Forum for Science, Industry and Business

Sponsored by:     3M 
Search our Site:

 

NASA-funded mission studies the Sun in soft X-rays

25.03.2015

At any given moment, our sun emits a range of light waves far more expansive than what our eyes alone can see: from visible light to extreme ultraviolet to soft and hard X-rays. Different wavelengths can have different effects at Earth and, what's more, when observed and analyzed correctly, those wavelengths can provide scientists with information about events on the sun. In 2012 and 2013, a detector was launched on a sounding rocket for a 15 minute trip to look at a range of sunlight previously not well-observed: soft X-rays.

Each wavelength of light from the sun inherently carries information about the kind of process that emitted the light, so looking at soft X-rays provides a new way to figure out what is happening on our closest star. For example, the sun's atmosphere, the corona, is 1,000 times hotter than its surface, and scientists do not yet understand the details of why.


The NASA-funded MinXSS CubeSat will launch in late 2015 to study soft X-rays from the sun. There have not yet been long term studies of these soft X-rays, but observations show they may be important clues to understanding what heats the sun's atmosphere to 1000 times the temperature of its surface.

Credit: NASA/U.Colorado

The soft X-ray detector brought home data showing that a significant amount of soft X-rays - more than expected - were seen when there are even a small amount of magnetically complex sunspots. Identifying what process within these magnetically active regions contributes to the great increase in soft X-rays could hold clues for what's helping to heat the corona. A paper on these results appeared in the Astrophysical Journal Letters on March 18, 2015.

"Not only did we gather measurements that haven't been made routinely," said Amir Caspi, first author on the paper and a solar scientist at Southwest Research Institute in Boulder, Colorado, who worked at the University of Colorado in Boulder during the course of this study. "The detector we used also allowed us to gather the best measurements so far made in this energy range."

This soft X-ray detector hitched a ride into space on a NASA sounding rocket. During a 15 minute total flight, sounding rockets have about six minutes of time to gather data from space. The soft X-ray detector and its related components are only about the size of a pack of cards, so it could easily fly on board a rocket carrying another experiment - in this case, one that helps calibrate the Extreme Ultraviolet Variability Experiment, or EVE, on NASA's Solar Dynamics Observatory. Sounding rockets and combining missions on a single launch vehicle provide an opportunity to conduct world-class science with a lower price tag.

The soft X-ray detector flew first on June 23, 2012, and again on October 21, 2013.

During both flights, there were only a few complex active regions on the sun's surface - indeed, very few during the 2012 flight. Yet, in both flights the detector saw 1000 times more soft X-rays than had been seen by another experiment in 2009. Even a slight extra amount of solar activity in the form of these active regions, led to substantially more output in the soft X-ray wavelengths.

Wavelengths of light correlate to particular temperatures of material on the sun, and this abundance of soft X-rays points to clouds of hot - 5 to 10 million degrees - gases above the active regions that wasn't present during the 2009 measurements when there were no active regions on the sun. That kind of information makes it clear that different heating mechanisms occur on the quiet sun and active regions, opening the door to determining the differences. One theory for the source of this mysterious heating is that numerous tiny explosions called nanoflares are constantly erupting on the sun. Nanoflares are too small to be seen by our telescopes, but powerfully energetic nonetheless. The soft X-rays might well be a result of nanoflares, thus giving us a way of investigating them.

The new soft X-ray data differed from previous data studies in another respect as well. By parsing out the amounts of each individual wavelength of light gathered, the team could identify what elements were present in the corona. Typically, the abundance of some of these atoms in the corona is greater than at the sun's surface. But not so in these recent observations. The mix of material in the corona was more similar to the mix seen at the solar surface, suggesting that some material from the surface was somehow rising up higher into the atmosphere.

"The difference we see in the abundances of the elements compared to previous studies suggest there may be a link between the heating mechanism and the coronal composition," said Caspi.

Untangling the elements present on the sun's surface and in its atmosphere during different events on the sun could offer another set of tools for interpreting what heats the corona.

Discovering that the soft X-ray emission was brighter than supposed has effects for understanding space weather events near Earth as well. Different wavelengths of light from the sun penetrate to different layers of Earth's atmosphere, causing different effects.

"The solar soft X-rays are deposited lower in Earth's atmosphere than the sun's extreme ultraviolet radiation," says Tom Woods, a co-author on the paper and the principal investigator for this experiment at the University of Colorado in Boulder. "The soft X-rays cause almost instantaneous changes in the ionosphere that can disturb radio communications and the accuracy of GPS navigation systems."

Such changes in the ionosphere happen during large explosions on the sun called solar flares. As humans attempt to better understand - and predict - the sun's effects on the space through which our communication signals travel, it's crucial that we have accurate models to simulate what the sun is sending our way and when.

The soft X-ray results so far are based on what amounts to only 10 minutes worth of data. However, this early data clearly shows the value of observing the previously understudied soft X-ray emissions. In the hopes of getting a longer data record - and of observing soft X-rays from solar flares -- the team has been working to place the same kind of detector into the NASA-funded Miniature X-ray Solar Spectrometer, or MinXSS, CubeSat, currently scheduled to launch in late 2015. About the size of a loaf of bread, the MinXSS is part of NASA's CubeSat program, which started in October 2013. CubeSats are small satellites that ride along with larger missions to take advantage of yet another low cost way to perform experiments in space. MinXSS will provide 6-12 months of observations to advance our understanding of soft-X-ray emissions from the sun both from solar flares and during quiescent periods.

The soft X-ray detector used for this experiment was an Amptek X123-SDD.

###

For more on NASA's sounding rocket program:

http://www.nasa.gov/soundingrockets

Susan Hendrix | EurekAlert!

Further reports about: Atmosphere Flight Center Goddard Space Flight Center NASA X-ray detector heating small

More articles from Physics and Astronomy:

nachricht Airborne thermometer to measure Arctic temperatures
11.01.2017 | Moscow Institute of Physics and Technology

nachricht Next-generation optics offer the widest real-time views of vast regions of the sun
11.01.2017 | New Jersey Institute of Technology

All articles from Physics and Astronomy >>>

The most recent press releases about innovation >>>

Die letzten 5 Focus-News des innovations-reports im Überblick:

Im Focus: Designing Architecture with Solar Building Envelopes

Among the general public, solar thermal energy is currently associated with dark blue, rectangular collectors on building roofs. Technologies are needed for aesthetically high quality architecture which offer the architect more room for manoeuvre when it comes to low- and plus-energy buildings. With the “ArKol” project, researchers at Fraunhofer ISE together with partners are currently developing two façade collectors for solar thermal energy generation, which permit a high degree of design flexibility: a strip collector for opaque façade sections and a solar thermal blind for transparent sections. The current state of the two developments will be presented at the BAU 2017 trade fair.

As part of the “ArKol – development of architecturally highly integrated façade collectors with heat pipes” project, Fraunhofer ISE together with its partners...

Im Focus: How to inflate a hardened concrete shell with a weight of 80 t

At TU Wien, an alternative for resource intensive formwork for the construction of concrete domes was developed. It is now used in a test dome for the Austrian Federal Railways Infrastructure (ÖBB Infrastruktur).

Concrete shells are efficient structures, but not very resource efficient. The formwork for the construction of concrete domes alone requires a high amount of...

Im Focus: Bacterial Pac Man molecule snaps at sugar

Many pathogens use certain sugar compounds from their host to help conceal themselves against the immune system. Scientists at the University of Bonn have now, in cooperation with researchers at the University of York in the United Kingdom, analyzed the dynamics of a bacterial molecule that is involved in this process. They demonstrate that the protein grabs onto the sugar molecule with a Pac Man-like chewing motion and holds it until it can be used. Their results could help design therapeutics that could make the protein poorer at grabbing and holding and hence compromise the pathogen in the host. The study has now been published in “Biophysical Journal”.

The cells of the mouth, nose and intestinal mucosa produce large quantities of a chemical called sialic acid. Many bacteria possess a special transport system...

Im Focus: Newly proposed reference datasets improve weather satellite data quality

UMD, NOAA collaboration demonstrates suitability of in-orbit datasets for weather satellite calibration

"Traffic and weather, together on the hour!" blasts your local radio station, while your smartphone knows the weather halfway across the world. A network of...

Im Focus: Repairing defects in fiber-reinforced plastics more efficiently

Fiber-reinforced plastics (FRP) are frequently used in the aeronautic and automobile industry. However, the repair of workpieces made of these composite materials is often less profitable than exchanging the part. In order to increase the lifetime of FRP parts and to make them more eco-efficient, the Laser Zentrum Hannover e.V. (LZH) and the Apodius GmbH want to combine a new measuring device for fiber layer orientation with an innovative laser-based repair process.

Defects in FRP pieces may be production or operation-related. Whether or not repair is cost-effective depends on the geometry of the defective area, the tools...

All Focus news of the innovation-report >>>

Anzeige

Anzeige

Event News

12V, 48V, high-voltage – trends in E/E automotive architecture

10.01.2017 | Event News

2nd Conference on Non-Textual Information on 10 and 11 May 2017 in Hannover

09.01.2017 | Event News

Nothing will happen without batteries making it happen!

05.01.2017 | Event News

 
Latest News

Solar Collectors from Ultra-High Performance Concrete Combine Energy Efficiency and Aesthetics

16.01.2017 | Trade Fair News

3D scans for the automotive industry

16.01.2017 | Automotive Engineering

Nanoparticle Exposure Can Awaken Dormant Viruses in the Lungs

16.01.2017 | Life Sciences

VideoLinks
B2B-VideoLinks
More VideoLinks >>>