Forum for Science, Industry and Business

Sponsored by:     3M 
Search our Site:

 

NASA Study Using Cluster Reveals New Insights Into Solar Wind

25.10.2012
A new study based on data from European Space Agency’s Cluster mission shows that it is easier for the solar wind to penetrate Earth’s magnetic environment, the magnetosphere, than had previously been thought.

Scientists from NASA's Goddard Space Flight Center in Greenbelt, Md. have, for the first time, directly observed the presence of certain waves in the solar wind—called Kelvin-Helmholtz waves that can help transfer energy into near-Earth space—under circumstances when previous theories predicted they were not expected.


When the interplanetary magnetic field (IMF) is oriented westward (dawnward) or eastward (duskward), magnetopause boundary layers at higher latitude become most subject to Kelvin–Helmholtz instabilities — shown here in an artist’s representation as giant swirls. Credit: AOES Medialab

The recent paper, published on Aug 29, 2012, in the Journal of Geophysical Research shows that the presence of these waves help the incoming charged particles of the solar wind breach the magnetopause—the outer region of the magnetic "shield" around our planet. http://cms.nasa.gov/
support/cms/templates/authoring
/detail_page_template.html#4
As a result, the boundary of Earth’s magnetic bubble behaves less like a continuous barrier and more like a sieve allowing entry to the continuous onslaught of energetic electrons and protons.

"The complex environment near Earth varies continuously, but it is always filled with strong and complex magnetic fields. Variations in the pressure of the solar wind and in the orientation of the magnetic field can lead to changes in how the magnetosphere responds to the solar wind," says Melvyn Goldstein, a geospace scientist at Goddard and an author on the paper. "And understanding how the solar wind impacts these changes by transferring material, momentum and energy across the magnetopause, is one of the most important questions in magnetospheric physics in general and space weather effects in particular."

This latest discovery was made possible by the unique configuration of the four identical Cluster spacecraft, which fly in a closely controlled formation through near-Earth space. As they sweep from the magnetosphere into interplanetary space and back again, the flotilla provides unique three-dimensional insights on the processes that connect the sun to Earth.

Previous discoveries derived from Cluster measurements have shown that the magnetopause is commonly subject to Kelvin-Helmholtz waves. These waves have a distinctive shape that is quite familiar: they look like large amplitude ocean waves that are whipped up by strong winds. Such waves generate turbulence as they crest and break. In the case of the solar wind, the waves are made of huge swirls of electrified gas called plasma, up to 25,000 miles across, which develop along the outer edge of the magnetosphere. Moving plasma, and therefore the Kelvin-Helmholtz waves, trap magnetic fields along with them, which turn out to be crucial in trying to determine how the solar wind can enter the magnetosphere. As the magnetic field becomes wrapped up in the Kelvin-Helmholtz waves, oppositely directed fields can "reconnect", allowing plasma to move from the solar wind into the magnetosphere.

"The space weather community pays considerable attention to Kelvin-Helmholtz waves," says Kyoung-Joo Hwang, a research scientist at Goddard and the University of Maryland Baltimore County and lead author of the paper. "Because they have global influence on Earth's magnetic system and are important for understanding Earth’s response to changes on the sun."

Medialab In general, the solar wind's ability to penetrate into near-Earth space is thought to rely on the magnetic alignment of the interplanetary magnetic fields, often shortened to IMF. As the solar wind streams from the sun toward the day side of Earth, its magnetic fields connect up to those of Earth, resulting in a sudden and dramatic reconfiguration or reconnection of the field lines. This is most efficient when the IMF is aligned southward – opposite to the northward alignment of Earth’s magnetic field. The temporary tangling of the field lines creates ideal conditions for magnetic reconnection, allowing large amounts of plasma and magnetic energy to be transferred from the solar wind to the magnetosphere.

Magnetic reconnection also occurs more weakly with a northward orientation of the IMF, generally only seen at higher latitudes. Spacecraft observations have indicated that Kelvin-Helmholtz waves may play an important role in the transfer of solar wind material into the magnetosphere during a northward IMF – a hypothesis bolstered by the fact that the waves can facilitate magnetic reconnection. However, previous identification of Kelvin-Helmholtz waves during northward IMF were limited to the low latitude flanks of the magnetosphere.

The team of scientists has now directly observed these Kelvin-Helmholtz waves at high latitudes under other orientations of the IMF. Instead of pointing north or south, the IMF was pointing west, towards the dawn side of Earth. Under these conditions, the Cluster data showed the waves on the dusk side of the high-latitude magnetopause. The magnetopause is the boundary between the relatively undisturbed magnetosphere and the magnetosheath, the region containing solar wind plasma that has come across the bow shock that protects Earth from the direct onslaught of solar wind plasma. The scientists were also able to characterize how differences in IMF orientation greatly influenced the Kelvin-Helmholtz waves as a result of variations in the thickness and other characteristics of the boundary layer.

The data were obtained between 7:00 a.m. and noon EST on 12 Jan., 2003. The four Cluster spacecraft were in tetrahedral formation, about 2,500 miles apart, flying close to the northern duskward region of Earth’s magnetosphere. The quartet was outbound, heading toward the evening side magnetopause.

"This was the first time that the presence of Kelvin-Helmholtz waves at the magnetopause had been demonstrated at high latitude for a dawnward orientation of the IMF," said Hwang. "We are seeing these waves in unpredictable places, under solar wind conditions that were previously thought to be unfavorable for their generation."

While the paper reports on only one case study, similar conditions are frequently found in the magnetosphere, says Goldstein. "Since this and similar geometrical orientations of the IMF are common, the process we describe might act as a fairly continuous mechanism of solar wind transport into the magnetosphere."

Hwang is now undertaking a statistical study to determine how ubiquitous the Kelvin-Helmholtz waves are and how they evolve and develop.

"This discovery shows how Earth’s magnetosphere can be penetrated by solar particles under certain interplanetary magnetic field conditions," said Matt Taylor, ESA project scientist for Cluster. "The study of the high-latitude, dayside magnetopause would not have been possible without the in-situ measurements sent back by Cluster. The relatively small spatial separation of the four spacecraft made it possible to analyze the spatial structures and characteristics of the Kelvin-Helmholtz waves."

These results are also relevant to studies of magnetospheric processes around other planets in the solar system. For example, Kelvin-Helmholtz instabilities are commonly observed at the boundary of Mercury’s magnetosphere and on the dawnward flank of Saturn’s magnetopause. This new study opens up the possible locations where such waves may be generated, suggesting that they can be a common, and possibly continuous, mechanism for the entry of solar wind into planetary magnetospheres under various IMF orientations.

Karen C. Fox
NASA Goddard Space Flight Center, Greenbelt, MD

Karen C. Fox | EurekAlert!
Further information:
http://www.nasa.gov
http://www.nasa.gov/mission_pages/sunearth/news/solarwind-insight.html

More articles from Earth Sciences:

nachricht Colorado River's connection with the ocean was a punctuated affair
16.11.2017 | University of Oregon

nachricht Researchers create largest, longest multiphysics earthquake simulation to date
14.11.2017 | Gauss Centre for Supercomputing

All articles from Earth Sciences >>>

The most recent press releases about innovation >>>

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

Im Focus: A “cosmic snake” reveals the structure of remote galaxies

The formation of stars in distant galaxies is still largely unexplored. For the first time, astron-omers at the University of Geneva have now been able to closely observe a star system six billion light-years away. In doing so, they are confirming earlier simulations made by the University of Zurich. One special effect is made possible by the multiple reflections of images that run through the cosmos like a snake.

Today, astronomers have a pretty accurate idea of how stars were formed in the recent cosmic past. But do these laws also apply to older galaxies? For around a...

Im Focus: Visual intelligence is not the same as IQ

Just because someone is smart and well-motivated doesn't mean he or she can learn the visual skills needed to excel at tasks like matching fingerprints, interpreting medical X-rays, keeping track of aircraft on radar displays or forensic face matching.

That is the implication of a new study which shows for the first time that there is a broad range of differences in people's visual ability and that these...

Im Focus: Novel Nano-CT device creates high-resolution 3D-X-rays of tiny velvet worm legs

Computer Tomography (CT) is a standard procedure in hospitals, but so far, the technology has not been suitable for imaging extremely small objects. In PNAS, a team from the Technical University of Munich (TUM) describes a Nano-CT device that creates three-dimensional x-ray images at resolutions up to 100 nanometers. The first test application: Together with colleagues from the University of Kassel and Helmholtz-Zentrum Geesthacht the researchers analyzed the locomotory system of a velvet worm.

During a CT analysis, the object under investigation is x-rayed and a detector measures the respective amount of radiation absorbed from various angles....

Im Focus: Researchers Develop Data Bus for Quantum Computer

The quantum world is fragile; error correction codes are needed to protect the information stored in a quantum object from the deteriorating effects of noise. Quantum physicists in Innsbruck have developed a protocol to pass quantum information between differently encoded building blocks of a future quantum computer, such as processors and memories. Scientists may use this protocol in the future to build a data bus for quantum computers. The researchers have published their work in the journal Nature Communications.

Future quantum computers will be able to solve problems where conventional computers fail today. We are still far away from any large-scale implementation,...

Im Focus: Wrinkles give heat a jolt in pillared graphene

Rice University researchers test 3-D carbon nanostructures' thermal transport abilities

Pillared graphene would transfer heat better if the theoretical material had a few asymmetric junctions that caused wrinkles, according to Rice University...

All Focus news of the innovation-report >>>

Anzeige

Anzeige

Event News

Ecology Across Borders: International conference brings together 1,500 ecologists

15.11.2017 | Event News

Road into laboratory: Users discuss biaxial fatigue-testing for car and truck wheel

15.11.2017 | Event News

#Berlin5GWeek: The right network for Industry 4.0

30.10.2017 | Event News

 
Latest News

NASA detects solar flare pulses at Sun and Earth

17.11.2017 | Physics and Astronomy

NIST scientists discover how to switch liver cancer cell growth from 2-D to 3-D structures

17.11.2017 | Health and Medicine

The importance of biodiversity in forests could increase due to climate change

17.11.2017 | Studies and Analyses

VideoLinks
B2B-VideoLinks
More VideoLinks >>>