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April 2008

April 29, 2008

Meet "Cheatgrass!"

I got this e-mail from one of the volunteers working to rid Mt. Lemmon of Cheatgrass.  Below is her plea for more volunteers. 

Dear Chuck --

I am on the Board of Directors of Trees for Mt. Lemmon, a volunteer group dedicated to re-vegetating and protecting the flora on Mt. Lemmon following the devastating Aspen Fire of 2003.  Our latest challenge is the eradication of cheatgrass, which is an invasive, highly flammable grass--much like the buffalo grass of the desert--that has emerged in large patches on Mt. Lemmon over the past years since the Aspen Fire.  Our organization is looking for volunteers from the Tucson community to help us control the invasion of this plant.

Our first Cheatgrass Pull is scheduled for this Saturday, May 3rd, beginning at 9:00 AM.  We will meet in the parking lot across from the Mt. Lemmon Community Center.  Bring water and a bag lunch; we will provide all the information needed, as well as garbage bags to collect the pulled grass.  Escape the heat and help with a worthy cause!

I am also attaching an article on Cheatgrass and its threat to the forests and basins all over the U.S., as well as a flyer that pertains specifically to Mt. Lemmon and our project.

Thank you, Chuck!

Linda Benziger

Attached Files with information:

Download CheatgrassEradication2008.pdf

Download cheatgrass_dangers_in_the_u.S. forests.doc

RENO QUAKES UPDATE

The Mogul area just west of Reno continues to shake from a swarm of earthquakes that began on February 28th and continued right through the weekend.  On Friday night a magnitude 4.7 hit the area.  It was the most powerful quake to date.  When a quake of this magnitude strikes it raises the risk slightly for a stronger earthquake to occur.  There have been almost 400 temblors with the most powerful.  Check out the latest information from this series of quakes here. -  First Alert Meteorologist Erin Jordan

April 28, 2008

Unusual Solar Flare

Check out this story from SpaceWeather.com.

SOLAR BLAST: No sunspots? No problem. On April 26th the blank sun unleashed a solar flare without the usual aid of a sunspot. At 1408 UT, Earth-orbiting satellites detected a surge of X-rays registering B3.8 on the Richter scale of solar flares. Shortly thereafter, SOHO coronagraphs recorded a coronal mass ejection (CME) billowing away from the sun:

The expanding cloud could deliver a glancing blow to Earth's magnetic field late on April 28th or 29th. High-latitude sky watchers should be alert for auroras when it arrives.

This strange solar flare came from a patch of sun (N08,E08) where magnetic fields were not intense enough to form a visible sunspot (sunspots are made of magnetism). Nevertheless, magnetic fields were present with sufficient energy and instability to produce a powerful explosion. NASA's twin STEREO spacecraft, observing the sun from widely separated vantage points, recorded a million mph shock wave or "solar tsunami" spreading from the blast site through the sun's atmosphere: movie.

Not bad for a "blank sun."

April 24, 2008

Cooking With The Sun

Want to reduce your carbon footprint?  An easy way to do so is to invest in a solar oven.  And since our sun is so strong year round, these work very well in southern Arizona.  They are also great for camping.  Imagine putting in a pot roast before going out hiking and having it done when you get back to camp?  Yummy! 

You can check out solar ovens in action this weekend at the 2008 Solar Potluck and Festival in the Sun at Catalina State Park.  Admission to the park is free on Saturday so pack in the family and put on your hiking shoes.  Enjoy the day! - First Alert Meteorologist Erin Jordan

April 22, 2008

Earth Day News from Kitt Peak

GLOBE at Night 2008 Results a Solid Step Toward IYA 2009

The international star-hunting activity known as GLOBE at Night inspired 6,838 measurements of night-sky brightness by citizen scientists around the world, including 660 digital measurements using handheld sky-quality meters.

The third edition of GLOBE at Night was held from February 25-March 8, with assistance from the educational outreach networks of the Astronomical Society of the Pacific (ASP) to help spread the campaign to amateur astronomers and science centers.

The 2008 campaign received measurements from 62 countries, surpassing last year's total of 60 countries.  Just over 4,800 of the measurements came from the United States (with 48 states and the District of Columbia reporting at least one measurement).  Observers in Hungary submitted the most measurements (380) from outside the U.S., followed by Romania, the Czech Republic, Costa Rica, and Spain, all with over 100 observations; Canada was next largest, with 95 measurements reported.

A representative map of GLOBE at Night 2008 observations is available at www.noao.edu/outreach/press/pr08/pr0805.html

These basic numbers fall roughly midway between the 2007 and 2006 results from GLOBE at Night, which may result from several factors.

"While we have just begun to analyze the data, we have strong anecdotal evidence from our citizen-scientist network in North America that they experienced abnormally cloudy skies this year," says Connie Walker, GLOBE at Night project manager at the National Optical Astronomy Observatory (NOAO) in Tucson, AZ.  "The timing of the March new Moon this year­which is required to give everyone sufficiently dark skies to properly observe the constellation Orion­also fell further into summer vacation for our partners in Chile and some other Southern Hemisphere countries, which made it more difficult to attract large numbers of students."

The classic GLOBE at Night program directs students, families, and the general public how to observe and record the number of stars visible in the constellation Orion, as seen from different locations.

Observers report their results online by comparing their view of Orion with a set of template images on the program's Web site, which shows the number of stars in the constellation for a range of visibilities from bright skies to very dark.

The digital version of GLOBE at Night takes advantage of low-cost digital sky-quality meters manufactured by Unihedron of Ontario, Canada, which can make a highly repeatable direct measurement of integrated sky brightness.

Both the "classic" GLOBE at Night exercise that anyone can have fun doing with their unaided eyes, and a digital effort to obtain precise measurements of urban dark skies will be conducted again in March 2009, as one of several start-hunting efforts connected to the "dark-skies awareness" cornerstone program of the International Year of Astronomy (IYA) 2009.

GLOBE at Night 2009 will occur in the latter half of March.  These dates should provide better conditions for schools in the Southern Hemisphere, and will likely coincide with Earth Hour 2009 as well, Walker says.

A first-look at results from GLOBE at Night 2008 was presented by project leaders who attended the March 2008 meeting of the National Science Teachers Association in Boston.  More detailed analysis of the GLOBE at Night 2008 data will be presented at the May 31-June 4 annual meeting of the Astronomical Society of the Pacific in St. Louis, to be held jointly with the American Astronomical Society.  The meeting's primary focus is national and regional training and planning related to IYA 2009.  See www.astrosociety.org/events/meeting.html for more details.

For more information and access to the data sets, see the program's Web page at www.globe.gov/globeatnight, or contact globeatnight@globe.gov or outreach@noao.edu.

Information about the emerging global plans for the IYA 2009 is available at www.astronomy2009.org

GLOBE at Night is a collaboration between The Global Learning and Observations to Benefit the Environment (GLOBE) Program, Boulder, CO; the National Optical Astronomy Observatory (NOAO) in Tucson, AZ; Centro de Apoyo a la Didactica de la Astronomia (CADIAS) in Chile; Environmental Systems Research Institute, Inc. (ESRI); and the International Dark-Sky Association (IDA).

The National Optical Astronomy Observatory (NOAO) consists of Kitt Peak National Observatory near Tucson, AZ; Cerro Tololo Inter-American Observatory near La Serena, Chile; and, the NOAO Gemini Science Center, the route for U.S. astronomers to observe with the Gemini North telescope in Hawaii and the Gemini South telescope in Chile.

NOAO is operated by the Association of Universities for Research in Astronomy Inc. (AURA), under a cooperative agreement with the National Science Foundation.

GLOBE (Global Learning and Observations to Benefit the Environment) is a worldwide, hands-on, primary and secondary Earth science and education program. GLOBE promotes and supports student-teacher-scientist collaborations on inquiry-based investigations of Earth's environment. To date, over 1 million students and 40,000 teachers from more than 100 countries have participated in GLOBE. GLOBE is funded by the National Aeronautics and Space Administration (NASA), supported by the National Science Foundation (NSF) and the U.S. Department of State, and implemented through a cooperative agreement between NASA, the University Corporation for Atmospheric Research (UCAR) in Boulder, Colorado and Colorado State University in Fort Collins, Colorado.

April 21, 2008

Watch a Map of Ozone

Unlike the Ozone Layer, which is in the upper atmosphere and prevents the entry of most of the

sun's harmful rays, ground level ozone is a bad thing for us to breathe.

Add wildfire smoke and exhaust from our cars to sunlight and you get ozone. Watch an animation

Of ozone on Pima County's site at http://www.airinfonow.org/ . You can find the animation under OZONE

MAPPING at the top.

Give it a try and let us know what you think!

Happy Weather!

Chuck George

It's That Time Of Year...Triple Digits Temps Are Possible!

The following information is from the Tucson National Weather Service.

First date of 100 degree or greater across southeast Arizona

Location Average date Earliest Latest
Pima County
Organ Pipe N.M May 10 May 6, 1989 June 16, 1982
Ajo May 18 April 7, 1930 May 18, 1954
Anvil Ranch May 25 April 19, 1989 June 16, 1982
Tucson May 26 April 19, 1989 June 22, 1905
                                         Click on Tucson Line for yearly listing
Pinal County
Eloy May 10 April 7, 1989 June 11, 1972
San Manuel June 8 May 18, 1970 June 29, 1965
Oracle June 25 May 26, 1951 August 2, 1918
San Carlos Res. June 2 May 13, 1959 June 23, 1965
Santa Cruz County
Tumacacori N.M. May 27 April 20, 1989 June 20, 1999
Nogales June 6 May 12, 1996 June 26, 1982
Canelo June 19 May 12, 1996 July 26, 1995
Santa Rita Exp. June 19 May 12, 1996 July 31, 1986
Cochise County
Cascabel May 24 April 19, 1989 June 18, 1976
Bowie May 31 May 3, 1923 June 19, 1972
San Simon June 2 May 3, 1947 June 21, 1999
Benson June 6 May 3, 1947 June 22, 1999
Willcox June 13 May 8, 1989 June 26, 1935
Douglas June 13 May 12, 1996 June 29, 1986
Tombstone June 14 May 6, 1989 July 5, 1905
Pearce-Sunsites June 14 May 11, 1996 July 1, 1967
Sierra Vista June 17 May 22, 1989 June 29, 1986
Coronado N.M. June 23 May 28, 1984 July 31, 1986
Chiricahua N.M. June 24 May 28, 1910 July 27, 1995
Portal June 30 June 25, 1994 July 11, 1958
Graham County
Fort Thomas May 31 April 21, 1989 June 20, 1998
Safford June 1 April 28, 2000 June 23, 1967
Black River Pumps July 8 June 24, 1990 July 25, 1995
Greenlee County
Clifton June 1 May 2, 1947 July 6, 1943
Duncan June 10 April 27, 2000 July 10, 1958

April 18, 2008

5.2 Earthquake In Illinois

A 5.2 magnitude earthquake hit southeastern Illinois early Friday morning.  There were reports of minor structural damage in West Salem, IL and Louisville, KY.  No one was hurt.  However this is a powerful earthquake for this area.  The last time this area saw a quake of this magnitude was in 1968.  Check out details at the United States Geological Survey.

Usgs_earthquake Check out the image at left. The brighter the color, the higher the earthquake danger in the United States.  You can see the usual suspects of coastal California, Oregon, and Washington.  But look towards the center of the coutnry.  The red area and surrounding bright colors is the New Madrid Region.  This area is know for numerous small earthquakes and even a few large ones.  This area ecompasses cities like Memphis and St. Louis.  On the edge of this area is where this morning's earthquake occured.  Every 10 to 20 years there is a moderate eathquake in the region where today's earthquake struck.  Smaller earthquakes are felt once or twice a year. 

Even farther east,along the coast of South Carolina, is another high risk earthquake zone.  In 1886 a 7.6 magnitude earthquake struck Charleston.  Historically there have been similar strong earthquakes in the last 5000 years. 

April 17, 2008

The Earth Hums It's Own Tune

Check out this article by Charles Q. Quoi published on LiveScience.com.  The earth is always humming...and we aren't really sure why.  But it's pretty cool! - First Alert Meteorologist Erin Jordan

Earth gives off a relentless hum of countless notes completely imperceptible to the human ear, like a giant, exceptionally quiet symphony, but the origin of this sound remains a mystery.

Now unexpected powerful tunes have been discovered in this hum. These new findings could shed light on the source of this enigma.

The planet emanates a constant rumble far below the limits of human hearing, even when the ground isn't shaking from an earthquake. (It does not cause the ringing in the ear linked with tinnitus.) This sound, first discovered a decade ago, is one that only scientific instruments — seismometers — can detect. Researchers call it Earth's hum.

Investigators suspect this murmur could originate from the churning ocean, or perhaps the roiling atmosphere. To find out more, scientists analyzed readings from an exceptionally quiet Earth-listening research station at the Black Forest Observatory in Germany, with supporting data from Japan and China.

Different types

In the past, the oscillations that researchers found made up this hum were "spheroidal" — they basically involved patches of rock moving up and down, albeit near undetectably.

Now oscillations have been discovered making up the hum that, oddly, are shaped roughly like rings. Imagine, if you will, rumbles that twist in circles in rock across the upper echelons of the planet, almost like dozens of lazy hurricanes.

Scientists had actually expected to find these kinds of oscillations, but these new ring-like waves are surprisingly about as powerful as the spheroidal ones are. The expectation was they would be relatively insignificant.

New thinking

This discovery should force researchers to significantly rethink what causes Earth's hum. While the spheroidal oscillations might be caused by forces squeezing down on the planet — say, pressure from ocean or atmospheric waves — the twisting ring-like phenomena might be caused by forces shearing across the world's surface, from the oceans, atmosphere or possibly even the sun.

Future investigations of this part of the hum will prove challenging, as "this is a very small signal that is hard to measure, and the excitation is probably due to multiple interactions in a complex system," said researcher Rudolf Widmer-Schnidrig, a geoscientist at the University of Stuttgart, Germany.

Still, a better understanding of this sound will shed light on how the land, sea and air all interact, he added.

Researcher Dieter Kurrle and Widmer-Schnidrig detailed their findings March 20 in the journal Geophysical Research Letters.

April 15, 2008

UA SCIENCE NEWS!

FROM: Lori Stiles (520-626-4402; lstiles@u.arizona.edu)

The High Resolution Imaging Science Experiment, run from The University of Arizona, has produced a new color stereo view of Phobos, the larger and inner of Mars' two tiny moons.  The HiRISE camera aboard NASA's Mars Reconnaissance Orbiter took two images of Phobos 10 minutes apart on March 23. Scientists combined the images for a stereo view.

"Phobos is of great interest because it may be rich in water ice and carbon-rich materials," professor Alfred McEwen of the UA's Lunar and Planetary Laboratory, and HiRISE principal investigator, said.

Previous spacecraft, notably Mars Global Surveyor, have taken higher resolution pictures of Phobos because they flew closer to it, HiRISE team member Nathan Bridges of NASA's Jet Propulsion Laboratory, in Pasadena, Calif., said.

"But the HiRISE images are higher quality, making the new data some of the best ever for Phobos," Bridges said. "The new images will help constrain the origin and evolution of this moon."

By combining information from the HiRISE camera's blue-green, red and near-infrared color channels, scientists confirmed that material around the rim of Phobos' largest surface feature, Stickney crater, appears bluer than the rest of Phobos. The impact that excavated 9-kilometer, or 5-and-a-half mile, Stickney is thought to have almost shattered the moon.  If Phobos' surface is analogous with surface of our own moon, "the bluer color could mean that the regolith is fresher, or hasn't been exposed to space as long as the rest of Phobos' surface has," Bridges said.

The HiRISE view also shows landslides along the walls of Stickney and other large craters, Phobos' striking surface grooves and crater chains, and craters hidden on the moon's dark side illuminated by "Marsshine."  "Marsshine" is sunlight reflected by Mars onto the moon. The phenomenon is analogous to "Earthshine," where Earth reflects sunlight that illuminates the dark side of our moon. Like Earth's moon, Mars' moons Phobos and Deimos are "tidally locked" on their planet – that is, they always present the same side to the planet they orbit.

The HiRISE images are among several new HiRISE images being released today on the HiRISE Web site at http://hirise.lpl.arizona.edu. The images include an anaglyph, or 3-D view of Phobos that can be viewed with red-blue glasses.  MRO flies at about 7,800 mph between 155 and 196 miles, or between 250 and 316 kilometers, above the surface of Mars. Phobos was 6,800 kilometers, or about 4,200 miles, away when the HiRISE camera took the first photograph. At that distance, the HiRISE camera was able to resolve surface features at a scale of 6.8 meters, or about 22 feet, per pixel, and see features as small as 20 meters, or 65 feet, across. Phobos was 5,800 kilometers, or about 3,600 miles, away when the HiRISE camera took the second picture minutes later. At that distance, the HiRISE camera was able to resolve features about 15 meters, or 50 feet, across.  Phobos, only about 13 and a half miles, or 22 kilometers, in diameter, has less than one-thousandth the gravity of Earth. That's not enough gravity to pull the moon into a sphere, so it's oblong. Mars' second moon, Deimos, is even smaller, at about 7 and a half miles, or 12 kilometers, across. The very dark, diminutive moons may be captured asteroids from the outer, carbon-rich, Mars-Jupiter asteroid belt. The Mars Reconnaissance Orbiter's Compact Reconnaissance Imaging Spectrometer for Mars, or CRISM, observed both Martian moons last year. By combining HiRISE and CRISM data on Phobos, scientists can map minerals and soil types on the moons.