A new look 100 miles beneath a massive tectonic plate as it dives under North America has helped clarify the subduction process that generates earthquakes, volcanoes and the rise of the Cascade Range in the Pacific Northwest.

The largest array of seismometers ever deployed on the seafloor, coupled with hundreds of others operating in the continental U.S., has enabled University of California, Berkeley, researchers to essentially create CT scans of the Juan de Fuca plate and part of the earth’s mantle directly below it.

The plate, about the size of the state of Michigan, is grinding under the continent along an 800-mile swath that runs from Northern California to Vancouver Island, known as the Cascadia subduction zone.

The 3-D imaging process, known as seismic tomography, has revealed with unprecedented clarity a huge, buoyant, sausage-shaped region of the upper mantle, or asthenosphere, pressing up on the oceanic plate.

The imaging casts new light on the competing hypotheses about the drivers of plate tectonics, a dynamic earth process that has been studied for more than 50 years but is still poorly understood.

Different evidence has led to three different plate movement scenarios: either the plates are pushed from mid-ocean ridges; or they are pulled from their subducting slabs; or their movement is driven by the drag of the viscous mantle material that lies directly below.

The new research suggests that the third scenario does not apply to the Cascadia subduction zone. Rather, it reveals that a distinct, thin – and difficult to observe – layer separates the plate from the mantle beneath, at least in the Cascadia subduction zone.

The layer acts as a kind of berm that the plate rolls over before descending beneath the continent, says UC Berkeley seismologist Richard Allen, leader of the research and co-author of a paper appearing in the Sept. 23 edition of the journal Science.

“What we observe is an accumulation of low-viscosity material between the plate and the mantle. Its composition acts as a lubricant, and decouples the plate's movement from the mantle below it,” Allen explains. The plates may move independently of the mantle below, he adds.

The finding, he says, will help refine models of plate tectonic dynamics, aiding the long-range effort to understand the connection between tectonics and earthquakes.

“It is the motion of the plates that causes earthquakes,” Allen says. “Models like this help us understand that linkage so we can be better informed of the coastal hazards.

“First though, we need to learn if what we find here is typical of subduction zones across the planet, or if it is unique for some reason.”

Japan has recently deployed a massive seafloor seismic network to study subduction and earthquakes. Allen hopes to next apply the tomography strategy there. Alaska also beckons.

Lead author on the Science paper is William Hawley, a graduate student in Allen’s lab.

“Plate tectonics is the most fundamental concept explaining the formation of features we see on the earth’s surface,” Hawley said, “but despite the fact that the concept is simple, we still do not know exactly why or how it operates.

“If the asthenosphere acts as a lubricant for tectonic plate movement throughout the planet, it will really change our long-term models of the process” – dynamic changes that occur over a 100 million years, Hawley said.

“Modelers will have to take this lubricating layer into account because it changes the way the mantle and the plates talk to each other,” according to Hawley.

Seismic tomography generates 3-D images of the earth’s interior by measuring how differences in shape, density, rock type and temperature affect the path, speed and amplitude of seismic waves traveling through the planet from an earthquake.

Much as in CT scans, computers process differences in energy measured at the receiving end to infer interior 3-D detail. CT scans use X-rays as the energy source, while seismic tomography measures energy from seismic waves.

A dense array of seismometers directly over the region of interest yields the best images and provides the highest resolution of the structures, which can then inform models of the process.

This study used the data from the largest scale ocean-floor deployment to complement the onshore data already available. Together, they generated the best images of the region to date.

The four-year seafloor research effort was made possible by the National Science Foundation’s ambitious $20 million Cascadia Initiative.

The NSF aimed to spur greater understanding of plate structure, subduction processes, earthquakes and volcanism by deploying seismometers at 120 sites on the ocean floor, arrayed throughout the 95,000-square-mile Juan de Fuca plate.

Over the four years, the offshore and onshore seismometer array measured thousands of earthquakes throughout the planet, ranging from magnitudes of 5 to about 9 on the Richter scale. The study examined a subset of 321 quakes with magnitudes between about 6 and 7.5.

Grad students and faculty scientists participated in 24 research cruises to deploy the instruments and move them between two swaths of the Juan de Fuca plate. Several of the seismic tomography cruises invited undergraduate students on the two-week trips.

On one Berkeley-led cruise aboard the R/V Thomas Thompson, the undergrads dubbed the trip the “Tom Cruise,” and sent daily video blogs ( https://www.youtube.com/playlist?list=PLaLpP50ifUEiz1cLei4aNZNfS4wtGihey ) .

Wallace Ravven writes for the UC Berkeley News Center.

LAKE COUNTY, Calif. – After a break in the rain, forecasters are predicting some more precipitation on Saturday for Lake County.

The National Weather Service said there are chances of rain around Lake County during the day and night on Saturday.

Up to a tenth of an inch is expected during the daytime, with another quarter of an inch possible Saturday night, according to the forecast.

Light winds also are expected, with temperatures in the high 60s during the day and in the low 50s at night.

Conditions are expected to clear on Sunday and remain mostly clear through next weekend, the National Weather Service said.

Email Elizabeth Larson at This email address is being protected from spambots. You need JavaScript enabled to view it. . Follow her on Twitter, @ERLarson, or Lake County News, @LakeCoNews.

NORTH COAST, Calif. – The Sonoma County Sheriff's Office is continuing it investigation into the death of a man whose body was found in a shallow grave on Sonoma State University property this past week, releasing new details on Saturday.

The body of Kirk Ryan Kimberly, 18, of Cotati was found in a wooded area on the outskirts of the campus by an employee on Wednesday, as Lake County News has reported.

Kimberly had been reported missing about two weeks before his body was found, officials said.

On Saturday Lt. Tim Duke of the Sonoma County Sheriff's Office Investigations Division offered new details on the case.

Duke said the investigation has revealed that Kimberly was stabbed multiple times by his assailant – or assailants. However, Duke did not release specifics about where Kimberly was wounded, how many wounds he had or the weapon authorities believe was used in the homicide.

“Preliminarily, detectives believe this was not a random act of violence but an isolated incident,” Duke said in his report. “Thus far, detectives have found no affiliation with the homicide and Sonoma State University or its students, other than where the body was found, which was on the property, in an isolated and secluded area of the campus.”

Duke said detectives, as well as other sheriff’s office personnel, are continuing to work around the clock on this case collecting and processing physical, trace and forensic evidence.

Anyone with information about Kimberly disappearance or who has knowledge of this incident is encouraged to call Detective Joseph Horsman of the Sonoma County Sheriff’s Office Violent Crimes Unit at 707-565-2185.

LAKE COUNTY, Calif. – Veterans with stories to share and volunteers to help collect personal accounts are being sought for the Veterans History Project.

The Veterans History Project is an ongoing effort of the American Folklife Center of the Library of Congress.

The project collects, preserves and makes accessible to the public the personal accounts of American war veterans.

The goal is that future generations may hear directly from veterans and better understand the realities of war.

This week it was announced that Karen D. Lloyd, a retired colonel and former US Army aviator, has been appointed as the new director of the Veterans History Project.

In her previous assignment in the Office of the Librarian of Congress, Lloyd worked to expand the Veterans History Project's outreach efforts and developed products to facilitate the implementation of a project volunteer corps.

Volunteers for the project are needed. Veterans are asked to share their stories, and interested individuals are needed to help record the veterans' accounts.

Students in the 10th grade and above also may participate and there are special resources for educators and students.

Help honor our veterans by making their stories known.

To participate, contact Congressman Mike Thompson's Napa District office at 707-226-9898 or email This email address is being protected from spambots. You need JavaScript enabled to view it. .

For more information about the project, visit http://www.loc.gov/vets/ .

LAKE COUNTY, Calif. – Lake County Animal Care and Control has another group of big dogs ready for homes this week.

This week's dogs include mixes Labrador Retriever, pit bull, Rottweiler and shepherd.

Dogs that are adopted from Lake County Animal Care and Control are either neutered or spayed, microchipped and, if old enough, given a rabies shot and county license before being released to their new owner. License fees do not apply to residents of the cities of Lakeport or Clearlake.

If you're looking for a new companion, visit the shelter. There are many great pets hoping you'll choose them.

The following dogs at the Lake County Animal Care and Control shelter have been cleared for adoption (additional dogs on the animal control Web site not listed are still “on hold”).

'Perchuan'

“Perchuan” is a male Rottweiler mix with a short black and tan coat.

He's in kennel No. 11, ID No. 3557.

Rottweiler-shepherd mix

This young male Rottweiler-shepherd mix has a medium-length black and brown coat with white markings.

He's in kennel No. 19, ID No. 6412.

Labrador Retriever mix

This female Labrador Retriever mix has a short black coat with white markings.

She already has been spayed.

She's in kennel No. 21, ID No. 6308.

Rottweiler-shepherd mix

This young male Rottweiler-shepherd mix has a medium-length black and tan coat.

He's in kennel No. 22, ID No. 6411.

Rottweiler mix

This female Rottweiler mix has a black coat with some brindle markings.

Shelter staff said she need some training and is manageable on a leash. They said she is a very nice dog and knows not to jump when excited. After proper introductions, she has gotten along with other dogs she has met, including off-leash play. She would do best in a home with no cats.

She's in kennel No. 25, ID No. 5947.

To fill out an adoption application online visit http://www.co.lake.ca.us/Government/Directory/Animal_Care_And_Control/Adopt/Dog___Cat_Adoption_Application.htm .

Lake County Animal Care and Control is located at 4949 Helbush in Lakeport, next to the Hill Road Correctional Facility.

Office hours are Monday through Friday, 11 a.m. to 5 p.m., and 11 a.m. to 3 p.m., Saturday. The shelter is open from 11 a.m. to 4 p.m. Monday through Friday and on Saturday from 11 a.m. to 3 p.m.

Visit the shelter online at http://www.co.lake.ca.us/Government/Directory/Animal_Care_And_Control.htm .

For more information call Lake County Animal Care and Control at 707-263-0278.

Email Elizabeth Larson at This email address is being protected from spambots. You need JavaScript enabled to view it. . Follow her on Twitter, @ERLarson, or Lake County News, @LakeCoNews.

Save

LAKE COUNTY, Calif. – Going to sleep “later” as a result of the upcoming Daylight Saving Time change on Sunday, Nov. 6, can disrupt sleep patterns and may result in sleep-deprived drivers struggling with performance and concentration behind the wheel.

The California Highway Patrol is joining with the National Sleep Foundation to promote Drowsy Driving Awareness Week, Nov. 6 to 13, and increase awareness of the dangers associated with the deadly driving behavior.

California has seen an increase in collisions involving sleepy or fatigued drivers over the last three years, the CHP said.

In 2013, there were 4,284 collisions involving sleepy or fatigued drivers. The number increased to 4,693 in 2014 and to 5,511 in 2015, according to the CHP.

Over the same time span, the CHP said those collisions resulted in the deaths of 28 people in 2013, 44 people in 2014 and 45 in 2015.

“Most people are aware of the dangers of driving while intoxicated, but many do not know that drowsiness also impairs judgment, performance, and reaction time just like alcohol and drugs,” CHP Commissioner Joe Farrow said. “Teens and young adults are at the highest risk of drowsy driving, due to their chronic sleepiness and overall lack of driving experience.”

According to the National Highway Traffic Safety Administration, there are an estimated 100,000 collisions annually in the United States that are a result of drowsy driving. These collisions result in more than 1,550 deaths, 71,000 injuries, and an estimated $12.5 billion in monetary losses.

Here are some tips to avoid drowsy driving:

· Get a good night’s sleep before a long drive.
· Get off the road if you notice any signs of fatigue.
· Take a nap. Exit the freeway, pull off the road and find a safe place to take a 15- to 20-minute nap.
· Consume caffeine. The equivalent of two cups of coffee can increase alertness for several hours, but do not rely on it for long periods.
· Drive with a friend. A passenger who remains awake can help watch for signs of fatigue in the driver and take a turn driving if necessary.

The mission of the CHP is to provide the highest level of safety, service and security to the people of California.

Earth’s moon is an unusual object in our solar system, and now there’s a new theory to explain how it got where it is, which puts some twists on the current “giant impact” theory.

The work is published Oct. 31 in the journal Nature.

The moon is relatively big compared to the planet it orbits, and it’s made of almost the same stuff, minus some more volatile compounds that evaporated long ago.

That makes it distinct from every other major object in the solar system, said Sarah Stewart, professor of earth and planetary sciences at the University of California, Davis, and senior author on the paper.

“Every other body in the solar system has different chemistry,” she said.

The textbook theory of lunar formation goes like this: Late in the formation of the solar system came the “giant impact” phase, when hot, planet-sized objects collided with each other.

A Mars-sized object grazed what would become Earth, throwing off a mass of material from which the moon condensed. This impact set the angular momentum for the Earth-moon system, and gave the early Earth a five-hour day.

Over millennia, the moon has receded from the Earth and the rotation has slowed to our current 24-hour day.

Scientists have figured this out by looking at the moon’s current orbit, working out how rapidly angular momentum of the Earth-moon system has been transferred by the tidal forces between the two bodies, and working backward.

But there are a couple of problems with the textbook theory. One is the moon’s surprisingly Earth-like composition. Another is that if the moon condensed from a disk of material rotating around Earth’s equator, it should be in orbit in the plane of the ecliptic – the same plane as the other planets.

But the moon’s current orbit is tilted 5 degrees off the ecliptic, meaning some more energy must have been put in to move it.

An alternative to explain it all

Stewart, her former postdoctoral fellow Matija Ćuk (now a scientist at the SETI Institute in Mountain View, California), with Douglas Hamilton at the University of Maryland and Simon Lock, Harvard University, have come up with an alternative model.

In 2012, Ćuk and Stewart proposed that some of the angular momentum of the Earth-moon system could have been transferred to the Earth-sun system. That allows for a more energetic collision at the beginning of the process.

In the new model, a high-energy collision left a mass of vaporized and molten material from which the Earth and moon formed. The Earth was set spinning with a two-hour day, its axis pointing toward the sun.

Because the collision could have been more energetic than in the current theory, the material from Earth and the impactor would have mixed together, and both Earth and moon condensed from the same material and therefore have a similar composition.

As angular momentum was dissipated through tidal forces, the moon receded from the Earth until it reached a point called the “LaPlace plane transition,” where the forces from the Earth on the moon became less important than gravitational forces from the sun.

This caused some of the angular momentum of the Earth-moon system to transfer to the Earth-sun system.

This made no major difference to the Earth’s orbit around the sun, but it did flip Earth upright. At this point, the models built by the team show the moon orbiting Earth at a high angle, or inclination, to the ecliptic.

Over a few tens of million years, the moon continued to slowly move away from Earth until it reached a second transition point, the Cassini transition, at which point the inclination of the moon – the angle between the moon’s orbit and the ecliptic – dropped to about 5 degrees, putting the moon more or less in its current orbit.

The new theory elegantly explains the moon’s orbit and composition based on a single, giant impact at the beginning, Stewart said. No extra intervening steps are required to nudge things along.

“One giant impact sets off the sequence of events,” she said.

The research was supported by NASA.

Andy Fell writes for UC Davis News and Media Relations.

CLEARLAKE OAKS, Calif. – A Friday morning vehicle crash led to a propane leak, brief evacuations of some nearby homes and a closure of Highway 20.

The California Highway Patrol said the crash happened just before 8:30 a.m. on Highway 20 at Paradise Valley Boulevard.

A small green four-door sedan went off the highway and down an embankment next to the Paradise Cove subdivision, according to reports from the scene.

Northshore Fire Chief Jay Beristianos said the crash resulted in no injuries, but the vehicle hit a residential propane tank and knocked it over.

The result was that the overturned tank was leaking liquid propane in the backyard of the residence, Beristianos said.

Northshore and Cal Fire firefighters used water streams to disburse a propane gas cloud away from the home. Beristianos said a winch had to be used to upright the tank so the value could be turned off.

He said residents in nearby homes were asked to evacuate while the work at the scene involving the propane tank was taking place.

At the same time, Highway 20 was closed for about an hour to reduce the chance of igniting the propane cloud, Beristianos said.

Beristianos said Northshore Fire sent two engines, a heavy rescue and a medic unit, and Cal Fire sent two engines, with a total of 13 personnel on scene.

Email Elizabeth Larson at This email address is being protected from spambots. You need JavaScript enabled to view it. . Follow her on Twitter, @ERLarson, or Lake County News, @LakeCoNews.

Humans sometimes struggle to adjust to Daylight Saving Time, but just measuring the exact length of a Saturn day is one of the big challenges for scientists on NASA's Cassini mission.

Over more than a decade in Saturn orbit, Cassini's instruments have wrestled with confusing measurements to determine the planet's precise rotation rate.

The mission's final year and unprecedented trajectory will carry Cassini to unexplored regions so near to Saturn that scientists might finally answer the question:

Just how long is a day on Saturn?

Michele Dougherty used to say that measuring the length of a Saturn day was like searching for a needle in a haystack. Now she thinks the old cliché falls short. "It's more like searching for several needles that change color and shape unpredictably," she said.

Based at Imperial College, London, Dougherty is principal investigator for the magnetometer instrument (MAG) on board Cassini, studying the planet more closely than any spacecraft before. Yet Cassini's instruments can't seem to nail down something fundamental about Saturn that, for Earth, is hard to miss: the length of a day. Part of the challenge stems from what a day truly is.

When a person says, "It's been cloudy for days," they're conveying how long (that is, for how much time) the sky's been cloudy. But a day is really a description of motion, not time. The sun doesn't rise or set. Instead, the sun's apparent motion is the result of Earth spinning on its axis. And an observer need not be on Earth to figure out the length of an Earth day.

Someone in space or on another planet in our solar system could choose a distinct surface feature on Earth, such as Madagascar, then note its position and click a stopwatch. When Madagascar returns to the position it was in when the stopwatch was started, the observer could note the elapsed time.

If they measured precisely enough, they would find that Earth rotates once per 23.934 hours. That's Earth's rotation rate – the very definition of a day.

Using the same principle, Earthlings have learned the rotation rates of other planets. A day on Mercury lasts about two Earth months. And a Mars day lasts 24.623 Earth hours, barely longer than Earth's. But watching surface features does not work equally well for all planets.

When the bulk of a planet swims beneath thousands of miles of atmosphere, the challenge of clocking its rotation rate is even tougher. The swirling cloud bands on a gas planet like Saturn and Jupiter move at different rates, making it impossible to use the clouds to measure the planet's rotation rate. But even then, scientists have a couple aces up their sleeve: the planet's magnetic field and radio wave emissions.

In a planet's interior, heat causes electrically conductive fluids to move, and those currents generate a magnetic field that can extend out into space many times the diameter of the planet.

On Earth and Jupiter, the magnetic north pole is tilted from each planet's rotation axis by about 10 degrees, meaning it's not aligned with the "true north" pole on either planet.

If you could see Jupiter's or Earth's magnetic field from space, and you sped up time, the magnetic field would appear to wobble like a hula hoop as the planet spins.

Since the magnetic field is generated in a planet's deep interior, for most planets, the field's rotation rate tells scientists the rotation rate of the planet itself. One full wobble equals one day.

We can't see magnetic fields, but instruments called magnetometers can, and radio antennas can detect radio emissions from a planet with patterns that repeat each time the planet rotates.

In fact, almost as soon as radio antennas were invented, scientists figured out that Jupiter has a nine-hour and 55-minute day, according to Bill Kurth, a University of Iowa physicist and leader of Cassini's Radio and Plasma Wave Science (RPWS) team.

"Jupiter is like a clock. It doesn't lose time. It doesn't gain time," he said.

But Saturn is like no other planet orbiting our sun. Its magnetic field seems to be offset from its rotation axis by very much less than a degree, so Saturn's magnetic field doesn't hula but instead appears to spin smoothly with no wobble. Scientists might then expect to observe a steady signal of magnetic strength and direction at Saturn, but they don't.

The Cassini MAG instrument has detected a signal in Saturn's magnetic field which looks like a wave in the data that repeats about every 10 hours and 47 minutes. Scientists call that regularly repeating signal a "periodicity."

But this periodicity has a different value whether you're observing Saturn's northern or southern hemisphere, and it also seems to change with the seasons.

The RPWS instrument has also detected periodicities, and another of Cassini's instruments, the Magnetospheric Imaging Instrument (MIMI) has observed energetic charged particles (protons, electrons, ions) being whipped around Saturn periodically by its magnetic field.

"The MIMI instrument sees these blobs that move about the planet," Kurth said. But observations of the blobs, the radio emissions, and the magnetic field don't agree enough for scientists to feel they're sure about Saturn's rotation rate.

Cassini scientists didn't think Saturn's rotation rate was a puzzle they'd have to solve. "We thought we already knew, because Voyager measured it," Kurth said. Voyager data had suggested a Saturn day was about 10.7 hours. But Cassini's magnetometer measures it as a bit longer, or a bit shorter, depending on whether the spacecraft is observing Saturn's northern or southern hemisphere.

"Saturn has stymied us," Dougherty said. "Its rotation rate is somewhere between 10.6 and 10.8 hours, probably, but the signal we're seeing, we're not sure it's linked to the interior at all. All we know is that, in our MAG data, we see oscillations that are different in the north or the south, and they change over time."

One possible cause is that something in Saturn's atmosphere is disrupting or canceling out the effects of the true planetary magnetic field, Dougherty said. If that's the case, getting closer to Saturn might help.

For the final phase of Cassini's mission, the spacecraft will perform 20 orbits just outside of Saturn's main rings starting in November 2016, followed by 22 orbits flying through the unexplored space between Saturn's upper atmosphere and its innermost ring starting in April 2017. There, Cassini should have a better shot at seeing Saturn's rotation rate more clearly and resolving the mystery of Saturn's day.

"By the end of May 2017," Dougherty said, "we should know whether we'll be able to solve it."

For more information on Cassini and its mission to Saturn, visit http://saturn.jpl.nasa.gov .