. However, significant risk of sunburn (short - term) and skin cancer (long - term) attributable to sunlight exposure, especially in younger children, makes it prudent to counsel against exposure to sunlight.
Images were obtained from viewing the galaxy in near - ultraviolet, visible, and near - infrared wavelengths, using the Advanced Camera for Surveys and the Wide Field Camera 3 aboard Hubble.
The team observed the star with the infrared Spitzer and ultraviolet Swift space telescopes from October 2015 to December 2016 — the first observations in multiple wavelengths of light.
One of the most complex eyes in the animal kingdom can be found in species of stomatopod crustaceans (mantis shrimp), some of which have 12 different photoreceptor types, each sampling a narrow set of wavelengths ranging from deep ultraviolet to far red (300 to 720 nanometers)(1 — 3).
Light — in wavelengths ranging from ultraviolet to deep red — was projected onto the dancers and reflected to a target surface.
Watching the sun in ultraviolet wavelengths of light from space — above our UV light - blocking atmosphere — reveals constant activity, including bursts of light, particles, and magnetic fields.
The scientists then mapped the quasars with other telescopes and at wavelengths ranging from ultraviolet to far infrared.
Even down on the Red Planet's surface, the Curiosity rover might be able to get in on the act: Because Mars's atmosphere has no ozone to block ultraviolet light, sensors on the rover will be able to detect those wavelengths and thereby monitor certain trace gases spewing from the comet — unless a dust storm blocks the view to space, Lemmon says.
His team's study, «Ultraviolet Flux Decrease Under a Grand Minimum from IUE Short - wavelength Observation of Solar Analogs,» appears in the publication Astrophysical Journal Letters and was funded by the state of California.
The laser light that emerged from the frozen gas was in the extreme ultraviolet range, with wavelengths about 40 times shorter than the light that went in, they report today in the journal Nature.
By studying such a large data set — over 200,000 galaxies in 21 different wavelengths, or colors of light, from ultraviolet to infrared — astronomers compared the energy emissions from galaxies across a wide swath of space and time to read the history of the universe.
«We tested ultraviolet LEDs from different sources and at different wavelengths.
Stuart Bowyer, from the University of California at Berkeley and a principal investigator of the EUVE, built an extreme ultraviolet detector for the mission, which found four stars at these wavelengths.
At the same time, an extreme ultraviolet imager on SDO can follow small features at eight different ultraviolet wavelengths that gauge temperatures from 20,000 ˚C to 1 million˚C.
They determined the planet's radius at 10 different wavelength bands, from 300 - nanometer ultraviolet light to 1000 - nanometer infrared.
The light - absorbing molecules break off from the chains when exposed to ultraviolet light at 350 nanometers wavelength, triggering degradation of the plastics.
By the time it stops working, the JWST should be in orbit, but the newer telescope will operate in different wavelengths from Hubble — using infrared rather than optical and ultraviolet light.
The EBL is essentially all the accumulated light from stars over the history of the universe and ranges in wavelength from the ultraviolet, through the optical, and to the infrared.
After all, almost every photon (particle of light) from ultraviolet to far infrared wavelengths ever radiated by all galaxies that ever existed throughout cosmic history is still speeding through the Universe today.
The other part of the process, as explained in the paper, is using the high harmonic generation process to produce bright spatially coherent beams from a tabletop laser, spanning the range from the vacuum ultraviolet (wavelengths less than 200 nm) to the soft X-ray region of the spectrum (wavelengths less than 10 nm)
This large range of wavelength coverage, combined with the instrument's high sensitivity, allows the study of everything from comets (which have interesting features in the ultraviolet part of the spectrum), to the blue light from star formation, to the red light of very distant objects.
When the star's ultraviolet radiation strikes the gases in the nebula, they heat up, giving out radiation ranging in wavelength from blue — emitted by hot oxygen in the bubble near the star — to yellow — emitted by hot hydrogen and nitrogen.
XMM - Newton observed this output in optical, ultraviolet and X-ray wavelengths, enabling the astronomers to measure how far the disk sits from the black hole.
The distance to the quasar is so great (about 10 billion light - years) that the emitted light is «stretched» by the expansion of the universe from an invisible ultraviolet wavelength to a visible shade of violet by the time it reaches the 10 - meter Keck I telescope and the LRIS (Low Resolution Imaging Spectrometer) used for this discovery.
Observing in wavelengths ranging from the ultraviolet to the mid-infrared, this unique instrument will allow astronomers to address fundamental questions in astronomy ranging from understanding star and planet formation to unraveling the history of galaxies and the development of large - scale structure in the universe.
At ultraviolet wavelengths, Hubble's Cosmic Origins Spectrograph (COS) is sensitive to absorption from hot gas, which shows up as reduced brightnesses at specific colors in a spectrum.
The shortwave extreme ultraviolet flux is much higher in the distant past, which could pose problems for early Mars to develop a very dense CO2 atmosphere early on for example, since C and O could escape from Mars early in its history (driven by these energetic wavelengths).
The cell also overcomes some of the major problems with current solar tech like wear out or damage from high heat that comes from the absorption of great amounts of ultraviolet and infrared radiation that can't actually be turned into electricity due to a narrow band gap (the wavelength of light that can effectively be used to generate electricity).
Ultraviolet light is radiation in wavelengths from 200 to 300 nm (nautical miles) found in natural sunlight, sun lamps and tanning beds.
The Earth receives energy from the Sun in the form of visible light and ultraviolet radiation, which is then re-radiated away from the surface as thermal radiation in infrared wavelengths.
Although only 1 percent of the sun's energy is emitted at ultraviolet wavelengths between 200 and 300 nanometers, the decrease in this radiation from 1 July 1981 to 30 June 1985 accounted for 19 percent of the decrease in the total irradiance over the same period.»
Very few organizations match our expertise which spans the complete spectrum from the shortest (ultraviolet) to the longest (microwave) wavelengths, and from the surface to the upper reaches of the atmosphere.
According to their modeling studies, the difference in the amount of incoming solar radiation, in this case, primarily in the ultraviolet (UV) wavelengths, during the minima and maxima of the 11 - yr solar cycle are large enough to produce a characteristic change in the winter circulation pattern of the atmosphere over North America... When the NAO is in its negative phase, more cold air can seep south from the Arctic and impact the lower latitudes of Europe and the eastern U.S., which helps spin up winter storm systems.
Earth receives energy that travels from the sun in a variety of wavelengths, some of which we see as sunlight and others that are invisible to the naked eye, such as shorter - wavelength ultraviolet radiation and longer - wavelength infrared radiation.
Observational evidence suggests that some organic aerosol compounds from fossil fuels are relatively weakly absorbing but do absorb solar radiation at some ultraviolet and visible wavelengths (e.g., Bond et al., 1999; Jacobson, 1999; Bond, 2001) although organic aerosol from high - temperature combustion such as fossil fuel burning (Dubovik et al., 1998; Kirchstetter et al., 2004) appears less absorbing than from low - temperature combustion such as open biomass burning.
From smartphone apps to smart wearables, there are a variety of high - tech ways we can make sure we're not being exposed to too many harmful ultraviolet wavelengths by being out in the sun.
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