Sounding rocket to study active regions on the sun

Aug 02, 2013
The bright regions in this solar image, known as active regions in the solar atmosphere, are areas that can spawn giant eruptions on the sun. The VERIS rocket will study the physical properties of these regions in exquisite detail during a 15-minute flight in early August 2013. Credit: NASA/SDO

(Phys.org) —At NASA's White Sands Test Facility in Las Cruces, N.M., a sounding rocket is being readied for flight. Due to launch on Aug. 8, 2013, the VERIS rocket, short for Very high Resolution Imaging Spectrometer, will launch for a 15-minute trip carrying an instrument that can measure properties of the structures in the sun's upper atmosphere down to 145 miles across, some eight times clearer than any similar telescope currently in space.

When it comes to observing the sun, different instruments and techniques must be used to study different temperatures of material or different layers of the sun from its surface out into its active , the corona. VERIS will focus on the very hot material present in what's known as active regions, magnetically complex spots in the corona that are often the location of eruptions on the sun such as and coronal , which can send radiation and solar material toward Earth, potentially disrupting satellite systems and .

"On the sun, these large scale energy releases are driven by small scale ," said Clarence Korendyke, principal investigator for VERIS at the United States Naval Research Laboratory in Washington, D.C. "So we need to look at and understand the tiny details of those processes."

After VERIS launches, it will begin to soar 150 miles up into space. When the rocket passes 60 miles, it will be above the bulk of hydrogen and water in Earth's atmosphere that block solar emissions from reaching Earth, and the instruments will begin collecting useful scientific data. Engineers on the ground will point the telescope at a pre-selected active region on the sun and gather observations for some six minutes. During that time, the rocket will reach the peak of its trajectory and then fall back towards Earth to re-enter the atmosphere. At that point, a parachute deploys and the rocket floats back down to the ground – still within White Sands, but some 60 miles away from the launch site—where it will be retrieved by a helicopter.

"Sounding rockets only gather five to six minutes worth of data," said Angelos Vourlidas, project scientist for VERIS at the Naval Research Laboratory. "But then scientists spend years analyzing and debating the information."

VERIS's six-minute flight can yield such rich information partly because of the flexibility of instrument size possible on a . The mirror diameter is 17 inches while the entire telescope length spans almost 10 feet and weighs almost 1000 pounds, making it much too large to fly on a satellite. VERIS's telescope is unique because it is the first to gather a kind of data known as spectra of this region of the sun at such high resolution. Spectra provide information on how much of any given wavelength of light is present. The instrument works by passing the light from the telescope through a slit and onto a grating that separates the light into its constituent wavelengths, much the way a prism can. Each wavelength corresponds to a different temperature of material – a charged gas, called plasma – present on the sun. So looking at any given wavelength can give information about just one temperature of material at a time. The spectra can also be used to collect density and velocity information about the active region. Together, this information can help scientists distinguish between theories on what causes heat to well up from the lowest layers of the sun's atmosphere to its highest, resulting in a corona that is a mysterious 10,000 times hotter than its surface.

"There are two categories of theories on how the corona is heated. One proposal is that small bursts of energy, called microflares, constantly erupt, heating the material. Another is that waves flow up from the surface to the corona," said Vourlidas. "VERIS will be able to provide temperature information at the smallest level, and help distinguish between these theories."

To support the VERIS observations, scientists will also turn to data sets gathered simultaneously by other solar observatories, such as the joint NASA-Japanese Aerospace Exploration Agency's Hinode and NASA's newly-launched Interface Region Imaging Spectrograph, which observes the lower, cooler layers of the sun's atmosphere.

A success of a mission like this also serves as a significant test to see if a similar instrument should be part of the next generation of solar telescopes, which will continue to help unravel the complex behavior of our closest star.

"Understanding the sun does not, by itself, lead to the capability for us to predict when the sun will send a burst of radiation or particles toward Earth," said Korendyke. "But at the end of the day, you can't have such a capability without first having that understanding."

VERIS was built at NRL with funding for the NASA Low Cost Access to Space program. It will launch aboard a Terrier-Black Brant IX rocket. The NASA sounding rocket program is managed for the agency at the Wallops Flight Facility in Virginia.

Explore further: NASA's IRIS mission readies for a new challenge

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cantdrive85
1 / 5 (3) Aug 02, 2013
this information can help scientists distinguish between theories on what causes heat to well up from the lowest layers of the sun's atmosphere to its highest, resulting in a corona that is a mysterious 10,000 times hotter than its surface.


"Essential to the received theory is the conviction that inside the sun is a steep temperature gradient, falling toward the photosphere, along which the internal energy flows outward. If we stack this internal temperature gradient against the observed temperature gradient in the solar atmosphere, which falls steeply inward, toward the photosphere, we find we have diagrammed a physical absurdity: The two gradients produce a trough at the photosphere, which implies that thermal energy should collect and become stuck there until it raises the temperature and eliminates the trough. That this does not occur seems to bother no one."
Jeurgens
Who cares about thermodynamics or physics? Apparently not solar physicists.

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