The Sun Doesn’t Cause Earthquakes

SDO/AIA image of the Sun from April 12

If that title seems like an obvious statement to you, it’s ok… it seems pretty obvious to me too. But there are those who have been suggesting — for quite some time, actually — that earthquakes can be triggered or strengthened by solar activity; that, in fact, exceptionally powerful solar flares, coronal mass ejections, and other outpourings from our home star can cause the planet’s crust to shift, shake, and shudder.

Except that that’s simply not true — at least, not according to a recent study by researchers from the USGS.

Researchers Dr. Jeffrey Love from the United States Geological Survey and Dr. Jeremy Thomas from Northwest Research Associates compared historical data of solar activity with earthquake occurrences around the world and found no definitive correlations… nothing to suggest that one directly influenced the other.

“Recently there’s been a lot of interest in this subject from the popular press, probably because of a couple of larger and very devastating earthquakes. This motivated us to investigate for ourselves whether or not it was true.”

– Jeffrey Love, USGS Research Geophysicist

Even when an earthquake may have been found to occur on the same day as increased solar activity, at other times during even stronger quakes the Sun may have been relatively quiet, and vice versa.

Damage in Anchorage from an earthquake on March 27, 1964. Solar activity at the time was unexceptional. (U.S. Army photo)
Damage in Anchorage from an earthquake on March 27, 1964. Solar activity at the time was unexceptional. (U.S. Army photo)

“There have been some earthquakes like the 9.5 magnitude Chile quake in 1960 where, sure enough, there were more sunspots and more geomagnetic activity than on average,” said Dr. Love. “But then for the Alaska earthquake in 1964 everything was lower than normal. There’s no obvious pattern between solar activity and seismicity, so our results were inconclusive.”

Basically, even though our planet orbits within the Sun’s outer atmosphere and we are subject to the space weather it creates — and there’s still a lot to be learned about that — observations do not indicate any connection between sunspots, flares, and CMEs and the shifting of our planet’s crust (regardless of what some may like to suggest.)

“It’s natural for scientists to want to see relationships between things,” said Love. “Of course, that doesn’t mean that a relationship actually exists!”

The team’s findings were published in the March 16, 2013 online edition of Geophysical Research Letters.

Read more in Harriet Jarlett’s article on Planet Earth Online, and for results from another study see Dr. Ryan O’Milligan’s article on TheSunToday.org.

(Oh, and the Moon doesn’t cause earthquakes either.)

Weekend Aurora Alert: The Sun Lets Loose an Earth-Directed CME

NASA's Solar Dynamics Observatory captured this image of an M6.5 class flare at 3:16 EDT on April 11, 2013. This image shows a combination of light in wavelengths of 131 and 171 Angstroms. Credit: NASA/SDO.

The Solar Dynamics Observatory captured this view as the Sun let loose with its biggest solar flare of the year so far. It’s not a real big one — a mid-level flare classified as an M6.5 – but an associated coronal mass ejection is heading towards Earth and could spur some nice auroae by this weekend. Spaceweather.com predicts the expanding cloud (see animation below) will probably deliver a glancing blow to Earth’s magnetic field late on April 12th or more likely April 13th. The NOAA Space Prediction Center forecasts this event to cause moderate (G2) Geomagnetic Storm activity, and predicts geomagnetic activity to start in the mid to latter part (UTC) of April 13. They add that the source region is still potent and well-positioned for more geoeffective activity in the next few days.

 The magnetic field of sunspot AR1719 erupted on April 11th at 0716 UT, producing an M6-class solar flare. Coronagraph images from the Solar and Heliospheric Observatory show a CME emerging from the blast site of the M6.5 solar flare. Credit: NASA
The magnetic field of sunspot AR1719 erupted on April 11th at 0716 UT, producing an M6-class solar flare. Coronagraph images from the Solar and Heliospheric Observatory show a CME emerging from the blast site of the M6.5 solar flare. Credit: NASA

See this NASA page for info on solar flares, CMEs, and more.

NASA's Solar Dynamics Observatory captured this image of an M6.5 class flare at 3:16 am EDT on April 11, 2013. This image shows a combination of light in wavelengths of 131 and 171 Angstroms. Credit: NASA/SDO.
NASA’s Solar Dynamics Observatory captured this image of an M6.5 class flare at 3:16 am EDT on April 11, 2013. This image shows a combination of light in wavelengths of 131 and 171 Angstroms. Credit: NASA/SDO.

Solar Spacecraft Gets a Little Loopy

Our own Sun produces flares, but we are protected by our magnetosphere, and by the distance from the Sun to Earth. Credit: NASA/ Solar Dynamics Observatory,

Twice a year, the Solar Dynamics Observatory performs a 360-degree roll about the axis on which it points toward the Sun. This produces some unique views, but the rolls are necessary to help calibrate the instruments, particularly the Helioseismic and Magnetic Imager (HMI) instrument, which is making precise measurements of the solar limb to study the shape of the Sun. The rolls also help the science teams to know how accurately the images are aligned with solar north.

But take this rolling imagery, add some goofy music and hopefully it adds a smile to your day!

Astrophotos: We Have Liftoff from the Sun!

A large prominence from the Sun, on April 1, 2013. Credit and copyright: Paul Andrew.

Here are three images showing large prominences recently lifting off from the Sun’s surface. Solar prominences are sheets or arcs of luminous gas emanating from the Sun’s surface. They can loop hundreds of thousands of kilometers into space. In the image below by noted Australian amatuer Monty Leventhal, he estimates the prominence he captured stretches 233,000 km! Against the Sun, prominences appear dark, but against the sky they appear brighter. Prominences are held above the Sun’s surface by strong magnetic fields and can sometimes last for long periods of time.

See more and varied views below:

A negative image of the Sun and large prominences on March 31, 2013. Credit and copyright: César Cantú.
A negative image of the Sun and large prominences on March 31, 2013. Credit and copyright: César Cantú.
This digital filtergram shows an active prominence on the SE limb of the Sun, stretching across for approximately 233,000 km on March 27, 2013. Credit and copyright: Monty Leventhal.
This digital filtergram shows an active prominence on the SE limb of the Sun, stretching across for approximately 233,000 km on March 27, 2013. Credit and copyright: Monty Leventhal.

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Astrophoto: Jungle Sunset

A big Sun sets behind the trees in Cairns, Queensland, Australia. Credit and copyright: Joseph Brimacombe.

They say that perspective is everything. In this case perspective and filters are what makes this such a great astrophoto! We’ve been following Joseph Brimacombe’s astrophotography for years, and have come to appreciate his ‘perspective!” This great zoom shot of the setting Sun was taken on March 31, 2013 using a calcium K-line Filter, using a a 60 mm Lunt CaK Solar Telescope at F/8.3 and a Skynyx 2-2 camera. It’s a single shot, but below, you can watch a negative version of the Sun sink below the horizon in a video of 1,350 frames shown at double speed.

Jungle Sunset Calcium K-line Filter: Long Video – March 31, 2013 from Joseph Brimacombe on Vimeo.

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A Rather Quiet Solar Maximum … For Now

Recent sunspot counts fall short of predictions. Credit: Dr. Tony Philips & NOAA/SWPC.

2013 was supposed to be the year of Solar Max, the peak of the 11-year sunspot cycle. But so far, solar activity has been fairly low, with sunspot numbers well below expectations as well as infrequent solar flares.

Back in 2008, the NOAA/NASA Solar Cycle Prediction Panel, said that due to the extrememly deep and quite solar minimum going on at that time, they anticipated Solar Cycle 24 – our current cycle – to be below average in intensity. They’ve certainly been right about that.

In this video, solar physicist Dean Pesnell of the Goddard Space Flight Center says that this solar max looks different from what we expected because it may end up being “double peaked.”

This video shows the low amount of sunspots so far in 2013:

Read more at Science@NASA
.

Astrophoto: Giant Sunspot Group on the Sun

Sunspot 1678 in Hydrogen alpha light, taken on February 19, 2013. Credit and copyright: Paul Andrew.

On February 19 and 20, 2013, scientists watched a giant sunspot form in under 48 hours. It has grown to over six Earth diameters. This image by astrophotographer Paul Andrew shows a detailed, close-up view of this sunspot group, named AR 1678, imaged with a hydrogen alpha filter.

NASA said the spot quickly evolved into what’s called a delta region, which has a magnetic field that harbors energy for strong solar flares. NOAA forecasters estimate a 45% chance of M-flares and a 15% chance of X-flares during the next day.

Below is an image from the Solar Dynamics Observatory of this region on the Sun:

This image of AR 1678 combines images from two instruments on NASA's Solar Dynamics Observatory (SDO): the Helioseismic and Magnetic Imager (HMI), which takes pictures in visible light that show sunspots and the Advanced Imaging Assembly (AIA), which took an image in the 304 Angstrom wavelength showing the lower atmosphere of the sun, which is colorized in red. Credit: NASA/SDO/AIA/HMI/Goddard Space Flight Center
This image of AR 1678 combines images from two instruments on NASA’s Solar Dynamics Observatory (SDO): the Helioseismic and Magnetic Imager (HMI), which takes pictures in visible light that show sunspots and the Advanced Imaging Assembly (AIA), which took an image in the 304 Angstrom wavelength showing the lower atmosphere of the sun, which is colorized in red. Credit: NASA/SDO/AIA/HMI/Goddard Space Flight Center

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New Video Shows Fire and ‘Rain’ on the Sun

Screenshot of a dazzling magnetic display on the Sun, a phenomenon known as coronal rain. Credit: NASA/SDO

This footage was obtained by the AIA instrument on the Solar Dynamics Observatory on July 19, 2012. It provides a stunning display of solar activity and shows how wildly different events on the Sun can be. Some come just with a solar flare, some with an additional ejection of solar material called a coronal mass ejection (CME), and some with complex moving structures in association with changes in magnetic field lines that loop up into the Sun’s atmosphere, the corona.

This eruption produced all three.

A moderately powerful solar flare exploded on the Sun’s lower right hand limb, sending out light and radiation. Next came a CME, which shot off to the right out into space. And then, the Sun treated viewers to one of its dazzling magnetic displays — a phenomenon known as coronal rain.

Over the course of the next day, hot plasma in the corona cooled and condensed along strong magnetic fields in the region. Magnetic fields, themselves, are invisible, but the charged plasma is forced to move along the lines, showing up brightly in the extreme ultraviolet wavelength of 304 Angstroms, which highlights material at a temperature of about 50,000 Kelvin. This plasma acts as a tracer, helping scientists watch the dance of magnetic fields on the Sun, outlining the fields as it slowly falls back to the solar surface.

SDO collected one frame every 12 seconds, and the movie plays at 30 frames per second, so each second in this video corresponds to 6 minutes of real time. The video covers 12:30 a.m. EDT to 10:00 p.m. EDT on July 19, 2012.

Stunning Compilation of the Solar Dynamic Observatory’s Observations

Magnificent eruption from the Sun, shown in 304 and 171 Angstrom wavelength light, on August 31, 2012. Credit: NASA

Three years ago today, (February 11, 2010) I was standing at Kennedy Space Center watching the launch of the Solar Dynamics Observatory. The launch was spectacular, and included a unique effect as the Atlas rocket flew close to a sundog just as the spacecraft reached Max-Q, creating a ripple effect around the spacecraft. And so, SDO started off with a bang and she’s been producing incredible data ever since. The folks at Goddard Spaceflight Center’s Scientific Visualiation Studio have put together a highlight reel for the third year of SDO operations. You’ll see morphing sunspots, fountains of solar plasma, sun-grazing comets and more. Throughout its mission, SDO has not only studied the Sun, but also opened up several new, unexpected doors to scientific inquiry. Enjoy this “greatest hits” video of SDO’s third year.

Astrophotos: An Amazing Rush from the Sun

The Sun in H-Alpha with close-up on a rushing prominence on 02-07-2013. Credit and copyright: John Chumack.

“The Sun was amazing yesterday!” wrote John Chumack, one of our favorite astrophotographers, sending us these great shots of incredible prominences on the western limb, and one detached solar prominence, along with several filaments on the disk and 3 Sunspots!

You might get a “rush” from the close-ups of the large prominences blasting from the Sun. John shot these with a hydrogen alpha filter from his backyard in Dayton, Ohio. See more below:

Full disk of the Sun in Hydrogen Alpha Light on 02-07-2013. Credit and copyright: John Chumack.
Full disk of the Sun in Hydrogen Alpha Light on 02-07-2013. Credit and copyright: John Chumack.

John’s tools of the trade for these images were a Lunt 60mm/50F H-Alpha Solar telescope, DMK 21 AF04, 2x barlow, for close-up, 1/54 Sec exposure, 724 frames; a DMK 31 Camera for Full Disk, 1/387 second exposure, 561 Frames, Stacked in Registax 6.

Prominences from the Sun on 02-07-2013, with one detached prominence achieving liftoff! Credit and copyright: John Chumack.
Prominences from the Sun on 02-07-2013, with one detached prominence achieving liftoff!. Credit and copyright: John Chumack.

These Sun has been fairly active the past few days. Here’s a video from the Solar Dynamics Observatory of a C9-class solar flare. produced from Active Region AR1667 on February 6, 2013:

And John wasn’t the only one imaging the active Sun in the last few days. Here’s another photo of the Sun captured by Paul Stewart in New Zealand.

The Sun by Paul Stewart
The Sun by Paul Stewart

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