Sentences with phrase «ultraviolet emission»

This image of the Mars night side shows ultraviolet emission from nitric oxide (abbreviated NO).

Ultraviolet data collected by NASA's MAVEN spacecraft was used to construct these images showing ultraviolet emissions before (left) and during (right) the storm (Credit: NASA / Goddard / University of Colorado)

Ultraviolet data collected by NASA's MAVEN spacecraft was used to construct these images showing ultraviolet emissions before (left) and during (right) the storm

The remote - sensing Imaging Ultraviolet Spectrograph (IUVS) designed and built at CU - Boulder observed intense ultraviolet emissions from magnesium and iron ions high in the atmosphere in the aftermath of the meteor shower.

Using Keck Observatory's powerful infrared spectrograph called MOSFIRE, the team dated the galaxy by detecting its Lyman - alpha emission line — a signature of hot hydrogen gas heated by strong ultraviolet emission from newly born stars.

Rogier Windhorst, Sam Pascarelle, Arizona State University, STScI, NASA Larger true - color image of ultraviolet emission redshifted to visible light.

Skylab made the first time - resolved observations of the solar transition region and of ultraviolet emissions from the solar corona.

Instead, it detects the ultraviolet emission from the cooler plasma (~ 18,000 to 180,000 degrees Fahrenheit) at their footpoints.

The interface region also is where most of the sun's ultraviolet emission is generated.

A detector placed at the end of the optical path highlights any portions of the light signal that are absorbed as the ultraviolet emission passes through the gas sample.

IRIS will advance our understanding of the interface region, a region in the lower atmosphere of the sun where most of the sun's ultraviolet emissions are generated.

Information about the shadow of the electron orbital as seen by the traveling electron wave is imprinted on the ultraviolet emission.

When hydrogen gas is heated by the ultraviolet emissions of new stars, it produces a spectral signature called the Lyman - alpha line.

Small stars harbor most of the planets in the universe, and their ultraviolet emission could be a determining factor in the evolution and present chemical state of the atmospheres of orbiting planets.

One spacecraft instrument can see through the sun to the backside, while another one can sense activity through ultraviolet emissions.

Figure 1 (a) represents the corrected visible light from Neptune from 1950 to 2006; (b) shows the temperature anomalies of the Earth; (c) shows the total solar irradiance as a percent variation by year; (d) shows the ultraviolet emission from the Sun (Source: Hammel and Lockwood (2007)-RRB-.