Solar Dynamics Observatory: The 'Variable Sun' Mission

Feb 05, 2010 by Dr. Tony Phillips
An artist's concept of the variable sun.

For some years now, an unorthodox idea has been gaining favor among astronomers. It contradicts old teachings and unsettles thoughtful observers, especially climatologists.

"The sun," explains Lika Guhathakurta of NASA headquarters in Washington DC, "is a variable star."

But it looks so constant...

That's only a limitation of the human eye. Modern telescopes and spacecraft have penetrated the sun's blinding glare and found a maelstrom of unpredictable turmoil. Solar flares explode with the power of a billion atomic bombs. Clouds of magnetized gas (CMEs) big enough to swallow planets break away from the stellar surface. Holes in the sun's atmosphere spew million mile-per-hour gusts of solar wind.

And those are the things that can happen in just one day.

Over longer periods of decades to centuries, waxes and wanes with a complex rhythm that researchers are still sorting out. The most famous "beat" is the 11-year sunspot cycle, described in many texts as a regular, clockwork process. In fact, it seems to have a mind of its own.

"It's not even 11 years," says Guhathakurtha. "The cycle ranges in length from 9 to 12 years. Some cycles are intense, with many sunspots and solar flares; others are mild, with relatively little solar activity. In the 17th century, during a period called the 'Maunder Minimum,' the cycle appeared to stop altogether for about 70 years and no one knows why."
There is no need to go so far back in time, however, to find an example of the cycle's unpredictability. Right now the sun is climbing out of a century-class solar minimum that almost no one anticipated.

"The depth of the in 2008-2009 really took us by surprise," says sunspot expert David Hathaway of the Marshall Space Flight Center in Huntsville, Alabama. "It highlights how far we still have to go to successfully forecast solar activity."

Areas of the USA vulnerable to power system collapse in response to an extreme geomagnetic storm. Source: National Academy of Sciences.

That's a problem, because human society is increasingly vulnerable to solar flare ups. Modern people depend on a network of interconnected high-tech systems for the basics of daily life. Smart power grids, GPS navigation, air travel, financial services, emergency radio communications—they can all be knocked out by intense solar activity. According to a 2008 study by the National Academy of Sciences, a century-class solar storm could cause twenty times more economic damage than Hurricane Katrina.

"Understanding solar variability is crucial," says space scientist Judith Lean of the Naval Research Lab in Washington DC. "Our modern way of life depends upon it."

Enter the Solar Dynamics Observatory—"SDO" for short—slated to launch on Feb. 9, 2010, from the Kennedy Space Center in Florida.

SDO is designed to probe solar variability unlike any other mission in NASA history. It will observe the sun faster, deeper, and in greater detail than previous observatories, breaking barriers of time-scale and clarity that have long blocked progress in solar physics.

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SDO Project Scientist Dean Pesnell explains how the SDO's Atmospheric Imaging Assembly (AIA) instrument suite will allow us to take pictures of the sun at multiple temperatures and at resolutions never before seen.

Guhathakurta believes that "SDO is going to revolutionize our view of the sun."

The revolution begins with high-speed photography. SDO will record IMAX-quality images of the sun every 10 seconds using a bank of multi-wavelength telescopes called the Atmospheric Imaging Assembly (AIA). For comparison, previous observatories have taken pictures at best every few minutes with resolutions akin to what you see on the web, not at a movie theatre. Researchers believe that SDO's rapid-fire cadence could have the same transformative effect on solar physics that the invention of high-speed photography had on many sciences in the 19th century.

SDO doesn't stop at the stellar surface. SDO's Helioseismic Magnetic Imager (HMI) can actually look inside the sun at the solar dynamo itself.

The solar dynamo is a network of deep plasma currents that generates the sun's tangled and sometimes explosive magnetic field. It regulates all forms of solar activity from the lightning-fast eruptions of solar flares to the slow decadal undulations of the sunspot cycle.

"Understanding the inner workings of the solar dynamo has long been a 'holy grail' of solar physics," says Dean Pesnell of the Goddard Space Flight Center in Greenbelt, Maryland. "HMI could finally deliver this to us."

The dynamo is hidden from view by about 140,000 miles of overlying hot gas. SDO penetrates the veil using a technique familiar to geologists—seismology. Just as geologists probe Earth's interior using waves generated by earthquakes, solar physicists can probe the sun's interior using acoustic waves generated by the sun's own boiling turbulence. HMI detects the waves, which researchers on Earth can transform into fairly clear pictures.

"It's a little like taking an ultrasound of a pregnant mother," Pesnell explains. "We can see 'the baby' right through the skin."

Finally - and of most immediate relevance for Earth--SDO will observe the sun at wavelengths where the sun is most variable, the extreme ultraviolet (EUV). EUV photons are high-energy cousins of regular UV rays that cause sunburns. Fortunately, our atmosphere blocks solar EUV; otherwise a day at the beach could be fatal. In space, solar EUV emission is easy to detect and arguably the most sensitive indicator of solar activity.

"If human eyes could see EUV wavelengths, no one would doubt that the sun is a ," says Tom Woods of the University of Colorado in Boulder.

During a , the sun's extreme ultraviolet output can vary by factors of hundreds to thousands in a matter of seconds. Surges of EUV photons heat Earth's upper atmosphere, causing the atmosphere to "puff up" and drag down low-orbiting satellites. EUV rays also break apart atoms and molecules, creating a layer of ions in the upper atmosphere that can severely disturb radio signals. According to Judith Lean, "EUV controls Earth's environment throughout the entire atmosphere above about 100 km."

"EUV is where the action is," agrees Woods.

That's why Woods and colleagues built an extreme ultraviolet sensor for SDO called the EUV Variability Experiment ("EVE"). "EVE gives us the highest time resolution (10 sec) and the highest spectral resolution (< 0.1 nm) that we've ever had for measuring the sun, and we'll have it 24/7," he says. "This is a huge improvement over past missions."

Woods expects EVE to reveal how fast the sun can change—"we really don't know," he points out—and to surprise astronomers with the size of the outbursts.

EVE, AIA, HMI. For the next five years, the will use these instruments to redefine our star and its potential for variability. What unorthodox ideas will they beam back? Old teachings beware!

Explore further: SDO captures images of two mid-level flares

Source: Science@NASA, by Dr. Tony Phillips

4.9 /5 (18 votes)

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User comments : 2

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Jarek
5 / 5 (1) Feb 06, 2010
I believe that understanding why corona has millions of kelvins, while the surface only thousands - why magnetic reconnections effect "once started, it proceeds many orders of magnitude faster than predicted by standard models" is one of the most important fundamental lacks of todays physics.
http://en.wikiped...nnection
I think that the answer could be treating magnetic lines as physical objects not only in superconductor, but also in vacuum as QM suggest ( http://arxiv.org/abs/0910.2724 ) - giving them additional energy(mass) density per length should explain observed effects.
rgw
Feb 06, 2010
This comment has been removed by a moderator.
ormondotvos
1 / 5 (1) Feb 07, 2010
It's Lord Kelvin and his many male descendants. The women go to Gaia. It's where they go when they die. Occasionally the family feuds and that's what causes solar flares.

Ain't the Intertubes great?

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