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Showing posts with label magnetic. Show all posts
Showing posts with label magnetic. Show all posts

Saturday, April 19, 2014

Fierce 2012 magnetic storm just skipped us: Earth dodged huge magnetic bullet in the sun

Earth dodged an enormous magnetic bullet in the sun on This summer 23, 2012.

Based on College of California, Berkeley, and Chinese scientists, an immediate succession of coronal mass ejections -- probably the most intense eruptions around the sun -- sent a pulse of magnetized plasma barreling into space and thru Earth's orbit. Had the eruption come nine days earlier, it might have hit Earth, potentially causing havoc using the electrical power grid, crippling satellites and Gps navigation, and interfering with our progressively electronic lives.

The photo voltaic bursts might have surrounded Earth in magnetic fireworks matching the biggest magnetic storm ever reported on the planet, the so-known as Carrington event of 1859. The dominant mode of communication in those days, the telegraph system, was bumped out over the U . s . States, literally shocking telegraph operators. Meanwhile, the Northern Lights illuminated the evening sky as far south as Hawaii.

Inside a paper showing up today (Tuesday, March 18) within the journal Character Communications, former UC Berkeley postdoctoral fellow and research physicist Ying D. Liu, now a professor at China's Condition Key Laboratory of Space Weather, UC Berkeley research physicist Jesse G. Luhmann as well as their co-workers report their research into the magnetic storm, that was detected by NASA's Stereo system A spacecraft.

"Been with them hit Earth, it most likely could have been such as the large one out of 1859, however the effect today, with this modern technologies, could have been tremendous," stated Luhmann, who belongs to the Stereo system (Photo voltaic Terrestrial Observatory) team and based at UC Berkeley's Space Sciences Laboratory.

Research this past year believed that the price of a photo voltaic storm such as the Carrington Event could achieve $2.6 trillion worldwide. A substantially more compact event on March 13, 1989, brought towards the collapse of Canada's Hydro-Quebec energy power grid along with a resulting lack of electricity to 6 million people for approximately nine hrs.

"A serious space weather storm -- a photo voltaic superstorm -- is really a low-probability, high-consequence event that poses severe risks to critical infrastructures from the society,Inch cautioned Liu, who's using the National Space Science Core Chinese Academy of Sciences in Beijing. "To buy a extreme space weather event, whether it hits Earth, could achieve billions of dollars having a potential time to recover of four-ten years. Therefore, it's vital towards the security and economic interest from the society to know photo voltaic superstorms."

According to their research into the 2012 event, Liu, Luhmann as well as their Stereo system co-workers came to the conclusion that a large episode around the sun on This summer 22 powered a magnetic cloud with the photo voltaic wind in a peak speed in excess of 2,000 kilometers per second -- four occasions the normal speed of the magnetic storm. It tore through Earth's orbit but, fortunately, Earth and yet another planets were on the other hand from the sun at that time. Any planets within the type of sight might have experienced severe magnetic storms because the magnetic area from the episode twisted using the planets' own magnetic fields.

The scientists determined the huge episode resulted from a minimum of two nearly synchronised coronal mass ejections (CMEs), which generally release powers equal to those of in regards to a billion hydrogen tanks. How quickly the magnetic cloud plowed with the photo voltaic wind am high, they came to the conclusion, because another mass ejection four days earlier had removed the road of fabric that will have slowed down it lower.

"The authors believe this extreme event was because of the interaction of two CMEs separated by only ten to fifteen minutes," stated Joe Gurman, the work researcher for Stereo system at NASA's Goddard Space Flight Center in Greenbelt, Md.

One good reason the big event was potentially so harmful, apart from its high-speed, is it created a really lengthy-duration, southward-oriented magnetic area, Luhmann stated. This orientation drives the biggest magnetic storms once they hit Earth since the southward area merges strongly with Earth's northward area inside a process known as reconnection. Storms that normally might dump their energy limited to the rods rather dump it in to the radiation devices, ionosphere and upper atmosphere and make auroras lower towards the tropics.

"These gnarly, twisty ropes of magnetic area from coronal mass ejections come raging in the sun with the ambient photo voltaic system, mounting up material before them, so when this double whammy hits Earth, it skews our planet's magnetic area to odd directions, dumping energy all over the planet," she stated. "Some people wish Earth have been in the manner how much of an experiment that could have been.Inch

"People continue to say these are rare natural hazards, but they're happening within the photo voltaic system despite the fact that we do not always discover their whereabouts,Inch she added. "It's as with earthquakes -- it's difficult to impress upon people the significance of planning unless of course a person suffers a magnitude 9 earthquake."

All of this activity could have been skipped if Stereo system A -- the Stereo system spacecraft in front of us in Earth's orbit and also the twin to Stereo system B, which trails within our orbit -- was not there to record the blast.

The aim of Stereo system along with other satellites probing the magnetic fields from the sun and Earth would be to understand why and how the sun's rays transmits out these large photo voltaic storms and also to have the ability to predict them throughout the sun's 11-year photo voltaic cycle. The wedding was particularly unusual since it happened throughout a really calm photo voltaic period.

"Findings of photo voltaic superstorms happen to be very missing and limited, and our current knowledge of photo voltaic superstorms is extremely poor," Liu stated. "Questions fundamental to photo voltaic physics and space weather, for example how extreme occasions form and evolve and just how severe it may be in the Earth, aren't addressed due to the ultimate insufficient findings."


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Tuesday, February 25, 2014

Satellite trio to explore the Earth's magnetic field

In a dense fog, a Russian Rockot rocket on 22 November 2013 cleared the launchpad of the Baikonur Cosmodrome on schedule at 13:02:15 CET. In the tip of the rocket: three identical satellites to measure the Earth's magnetic field. A good hour and a half later, at 14:37:48 CET, the report of success: all three satellites separated seamlessly from the carrier rocket and the ground stations Kiruna (Sweden) and Longyearbyen /Svalbard (Norway) were able to establish radio contact with them. GFZ scientists and invited guests observed the start of the mission called SWARM of the European Space Agency in Darmstadt via remote transmission.

Professor Johanna Wanka, Federal Minister of Education and Research said on the occasion of the perfect start of the mission: "We are very pleased that this European mission has started so smoothly.The magnetic field of the Earth is our shield against cosmic particle radiation. But it is subject to natural fluctuations, from the Earth's interior or eruptions on the Sun. Improving the exploration of its function and recording space weather data more accurately allows us to draw conclusions for life on our planet."

Professor Reinhard Huettl, Chairman of the Board of the GFZ German Research Centre for Geosciences pointed out a Potsdam success story: "The three satellites are direct developments from the CHAMP mission of the GFZ, which was launched in 2000. CHAMP with his followers GRACE and SWARM proves to be the founding father of a whole generation of satellites and space-based measurement methods."

A trio for the magnetic field

SWARM is an ESA mission as part of its "Living Planet" program. "The satellite swarm -- hence the name -- is to measure the Earth's magnetic field from space with unprecedented precision for at least four years," elaborated Professor Huettl. For this, the three satellites fly in an optimized formation: two satellites (SWARM-A, SWARM-B) fly in an altitude of 450 kilometers with a distance of 150 kilometers alongside one another, the third (SWARM-C) ascends into a higher orbit at 530 km altitude. The reason for this complex formation flight lies in the magnetic field itself: it is generated by the flow of electrically conducting liquid iron in the outer core oft he Earth, 2900 kilometers beneath our feet. It is influenced by the conductivity and the dynamics of the overlying mantle (up to 40 kilometers below the Earth's surface). Finally, the magnetized rocks of the Earth's crust contribute to the Earth's magnetic field. In addition, the sun and currents in near-Earth space influence the Earth's magnetic field from the outside. In order to study these individual components, the total signal of the magnetic field measured by the satellite needs to be separated into its individual components. "From its distance of 150 kilometers, the lower flying SWARM pair can look at the magnetic field of the Earth's crust with a stereo view," explains Professor Hermann L?hr , one of the three Principle Investigators of the mission, member of the SWARM Mission Advisory Group and Head of the German SWARM Project Office at the GFZ. "We can therefore analyze this component with very high accuracy." The third, upper SWARM satellite can in turn precisely determine the force of the magnetic field as it decreases with increasing altitude. Also, over time this satellite flies in a progressively increasing angle to the path of the lower pair. The total measurement will give a picture of the earth's magnetic field with a precision never achieved before.

Almost as a side effect, the possibility arises to observe space weather more accurately. What is understood by this are flares of our sun, but also magnetic storms generated by distant stars that can interfere with or even paralyze our technical civilization. For example, a strong solar storm in 1989 caused a breakdown of the electricity supply in Canada.

About the satellites

The three SWARM satellites together cost about 220 million euros, each weighs 500 kg. Inside the carrier rocket, a four-meter long measuring arm is folded on the back of the five meter long satellite body. This boom is folded out several hours after the deployment of the satellite, once the on-board operating system has been initiated. The reason for this is that the surface of the satellite is equipped with solar cells for the power supply. The magnetic field generated by the current, however, would interfere with the measurement, therefore, the magnetic field measuring instruments are mounted on the measuring arm.

At the tip of the boom, the particularly sensitive apparatus for measuring the magnetic field strength is installed, the sensors for determining the direction of the magnetic field are in its center. In the same position, three star sensors allow the satellite to determine and corrected its location.

To begin with, the three satellites fly parallel on a north-south path at about 88? inclination. Swarm-C is then slowly deflected by 30? per year and thus continues to fly at an increasing angle to the orbit of Swarm-A and -B.

Cite This Page:

Helmholtz Centre Potsdam - GFZ German Research Centre for Geosciences. "Satellite trio to explore the Earth's magnetic field." ScienceDaily. ScienceDaily, 22 November 2013. .Helmholtz Centre Potsdam - GFZ German Research Centre for Geosciences. (2013, November 22). Satellite trio to explore the Earth's magnetic field. ScienceDaily. Retrieved February 1, 2014 from www.sciencedaily.com/releases/2013/11/131122103703.htmHelmholtz Centre Potsdam - GFZ German Research Centre for Geosciences. "Satellite trio to explore the Earth's magnetic field." ScienceDaily. www.sciencedaily.com/releases/2013/11/131122103703.htm (accessed February 1, 2014).

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