February
2010

 

Our Vision
The world’s finest educators supporting science, technology, engineering, and math learning for pre-kindergarten to post-graduate students using real-world applications from satellites and satellite data.

Our Mission
To enhance the education environment to excite students about science, technology, engineering, and math through space-based technology – satellites and satellite data.

TABLE OF CONTENTS CLICK ON THE RED LINKS BELOW TO VIEW ARTICLES

Discussions With Dennis

Where Do You Fit in the Universe?

Nature Geoscience

How the Bering Strait influences Earth's climate

Goddard News

Giovanni Air Quality Instance Now Available

Comment

It Only Hurts When I Laugh
and
Challenges Are Gifts

Government & Education

Obama directs $250 million for science and math education

News From NOAA

Ocean Policy Task Force Releases Interim Framework for Effective Coastal and Marine Spatial Planning
And
Funding Opportunity

News From NASA

As the World Churns
And
Nasa mission to unravel sun’s threat to Earth

Go to SEA's Home Page

Visit the Satellite Educators Association home page


Where Do You Fit in the Universe?
By Dennis Bauer  www.DennisBauer.com

If you had been there on Voyager 1, thirteen years after leaving Earth, as NASA commanded the spacecraft to turn for final photos of our solar system, you would have seen the earth as the tiniest of dots 3.7 billion miles away. You might have been awed by the size of the earth against the huge backdrop of the universe.

How do you develop a sense of personal place and significance when you consider how small you are? Expand the view to our Milky Way Galaxy, and we are very small indeed. Estimates of the number of stars in our galaxy range from 100-400 billion, and there are billions more galaxies.

Our own sun is in the minor leagues compared to several other stars. The largest in our galaxy is Canis Major which means something like “Big Dog”. Indeed! Seven quadrillion earths would fit inside Canis Major. That many golf balls would cover the entire State of Washington (my home) 6 ½ feet deep, +/- an inch or two.

The universe is awesomely big! I cannot get my head around the numbers. The statistics make me feel numbingly small indeed.

Now turn the telescope around. Under the microscope, how small is small? Next to oxygen, we’re mostly made up of carbon. In a one-carat diamond there are around ten sextillion carbon atoms. Amazingly, the electron cloud is 100,000 times larger than the nucleus. If the nucleus were a golf ball and you put it at sea level, the electron cloud would be over 14,000 feet across!

Awesomely big! Awesomely small! Yet, the most amazing fact of all is this: Compare the size of the known universe to the size of the smallest known particle ...the size of a human being is right in the middle. What an amazing place to be! Right in the middle of it all.

To develop a sense of purpose requires that you first have a sense of place, that you know where you stand in relation to other people or to an objective. Looking through a telescope can make you feel incredibly small. Looking through a microscope can make you feel incredibly big. Being right in the middle can make you feel right at home in the universe. Awesome big! Awesome small! Awesome you!

Dennis Bauer is an award winning professional public speaker. Working with people to reach new levels of leadership, critical thinking, personal potential and a deeper sense of mission, Dennis declares, "You can change the world! (or at least make a dent in it.)". Through engaging humor, true-life stories and unique perspectives, he leads his audience to new heights of personal insight, motivation and achievement. www.dennisbauer.com

 

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How the Bering Strait influences Earth's climate
By Moises Velasquez-Manoff Staff writer, The Christian Science Monitor

At 50 miles wide, the Bering Strait, which separates Alaska from Russia, hardly seems like a major player in Earth's climate.

But a new study in the journal Nature Geoscience concludes that this shallow strait between the North Pacific and the Arctic oceans has played a large role in climate fluctuations during recent ice ages. Depending on whether it's closed or open, the strait dramatically changes the distribution of heat around the planet.

When sea levels decline enough that water can no longer flow from the Pacific to the Arctic through the strait, the North Atlantic responds by growing warmer. That warmth is strong enough to melt ice sheets and temporarily reverse the glaciation of the Northern Hemisphere.

Generally, scientists think that changes in Earth's orbit around the sun have driven the repeated advance and retreat of glaciers during the Pleistocene — the period starting 2.58 million years ago and ending about 10,000 years ago.

When less sun reaches the Northern Hemisphere during summer months, winter snows don't melt. The white snow reflects more of the sun's energy back into space, further cooling the region. Glaciers form and begin creeping southward. These ice sheets, a mile or more thick in places, suck up large quantities of water.

Compared to today, sea levels dropped by as much as 400 feet during the Pleistocene.

But while glacial periods follows Earth's orbital variations quite closely — they occur very roughly on 100,000-year cycles — for the past 100,000 years or so, a shorter warming and cooling cycle has played out over the larger one.

Even as the amount of sunlight hitting the region diminished, parts of Greenland and North America warmed by nearly 3 degrees F. Glaciers then shrank and sea levels rose by up to 100 feet, only to reverse. This cycle repeated every few thousand years. Why?

The authors argue that the Bering Strait, a choke point, is the critical factor. When sea levels dropped sufficiently, dry land emerged between North America and Asia. This dam halted the flow of water from the North Pacific into the Arctic.

At present, about 800,000 cubic meters (211 million gallons) of water per second flow into the Arctic from the North Pacific. That's about 3.6 times the discharge of the Amazon, the world's largest river.

This water from the north Pacific eventually flows to the north Atlantic. Water in the north Pacific is much fresher, and therefore much lighter, than the saltier water of the North Atlantic. And the influx of freshwater into the North Atlantic impedes a process that's critical to heat distribution around the globe.

In the north Atlantic, warm water flows north from equatorial regions. As it cools between Iceland and Norway, this water sinks and, once at a certain depth, begins flowing back south.

Scientists call this conveyor-beltlike flow the "meridional overturning circulation." And it's responsible for keeping Europe balmy compared to regions at similar latitudes elsewhere.

When the overturning is impeded, however, the transport of tropical heat to high northern latitudes slows, and the north Atlantic grows colder.

In other words, freshwater flowing into the north Atlantic can bring temperatures down in the region. Conversely, lessening the flow of freshwater into the north Atlantic can cause temperatures to rise. That's what the authors of this paper say happened repeatedly during the past 100,000 years.

Here’s the cycle: Cooling brought on by changes in Earth's orbit caused glaciers to grow and sea levels to fall. Eventually, the seas dropped far enough that the Bering Strait was closed off. The flow of relatively fresh water from the north Pacific to the north Atlantic stopped, or was dramatically decreased. Without interference from this freshwater, the meridional overturning in the North Atlantic strengthened — by about 13 percent. Parts of Greenland, northeastern North America, and Europe warmed by 2.7 degrees F. Glaciers around thenNorth Atlantic then began melting.

Meanwhile, as the northward flow of water in the Pacific was stymied, temperatures there dropped by the same amount — 2.7 degrees F.

In the end, however, this warming was self-limiting. As increased warmth melted glaciers around the north Atlantic, sea levels began to rise.

Eventually they rose sufficiently to again engulf the Bering land bridge. The flow of water from the north Pacific into the Arctic resumed. The meridional overturning in the north Atlantic again weakened. And the glaciers of the Northern Hemisphere again began advancing southward.

None of this bears directly on the current trend of human-induced global warming. But it does indicate that scientists, enabled by ever-more powerful computers and more complicated — some might say "realistic" — climate models, are improving their understanding of Earth's climate system.

It also highlights an important lesson: In complex systems (Earth’s climate), seemingly small changes, such as closing the 50-mile-wide Bering Strait, can have large consequences, like temporarily reversing a hemisphere-wide cooling trend.

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Giovanni Air Quality Instance Now Available

A new Giovanni instance dedicated to air quality related data is now available. The instance includes global aerosol and cloud data from MODIS, global aerosol data from OMI, and the AIRNow Fine Particulate Matter (PM2.5) ground-based monitoring product for the continental United States.

The GES DISC has created the Giovanni Air Quality Instance for visualization and exploration of remotely- sensed and in situ data products related to air quality. For the continental United States, the Air Quality instance features Environmental Protection Agency AIRNow PM2.5 data from ground-based monitoring stations. PM2.5 is also known as Fine Particulate Matter, and it indicates the concentration of aerosol particles less than 2.5 μm in diameter. PM2.5 is a pollutant because particles of this size can lodge deep in human lungs and cause health problems, such as asthma, emphysema, respiratory difficulty, and chronic bronchitis. The PM2.5 product is provided by the cross-agency AIRNow program.

Correlation map, PM2.5 and MODIS Aerosol Optical Depth, July 2007, California and Pacific NorthwestIn addition to the PM2.5 data product, the Air Quality Instance also includes aerosol and cloud data products from the Moderate Resolution Imaging Spectroradiometer (MODIS) on the Terra and Aqua satellites, and aerosol products from the Ozone Monitoring Instrument (OMI) on the Aura satellite.   Unlike the PM2.5 data product, all of the remotely-sensed data products are available globally.

The Giovanni system provides several different rapid visualization and analysis capabilities that can be utilized to examine the data in the Air Quality instance.   Users can generate maps of specific data products, time-series, and Hovmöller plots.    Multiple data products can be plotted in the same time-series.   Users can also create maps of the correlations between different data products, which indicate if these data products are related to each other over a specific time interval.

Shown below are other types of events that influence air quality.   The "Haze" custom color palette was used to show how Giovanni has considerable flexibility in its visualization menu, providing an easy way to prepare graphics for presentations and research papers.  Click on each image to view it full-size.

Vog ("volcanic smog")  
MODIS true-color image of volcanic haze over the Hawaiian Islands, April 26, 2008

Giovanni visualization of MODIS Aerosol Optical Depth data on April 26, 2008

Southern California Wildfires, October 2003  
MODIS image of Southern California wildfires on October 26, 2003.
Giovanni visualization of PM2.5 data product for California in October 2003

MODIS image of smoke and fire location, October 26, 2003

Fine Particulate Matter (PM2.5) over California, October 2003
Saharan Dust Storm over the Atlantic  
MODIS image of a dust storm over the Atlantic Ocean, March 4, 2004
Giovanni visualization of MODIS Aerosol Optical Depth data for this dust storm.

MODIS true-color image of dust storm over the Atlantic Ocean March 4, 2004

Giovanni visualization of MODIS Aerosol Optical Depth data for the dust storm, March 2-6, 2004

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It Only Hurts when I Laugh
By: BJ Gallagher

 

Nobody ever promised you a rose garden, but who knew the thorns would be so sharp?File:Subway train in tunnel.jpg

 

Tough times are painful - your head hurts, your back aches, your heart breaks.

 

Sometimes everything seems to hurt. When will it end? Or will it ever end?

 

Discomfort and pain are easier to bear when you know they're not permanent

 

But it's harder when there's no end in sight.

 

Hang in there now. REMEMBER TO BREATHE

 

Nothing is forever and this too shall pass.

 

Watch for that light at the end of the tunnel and pray that its NOT A TRAIN!

 


 

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Ocean Policy Task Force Releases Interim Framework for Effective Coastal and Marine Spatial Planning

EXECUTIVE OFFICE OF THE PRESIDENT

COUNCIL ON ENVIRONMENTAL QUALITY

 

Ocean Policy Task Force Releases Interim Framework for Effective Coastal and Marine Spatial Planning

Comprehensive, Integrated Approach Helps to Determine how the Ocean, Coasts and Great Lakes are Used and Protected Now and in the Future

President Obama’s Ocean Policy Task Force released its Interim Framework for Effective Coastal and Marine Spatial Planning (Interim Framework) today for a 60-day public review and comment period. With competing interests in the ocean, our coasts and the Great Lakes, the Interim Framework offers a comprehensive, integrated approach to planning and managing uses and activities. Under the Framework, coastal and marine spatial planning would be regional in scope, developed cooperatively among Federal, State, tribal, local authorities, and regional governance structures, with substantial stakeholder and public input.

The Interagency Ocean Policy Task Force, which was established by President Obama on June 12,

2009, is led by White House Council on Environmental Quality Chair Nancy Sutley, consists of 24 senior-level officials from Administration agencies, departments, and offices. “The uses of our oceans, coasts and Great Lakes have expanded exponentially over time. These waters provide the United States with many commercial, recreational, cultural, energy, scientific, economic, conservation and national security benefits and they sustain diverse habitats and species. At the same time they are facing environmental challenges including pollution and habitat destruction that make them increasingly vulnerable,” said Nancy Sutley, Chair of the White House Council on Environmental Quality. “Without an improved, more thoughtful approach, we risk an increase in user conflicts and the potential loss of critical economic, ecosystem, social, and cultural benefits for present and future generations.”

"Coastal and marine spatial planning may sound like the stuff of policy wonks, but it is actually vital to anyone who works or plays on the oceans," said Dr. Jane Lubchenco, Under Secretary of Commerce for Oceans and Atmosphere and NOAA administrator. "In fact, coastal and marine spatial planning is an essential tool for anyone who depends on the oceans for sustainable jobs, healthy seafood, clean energy, recreation, or vibrant coastal communities."

“America is a maritime nation so we must consider how we can protect the environment, facilitate maritime commerce, and responsibly harness oceanic resources. By pursuing a “whole of government” approach, we can meet our broad goals while protecting our way of life,” said Coast Guard Commandant, Admiral Thad Allen. “Marine Spatial Planning is an important tool that will inform the decisions that the Department of the Interior makes under its many existing coastal and ocean authorities,” said Associate Deputy Secretary Laura Davis. “It is important that we make every effort to improve communication and coordination on these issues among the federal government, states and stakeholders.”

“The interim framework strengthens the work we do with states, tribes, partners and other stakeholders to protect vital resources in our oceans, coasts, and the Great Lakes,” said Peter Silva, EPA's Assistant Administrator for the Office of Water. “By opening up the flow of information and promoting transparent, sound science, we will be better equipped to deliver the environmental, economic, and health benefits the public rightly expects.” In developing the Interim Report and Interim Framework, the Task Force undertook a robust public engagement process. The Task Force heard from and involved stakeholders and interested parties, including holding six regional public meetings, convening 38 expert briefings, and receiving almost four thousand individual comments via the web.

The Interim Framework includes a number of important provisions that would significantly overhaul the Federal government’s approach to coastal and marine planning, including:

A New Approach to How We Use and Protect the Ocean, Coast, and Great Lakes.

The Interim Framework is designed to: decrease user conflicts; improve planning and regulatory efficiencies and decrease their associated costs and delays; and preserve critical ecosystem function and services. The Interim Framework describes how such plans would be developed and implemented, and provides timeframes and steps for phased implementation of the framework.

Moves us Away From Sector-by-Sector and Statute-by-Statute Decision-Making.

While many existing permitting processes include aspects of coordinated planning, most focus solely on a limited range of management tools and outcomes (e.g., oil and gas leases, fishery management plans, and marine protected areas). Comprehensive marine spatial spatial planning presents a more integrated, comprehensive, ecosystem-based, flexible, and proactive approach to planning and managing uses and activities.

Brings Federal, State, and Tribal Partners Together in an Unprecedented Manner to Jointly Plan for the Future.

The Interim Framework is not a top-down planning effort. Rather, it describes a new approach to Federal resource planning that is regionally based and developed cooperatively among Federal, State, tribal, and local authorities, and regional governance structures, through the establishment of nine regional planning bodies.

Places Science-Based Information at the Heart of Decision-Making:

Scientific data, information and knowledge, as well as relevant traditional knowledge, will be the underpinning of the regionally developed plans.

Emphasizes Stakeholder and Public Participation:

The planning process would be fully transparent and participatory – requiring frequent and robust stakeholder engagement throughout all steps of the process (i.e., development, adoption, implementation, adaptation and evaluation).

The Task Force’s Interim Framework is now available for a 60-day public review and comment period. After the close of the comment period on the Interim Framework, the Task Force will finalize its recommendations in both this report and the September 10, 2009 Interim Report, and provide a final report to the President in early 2010.

For more details on the Interagency Ocean Policy Task Force, including the Interim Framework, and to submit your comments, please go to www.whitehouse.gov/oceans.

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Challenges Are Gifts
Oprah Winfrey
Angry_Woman.jpg

Challenges are gifts that force us to search for a new center of gravity.

 

Don't fight them.

 

Just find a different way to stand.

 

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Obama directs $250 million for science and math education
By Amanda Paulson Staff writer, The Christian Science Monitor

President Obama on Wednesday announced a $250 million public-private effort to increase the number and quality of science, technology, engineering, and mathematics (STEM) teachers.

The partnerships expand the “Educate to Innovate” campaign Mr. Obama launched in November. But where the initial campaign focused on out-of-classroom science exposure – bringing in organizations like the Discovery Channel and Sesame Street – the latest efforts focus specifically the teaching part of the issue.

“The in-school intervention that has the highest impact on student achievement is a strong teacher,” says Arthur Levine, president of the Woodrow Wilson Foundation, whose teaching fellowship is one of the five programs the administration is helping to expand.

The push for more attention on STEM subjects has been building for some time, with educators, business leaders, scientists, and policymakers calling attention to American students’ lackluster math and science performance relative to other countries and sounding the alarm for what it means for the country’s future.

“Our future is on the line,” said Obama in announcing the new partnerships and honoring more than 100 science and math teachers. “The nation that out-educates us today is going to out-compete us tomorrow.”

US students' mediocre ranking

According to one measure, US students are 19th in math and 14th in science out of 31 countries ranked by the Organization for Economic Co-operation and Development (OECD). And in 2000, the number of foreign students studying physical sciences and engineering in US grad schools for the first time surpassed the number of American students.

Women and minority students are vastly underrepresented among undergraduate majors in science and math, and there is a growing shortage of qualified teachers for STEM subjects.

That shortage is what the programs highlighted Wednesday aims to address, trying to increase both the number and quality of STEM teachers, particularly in high-poverty schools.

Among the partnerships:

• An expansion of the UTeach program, which helps science and math undergraduates receive a teaching certificate along with their baccalaureate degree.

• A commitment by the presidents of more than 75 public universities to prepare 10,000 science and math teachers by 2015.

• An expansion of the Woodrow Wilson teaching fellowships, which will train more than 700 math and science teachers in Indiana, Ohio, and Michigan over the next three years.

The focus on teaching is the right one, says Tracy Gray, managing director for the Center on STEM Education and Innovation at the American Institutes for Research, though the key is in how the programs are implemented.

“It’s necessary to have not just some good ideas and good intentions, but a very solid program that is based on evidence of what works, and that is provided to teachers on an ongoing basis,” says Dr. Gray. “A one-shot professional development initiative in August does not help the teacher in February…. The hope is that this [administration] effort, working with the business community, will generate enough funding so that teachers get enough support … to really ensure they have both the content and the pedagogical knowledge to reach all students.”

Programs selected have good track records

Most of the programs being highlighted already have a significant track record, providing extensive support and both practical and theoretical training to the teachers they produce.

“The prevailing myth is that students majoring in math, chemistry, biology, or physics aren’t interested in teaching, and we’ve significantly debunked that myth,” notes John Winn, chief program officer for the National Math and Science Initiative, whose UTeach program had 2,700 students enroll this year at the 13 universities where it currently exists. (It is expanding this year to about 20 schools.) More than 90 percent of UTeach graduates become teachers, and 82 percent are still in the classroom after five years.

The Woodrow Wilson partnership, meanwhile, operates much like a teaching residency program, paying students during their fellowship and asking for a three-year commitment to teach in high-need schools, with on-site mentoring throughout that period.

Just a few teachers, notes Dr. Levine, can make a big difference: In Michigan, the 120 teachers a year that the program will train will be enough to fill all anticipated vacancies in Detroit, Grand Rapids, and Kalamazoo, and the 80 teachers a year it has trained in Indiana is enough to increase the number of certified STEM teachers in the state by 20 percent.

“What we’ve asked [universities] to do is to create brand new programs that focus on student achievement as the goal and the marker of success, are clinically based, and move the instruction from the ivory tower into schools,” says Levine. “Even after this program is completed what we’ll have is a series of leading universities that have changed the way they prepare STEM teachers.”

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Nasa mission to unravel sun’s threat to Earth
By

NASA is to embark on one of its most ambitious missions in an attempt to unlock the secrets of the sun.

The Sun

Following its launch in nine days’ time, the US space agency’s Solar Dynamics Observatory (SDO) will spend five years in orbit trying to discover the causes of extreme solar activity, such as sun spots and solar winds and flares.

Scientists have long been aware that disturbances on the sun can trigger dangerous x-rays, charged particles and magnetic fields that can disrupt power supplies, communication signals and aircraft navigation systems on Earth.

By understanding how such solar phenomena are created, they hope to be able to produce reliable forecasts of “space weather” and provide advance warnings of any threat.

Orbiting the Earth at a distance of 22,300 miles, the observatory will measure fluctuations in the sun’s ultraviolet output, map magnetic fields and photograph its surface and atmosphere.

Experts have likened the mission to a “giant microscope” that will capture for the first time every nuance of the sun’s exterior. The images relayed to Earth will be 10 times clearer than high-definition television.

Barbara Thompson, project scientist, said: “It is Nasa’s first weather mission and it aims to characterise everything on the sun that can impact on the Earth and near Earth.

“We know things happen on the sun which affect spacecraft, communications and radio signals. If we can understand the underlying causes of what is happening then we can turn this information into forecasts.

“The key thing about the mission is that it is not just pure science for its own sake. There is likely to be a direct and immediate benefit for people.”

Solar magnetic storms and space weather disturbances have had a number of dramatic consequences over the years.

On March 13, 1989, millions of people in Canada and the United States were left without electricity for more than nine hours after a magnetic storm sent shockwaves through the Hydro-Québec power grid.

Five years later, a geomagnetic storm temporarily knocked out two Canadian satellites and Intelsat-K, an international communications satellite.

The most powerful solar storm in history, known as a “superstorm”, occurred on September 1, 1859. It caused the failure of telegraph systems in Europe and North America.

The storm produced auroras — phenomena normally only seen near the poles — which were visible in Cuba, Mexico and Italy. The lights were so bright in California’s Rocky Mountains that gold prospectors mistook them for dawn and began preparing breakfast.

Transpolar aircraft are particularly sensitive to space weather because they rely on navigation systems for the entire duration of a flight.

Nasa estimates that the SDO will transmit as much as 50 times more scientific data than any other mission in the space agency’s history.

Each image will consist of more than 16m pixels and the amount of data sent back to Earth daily will be equivalent to downloading 500,000 songs a day from the internet.

In order to process the data, the organisation has set up a pair of dedicated radio antennae near Las Cruces, New Mexico.

The SDO’s orbit will match the speed of the rotation of the Earth, meaning that it will be in constant view of the two 59ft dishes throughout the mission.

The UK-based Science and Technology Facilities Council is supplying some of the equipment for the observatory.

Professor Richard Harrison, of the Rutherford Appleton Laboratory in Oxfordshire, said understanding the impact of the sun’s magnetic fields was key to the mission.

“The idea is to image different layers of the sun’s atmosphere all the way down to the surface and measure magnetic fields,” he said.

“The bottom line is that you are trying to understand how this atmosphere works. We can already see phenomena like the flares. The question is how does the magnetic field form to allow this sort of thing to happen.”

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Funding Opportunity

NOAA’s Office of Education (OEd) has issued a request for applications for informal/nonformal science education projects that engage the public in activities that utilize emerging and/or advanced technologies and leverage NOAA assets to improve understanding and stewardship of the local and global environment.  There is specific interest in projects that use emerging and/or advanced technologies to (1) facilitate outdoor experiences involving scientific inquiry and exploration of the natural world apart from formal K-12 curricula and (2) visualize, display, and interpret data to improve understanding and provide a systems perspective of Earth's dynamic processes. All projects must focus on one or more of the following informal/nonformal science education activities:

·                Technologically facilitated outdoor experiential learning for youth and adults;

·                Public participation in science related to one or more of NOAA's mission goals;

·                Exhibitions and online programs allowing the visualization and exploration of data supporting the interpretation of ocean, coastal, Great Lakes, weather and climate sciences for public audiences;

·                Spherical display system (including NOAA's Science On a Sphere) installations and programming; and

·                Professional development programs and training programs for informal/nonformal education staff.

                                                                         
Deadlines

Letters of Intent are required.  The deadline for letters of intent is 5:00 PM EST February 16, 2010.

 The deadline for full applications is 5:00 PM EDT on April 6, 2010.

  Additional Information
For further information please visit: http://www.oesd.noaa.gov/funding_opps.html

For automated updates on this funding opportunity, we recommend you subscribe to our RSS feed at http://www.oesd.noaa.gov/funding_opps_feed.xml.

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As the World Churns
By:
Alan Buis, Jet Propulsion Laboratory
Illustration of Earth core data

"Terra firma." It's Latin for "solid Earth." Most of the time, at least from our perspective here on the ground, Earth seems to be just that: solid. Yet the Earth beneath our feet is actually in constant motion. It moves through time and space, of course, along with the other objects in the universe, but it moves internally as well. The powerful forces of wind, water and ice constantly erode its surface, redistributing Earth's mass in the process. Within Earth's solid crust, faulting literally creates and then moves mountains. Hydrological changes, such as the pumping of groundwater for use by humans, cause the ground beneath us to undulate. Volcanic processes deform our planet and create new land. Landslides morph and scar the terrain. Entire continents can even rise up, rebounding from the weight of massive glaciers that blanketed the land thousands of years ago.

Indeed, the outermost layers of the celestial blue onion that is Earth-its crust and upper mantle-aren't very solid at all. But what happens if we peel back the layers and examine what's going on deep within Earth, at its very core?

Obviously, Earth's core is too deep for humans to observe directly. But scientists can use indirect methods to deduce what's going on down there. A new study in the journal Geophysical Research Letters, by Jean Dickey of NASA's Jet Propulsion Laboratory, Pasadena, Calif. and co-author Olivier deViron of the Institut de Physique du Globe de Paris, University Paris Diderot, Centre National de la Recherche Scientifique, Paris, has confirmed previous theoretical predictions that the churning cauldron of molten metals that make up Earth's liquid outer core is slowly being stirred by a very complex but predictable series of periodic oscillations. The findings give scientists unique insights into Earth's internal structure, the strength of the mechanisms responsible for generating Earth's magnetic field and its geology.

Peeling Back the Onion

In order to better understand what's going on inside our planet, it helps to first get a lay of the land, so to speak.

Earth has several distinct layers, each with its own properties. At the outermost layer of our planet is the crust, which comprises the continents and ocean basins. Earth's crust varies in thickness from 35 to 70 kilometers (22 to 44 miles) in the continents and 5 to 10 kilometers (3 to 6 miles) in the ocean basins. The crust is mainly composed of alumino-silicates.

Next comes the mantle. The mantle is roughly solid, though very slow motion can be observed inside of it. It is about 2,900 kilometers (1,800 miles) thick, and is separated into an upper and lower mantle. It is here where most of Earth's internal heat is located. Large convective cells in the mantle circulate heat and drive the movements of Earth's tectonic plates, upon which our continents ride. The mantle is mainly composed of ferro-magnesium silicates.

Earth's innermost layer is the core, which is separated into a liquid outer core and a solid inner core. The outer core is 2,300 kilometers (1,429 miles) thick, while the inner core is 1,200 kilometers (746 miles) thick. The outer core is mainly composed of a nickel-iron alloy (liquid iron), while the inner core is almost entirely composed of a pure solid iron body.

Earth's "Magnetic" Personality

Scientists believe Earth's magnetic field results from movements of molten iron and nickel within its liquid outer core. These flows, which are caused by interactions between Earth's core and its mantle, are neither even, nor evenly distributed. The electrical currents generated by these flows result in a magnetic field, which is similarly uneven, moves around in location and varies in strength over time. Earth's magnetic field is also slightly tilted with respect to Earth's axis. This causes Earth's geographic north and south poles to not line up with its magnetic north and south poles--they currently differ by about 11 degrees.

In just the last 200 million years alone, Earth's magnetic poles have actually reversed hundreds of times, with the most recent reversal taking place about 790,000 years ago. Scientists are able to reconstruct the chronology of these magnetic pole reversals by studying data on the spreading of the seafloor at Earth's mid-oceanic ridges. Unlike the doomsday scenario popularized by Hollywood in the movie "2012," however, such reversals don't occur over days, but rather on geologic timescales spanning hundreds to thousands of years-very short in geologic time but comparatively long in human time. The time span between pole reversals is even longer, ranging from 100,000 to several million years.

Earth's magnetic field is essential for life on Earth. Extending thousands of kilometers into space, it serves as a shield, deflecting the constant bombardment of charged particles and radiation known as the solar wind away from Earth. These solar winds would otherwise be fatal to life on Earth. At Earth's poles, the perpendicular angle of the magnetic field to Earth there allows some of these particles to make it into our atmosphere. This results in the Northern Lights in the northern hemisphere and the Southern Lights in the southern hemisphere.

Here on the ground, Earth's magnetic field has many practical applications to our everyday lives. It allows people to successfully navigate on land and at sea, making it a critical tool for commerce. Hikers use it to find their way. Archaeologists use it to deduce the age of ancient artifacts such as pottery, which, when fired, assumes the magnetic field properties that were present at the time of its creation. Similarly, the field of paleomagnetism uses magnetism to give scientists glimpses into Earth's remote past. In addition, geophysicists and geologists use geomagnetism as a tool to investigate Earth's structure and changes taking place in the Earth.

Getting to the Core of the Matter

Since Earth's liquid core is the primary source of Earth's magnetic field, scientists can use observations of the magnetic field at Earth's surface and its variability over time to mathematically calculate and isolate the approximate motions taking place within the core.

That's what Dickey and deViron did. They combined measurements of Earth's magnetic field taken by observatory stations on land and ships at sea dating back to 1840 with those of the Danish Oersted and German CHAMP geomagnetic satellite missions, both of which were supported by NASA investments. These measurements were then used as inputs for a complex model that employs statistical time series analyses to determine how fast liquid iron is flowing within Earth's core.

"Although we do not observe the core directly, it's amazing how much we can learn about Earth's interior using magnetic field observations," said Dickey.

In order to approximate the flow of liquid in the core, the scientists visualized its motion as a set of 20 rigid cylinders, each rotating about a common point that represents Earth's axis. "Imagine that each cylinder is slowly rotating at a different speed, and you'll get a sense of the complex churning that's taking place within Earth's core," Dickey said.

The scientists analyzed the data to identify common patterns of movement among the different cylinders. These patterns represent how momentum and energy are transferred from the liquid core-mantle interface inward through the liquid core toward the inner core with diminishing amplitudes.

Their analyses isolated six slow-moving oscillations, or waves of motion, occurring within the liquid core. The oscillations originated at the boundary between Earth's core and its mantle and traveled inward toward the inner core with decreasing strength. Four of these oscillations were robust, occurring at periods of 85, 50, 35 and 28 years. Since the scientist's data set goes back to 1840, the recurrence period of the longest oscillation (85 years) is less well determined than the other oscillations. The last two oscillations identified were weaker and will require further study.

The 85- and 50-year oscillations are consistent with a 1997 study by researchers Stephen Zatman and Jeremy Bloxham of Harvard University, Cambridge, Mass., who used a different analysis technique. A later purely theoretical study by Harvard researcher Jon Mound and Bruce Buffett of the University of Chicago in 2006 showed that there should be several oscillations of this type; their predicted periods agree with the first four modes identified in Dickey and deViron's study.

"Our satellite-based results are in excellent agreement with the previous theoretical and other studies in this field, providing a strong confirmation of the existence of these oscillations," said Dickey. "These results will give scientists confidence in using satellite measurements in the future to deduce long-term changes taking place deep within our restless planet."

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Artist concept of the albedo effect

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