Shown here is the “first light” image of ultraviolet atomic oxygen emission (135.6 nm wavelength) from the Earth’s upper atmosphere captured by NASA’s GOLD instrument. It was taken at approximately 6 a.m. local time, near sunrise in eastern South America. The colors correspond to emission brightness, with the strongest shown in red and the weakest in blue. This emission is produced at altitudes around 160 km (note how it extends above the Earth’s surface on the horizon), when the Earth’s upper atmosphere absorbs high energy photons and particles. The aurora, at the top and bottom of the image, and daytime airglow, on the right hand side, are also visible. An ultraviolet star, 66 Ophiuchi (HD 164284), is visible above the western horizon of the Earth. Outlines of the continents and a latitude-longitude grid have been added for reference. (Courtesy LASP/GOLD science team)
NASA’s Global-scale Observations of the Limb and Disk, or GOLD, instrument powered on and opened its cover to scan the Earth for the first time, resulting in a “first light” image of the Western Hemisphere in the ultraviolet. GOLD will provide unprecedented global-scale imaging of the temperature and composition at the dynamic boundary between Earth’s atmosphere and space.
The instrument was launched from Kourou, French Guiana, on Jan. 25, 2018, onboard the SES-14 satellite and reached geostationary orbit in June 2018. After checkout of the satellite and communications payload, GOLD commissioning—the period during which the instrument performance is assessed—began on Sept. 4.
Team scientists conducted one day of observations on Sept. 11, during instrument checkout, enabling them to produce GOLD’s “first light” image shown here. Commissioning will run through early October, as the team continues to prepare the instrument for its planned two-year science mission.
Built by LASP, and managed by NASA’s Goddard Space Flight Center in Greenbelt, Maryland, GOLD is the first NASA science mission to fly an instrument as a hosted payload on a commercial satellite. Data from the instrument—comprised of two, identical ultraviolet-imaging spectrographs—will improve our understanding of the Sun’s impact on the Earth’s upper atmosphere, as well as the effects from terrestrial weather below.
“GOLD is an amazing technological breakthrough,” said GOLD Principal Investigator Richard Eastes, a research scientist at LASP. “After years of reviews, testing, testing, and more testing, the instrument is finally making observations of the Earth. The main act has begun. It’s a testament to the engineering and science teams, who were responsible for building and calibrating the instrument, that we’ve reached this significant mission milestone.”
Along with NASA’s Ionospheric Connection Explorer, or ICON, scheduled for launch later this fall, GOLD is a key element of NASA’s program to explore Earth’s boundary with space, as the two missions explore this unpredictable near-Earth region to determine how it responds to solar and atmospheric inputs.
“The successful launch of GOLD and acquisition of initial data is a fantastic result,” said Bill McClintock, GOLD instrument scientist at LASP. “Its data will help us understand the critical role the Sun plays in space weather and allow us to better protect astronauts and our technological assets that we’ve become so reliant upon in today’s society.”
Changes in near-Earth space can affect our lives on Earth by disrupting the use of satellites for communications and navigation. The result can be lost messages, aircraft flight delays, interruptions in GPS signals, and satellite TV outages. Incoming solar energy can also damage spacecraft electronics and detectors, and expose astronauts to health risks from radiation. The more we understand about the fundamental nature of our space environment, the better we can protect these interests.
Scientists expect to begin operations of the GOLD instrument in early October 2018.
Quelle: LASP Laboratory for Atmospheric and Space Physics