The Sun’s Conveyor Belt May Lengthen Solar Cycles

The conveyor belt of the Sun - a large flow of plasma that circulates under the surface - may be responsible for the duration of solar cycles. Image Credit: Science@NASA

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The Sun seems to finally be waking up in earnest from the long slumber of the past cycle. Solar cycles tend to last on average about 11 years, but the last cycle – solar cycle 23 – was 12.5 years long. The cause of the most recent lull in the Sun’s activity is somewhat enigmatic, but it may be explained by the “conveyor belt” of plasma that circulates in the Sun’s chromosphere and photosophere. Just how far this conveyor belt of plasma extends underneath the Sun may heavily influence the duration of solar cycles.

In a recent paper published in Geophysical Research Letters, Dr. Mausumi Dikpati of the High Altitude Observatory National Center for Atmospheric Research in Boulder, Colorado and her team modeled data from the Mount Wilson Observatory for the duration of the last solar cycle. When they analyzed and modeled surface Doppler measurements of the flow of plasma currents that course underneath the surface of the Sun, they discovered that the flow extended all the way to the poles.

This is in contrast to data from previous, average-length solar cycles, in which the meridional plasma flow – or the Sun’s conveyor belt – flowed only to about 60 degrees latitude. This flow is not unlike thermohaline circulation here on Earth, in which the ocean transports heat around the globe.

Dr. Dikpati said in an email interview, “This is the first time that the Sun’s conveyor-belt has been measured accurately enough for two consecutive cycles (cycles 22 spanning approximately 1986-1996.5 and cycle 23 spanning 1996.5-2009). From these data we now know that cycle 22 had a shorter conveyor-belt reaching only to 60-degree latitude, while cycle 23 had a long conveyor-belt extending all the way to the pole.”

The cycles of the Sun are intricately linked to the magnetic field permeating our nearest star. Gigantic loops of the magnetic field of the Sun are what cause sunspots, and as the contours of the magnetic field change over the cycle of the Sun, more or fewer sunspots are seen, as well as solar flares and other activity. There is always a lack of sunspots between the cycles, but the minimum at the end of cycle 23 was unusually long.

The conveyor belt of plasma flowing in the chromosphere and photosphere essentially drags along with it the magnetic flux of the Sun. Because the extent of the conveyor belt reached a higher latitude, it took the magnetic flux longer to return to the equator, resulting in the delay of sunspots marking the onset of cycle 24.

Dr. Dikpati and her team determined that it wasn’t the speed of the flow of plasma conveyor belt that lengthened the solar cycle, but the extent into higher latitudes, and slower return to the equator. Though the speed of the conveyor belt was a bit higher than usual over the past five years, it also stretched much further than during a normal cycle.

Dr. Dikpati said of using data from previous solar cycles to better refine their model of the conveyor belt:

From the same data source (Mount Wilson data from Roger Ulrich) there is evidence of a short conveyor-belt in cycles 19, 20 and 21 also. All these cycles had periods (10.5 years) like cycle 22. Back beyond that we are hoping that others in the community will search for evidence of the latitudinal extent of the conveyor-belt in even earlier cycles. In fact, theory of the conveyor-belt in high-latitudes indicates that a shorter conveyor belt should be more common in the Sun, rather this long conveyor belt in cycle 23 may be the exception. There is already evidence from Mount Wilson data that, at the start of cycle 24, the conveyor-belt is shortening again, suggesting that cycle 24 is going to be more like cycles 19 – 22 in length.

By getting a better model of the interplay between the plasma flow and the Sun’s magnetic field, solar scientists may be able to better predict and explain the length of future and past solar cycles.

Dr. Dikpati said, “The conveyor belt also governs the memory of the Sun about its past magnetic features. This is an important ingredient for building prediction models for solar cycles.”

Source: Geophysical Research Letters, email interview with Dr. Mausumi Dikpati

Solar Storm Update: Best Times for Viewing Aurorae

Why is the Sun So Hot?
Image from the Solar Dynamics Observatory of the filaments coming from the Sun's surface. Credit: NASA

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The Harvard Smithsonian Center for Astrophysics released the latest information on the July 31/August 1 activity on the Sun that is just now reaching Earth. They predict we’ll have multiple opportunities for a display of the Northern Lights over the next two days. The latest word from the solar scientists is that the Sun erupted not just once, but four times. All four coronal mass ejections are headed toward Earth.

Space weather forecasts are even more challenging than regular weather forecasts, said Dr. Leon Golub, and a coronal mass ejection is like a hurricane: it’s large and fuzzy, and doesn’t always move at the same speed. Currently, the estimated arrival times are:

Wednesday, Aug. 4 – 3:00 a.m. EDT (0700 GMT on Aug. 5; aurorae not visible in daylight)
Wednesday, Aug. 4 – 1:00 p.m. EDT (1600 GMT, again the daylight issue)
Wednesday, Aug. 4 – 8:00 p.m. EDT (0000 GMT on Aug. 5)
Thursday, Aug. 5 – 2:00 a.m. EDT (0600 GMT)

Any one of these events may or may not generate an aurora. It depends on details like magnetic field orientation. If the magnetic field in the oncoming solar plasma is directed opposite Earth’s magnetic field, the result could be spectacular aurorae. If the fields line up, the coronal mass ejection could slide past our planet with nary a ripple.

The Center for Astrophysics suggested these two resources:

Map of current auroral activity

Chart of proton flux (watch for the numbers to go up as each wave arrives)

Source: Harvard Smithsonian Center for Astrophyics

Aurora Alert! Solar Storm Reaches Earth

Finally, some excitement from the Sun! On August 1, 2010, the entire Earth-facing side of the sun erupted with all sorts of activity. There was a C3-class solar flare, a solar tsunami, multiple filaments of magnetism lifting off the stellar surface, large-scale shaking of the solar corona, radio bursts, a coronal mass ejection (CME) and more. (Watch the movie from the Solar Dynamics Observatory spacecraft for all the action!) As I write this, the solar storm is beginning to reach Earth with one, and possibly two CMEs, according to Spaceweather.com. You can actually watch realtime data coming in from two of the GOES satellites at this link from NOAA’s Space Weather Prediction Center, which measures proton flux in the space environment around Earth. The page refreshes every 5 minutes.
Continue reading “Aurora Alert! Solar Storm Reaches Earth”

July 11 Total Eclipse Among the Mysterious Moai

The Moai statues on Easter Island.

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A group of astronomers are now on the mysterious Easter Island, one of the few solid places to stand on Earth where a total solar eclipse will be visible on July 11, 2010. The majority of the eclipse’s path is over the ocean, so this will be one of the least observed eclipses ever. “This is one of the most interesting things that is possible for anyone on Earth to see in one of the most interesting places on the Earth that people can go,” said Jay Pasachoff from Williams College, who is the Chair of the International Astronomical Union’s Working Group on Eclipses. This will be his 51st eclipse.

Williams astronomer Jay Pasachoff during the partial phase of the March 29, 2006 solar eclipse. Photo by Anna Tsykalova.

While the eclipse is thousands of miles long in its is path of totality on Earth, it is just a few hundred miles wide. It will pass through French Polynesia on the Cook Islands, but, Pasachoff said, it doesn’t go through any of the main islands. “It misses Tahiti, but there are some atolls off the side of the path, and some eclipse scientists and ecotourists will be on cruise ships that are going into the path of totality. There will also be a group on an airplane observing the eclipse and we hope to compare all the other observations with the ones we get from Easter Island,” he said.

Easter Island is 4023 km (2,500 miles) west of Chile, and is famous for the Moai, giant statutes that were left by a Polynesian culture that mysteriously disappeared. But while the statues’ constant gaze look outward, all human eyes will be on the skies on July 11.

“The actual four minutes and forty-five seconds of totality that we are scheduled to have at Easter Island will be very exciting, as the last sliver of the sun is covered we can then take off the protective filters we’ve been using,” Pasachoff said, “and look at the next few minutes without any protection because the solar corona is about the same brightness as the full moon and is equally safe to look at. In fact we’ve been having a debate recently about whether we can get a very brief warning on the so-called eclipse glasses that many people use because those glasses are only for when any of the everyday sun is visible. They are so dense that they block the solar corona entirely, and the few people who don’t understand what is going on enough to take those glasses off during totality miss the whole event. There are people who have missed past eclipses by not knowing they had to take their glasses off.”

Pasachoff is joined by Professor Marek Demianski and two students. They will be carrying out high-resolution imaging to look for motions in the corona and to follow the varying magnetic-field configuration in the solar-corona as a function of the solar-activity cycle. Though the sunspot cycle remains in an extreme low, some other indications of solar activity have been increasing and we are eager to see the condition of the low and middle corona. They expect to see motions at least in polar plumes.

Also, they will be using the images to fill in gaps between the observations of the corona on the solar disk taken with NASA’s new Solar Dynamics Observatory and the observations of the outer corona taken with the Naval Research Laboratory’s coronagraph on the Solar and Heliospheric Observatory. Pasachoff and his team have contributed to similar images for the past several eclipses but now will have the improved SDO images as part of their montage. Several of the cameras will be computer controlled using software called Solar Eclipse Maestro written by Xavier Jubier of France.

Universe Today hopes to talk with Pasachoff after the eclipse to hear about his experiences.

The Williams College team is accompanied by a documentary crew filming for National Geographic Channel, and their activities will be covered in a special program entitled Easter Island Eclipse partly pre-recorded and partly expected to have new eclipse footage that will air on the National Geographic Channel on the evening of July 11th, at 11 pm.

Here are some resource Pasachoff provided for the eclipse:

On Sunday, July 11th: total solar eclipse on Easter Island (same time zone as Mountain Time in the US)
Partial eclipse begins 12:40:36 Altitude of Sun: 40°
Totality begins 14:08:30 Altitude of Sun: 40°
Totality ends 14:13:10 Altitude of Sun: 39°
Partial eclipse ends 15:34:16 Altitude of Sun: 32°
Duration of totality: 4 minutes and 40 seconds

Times in UT:
18:40 UT 1st contact
20:08 UT 2nd contact: total eclipse begins
20:13 UT 3rd contact: total eclipse ends

His eclipse site for the International Astronomical Union

Google maps by Xavier Jubier and Fred Espenak

Espenak’s NASA Website, with maps and details

An interactive map

An animation of eclipse phenomena

Also, Pasachoff will talk about the eclipse on the July 10 365 Days of Astronomy podcast.

Here’s a link to USTREAM channel of the eclipse.

Update: I just received a note from Robin Zimmerman at DISH Network, and for those of you who have the DISH Network, there is a special channel, DishEARTH, Ch. 287, that features live 24/7 views of the earth from space and this Sunday the eclipse be shown. Robin said their network will allow people in the US to see the phenomena, live.

And here’s a video from National Geographic:

New Weekly Sun Fix: SDO’s Pick of the Week

View of action on the Sun during this past week. Credit: NASA/SDO team

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Images and data are starting to roll in from the Solar Dynamics Observatory, and the images are nothing short of stunning. So, the SDO website has started a couple of new image gallery features, which will provide a “best of” weekly fix without overloading your Sun senses (and no sunscreen needed!) The first one is Pick of the Week. The image above is the first “pick” and what a pick it is! This SDO close-up shows a filament and active region on the Sun, taken in extreme UV light on May 18, 2010. It shows a dark and elongated filament hovering above the Sun’s surface, with bright regions beneath it. The filaments are cooler clouds of gas that are suspended by tenuous magnetic fields that are often unstable and commonly erupt. This one is estimated to be at least 60 Earth diameters long (about 805,000 km, or 500,000 miles). Wowza!

Click here to see a super-huge full disk image.

See below for another new SDO feature, Hot Shots.

Solar flare on May 17, 2010, as seen by the AIA instrument on SDO. Credit: NASA

Hot Shots will feature some great looking flares. This image from the Atmospheric Imaging Assembly (AIA) instrument shows a solar eruption and a flare. The dark regions show the site of evacuated material from the eruption, and the large magnetic loops were formed during the flare. AIA takes images of the solar atmosphere in multiple wavelengths to study link changes in the surface and how they related to interior changes in the Sun. AIA takes images of the Sun in 10 wavelengths every 10 seconds.

For more see the SDO website.

SDO Wows With ‘First Light’ Images, Videos

A full-disk multiwavelength extreme ultraviolet image of the sun taken by SDO on March 30, 2010. False colors trace different gas temperatures. Reds are relatively cool (about 60,000 Kelvin, or 107,540 F); blues and greens are hotter (greater than 1 million Kelvin, or 1,799,540 F). Credit: NASA
A full-disk multiwavelength extreme ultraviolet image of the sun taken by SDO on March 30, 2010. False colors trace different gas temperatures. Reds are relatively cool (about 60,000 Kelvin, or 107,540 F); blues and greens are hotter (greater than 1 million Kelvin, or 1,799,540 F). Credit: NASA

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NASA’s newest solar satellite is officially open for business and all we can say is, “Wow!” The Solar Dynamics Observatory (SDO) released its “first light’ images on Wednesday, showing incredible views of the sun, with extreme close-ups, never-before-seen detail of material streaming outward from sunspots and high-resolution looks at solar flares across a wide range of ultraviolet wavelength.

“These initial images show a dynamic sun that I had never seen in more than 40 years of solar research,” said Richard Fisher, director of the Heliophysics Division at NASA. “SDO will change our understanding of the sun and its processes, which affect our lives and society. This mission will have a huge impact on science, similar to the impact of the Hubble Space Telescope on modern astrophysics.”

SDO launched in February and has been billed as the “Crown Jewel” of NASA’s fleet of solar observatories. This technologically advanced spacecraft is able to take images of the sun every 0.75 seconds and daily send back about 1.5 terabytes of data to Earth — the equivalent of downloading 380 full-length movies every day. The following graphic compares the capabilities of SDO with other missions and resolutions.

This image compares the relative size of SDO's imagery to that of other missions. Credit: NASA

Serendipitously, shortly after the instruments opened their doors, our recently quiet Sun began to get a little more active. The video below was created from data from the Atmospheric Imaging Assembly, a group of four telescopes designed to photograph the sun’s surface and atmosphere. This data is from March 30, 2010, showing a wavelength band that is centered around 304. This extreme ultraviolet emission line is from singly ionized Helium, or He II, and corresponds to a temperature of about 50,000 degrees Celsius.

This movie captures only a fraction of SDO’s imaging capabilities. It shows the Sun’s magnetic field followed by only four of SDO’s 12 imaging wavebands. You’ll see an eruption, flare, and dimming (dark regions evacuated by the eruption) by observing the event in several different layers of the atmosphere. If you’re wondering why the movie doesn’t show all 12 layers at full resolution it’s because at high-res the movie would be nearly a third of a gigabyte in size.

The Helioseismic and Magnetic Imager maps solar magnetic fields and looks beneath the sun’s opaque surface. HMI was undergoing a series of adjustments when it captured an eclipse of sorts. SDO’s view was partially blocked by the Earth. At the edges of the shadow, the Sun’s shape bends, due to the light’s refraction by the Earth’s atmosphere. SDO will have two “eclipse seasons” each year, when the orbit of SDO will intersect the Sun-Earth line.

For more images and a high-res version of the top image, see the SDO website.

Just remember — this is only the beginning of SDO’s mission!

Source: NASA

Our Sun Gets Active!

This SOHO image shows a huge CME on 4/13/2010. Credit: NASA/ESA/SOHO

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The Sun erupted with one of the biggest prominences in years. This shot from the SOHO spacecraft on April 13, 2010 at 13:13 UT shows a Coronal Mass Ejection from the Sun’s northeastern limb. The massive plasma-filled structure rose up and burst during a ~2 hour period around 0900 UT. Emily Lakdawalla at the Planetary Society blog pointed out that you can watch a movie of the event by going to the “SOHO movie theater” . Just select “LASCO C2” from the “Image Type” menu, then click “Search.” As Emily explained, the movie viewer will automatically grab all the LASCO C2 images from the previous 24 hours and animate them for you. So, if you want to watch the eruption from April 13, and it is a few days later, just put in “2010-04-13” as the start date.

Images of the eruption can also be found at SpaceWeather.com, and Richard Bailey at the Society for Popular Astronomy captured this shot of a detached prominence from the eruption, taken at 9:56 UT.

And there’s more!

The SOHO folks put together a “Pick of the Week” movie from the past week of solar activity, and the STEREO spacecraft captured a nice profile view of spiraling corona loops above an active region after it had just popped off a coronal mass ejection (CME) on April 3, 2010. According to the SOHO website, “Faint clouds of material from the CME can be seen billowing into space at more than a million miles per hour. Right afterwards, magnetic forces trying to reorganize themselves generate a series of white arcs visible in extreme UV light. We are observing not the magnetic fields themselves, but electrically charged atoms spiraling along the field lines. The video clip covers one day of activity.”

So hot its cool!

SDO On Station Transmitting First Data as Solar Science Payloads Open Today

Blast off on Feb 11 of mighty Atlas V rocket and SDO from Pad 41 at Cape Canaveral as viewed from the KSC press site. Credit: Ken Kremer

Video Caption: EVE rediscovered the Van Allen Radiation Belt. These EVE data highlight where the energetic protons are in the inner Van Allen radiation belt. The red dots indicate the highest concentration of protons (lower altitude), and the blue-violet dots represents very little detection of particles (higher altitude of GEO). Visualization by Chris Jeppesen.

Following several precise propulsion burns to circularize its orbit, NASA’s Solar Dynamics Observatory (SDO) has arrived “On Station” and multiple tasks critical to check out of the science instruments are in progress this week, according to Dean Pesnell. Pesnell is the SDO project scientist from NASA’s Goddard Spaceflight Center which built the spacecraft and manages the nearly $1 Billion mission for NASA.

“We reached our final orbit on March 16, 2010”, Pesnell told me in an interview. “The SDO spacecraft is working great and all systems are behaving as expected”. SDO was launched on Feb. 11, 2010 from Cape Canaveral Air Force Station aboard an Atlas V rocket.

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The revolutionary science mission has been dubbed the “crown jewel” of NASA’s Solar Exploration research fleet, joining the twin STEREO spacecraft and SOHO. SDO is equipped with three science instruments (HMI, AIA, and EVE) to explore the Sun and its complex interior mechanisms in unprecedented detail.

Although the doors to the solar science payload will be opened starting just today (March 24), SDO has already managed to transmit its “first data”, Pesnell explained. This bonus science data from Earth’s radiation belt was unexpected he said. The first solar light data will come after the science instruments are fully activated.

SDO Instruments
“One detector in EVE was responding to the protons in the inner Van Allen radiation belt. We spent several orbits going through that part of space and EVE was able to produce a map of the radiation belt,” said Pesnell.

“The amount of proton data was not expected as we were not supposed to spend as much time in the belts as we did. By spending a few extra days in the inner belt the MEGS-P radiometer was able to measure a more complete picture of the radiation belt. It may be the only measurement of the proton fluxes in the inner radiation belt during the extremely low solar activity of the current solar minimum,” added Pesnell.

Check out of the science payload is moving ahead swiftly as planned. “The SDO instruments are working through their initial steps to turning them completely on”, Pesnell explained. A key activity was to “bake out” the instruments to remove any remaining harmful contaminants that could threaten to degrade the quality of the science data.

“CCD decontamination heaters had been turned on for several weeks to allow the instruments to outgas any residual contamination”, according to Pesnell. “During the first 40 days of the mission the instruments kept their CCDs hot with heaters. This prevents water vapor from condensing onto the surfaces of the CCDs while forcing water vapor out of the interior of the instruments. Two instruments, HMI and EVE, have turned off their decontamination heaters while AIA will turn them off next week. Those heaters are being turned off to allow the CCD’s to cool to their normal operating temperatures of about minus 100 C”.

“HMI will open their payload door Wednesday and begin checking out the instrument. EVE is cooling their CCDs getting ready to open their doors on Thursday. AIA will open their doors on Saturday”.

Pesnell mentioned that the SDO team expects to show off the initial data at a telecom in mid-April. “The science data should start to flow in early May, fully calibrated data will show up later. We will discuss the data at the SPD/AAS meeting in Miami, FL at the end of May”.

Van Allen Radiation Belts

SDO will collect a staggering 1.5 terabytes of data per day, equivalent to 380 full length movies per day on a 24/7 basis. “The data will be continuously beamed back to newly built receivers on Earth. We have no onboard recorders since nothing is available to handle such a huge data volume,” said Pesnell. “SDO will transmit 50 times more science data than any other mission in NASA history”.

Test data have already been transmitted via the spacecraft antenna to the receiving station on the ground in New Mexico, confirming that the vital communications systems are operating perfectly.

SDO’s measurements of the Sun’s interior, magnetic field and hot plasma of the solar corona will allow scientists to determine how violent solar events are created which then cause ‘space weather’ that ultimately affects every aspect of life here on Earth. The goal is create better predictions of ‘space weather’ in order to provide early warning to valuable satellites and astronauts operating in space, and to prevent disruption to navigation systems and failures in the power grid.

Rocket firing to raise SDO to its final orbit on March 16, 2010. click to enlarge
SDO was launched into a geosynchronous transfer orbit with an apogee altitude (farthest point from Earth) of 36,000 km (22,000 miles) and a perigee altitude (closest point to Earth) of 2500 km (1600 miles). Over the next 34 days the propulsion module was used to raise the perigee altitude to 36,000 km, with a few small burns to push both apogee and perigee to geosynchronous.

“SDO is in an inclined geosynchronous orbit at the longitude of New Mexico. The inclination of 28 degrees is the natural orbit when launched from Kennedy Space Center. Changing the inclination of an orbit requires a lot of fuel, so this orbit was less expensive than a geostationary orbit,” said Pesnell. This orbit will keep the observatory in constant view of the two newly constructed 18-meter dishes around the clock so that not a single bit of data should be lost.

Nancy Atkinson and Ken Kremer covered the Feb 11, 2010 SDO launch on site at KSC for Universe Today

Read SDO launch report by Nancy Atkinson here.

Read earlier SDO reports by Ken Kremer below, including from on site at the Atlas launch pad

NASA Sun Probe rolled to Pad; 10 hours to Blast off

NASA’s Solar Crown Jewel Bolted atop Atlas Rocket

NASA advanced Solar Observatory nearing February launch; will send IMAX like movies daily

Learn more at the NASA SDO Website

SDO soars to space from the Kennedy Space Center atop Atlas V rocket on Feb 11, 2010 as I observed from the KSC Press Site. Credit: Ken Kremer
Artist's concept of the Solar Dynamics Observatory in Orbit

New Citizen Science Opportunity: Solar Storm Watch

A coronal mass ejection. Credit: Solar Storm Watch

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Sun-worshiper alert! Now you can have the chance to help scientists spot and track solar storms and be involved in the latest solar research. The ‘hottest’ new Citizen Science project from the “Zooniverse” is Solar Storm Watch. Volunteers can spot storms and track their progress as they hurtle across space towards our planet. Your “clicks” and input will help solar scientists better understand these potentially dangerous storms and help to forecast their arrival time at Earth. “The more people looking at our data, the more discoveries we will make,” said Dr. Chris Davis, Project Scientist with the STEREO mission. “We encourage everyone to track these spectacular storms through space. These storms are a potential radiation hazard for spacecraft and astronauts alike and together we hope to provide advanced warning of their arrival at Earth.”

Solar Storm Watch has been in Beta testing for about two months, but is now officially open for business. “It’s been wonderful to watch the team get ready for a flood of data,” said Chris Lintott, one of the founders of the original Galaxy Zoo, and now Zooniverse — new citizen science projects that that use the Galaxy Zoo model — of which Solar Storm Watch is a part. ” I’m sure there are discoveries there already.”

“I’ve been sitting at my desk watching the results roll in and there are plenty of CMEs that just need a few more clicks,” said Arfon Smith from Oxford University, one of the developers of Zooniverse, who has helped solar astronomers at the Royal Observatory in Greenwich integrate their science projects into the Galaxy Zoo model.

STEREO spacecraft. Credit: NASA

The project uses real data from NASA’s STEREO spacecraft, a pair of satellites in orbit around the Sun which give scientists a constant eye on the ever-changing solar surface. STEREO’s two wide-field instruments, the Heliospheric Imagers provide Solar Stormwatch with its data. Each imager has two cameras helping STEREO stare across the 150 million kilometers from the Earth to the Sun.

“The Solar Stormwatch website has a game-like feel without losing any of the science,” said Julia Wilkinson, Solar Stormwatch volunteer. “I can click away identifying features and watch solar storms head towards Earth on the video clips and learn about solar science at the same time. It’s fun, it’s addictive, it’s educational and you get to contribute to real astronomy research without being an expert in astrophysics … The fact that any Solar Stormwatch volunteer could make a brand new discovery about our neighboring star is very cool indeed. All you need is a computer and an interest in finding out more about what the sun is really like. Solar astronomy has never been easier!”

Solar Storm Watch has made their project very interactive with social media, as you can share your discoveries on the user forum and Flickr, as well as follow the space weather forecast on Twitter. SSW also has a blog to shre the latest news and challenges.

To participate, go to the Solar Storm Watch website. You can get a “Mission Briefing”, or watch informative videos on why the solar science community needs you!

Sources: Royal Observatory, Zooniverse

ESA’s Tough Choice: Dark Matter, Sun Close Flyby, Exoplanets (Pick Two)

Thales Alenia Space and EADS Astrium concepts for Euclid (ESA)


Key questions relevant to fundamental physics and cosmology, namely the nature of the mysterious dark energy and dark matter (Euclid); the frequency of exoplanets around other stars, including Earth-analogs (PLATO); take the closest look at our Sun yet possible, approaching to just 62 solar radii (Solar Orbiter) … but only two! What would be your picks?

These three mission concepts have been chosen by the European Space Agency’s Science Programme Committee (SPC) as candidates for two medium-class missions to be launched no earlier than 2017. They now enter the definition phase, the next step required before the final decision is taken as to which missions are implemented.

These three missions are the finalists from 52 proposals that were either made or carried forward in 2007. They were whittled down to just six mission proposals in 2008 and sent for industrial assessment. Now that the reports from those studies are in, the missions have been pared down again. “It was a very difficult selection process. All the missions contained very strong science cases,” says Lennart Nordh, Swedish National Space Board and chair of the SPC.

And the tough decisions are not yet over. Only two missions out of three of them: Euclid, PLATO and Solar Orbiter, can be selected for the M-class launch slots. All three missions present challenges that will have to be resolved at the definition phase. A specific challenge, of which the SPC was conscious, is the ability of these missions to fit within the available budget. The final decision about which missions to implement will be taken after the definition activities are completed, which is foreseen to be in mid-2011.
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Euclid is an ESA mission to map the geometry of the dark Universe. The mission would investigate the distance-redshift relationship and the evolution of cosmic structures. It would achieve this by measuring shapes and redshifts of galaxies and clusters of galaxies out to redshifts ~2, or equivalently to a look-back time of 10 billion years. It would therefore cover the entire period over which dark energy played a significant role in accelerating the expansion.

By approaching as close as 62 solar radii, Solar Orbiter would view the solar atmosphere with high spatial resolution and combine this with measurements made in-situ. Over the extended mission periods Solar Orbiter would deliver images and data that would cover the polar regions and the side of the Sun not visible from Earth. Solar Orbiter would coordinate its scientific mission with NASA’s Solar Probe Plus within the joint HELEX program (Heliophysics Explorers) to maximize their combined science return.

Thales Alenis Space concept, from assessment phase (ESA)

PLATO (PLAnetary Transit and Oscillations of stars) would discover and characterize a large number of close-by exoplanetary systems, with a precision in the determination of mass and radius of 1%.

In addition, the SPC has decided to consider at its next meeting in June, whether to also select a European contribution to the SPICA mission.

SPICA would be an infrared space telescope led by the Japanese Space Agency JAXA. It would provide ‘missing-link’ infrared coverage in the region of the spectrum between that seen by the ESA-NASA Webb telescope and the ground-based ALMA telescope. SPICA would focus on the conditions for planet formation and distant young galaxies.

“These missions continue the European commitment to world-class space science,” says David Southwood, ESA Director of Science and Robotic Exploration, “They demonstrate that ESA’s Cosmic Vision programme is still clearly focused on addressing the most important space science.”

Source: ESA chooses three scientific missions for further study