Particle physics laboratory

LASP rocket flight to refine NASA’s study of the Sun


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It is best not to look directly at the Sun, unless you are one of NASA’s Sun Observation Instruments. And even then it will cause damage. Sun exposure degrades light sensors of all kinds, from the retinas of the human eye to instruments on board NASA Solar dynamics observatory satellite or SDO. Fortunately, with periodic calibrations, these can continue to transmit high-quality data to researchers on Earth.


SDO / EVE calibration rocket assembly at White Sands, New Mexico. Credit: LASP

SDO’s Extreme Ultraviolet Variability Experiment, or EVE, uses sounding rockets for calibration. During their approximately 15-minute flights, these suborbital rockets carry a duplicate of the EVE instrument for observing the Sun to about 180 miles above Earth, where it records measurements that will maintain its twin instrument. on board the SDO listening. Tom Woods, a solar physicist in the Atmospheric and Space Physics Laboratory at the University of Colorado, is the principal investigator of the SDO / EVE instrument.

The 30-minute launch window for EVE’s next calibration flight opens at 11:25 a.m. MDT on September 9, 2021, at the White Sands Missile Range in New Mexico.

SDO’s EVE is a space instrument that measures extreme ultraviolet light from the Sun. The activity of the Sun causes enormous variations in the output of this powerful radiation, which is invisible to our eyes and is absorbed by the Earth’s atmosphere before it reaches the ground.

Solar flares, for example, release massive amounts of extreme ultraviolet light. EVE allows researchers to keep an eye on the Sun in near real time. It takes less than a second for SDO data to reach Earth and an additional 15 minutes for the data to be processed into a usable form.

This speed is important because the impacts of this variation in extreme ultraviolet light can sometimes be felt on Earth. Bursts can disrupt the Earth’s atmosphere and, therefore, the GPS or radio signals passing through it. “Part of our science is providing these measurements to space weather operators who are concerned about how our communication and navigation systems might be disrupted due to a solar flare,” said Woods.

But solar radiation and the harshness of space degrade EVE’s sensors over time. So Woods’ team and NASA regularly send sounding rockets – from the nautical term “sound”, which means to measure – into space to recalibrate EVE and keep the data accurate.

On board the sounding rocket, the copy of the EVE instrument measures extreme ultraviolet light before parachuting back down to Earth for reuse. The instrument must be in space to record these measurements because the atmosphere absorbs most of the ultraviolet light. In addition to its brief and occasional forays into space, the duplicate instrument spends its time on Earth, sheltered from the harsh space environment and within reach of scientists for tune-ups. By comparing the measurements of this EVE instrument with those of its twin on SDO, researchers can correct any degradation on the satellite version. The information is also used to validate the calibration of ten instruments on board other spacecraft.

Image of the Sun at 304 Angstroms from the AIA instrument on SDO. The image of the Sun on the left is not calibrated. In comparison, the image on the right is the same image with a calibration correction (measured from rocket flight) applied. Credit: NASA / SDO

After SDO launched in 2010, Woods and his team aimed to recalibrate the instrument approximately every six months. Now they shoot about once every two years because the rate of decay slows down over time. However, the coronavirus pandemic delayed the last launch, so they are now past the three-year mark. “We can’t wait to launch this one and see how great it turns out,” said Woods. Once they have the new numbers, they will rerun the data from the past few years to ensure the most accurate measurements possible.

Between sounding rocket launches, the EVE team also uses weekly calibration measurements of SDO’s EVE instrument itself. But, said Woods, those calibrations aren’t that informative. “It doesn’t give you a direct measure of the degradation,” he said. “The only way to really pinpoint this degradation is to do this type of cross-calibration. ”

EVE, who lives on Earth, is preparing for its tenth space trip in 15 years (it started flying before SDO launched), and new questions still arise. “How many times can you throw this before something breaks?” Woods said. “The vibration of the launch is hard on him, and the landing is hard on him too. ”

The exact technology inside EVE no longer exists, having been superseded by newer versions, but Woods and his team are building a replacement in case anything breaks in the next few years. “It’s getting old,” he said. “I don’t know how many more missions he can survive, but so far – I’m knocking on the wood – he’s already been delayed for so many years. During that time, it allowed us to see our Sun like never before. Woods hopes he will continue to shed light on the activity of the Sun for years to come.

Related video: Get on a sounding rocket

By Anna Blaustein
NASA Goddard Space Flight Center

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