Aurora Archives

September 27, 2011December 24, 2015 by VirtualAstro

An Easy Guide To Observing the Aurora

[/caption]

With the recent solar activity and the high possibility of more coming up, here is an easy guide to observing the aurora. An aurora is a natural light display high in the Earth’s atmosphere, caused by energetic particles from the Sun, colliding with the Earth’s magnetic field.

These light displays are called the Aurora Borealis in the Northern hemisphere and Aurora Australis in the Southern hemisphere, but are commonly known as the Northern and Southern lights.

Viewing aurorae is incredibly simple, but the conditions need to be right for a display to appear.

Normally you can only see aurorae near the poles, such as in Canada, Iceland, and Norway or southern Australia and Antarctica, but when the Sun is highly active, more solar material is thrown in Earth’s direction, creating powerful geomagnetic storms. These storms can bring auroral displays further south to areas such as Southern UK and North to mid latitudes of the USA.

The intensity scale is known as the Planetary KP index and basically the higher the KP number the further south Aurorae can be seen, KP 8 or higher can be good for observers further south. To find out what current levels are check spaceweather.com or the Geophysical Institute at the University of Alaska Fairbanks

If aurora activity is predicted to be high and there is a possibility of seeing it at your location, try and find an area away from light pollution or bright lights and let your eyes adjust to the dark. This may require you to travel into the countryside to escape bright city light pollution.

The best time to spot aurora is around local midnight, but this can change depending on viewing conditions and the current intensity of the magnetic storm.

Once you are comfortable and your eyes have adjusted to the dark, face north (or south in the Southern Hemisphere).

You do not need binoculars, a telescope, or any other optical aid other than glasses if you wear them.

Look low and close to the horizon and look for the faint green/ reddish glow of aurora. It may be quite difficult to see at first, but if it is a powerful display it can be very easy to spot.

I live in the South of the UK and have seen the waving bands and curtain like structures quite easily in powerful geomagnetic storms.

If you have a camera that takes long exposures, use a tripod and try to image the aurora and send us your results.

Most of all, enjoy the show! Good luck!

Aurora September 26, 2011 From Acadia National Park Credit: hale_bopp37

Aurora Behind the Clouds Credit: Corinne Mills

September 27, 2011December 24, 2015 by Nancy Atkinson

Active Sun, Beautiful Aurora: Reader Photos

[/caption]

Readers have submitted some great images of aurorae taken last night (Sept. 26 or early morning of Sept. 27). Why all the auroral activity? Sunspot region 1302 is big and bad, spewing out some nasty stuff. NASA says the sunspot’s magnetic field is currently crackling with sub-X-class flares that could grow into larger eruptions as the sunspot continues to turn toward Earth.

Here are some reader photos of the sunspot and the aurorae it created. A stunning view from Karstad Sweden, from Flickr user Socrates 2013, is above.

Massive sunspot 1302 on Sept. 25, 2011, with an Earth inserted for size reference. Credit: Ron Cottrell

This massive sunspot region has already produced two X-flares (X1.4 on Sept. 22nd and X1.9 on Sept. 24th). The dark cores in the sunspots this image from reader Ron Cottrell is larger than Earth, (see inserted Earth for reference) and the entire active region stretches more than 100,000 km from end to end.

“Even with a small aperture, 40mm, Hydrogen – Alpha telescope the image details are amazing,” Cottrell emailed us. “I captured this image from my patio in Oro Valley, Arizona.” He used a webcam to do some image post processing.

Aurora on Sept. 26, 2011 at Porsgrunn, Norway. Credit: Kjetil Vinorum

Kjetil Vinorum sent us some aurora photos from Porsgrunn, Norway (59° 09′ 33.3″N, 9° 39′ 46.9″E) and says this is the first time he’s seen aurora so far south in a decade.

This all-sky time-lapse of the aurora on Sept. 26-27, 2011 is from Arne Danielsen of Vestby, Norway (N59°36’18” E10°45’40” A84m).
The video shows a total of 726 images, which were obtained from Sunset to Sunrise. North is up and West is right. Be patient to see the aurora! Via Cosmos4U on Twitter

The aurora over Vernon, British Columbia Canada, sent to us by UT reader Marcel.

This beautiful shot was taken on the evening of September 27, 2011 by Marcel in British Columbia, Canada. The view is overlooking an orchard in the Coldstream Municipality.

The H-Alpha Sunspot 1302 09-25-2011. Credit: John Chumack

Here’s another view of the active region 1302 from John Chumack of Galactic Images.

The region has unleashed M8.6 and M7.4 flares on Sept. 24 and an M8.8 flare early on Sept. 25. None of the blasts have been squarely Earth-directed, but this could change, NASA says, as the sunspot turns toward our planet in the days ahead. AR1302 is growing and shows no immediate signs of quieting down.

Aurora at 21:20 UTC on Sep. 26, 2011 from Königswinter, Germany. Credit: Daniel Fischer — Aurora at 21:20 UTC on Sep. 26, 2011 from Königswinter, Germany. Credit: Daniel Fische

This image from Monty Leventhal shows the sunspots in region 1302 spreading across the face of the Sun for approximately 186,000 km. He used a Canon 300D with an Hydrogen-alpha filter with a Meade S.C. 10 inch telescope.

More info on AR1302 from NASA

September 26, 2011April 26, 2016 by Nancy Atkinson

Aurora Alert for September 26 and 27!

Predicted auroral oval over the North Pole, for Sept. 27, 2011. Credit: NOAA Space Weather Center

[/caption]

Skywatchers in northern Europe are already seeing some aurora activity as a strong-to-severe geomagnetic storm is in progress, according to the NOAA Space Weather Prediction Center and SpaceWeather.com. The fuel for this storm was a coronal mass ejection over the weekend that has now reached Earth. This is great news for skywatchers, as both the Northern and Southern lights should be spectacular. But this is not so good news for satellite companies. The Goddard Space Weather Lab reports a “strong compression of Earth’s magnetosphere. Simulations indicate that solar wind plasma [has penetrated] close to geosynchronous orbit starting at 13:00 UT.” Geosynchronous satellites could therefore be directly exposed to solar wind plasma and magnetic fields.

Predicted auroral oval over the South Pole, for Sept. 27, 2011. Credit: NOAA Space Weather Prediction Center.

The active region on the Sun will be pointed straight at Earth in few days as the Sun rotates, so this could be a week of high auroral activity. If you are able to capture images, send the to Universe Today via email or upload them to our Flickr page, and we’ll share them! See an image below of the Sun from September 25, 2011, showing the Active Region 1302, courtesy of John Chumack.

For more information and updates see the links above, or the Geophysical Institute at the University of Alaska Fairbanks.

The Full Solar Disk in Hydrogen Alpha Light 09-25-2011. Credit: John Chumack. Click for larger version on Flickr.

September 26, 2011December 24, 2015 by VirtualAstro

Massive Sunspot 1302

[/caption]

A highly active region on the Sun threatens to deliver powerful geomagnetic storms over the week ahead. Highly energetic solar eruptions are likely heading in our direction to give Earth’s magnetic field a significant glancing blow!

Over the past few days the new sunspot AR1302 has been incredibly active, hurling massive X-class solar flares into space and it will soon face Earth.

The massive sunspot, many times larger than the Earth (see images below) is expected to increase in size and energy, and is expected to release powerful solar flares, sparking strong geomagnetic storms.

Sun Spot AR1302 through the clouds Credit: Tavi Greiner

What does this mean for the Earth and it inhabitants?

The Earth experiences material ejected from the Sun on a daily basis and we are protected by the Earth’s own magnetic field. This is normal and has been happening since the birth of the solar system. But occasionally the Sun erupts and sends vast quantities of solar material our direction in the form of Coronal Mass Ejections (CME’s).

This can trigger very powerful geomagnetic storms, which can damage satellites in orbit and cause problems for communications and power networks. One positive outcome, though, is amazing displays of aurorae at the poles (Northern and Southern Lights).

Sunspot 1302 is expected to eject material towards Earth over the next few days, so look for news of strong geomagnetic activity and displays of aurorae.

Several observers are reporting that AR1302 is easily visible on the Sun at sunset or sunrise. Never ever look at the sun with your eyes, or any other optical aid! This will damage your eyesight permanently! The Sun should only be viewed using specialist equipment.

For further updates see Spaceweather.com and NASA’ Heliophysics Science Division

Massive Sun Spot 1302 and Earth size Comparison taken with a specialist solar filter Credit: Will Gater www.willgater.com

September 8, 2011December 24, 2015 by Tammy Plotner

Exploring Geomagnetic Substorms

Schematic view of Cluster C3 and C1 satellite trajectories Copyright: ESA

[/caption]

Every now and again, a sudden pulse of energy in Earth’s magnetosphere just cuts loose. As a result, we have a bright polar auroral display. While we’re beginning to understand more about magnetism and the Sun/Earth connection, there’s still a few rogues left in the gallery. Just what is a geomagnetic substorm and what does it do?

Although we’ve known about them for years, the exact process behind a geomagnetic substorm has been a mystery… one that’s being solved with data from missions like ESA’s Cluster spacecraft. Earth is continually being bathed in incoming sheets of electrons and protons – the product of an active Sun. These highly energized particles are simply a part of solar winds flowing from coronal holes and even powerful blasts from events like coronal mass ejections. For the most part, we’re shielded by the magnetosphere – but sometimes a wee bit escapes and collects in the magnetotail – stored like a battery charge. At a point, it’s released… and when it does, it re-arranges our magnetic field lines. The energy then conducts itself along these lines like a filament in a light bulb. When the watts hit the fan? Wow… We have polar aurora!

It’s not a new concept, but there’s never been a clear understanding of where these geomagnetic storms originate. Do they come from a sudden disruption of electric current about 64 000 km from the planet? Or are the created by a process called magnetic reconnection which occurs much further down the magnetotail, at a distance of around 125 000 – 200 000 km? If you remember our recent study of Alfven waves, then you know current consensus points towards the reconnection theory. But there’s only one problem. Alfven waves are slow movers, traveling at a reconnection speed of about 250 seconds. What we’re seeing is an event that occurs about 60 seconds after reconnection… and the birth of a new movement. The kinetic Alfven wave (KAW).

“We ran a very simple system, and simulated how the reconnection event released energy in the plasma sheet of charged particles,” said Shay. “We were looking for a faster mechanism for propagating the signal from the explosion than the Alfven waves that were already widely recognized.”

Unlike its predecessor which motivates both ions and electrons, the KAW only excites the electron, moving them through the plasma at twice the speed. Through simulations, it’s been proved the kinetic Alfven wave could be spawned by reconnection, move away from the explosion and activate aurora. The data was returned by the Fluxgate Magnetometer (FGM) and the Electric Fields and Waves (EFW) instrument and found by Jonathan Eastwood, a Research Fellow at The Blackett Laboratory, Imperial College London.

“I found 18 events which occurred at the time the four spacecraft were flying through the tail region,” said Dr. Eastwood. “The fast signal predicted by Michael Shay showed up in the Cluster data, supporting the theory that kinetic Alfven waves generated by reconnection were rapidly energizing the auroras.”

“It’s rather like what happens in a thunderstorm,” he added. “The fast-moving lightning flash arrives first, followed some time later by the slower sound waves of the thunderclap.”

Fancy that… Coming from a substorm!

Original Story Source: ESA Science and Technology News. For Further Reading: Super-Alfvenic Propagation of Substorm Reconnection Signatures and Poynting Flux.

August 8, 2011April 26, 2016 by Jason Major

A Noctilucent Masterpiece

Noctilucent clouds over Reykjavíc. © Örvar Atli Þorgeirsson

[/caption]

Night-shining “noctilucent” clouds create a magical glow in the night skies over Reykjavíc, Iceland in this beautiful photo by Örvar Atli Þorgeirsson, taken on August 6. In the foreground is “The Sun Voyager” (Sólfar), an iconic steel sculpture located on the city waterfront representing a Viking ship.

Örvar did not set out to photograph this rare atmospheric phenomenon but had instead intended to shoot aurora triggered by recent solar outbursts.

“The forecast on the 6th of August was predicting extreme aurora activity,” Örvar says in his Flickr description. “Even though it was very early August and the night would not get fully dark I went out as the aurora can be seen in deep twilight conditions. I saw the aurora for 1 – 2 minutes that night. I did not get a good picture of it though. Instead we witnessed this even rarer phenomenon called noctilucent clouds.”

Noctilucent clouds are extremely high-level clouds made located in the mesosphere, around 76 to 85 kilometers (47 to 53 miles) high… nearly at the very edge of space. (Most commercial airplanes fly between 6 and 7 miles high.) They are high enough to reflect sunlight coming from beyond the horizon long after night has fallen over the land below. They usually appear as a wispy web of blue, white, purple and orange tendrils stretched across the sky.

“These clouds where extremely beautiful to look at and reminded me of the aurora but where much more stationary and had this beautiful blue color.”

– Örvar Atli Þorgeirsson

Noctilucent clouds are mainly visible at latitudes between 50º – 70º north and south during the months of June and July. This means Reykjavíc, located right in the middle, can get great views. (Of course it helps to have a talented photographer like Örvar to capture them so nicely!)

Oddly enough noctilucent clouds are a relatively recent phenomenon, only having been recorded for about 120 years. They have been connected with space shuttle passages through the upper atmosphere, and it’s even been suggested that they may be associated with the 1908 Tunguska impact.

_____________________

Jason Major is a graphic designer, photo enthusiast and space blogger. Visit his website Lights in the Dark and follow him on Twitter @JPMajor or on Facebook for the most up-to-date astronomy news and images!

August 6, 2011December 24, 2015 by VirtualAstro

Recent Active Sun Prompts Stunning Auroras Over England

Aurora over Cumbria 5/6th August 2011 Credit: Raymond Gilchrist

[/caption]
On the evening of the 5th of August 2011 the Aurora Borealis, Northern Lights were seen as far South as Southern England! At approximately 18:00 Universal Time (19:00 BST) the Earth’s magnetosphere was hit by a coronal mass ejection from the sun, triggering a powerful geomagnetic storm and Aurora.

This storm measured 8 on the K index (aurora richter scale) which ranges from 0 – 9 so this was a big storm.

It is quite common to see Aurora in Northern Scotland, but at approximately midnight, aurora was seen as far south as Berkshire, Wiltshire and Hampshire in Southern England. It is incredibly rare to see aurora this far south — the last time I remember was in 2003.

I was incredibly lucky to briefly see the pale greenish hue of the aurora through clouds from my back garden in West Berkshire.

Unfortunately a lot of people in England and Scotland were under thick cloud and missed this fantastic display, but thanks to fantastic astrophotographers such as Raymond Gilchrist (@RayGil on twitter) we are able to see the aurora through his images.

Did you see any aurora activity in your location? Geomagnetic activity remains high as I write this article, so I hope the sky clears and we are given another fantastic display of this rare phenomenon soon.

Aurora on the River Tay, Newburgh, Fife, Scotland Credit: photosbyzoe

July 23, 2011December 24, 2015 by Tammy Plotner

Exoplanet Aurora… Light ‘Em Up!

This artist's conception shows a "hot Jupiter" and its two hypothetical moons with a sunlike star in the background. The planet is cloaked in brilliant aurorae triggered by the impact of a coronal mass ejection. Theoretical calculations suggest that those aurorae could be 100-1000 times brighter than Earth's. Credit: David A. Aguilar (CfA)

[/caption]

One of the most beautiful and mysterious apparitions – be it north or south – here on Earth is an auroral display. We know it’s caused by the Sun-Earth connection, so could it happen around exoplanets as well? New research shows that aurorae on distant “hot Jupiters” could be 100-1000 times brighter than Earthly aurorae, creating a show that would be… otherworldly!

“I’d love to get a reservation on a tour to see these aurorae!” said lead author Ofer Cohen, a SHINE-NSF postdoctoral fellow at the Harvard-Smithsonian Center for Astrophysics (CfA).

As we are now aware, aurorae occur here on Earth when the Sun’s energetic particles encounter our magnetosphere and are shifted towards the poles. This in turn excites the atmosphere, ionizing the particles. Much like turning on your electric stove, this causes the “element” to glow in visible light. It happens here… and it happens on Jupiter and Saturn as well. If other suns behave like our own and other planets have similar properties to those in our solar system, then the answer is clear.

Exoplanets have aurorae, too.

Cohen and his colleagues used computer models to study what would happen if a gas giant in a close orbit, just a few million miles from its star, were hit by a stellar blast. He wanted to learn the effect on the exoplanet’s atmosphere and surrounding magnetosphere. In this scenario, the solar storm is much more focused and far more concentrated when it impacts a “hot Jupiter”. In our solar system, a coronal mass ejection spreads out before it reaches us, but what would happen if it collided with a nearer planet?

“The impact to the exoplanet would be completely different than what we see in our solar system, and much more violent,” said co-author Vinay Kashyap of CfA.

Using modeling, the team took a look at the scenario. The solar blast would slice into the exoplanet’s atmosphere and weaken its magnetic shield. The auroral activity would then form a ring around the equator, 100-1000 times more energetic than seen here on Earth. It would then travel up and down the planet’s surface from pole to pole for hours, gradually weakening – yet the planet’s magnetosphere would save it from erosion. This type of study is important for understating habitable properties of Earth-like worlds.

“Our calculations show how well the planet’s protective mechanism works,” explained Cohen. “Even a planet with a magnetic field much weaker than Jupiter’s would stay relatively safe.”

Original News Source: Harvard-Smithsonian Center for Astrophysics News.

July 16, 2011December 24, 2015 by Nancy Atkinson

Awesome Aurora Photographed by Shuttle/ISS Crews

A panoramic view of Earth taken from the ISS, with shuttle Atlantis docked to the station. Aurora Australis or the Southern Lights can be seen on Earth's horizon and a number of stars also are visible. Credit: NASA

[/caption]

The STS-135 crew of space shuttle Atlantis and the Expedition 28 crew of the International Space Station were treated with great views of the Aurora Australis. Here’s one shot the crews photographed, showing a panoramic view of the station/shuttle complex along with several different astronomical beauties! The aurora shows up brightly, but what else is in the image? Looking closely –and southern hemisphere observers might recognize some objects better — but do you see the globular cluster Omega Centauri, the Coalsack Nebula and the Southern Cross? Anyone see anything else?

See below for another great aurora shot from the ISS, where the green glow shows up even better:

The Southern Lights or Aurora Australis as seen from the space station and space shuttle. Credit: NASA

These images were taken on Thursday during one of the “night” passes for the station/shuttle. The astronauts mentioned the aurora during media interviews on Friday. “We saw an incredible Southern Lights aurora,” said STS-135 pilot Doug Hurley. “It was the best one I’ve seen in my two spaceflights. It was just unbelievable, the view out the cupola.”

See larger views on NASA’s mission gallery page.

July 13, 2011January 18, 2016 by Nancy Atkinson

How Does the Aurora Borealis Form?

Seeing the Northern or Southern Lights is an awe-inspiring experience, but do you know the science behind their beauty? This video from Per Byhring and the physics department at the University of Oslo explains how particles originating from deep inside the core of the Sun creates aurorae in the atmosphere of Earth.

The video takes a look at how cloud of electrically charged particles emanate from the Sun, and what happens when this plasma reaches the Earth and interacts with the planet’s magnetic field, which creates fantastic light shows in the extreme northern and southern latitudes.

Via Scientific American