mardi 10 décembre 2013

NASA's Juno Gives Starship-Like View of Earth Flyby












NASA - JUNO Mission logo.

Dec. 10, 2013

Juno Spacecraft Listens for a Greeting From Earth

Video above: This cosmic pirouette of Earth and our moon was captured by the Juno spacecraft as it flew by Earth on Oct. 9, 2013. Image Credit: NASA/JPL-Caltech.

When NASA’s Juno spacecraft flew past Earth on Oct. 9, 2013, it received a boost in speed of more than 8,800 mph (about 7.3 kilometer per second), which set it on course for a July 4, 2016, rendezvous with Jupiter, the largest planet in our solar system. One of Juno's sensors, a special kind of camera optimized to track faint stars, also had a unique view of the Earth-moon system. The result was an intriguing, low-resolution glimpse of what our world would look like to a visitor from afar.

"If Captain Kirk of the USS Enterprise said, ‘Take us home, Scotty,’ this is what the crew would see," said Scott Bolton, Juno principal investigator at the Southwest Research Institute, San Antonio. “In the movie, you ride aboard Juno as it approaches Earth and then soars off into the blackness of space. No previous view of our world has ever captured the heavenly waltz of Earth and moon."

The Juno Earth flyby movie is available at: http://www.youtube.com/watch?v=_CzBlSXgzqI&feature=youtu.be . The music accompaniment is an original score by Vangelis.

The cameras that took the images for the movie are located near the pointed tip of one of the spacecraft's three solar-array arms. They are part of Juno's Magnetic Field Investigation (MAG) and are normally used to determine the orientation of the magnetic sensors. These cameras look away from the sunlit side of the solar array, so as the spacecraft approached, the system's four cameras pointed toward Earth. Earth and the moon came into view when Juno was about 600,000 miles (966,000 kilometers) away -- about three times the Earth-moon separation.


video above: The Waves instrument aboard NASA's Juno spacecraft recorded amateur radio signals from ham radio operators from around the world. Image Credit: NASA/JPL-Caltech/University of Iowa.

During the flyby, timing was everything. Juno was traveling about twice as fast as a typical satellite, and the spacecraft itself was spinning at 2 rpm. To assemble a movie that wouldn't make viewers dizzy, the star tracker had to capture a frame each time the camera was facing Earth at exactly the right instant. The frames were sent to Earth, where they were processed into video format.

"Everything we humans are and everything we do is represented in that view," said the star tracker's designer, John Jørgensen of the Danish Technical University, near Copenhagen.

Also during the flyby, Juno's Waves instrument, which is tasked with measuring radio and plasma waves in Jupiter's magnetosphere, recorded amateur radio signals. This was part of a public outreach effort involving ham radio operators from around the world. They were invited to say "HI" to Juno by coordinating radio transmissions that carried the same Morse-coded message. Operators from every continent, including Antarctica, participated.

"With the Earth flyby completed, Juno is now on course for arrival at Jupiter on July 4, 2016," said Rick Nybakken, Juno project manager at NASA's Jet Propulsion Laboratory in Pasadena, Calif.

Junos Two Deep Space Maneuvers are Back To Back Home Runs

The Juno spacecraft was launched from Kennedy Space Center in Florida on August 5, 2011. Juno’s launch vehicle was capable of giving the spacecraft only enough energy to reach the asteroid belt, at which point the sun’s gravity pulled it back toward the inner solar system. Mission planners designed the swing by Earth as a gravity assist to increase the spacecraft’s speed relative to the sun, so that it could reach Jupiter. (The spacecraft’s speed relative to Earth before and after the flyby is unchanged.)

After Juno arrives and enters into orbit around Jupiter in 2016, the spacecraft will circle the planet 33 times, from pole to pole, and use its collection of science instruments to probe beneath the gas giant's obscuring cloud cover. Scientists will learn about Jupiter's origins, internal structure, atmosphere and magnetosphere.

Juno's name comes from Greek and Roman mythology. The god Jupiter drew a veil of clouds around himself to hide his mischief from his wife, but the goddess Juno used her special powers to peer through the clouds and reveal Jupiter's true nature.

NASA's Jet Propulsion Laboratory, Pasadena, Calif., manages the Juno mission for the principal investigator, Scott Bolton, of Southwest Research Institute in San Antonio. The Juno mission is part of the New Frontiers Program managed at NASA's Marshall Space Flight Center in Huntsville, Ala. Lockheed Martin Space Systems, Denver, built the spacecraft. JPL is a division of the California Institute of Technology in Pasadena.

More information about Juno is online at: http://www.nasa.gov/juno and http://missionjuno.swri.edu

Image, Videos (mentioned), Credits: NASA / Steve Cole / JPL / DC Agle.

Best regards, Orbiter.ch

lundi 9 décembre 2013

NASA-USGS Landsat 8 Satellite Pinpoints Coldest Spots on Earth












NASA / USGS - Landsat 8 LDCM Mission patch.

Dec. 9, 2013

What is the coldest place on Earth? It is a high ridge in Antarctica on the East Antarctic Plateau where temperatures in several hollows can dip below minus 133.6 degrees Fahrenheit (minus 92 degrees Celsius) on a clear winter night.

Scientists made the discovery while analyzing the most detailed global surface temperature maps to date, developed with data from remote sensing satellites including the new Landsat 8, a joint project of NASA and the U.S. Geological Survey (USGS). Ted Scambos, lead scientist at the National Snow and Ice Data Center in Boulder, Colo., joined a team of researchers reporting the findings Monday at the American Geophysical Union meeting in San Francisco.

The Coldest Place in the World

Video above: The coldest place on earth is in the East Antarctic Plateau, but not at the highest peak. Rather, the coldest spots develop just downhill from a ridge that runs from Dome A to Dome Fuji. Data from NASA-USGS Landsat 8 satellite, and NASA's MODIS sensor on the Aqua satellite. Video Credit: NASA's Goddard Space Flight Center.

Researchers analyzed 32 years' worth of data from several satellite instruments. They found temperatures plummeted to record lows dozens of times in clusters of pockets near a high ridge between Dome Argus and Dome Fuji, two summits on the ice sheet known as the East Antarctic Plateau. The new record of minus 136 F (minus 93.2 C) was set Aug. 10, 2010.

That is several degrees colder than the previous low of minus 128.6 F (minus 89.2 C), set in 1983 at the Russian Vostok Research Station in East Antarctica. The coldest permanently inhabited place on Earth is northeastern Siberia, where temperatures in the towns of Verkhoyansk and Oimekon dropped to a bone-chilling 90 degrees below zero Fahrenheit (minus 67.8 C) in 1892 and 1933, respectively.

Landsat 8 LDCM spacecraft. Image Credit: NASA's Goddard Space Flight Center

"We had a suspicion this Antarctic ridge was likely to be extremely cold, and colder than Vostok because it's higher up the hill," Scambos said. "With the launch of Landsat 8, we finally had a sensor capable of really investigating this area in more detail."

The quest to find out just how cold it can get on Earth -- and why -- started when the researchers were studying large snow dunes, sculpted and polished by the wind, on the East Antarctic Plateau. When the scientists looked closer, they noticed cracks in the snow surface between the dunes, possibly created when wintertime temperatures got so low the top snow layer shrunk. This led scientists to wonder what the temperature range was, and prompted them to hunt for the coldest places using data from two types of satellite sensors.

How to Get Colder Than Anywhere Else

Video above: This narrated animation shows the process by which the coldest place on Earth develops its extreme low temperatures. Video Credit: NASA's Goddard Space Flight Center.

They turned to the Moderate Resolution Imaging Spectroradiometer (MODIS) instruments on NASA's Terra and Aqua satellites and the Advanced Very High Resolution Radiometer (AVHRR) on several National Oceanic and Atmospheric Administration satellites. These sensitive instruments can pick up thermal radiation emitted from Earth's surface, even in areas lacking much heat.

Using these sensors to scan the East Antarctic Plateau, Scambos detected extremely cold temperatures on a 620-mile stretch of the ridge at high elevations between Argus and Fuji, and even colder temperatures lower elevations in pockets off the ridge. Then, with the higher resolution of the Thermal Infrared Sensor (TIRS) aboard Landsat 8, the research team pinpointed the record-setting pockets.

The team compared the sites to topographic maps to explore how it gets so cold. Already cold temperatures fall rapidly when the sky clears. If clear skies persist for a few days, the ground chills as it radiates its remaining heat into space. This creates a layer of super-chilled air above the surface of the snow and ice. This layer of air is denser than the relatively warmer air above it, which causes it to slide down the shallow slope of domes on the Antarctic plateau. As it flows into the pockets, it can be trapped, and the cooling continues.

"By causing the air to be stationary for extended periods, while continuing to radiate more heat away into space, you get the absolute lowest temperatures we're able to find," Scambos said. "We suspected that we would be looking for one magical site that got extremely cold, but what we found was a large strip of Antarctica at high altitude that regularly reached these record low temperatures."

The study is an example of some of the intriguing science possible with Landsat 8 and the TIRS instrument, which was built at NASA’s Goddard Space Flight Center in Greenbelt, Md. Since its launch Feb. 11, Landsat 8 has captured approximately 550 scenes per day of Earth's land surface. USGS processes, archives and distributes the images free of charge over the Internet.


Image above: With remote-sensing satellites, scientists have found the coldest places on Earth, just off a ridge in the East Antarctic Plateau. The coldest of the cold temperatures dropped to minus 135.8 F (minus 93.2 C) -- several degrees colder than the previous record. Image Credit: Ted Scambos, National Snow and Ice Data Center.

"With Landsat 8, we expect to see more accurate and more detailed maps of the landscape than we've ever been able to see," said James Irons, the mission's project scientist at Goddard. "If change is occurring, I think we'll be able to detect it earlier and track it."

Researchers also are eager to see what new results come out of Landsat 8, both from icy plateaus and Earth's warmer regions.

"What we've got orbiting Earth right now is a very accurate and consistent sensor that can tell us all kinds of things about how the land surface of Earth is changing, how climate change is impacting the surface of Earth, the oceans of Earth, and the icy areas of Earth," Scambos said. "Finding the coldest areas on Earth is just the beginning of the discoveries we're going to be able to make with Landsat 8."

Related Link:

NASA's Landsat 8 website: http://www.nasa.gov/landsat

Images (mentioned), Videos (mentioned), Text, Credit: NASA.

Greetings, Orbiter.ch

NASA Rover Results Include First Age Measurement on Mars and Help for Human Exploration










NASA - Mars Science Laboratory (MSL) logo.

Dec. 9, 2013

Erosion by Scarp Retreat in Gale Crater

Image above: This mosaic of images from the Mast Camera (Mastcam) instrument on NASA's Curiosity Mars rover shows a series of sedimentary deposits in the Glenelg area of Gale Crater, from a perspective in Yellowknife Bay looking toward west-northwest. Image Credit: NASA/JPL-Caltech/MSSS.

NASA's Curiosity rover is providing vital insight about Mars' past and current environments that will aid plans for future robotic and human missions.

In a little more than a year on the Red Planet, the mobile Mars Science Laboratory has determined the age of a Martian rock, found evidence the planet could have sustained microbial life, taken the first readings of radiation on the surface, and shown how natural erosion could reveal the building blocks of life. Curiosity team members presented these results and more from Curiosity in six papers published online today by Science Express and in talks at the Fall Meeting of the American Geophysical Union in San Francisco.

Possible Extent of Ancient Lake in Gale Crater, Mars

Image above: This illustration depicts a concept for the possible extent of an ancient lake inside Gale Crater. Image Credit: NASA/JPL-Caltech/MSSS.

The Age of  'Cumberland'

The second rock Curiosity drilled for a sample on Mars, which scientists nicknamed "Cumberland," is the first ever to be dated from an analysis of its mineral ingredients while it sits on another planet. A report by Kenneth Farley of the California Institute of Technology in Pasadena, and co-authors, estimates the age of Cumberland at 3.86 billion to 4.56 billion years old. This is in the range of earlier estimates for rocks in Gale Crater, where Curiosity is working.

"The age is not surprising, but what is surprising is that this method worked using measurements performed on Mars," said Farley. "When you're confirming a new methodology, you don't want the first result to be something unexpected. Our understanding of the antiquity of the Martian surface seems to be right."

The analysis of Cumberland from a sample drilled by Curiosity was a fundamental and unprecedented measurement considered unlikely when the rover landed in 2012. Farley and his co-authors adapted a 60-year-old radiometric method for dating Earth rocks that measures the decay of an isotope of potassium as it slowly changes into argon, an inert gas. Argon escapes when a rock is melted. This dating method measures the amount of argon that accumulates when the rock hardens again.

Before they could measure rocks directly on Mars, scientists estimated their ages by counting and comparing the numbers of impact craters on various areas of the planet. The crater densities are correlated with ages based on comparisons with crater densities on the moon, which were tied to absolute dates after  the Apollo lunar missions returned rocks to Earth.

Farley and co-authors also assessed how long Cumberland has been within about an arm's reach of the Martian surface, where cosmic rays that hit atoms in the rock produce gas buildups that Curiosity can measure.

View of Yellowknife Bay Formation, with Drilling Sites

Image above: This mosaic of images from Curiosity's Mast Camera (Mastcam) shows geological members of the Yellowknife Bay formation, and the sites where Curiosity drilled into the lowest-lying member, called Sheepbed, at targets "John Klein" and "Cumberland." Image Credit: NASA/JPL-Caltech/MSSS.

Analyses of three different gases yielded exposure ages in the range of 60 million to 100 million years. This suggests shielding layers above the rock were stripped away relatively recently. Combined with clues of wind erosion Curiosity observed, the exposure-age discovery points to a pattern of windblown sand chewing away at relatively thick layers of rock. The eroding layer forms a retreating vertical face, or scarp.

"The exposure rate is surprisingly fast," Farley said. "The place where you'll find the rocks with the youngest exposure age will be right next to the downwind scarps."

From Rocks to Building Blocks?

Finding rocks with the youngest exposure age is important in the mission's investigations of whether organic chemicals are preserved from ancient environments. Organic chemicals are building blocks for life, although they also can be produced without any biology.

"We're making progress on the path to determining whether there are Martian organics in there," Doug Ming, of NASA's Johnson Space Center, Houston, said of the Cumberland rock sample. "We detect organics but can't rule out that they might be brought along from Earth." Curiosity detected higher amounts in Cumberland than it did in in either test runs with Martian soil samples or analysis of empty sample cups. Increasing the amount of rock powder in the test cup increased the amount of organic content detected.

Favorable for Life

Ming is the lead author of a new report about a site called "Yellowknife Bay." The team reported 10 months ago that the first rock Curiosity drilled there, nicknamed "John Klein," yielded evidence that met the mission's goal of identifying a Martian environment favorable for microbial life long ago. Yellowknife Bay's clay-rich lakebed habitat offers the key chemical elements for life, plus water not too acidic or salty, and an energy source. The energy source is a type used by many rock-eating microbes on Earth: a mix of sulfur- and iron-containing minerals that are ready acceptors of electrons, and others that are ready electron donors, like the two poles of a battery.

Not only has Curiosity accomplished its primary goal of finding evidence for an ancient environment that could have supported life, but it also has provided evidence habitable conditions existed more recently than expected and likely persisted for millions of years.

 Mars Science Laboratory (MSL) "Curiosity" rover. Image Credit: NASA/JPL-Caltech

Additional new results from Curiosity are providing the first readings of radiation hazards at Mars' surface, which will aid planning of human missions to Mars. Other findings will guide the search for evidence of life on Mars by improving insight about how erosion may expose buried clues of molecular building blocks of life.

New estimates of when habitable conditions existed at Yellowknife Bay and how long they persisted come from details of rocks' composition and layering. It is thought that Mars had enough fresh water to generate clay minerals -- and possibly support life -- more than 4 billion years ago, but that the planet underwent drying that left any remaining liquid water acidic and briny. A key question was whether the clay minerals at Yellowknife Bay formed earlier, upstream on the rim of Gale Crater where the bits of rock originated, or later, downstream where the rock particles were carried by water and deposited.

Scott McLennan of Stony Brook University in Stony Brook, N.Y., and co-authors found that chemical elements in the rocks indicate the particles were carried from their upstream source area to Yellowknife Bay and that most chemical weathering occurred after they were deposited. The loss of elements that leach easily, such as calcium and sodium, would be noticeable if the weathering that turns some volcanic minerals into clay minerals had happened upstream. Scientists did not notice such leaching.

David Vaniman of the Planetary Science Institute in Tucson, Ariz., and co-authors found supporting evidence in a separate mineral analysis of sedimentary rocks at Yellowknife Bay. They noticed a lack of olivine and an abundance of magnetite, which suggests the rocks turned to clay after they washed downstream. The presence of smectite tells about conditions where the clay formed.

"Smectite is the typical clay mineral in lake deposits," Vaniman said. "It is commonly called a swelling clay -- the kind that sticks to your boot when you step in it. You find biologically rich environments where you find smectites on Earth."

John Grotzinger of Caltech and co-authors examined physical characteristics of rock layers in and near Yellowknife Bay and concluded the habitable environment there existed at a time "relatively young by Martian standards." It was a part of Martian history called the Hesperian Era, when parts of the planet were already becoming drier and more acidic, less than 4 billion years ago and roughly the same time as the oldest evidence for life on Earth.

"This habitable environment existed later than many people thought there would be one," Grotzinger said. "This has global implications. It's from a time when there were deltas, alluvial fans and other signs of surface water at many places on Mars, but those were considered too young, or too short-lived, to have formed clay minerals. The thinking was, if they had clay minerals, those must have washed in from older deposits. Now, we know the clay minerals could be produced later, and that gives us many locations that may have had habitable environments, too."

Research suggests habitable conditions in the Yellowknife Bay area may have persisted for millions to tens of millions of years. During that time rivers and lakes probably appeared and disappeared. Even when the surface was dry, the subsurface likely was wet, as indicated by mineral veins deposited by underground water into fractures in the rock. The thickness of observed and inferred tiers of rock layers provides the basis for estimating long duration, and the discovery of a mineral energy source for underground microbes favors habitability throughout.

Implications for Human Explorers

Today's reports include the first measurements of the natural radiation environment on the surface of Mars. Cosmic rays from outside our solar system and energetic particles from the sun bombarded the surface at Gale Crater with an average of 0.67 millisieverts per day from August 2012 to June 2013, according to a report by Don Hassler of Southwest Research Institute in Boulder, Colo., and co-authors. For comparison, radiation exposure from a typical chest X-ray is about 0.02 millisievert. That 10-month measurement period did not include any major solar storms affecting Mars, and more than 95 percent of the total came from cosmic rays.

Results from the surface-radiation monitoring provide an additional piece of the puzzle for projecting the total round-trip radiation dose for a future human mission to Mars. Added to dose rates Curiosity measured during its flight to Mars, the Mars surface results project a total round-trip dose rate for a future human mission at the same period in the solar cycle to be on the order of 1,000 millisieverts.

Long-term population studies have shown exposure to radiation increases a person’s lifetime cancer risk. Exposure to a dose of 1,000 millisieverts is associated with a 5 percent increase in risk for developing fatal cancer. NASA's current career limit for increased risk for its astronauts currently operating in low-Earth orbit is 3 percent. The agency is working with the Institute of Medicine of the National Academies to address the ethics, principles and guidelines for health standards for long duration and exploration spaceflight missions.

Mars Human Exploration. Image Credit: Voyage to Planets, BBC

The radiation detected by Curiosity is consistent with earlier predictions. The new data will help NASA scientists and engineers create better models to anticipate the radiation environment human explorers will face, as the agency develops new technologies to protect astronauts in deep space.

"Our measurements provide crucial information for human missions to Mars," Hassler said. "We're continuing to monitor the radiation environment and seeing the effects of major solar storms on the surface at different times in the solar cycle, will give additional important data. Our measurements also tie into Curiosity's investigations about habitability. The radiation sources that are concerns for human health also affect microbial survival as well as preservation of organic chemicals."

If any organic chemicals that are potential signs of life did exist within rocks at about 2 inches (5 centimeters), the depth of Curiosity's drill, Hassler estimated they would be depleted up to 1,000-fold in about 650 million years by radiation at the exposure rate measured in Curiosity's first 10 months. However, the Cumberland rock that Curiosity sampled with its drill at Yellowknife Bay had been exposed to cosmic rays' effects for only about 60 million to 100 million years, by Farley's estimate. Researchers calculate that, with such a young exposure age, enough organic material could still be present in Cumberland to be detectable. Even if Mars has never supported life, the planet receives organic molecules delivered by meteorites, which should leave a detectable trace.

NASA's Jet Propulsion Laboratory built Curiosity and manages the mission for NASA's Science Mission Directorate, Washington.

For more information about the mission, visit: http://www.nasa.gov/msl and http://mars.jpl.nasa.gov/msl

Images (mentioned), Text, Credits: NASA / Dwayne Brown / JPL / Guy Webster.

Greetings, Orbiter.ch

CryoSat measures European storm surge







ESA - CRYOSAT 2 Mission logo.

9 December 2013

ESA’s CryoSat satellite measured the storm surge from the recent North Sea storms, as high waters passed through the Kattegat sea between Denmark and Sweden.

During 5–6 December, a major storm passed through northern Europe causing flooding, blackouts, grounding flights and bringing road, rail and sea travel to a halt.

Since the storm coincided with a period of high tides in the North Sea, there were extremely high sea levels – a ‘storm surge’. In the UK, sea levels were at their highest since the 1953 North Sea Floods, while in Germany, parts of Hamburg were flooded.

Measuring the storm surge

On Friday night, CryoSat passed over Kattegat, providing an estimate of total water levels. The observations matched predictions, helping to confirm these models.

The measurements were made by CryoSat’s radar altimeter that – although designed to measure sea-ice thickness – is providing outstanding results over sea and, especially, coastal areas.

Until recently, altimeter measurements of sea-level height could only be made over open oceans because of land interference closer to the coast. In the last few years, however, progress has been made in reducing these effects, also thanks to the new generation of radar altimeters being heralded by CryoSat. This has allowed scientists not only to map water levels closer to the coast, but also profile land surfaces and inland water targets such as small lakes, rivers and their intricate tributaries.

Kattegat

Altimeter measurements from space can be used to validate storm surge models as well as provide near-realtime information that can be incorporated into predictions. Under ESA’s Data User Element, the eSurge project is helping to optimise the use of altimetry and other types of satellite data to improve storm surge forecasting.

The importance of realistic storm surge models was recently demonstrated by the devastation caused by Typhoon Haiyan in south Asia, where over 5900 people lost their lives in the Philippines alone.

CryoSat 2

“Even a small improvement to a storm surge model can have a significant impact in terms of the accuracy of warnings, and the potential to protect lives and property,” noted Kevin Horsburgh from the UK’s National Oceanography Centre.

The upcoming Sentinel-3 mission being developed for Europe’s Copernicus programme will carry altimeters similar to those on CryoSat, delivering more input for applications such as predicting storm surges.

Related links:

eSurge: http://www.storm-surge.info/

Data User Element: http://dup.esrin.esa.it/

National Oceanography Centre: http://noc.ac.uk/

Related mission:

CryoSat: http://www.esa.int/Our_Activities/Observing_the_Earth/CryoSat

Sentinel-3: http://www.esa.int/Our_Activities/Observing_the_Earth/Copernicus/Sentinel-3

Images, Text, Credits: ESA / NOC / AOES Medialab.

Greetings, Orbiter.ch

The Sun Reverses its Magnetic Poles











NASA logo.

Dec. 9, 2013

The Sun Reverses its Magnetic Poles

This visualization shows the position of the sun's magnetic fields from January 1997 to December 2013. The field lines swarm with activity: The magenta lines show where the sun's overall field is negative and the green lines show where it is positive. A region with more electrons is negative, the region with less is labeled positive. Additional gray lines represent areas of local magnetic variation.

The entire sun's magnetic polarity, flips approximately every 11 years -- though sometimes it takes quite a bit longer -- and defines what's known as the solar cycle. The visualization shows how in 1997, the sun shows the positive polarity on the top, and the negative polarity on the bottom. Over the next 12 years, each set of lines is seen to creep toward the opposite pole eventually showing a complete flip. By the end of the movie, each set of lines are working their way back to show a positive polarity on the top to complete the full 22 year magnetic solar cycle.

At the height of each magnetic flip, the sun goes through periods of more solar activity, during which there are more sunspots, and more eruptive events such as solar flares and coronal mass ejections, or CMEs. The point in time with the most sunspots is called solar maximum. Video Credit: NASA/GSFC/PFSS.

Video (mentioned), Text, Credit: NASA.

Cheers, Orbiter.ch

IRIS Provides Unprecedented Images of Sun










NASA - IRIS Mission patch.

Dec. 9, 2013


Image above: The fine detail in images of prominences in the sun's atmosphere from NASA's Interface Region Imaging Spectrometer – such as the red swirls shown here – are challenging the way scientists understand such events. Image Credit: NASA/LMSAL/IRIS.

The region located between the surface of the sun and its atmosphere has been revealed as a more violent place than previously understood, according to images and data from NASA's newest solar observatory, the Interface Region Imaging Spectrograph, or IRIS.

Solar observatories look at the sun in layers. By capturing light emitted by atoms of different temperatures, they can focus in on different heights above the sun's surface extending well out into the solar atmosphere, the corona. On June 27, 2013, IRIS, was launched, to study what's known as the interface region – a layer between the sun's surface and corona that previously was not well observed.

Over its first six months, IRIS has thrilled scientists with detailed images of the interface region, finding even more turbulence and complexity than expected. IRIS scientists presented the mission's early observations at a press conference at the Fall American Geophysical Union meeting on Dec. 9, 2013.

"The quality of images and spectra we are receiving from IRIS is amazing," said Alan Title, IRIS principal investigator at Lockheed Martin in Palo Alto, Calif. "And we're getting this kind of quality from a smaller, less expensive mission, which took only 44 months to build."

For the first time, IRIS is making it possible to study the explosive phenomena in the interface region in sufficient detail to determine their role in heating the outer solar atmosphere. The mission’s observations also open a new window into the dynamics of the low solar atmosphere that play a pivotal role in accelerating the solar wind and driving solar eruptive events.

Tracking the complex processes in the interface region requires instrument and modeling capabilities that are only now within our technological reach. IRIS captures both images and what's known as spectra, which display how much of any given wavelength of light is present. This, in turn, corresponds to how much material in the solar atmosphere is present at specific velocities, temperatures and densities. IRIS's success is due not only to its high spatial and temporal resolution, but also because of parallel development of advanced computer models. The combined images and spectra have provided new imagery of a region that was always known to be dynamic, but shows it to be even more violent and turbulent than imagined.

"We are seeing rich and unprecedented images of violent events in which gases are accelerated to very high velocities while being rapidly heated to hundreds of thousands of degrees," said Bart De Pontieu, the IRIS science lead at Lockheed Martin. "These types of observations present significant challenges to current theoretical models."


Image above: Artist's concept of the Interface Region Imaging Spectrograph, or IRIS, satellite in orbit. Image Credit: NASA.

DePontieu has been culling images of two particular types of events on the sun that have long been interesting to scientists. One is known as a prominence, which are cool regions within the interface region that appear as giant loops of solar material rising up above the solar surface. When these prominences erupt they lead to solar storms that can reach Earth. IRIS shows highly dynamic and finely structured flows sweeping throughout the prominence.

The second type of event is called a spicule, which are giant fountains of gas – as wide as a state and as long as Earth – that zoom up from the sun's surface at 150,000 miles per hour. Spicules may play a role in distributing heat and energy up into the sun's atmosphere, the corona. IRIS imaging and spectral data allows us to see at high resolution, for the first time, how the spicules evolve. In both cases, observations are more complex than what existing theoretical models predicted.

"We see discrepancies between these observations and the models and that is great news for advancing knowledge," said Mats Carlsson, an astrophysicist at the University of Oslo in Norway. "By seeing something we don't understand we have a chance of learning something new."

Carlsson helps support the crucial computer model component of IRIS' observations. The computer models require an intense amount of power. Modeling just an hour of events on the sun can take several months of computer time. IRIS relies on supercomputers at NASA's Ames Research Center in Moffett Field, Calif., the Norwegian supercomputer collaboration and the Partnership for Advanced Computing in Europe.

Such computer models had helped design the IRIS instruments by providing a basis for the instrument performance requirements. Currently, they are used for analysis of IRIS data, as they represent the state of knowledge about what scientists understand about the interface region. By comparing models with actual observations, researchers figure out where the models fail, and therefore where the current state of knowledge is not complete.

By filling in these gaps, IRIS observations are helping round out our images of the solar atmosphere. The Japanese Aerospace Exploration Agency/NASA Hinode mission provides detailed imagery of the solar surface. NASA's Solar Dynamics Observatory offers imagery of what's higher up in the corona. Now, IRIS provides unprecedented information about the crucial layer in between, to finally help us understand how energy moves through the lower levels of the solar atmosphere driving the solar wind and heating the corona.

The IRIS Observatory was designed and the mission is managed by Lockheed Martin. The Harvard-Smithsonian Center for Astrophysics in Cambridge, Mass., built the telescope. Montana State University in Bozeman, Mont. designed the spectrograph. NASA Ames provides mission operations and ground data systems. NASA's Goddard Space Flight Center, in Greenbelt, Md. manages the Small Explorer Program for NASA's Science Mission Directorate in Washington, D.C. The Norwegian Space Centre is providing regular downlinks of science data. Other contributors include the University of Oslo and Stanford University in Stanford, Calif.

For more information about IRIS, visit: http://www.nasa.gov/iris

Images (mentioned), Text, Credits: NASA's Goddard Space Flight Center / Karen C. Fox.

Best regards, Orbiter.ch

Long March 4B launch failure with CBERS-3












CASC - China Aerospace Science and Technology Corporation logo.

Dec. 9, 2013

 Long March 4B launch with CBERS-3

CBERS-3, the latest Earth resources satellite of the long-running China–Brazil Earth Resources Satellite program between the Chinese and Brazilian space agencies, was launched on a Long March 4B rocket earlier today at 03:26 UTC.

For some yet-to-be-determined reason the satellite did not reach orbit despite separating from the rocket 12 minutes after liftoff. This is the first launch failure of the Long March 4 series since its debut in 1988 - 34 launches earlier. If the similar Long March 2D is also counted (also built in Shanghai like the LM-4 series) this is its first failure in 55 launches.

Already running at least 3 years late due to electric system problems, this should have some impact on the Brazilian space program with the gap on its Earth resources program further lengthened to 2015 (when the similar CBERS-4 is planned to launch); although impact on the Chinese should not be significant with several similar satellites already up and running in orbit.

However, despite initial news of a launch success, the Chinese media are now claiming the launch vehicle suffered a problem during ascent, failed to insert the satellite into its required orbit, leading to the satellite being classed as lost and potentially re-entering Earth’s atmosphere.

China-Brazil Earth Resources Satellite (CBERS 3)

No specific information has been provided by the Chinese media other than the mission failed. This came several hours after the Brazilians published the launch was successful.

The Brazilians have since claimed the spacecraft was inserted into an orbit much lower than required due to the unknown problem with the Long March 4B. The spacecraft apparently communicated for 15 minutes before falling silent, potentially – as is being claimed – as it began to re-enter Earth’s atmosphere.

More will follow when information is available (video).

For more information about China Aerospace Science and Technology Corporation (CASC), visit: http://www.spacechina.com/n25/jtindex.html

Images, Text, Credits: CASC / Orbiter.ch Aerospace.

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