Yeah Alaska! Yeah Brazil! Yeah California?

The people of Juneau saved electricity in a hurry– when electricity
went to 55 cents per kilowatt-hourIn Juneau, Alaska, an avalanche on April 16th downed transmission lines and cut off the city from it’s cheap source of hydroelectric power; electricity prices jumped by 500%. Alan Meier-a scientist at Lawrence Berkeley National Laboratory, Home Energy Magazine’s Senior Executive Editor, and an expert in how to cut energy use in a hurry-was called in to help. Within a few weeks the city reduced its electricity use by 30%. Remember that we reduced our electricity use in California by 15% in response to Enron and other power companies manipulating the power markets in 2001? Alaska reduced its electricity use by twice as much and did it in a hurry.

How did the Alaskan’s do it? They lowered their thermostats. They bought out all the CFLs from the hardware stores and you bet they turned out the lights when they left the room-wouldn’t you if electricity cost 55 cents per kilowatt hour? They took shorter showers and used cold water to wash their clothes. The city ran out of clothespins since so many people were hanging out there clothes to dry (anecdotal evidence suggests it takes two days to dry jeans).

The people of Juneau bought power strips in record numbers, so that they could really turn off power to all those devices that still use power when they are supposed to be off, like TVs and stereos, microwave ovens and cell phone chargers. And there was a lot of talk from city leaders, on the radio, and among neighbors and classmates about the best ways to save.

(Note: You generally use more energy when you wash your dishes by hand rather than washing full loads in a dishwasher-not everything they did helped.)

We may not face rolling blackouts in California this summer, but we probably will in the near future. There will be other natural disasters like Juneau’s that spike the price of electricity or natural gas. How will we save energy in a hurry? And here’s a bigger question: How will we keep saving energy after the crisis is over?

The Juneau transmission lines should be up and running by June 8. Will the people who were used to cheap electricity fall back into old habits when prices decrease? Brazil faced a similar crisis in 2001 when severe drought shut down hydroelectric plants all over the country. They cut their electricity use by 20%, and they haven’t changed their consumptions habits very much since the drought subsided.

We are still dependent on a diminishing store of fossil fuels mostly located in politically turbulent parts of the world where even the hint of conflict raises oil prices. For Californians, Alaskans, Brazilians, and everyone else, it might be best if we permanently changed our energy use habits and considered every day an emergency that calls for conservation.

There are times when you are in the production trenches, plumbing the depths of a story, that you realize how lucky you are to work on QUEST. Assisting QUEST Producer Amy Miller on this segment was yet another occasion to experience such a sentiment, as we found out about the amazing work of Ashok Gadgil and his colleagues to help the women and families who’ve been displaced as a result of the genocide in Darfur.

For those of you who aren’t familiar with the story, in 2005, Ashok Gadgil, a physicist at Lawrence Berkeley National Laboratory, led a team of four people to north and south Darfur to determine how families were cooking their meals. This may seem like an odd fact-finding mission but it had very real consequences for alleviating the suffering and violence the Darfuri women experience. Every other day, many women leave the relative safety of the refugee camps to travel six to seven hours to collect fuel wood for their meals. In the process, they risk rape and mutilation at the hands of the Janjaweed, a state-sponsored militia which has been lodged in a genocidal fight against Darfuri rebel groups pressing for more autonomy from the government in Khartoum. Three years later, Ashok Gadgil and Ken Chow of Engineers Without Borders are on version eight of the Berkeley Darfur stove, an elegantly simple yet effective ten pound metal stove which is four times more efficient than the traditional three-stone fire with which the Darfur refugees have traditionally cooked. Ashok and his colleagues on the Darfur Stoves Project hope to have five to six manufacturing plants operating in north, west and south Darfur, producing hundreds of thousands of stoves a year from the flat-pack kits of the stove Ken Chow has engineered.

For me, this QUEST segment highlighted how scientists with the brilliance and dedication of Ashok Gadgil can think up solutions to problems that have the potential to alleviate suffering and help the economic lot (each stove saves roughly $250 dollars in fuel wood annually for a Darfuri family) of hundreds of thousands of people existing within the margins of survival. Fortunately, there are organizations, in addition to the Darfur Stoves Project, that are also helping to get more stoves into the hands of Darfuri refugees, including The Hunger Site, Global Giving, The Child Health Site. You can visit these non-profit organizations and purchase a Berkeley Darfur stove on behalf of a family in Darfur, and also make a donation to the U.S. chapter of Engineers Without Borders to support their projects in Asia and Africa.

On a final production note, our QUEST segment about the Darfur Stoves Project was immensely helped by U.N.’s archival footage department and the U.N. Mission in Sudan, both of which gave us footage of the stark conditions in the Darfuri refugee camps. The U.N. High Commission for Refugees also accepts donations for their international humanitarian activities.

Watch the “Darfur Stoves Project” TV Story online, as well as find additional links and resources.


Sheraz Sadiq is an Associate Producer for QUEST on KQED Television.

Making Every Photon Count

Last week I went to a talk given by the leader of the Supernova Factory collaboration at LBNL. What is SN factory? This is an ambitious project to study supernovae like never before. I mentioned this project briefly in a previous post , now that they are so close to releasing their results I want to discuss it a bit more.

The main idea of this project is to study several hundred nearby supernovae using an instrument known as the Supernova Integral Field Spectrograph, or SNIFS. This type of instrument is essentially a blend between a traditional imaging camera and a spectrograph.

The resolution in an integral field spectrograph is defined in spaxels instead of the pixels that have become all too familiar with the advent of digital cameras. A spaxel is quite similar to a pixel, there aren’t nearly as many and each one carries at least a 1000 times as much information.

In your digital camera, the light passes through the lens and directly onto the CCD. Each pixel on the CCD counts the number of photons in the red, the blue, and the green. Typically, there are millions of pixels, each counting photons from a slightly different region of the subject of your photograph.

Now imagine that instead of just counting red, green, and blue, that each pixel counts the entire rainbow of light from your subject. Now you have a spaxel. In an intregral field unit, the light passes through an array of microlenses and prisms before landing on the detector. We would call each set of microlenses and prisms a spaxel. The resulting image carries information about every wavelength of light from every region of your target.

Spectrum of the first SN observed with SNIFSThe advantage to an integral field spectrograph like SNIFS is that you gain a lot more information than either an imager or spectrograph alone. With an integral field spectrograph you can basically identify and organize every photon that reaches the telescope.

Specifically designed to observe supernovae, SNIFS is being operated at the 88-inch telescope on Mauna Kea. Spaxels are quite expensive - this particular instrument has only 225. However, this is more than enough to observe the entirety of a galaxy, a supernova, and the background.

The members of the SN Factory have now observed over 100 SNe using this new camera. Last Thursday, I saw the data from the first 25 well-calibrated supernovae and was very impressed. The data showed the evolution of each supernova and the properties of the host galaxy in great detail. I’m sure the supernova community will be equally impressed when they first see these new results.

Kyle S. Dawson is engaged in post-doctorate studies of distant supernovae and development of a proposed space-based telescope at Lawrence Berkeley National Laboratory.

Last night we completed our observations for the Supernova Legacy Survey. This was a five year program to study supernovae using a 4-meter telescope in Hawaii in combination with several of the largest optical telescopes in the world.

The project was headed by a group at a university in Toronto and a group at a university in Paris. Canada and France sponsor the 4-meter telescope that is used to discover and observe the supernovae from the point of explosion to the final days when the supernova fades from view. We call this the imaging part of the program. This data constrains the apparent brightness and life cycle of the supernova, and eventually the absolute distance to the supernova.

Our contribution to the project was primarily through our affiliation with Keck Observatory. We were typically awarded four nights a year to observe recently discovered supernovae spectroscopically. The data is used to determine the redshift and the kind of supernova explosion.

The supernovae are used to study the rate of expansion of the universe. It was this type of experiment that was first used to discover that the universe is actually dominated by dark energy.

No one really suspected the presence of dark energy for almost the entirety of the 20^th century. Now, we not only know it exists but are actually trying to understand it in the same way we understand gravity, protons, and electrons. That is where projects like the Supernova Legacy Survey come in. With projects like this, we work to collect enormous samples of well-studied supernovae that can improve our understanding of dark energy.

We use a certain type of supernova as yardsticks to measure distances in the universe. We then model the affects of dark energy on the expansion history of the universe by comparing distances and rates of expansion. This comparison is typically represented in a Hubble Diagram.

The Supernova Legacy Survey has been very successful in its attempts thus far. On the right, I show the Hubble Diagram from the first year of data. This is less than 20% of the full sample. The dotted line outlines the expectations of the 1990’s cosmology crowd. The solid line shows the prediction from the more sophisticated cosmologists of the 21^st century. As you can see, the original expectations were pretty far off the mark - the supernovae just don’t lie on top of the dotted line.

Now that this program is finishing up, we should be seeing similar figures that are teeming with supernovae. Future programs should do an even better job of making these measurements. Someday we may actually understand this dark energy thing, it may turn out to be something else completely new and unexpected!

Kyle S. Dawson is engaged in post-doctorate studies of distant supernovae and development of a proposed space-based telescope at Lawrence Berkeley National Laboratory.

A sample of switchgrass at Sandia National
LaboratoriesIt doesn’t need to be said that there’s a heated debate about how to mitigate greenhouse gas emissions with actions that lessen our society’s carbon footprint. Biofuels like ethanol or biodiesel are one option. They’re touted as being carbon neutral because the CO2 they emit comes from crops which had previously sequestered them in the atmosphere. In contrast, petroleum produces CO2 emissions that had previously been buried deep in the earth’s crust, adding to the other green house gases in the environment. For example, the U.S. Department of Energy - citing research by the Argonne National Laboratory – states that ethanol derived from corn emits 25% less greenhouse gas emissions than petroleum and that the savings with cellulosic ethanol, made from a feedstock like switchgrass, are much higher, in effect producing no additional greenhouse gases.

So when QUEST decided to move forward on producing a story about biofuels, I welcomed the opportunity to assist Series Producer Josh Rosen in its crafting. Being QUEST, we weren’t content to merely renumerate the different kinds of biofuels and how cellulosic ethanol is more efficient than corn-based ethanol. Instead, our story focuses on the pioneering work being done by researchers affiliated with the Joint BioEnergy Initiative (JBEI), a multi-billion dollar research initiative based in Emeryville, as they look beyond ethanol to the next generation of biofuels. So not only is JBEI looking at various feedstocks like switchgrass, rice, poplar and innovative ways to “deconstruct” the cellulosic material, it also attempts to synthesize fuels that work more efficiently in America’s automotive fleet, still overwhelmingly reliant on gasoline.

But even top researchers at JBEI like Jay Keasling and Blake Simmons caution that this next generation of biofuels won’t be coming online for years. Moreover, new research suggests that the net production cycle of biofuels, from the clear-cutting of trees to grow the crops to their transport to markets far away, may yield as many or more emissions as the use of petroleum-based fuel. A recent Op-Ed piece in the San Francisco Chronicle by UC Berkeley Alex Farrell cites the reason for this as primarily one of production– the way we clear land for growing biofuels, as well as our emphasis on the use of food-based crops like corn and soybean, which aren’t terribly efficient sources of ethanol to begin with.

Tad Patzek, also at UC Berkeley, has been an ardent critic of the carbon-neutral reputation of biofuels, garnering controversy for conducting studies that some other researchers have criticized for their calculations of emissions arising from biofuel production. (See Patzek’s co-authored article on page 19 of the March 2007 edition of Energy Tribune). Earlier this year, a study by researchers at the Smithsonian Tropical Research Institute suggests that biofuels are not created equal, as those made from U.S. corn, Malaysian palm oil and Brazilian soy yield more emissions than their petroleum-based counterparts, given the environmental damage they reap when grown for fuel. The study cites recycled cooking oil and biofuel made from grassy and woody cellulosic material as being more intelligent choices for cutting down on emissions.

And so the debate continues, struggling to keep pace with the technological progress made by scientists toiling away in their quest to find the holy grail of an efficient, cheap and environmentally-friendly biofuel.

Watch the “Biofuels: Beyond Ethanol” TV Story online, as well as find additional links and resources.

Sheraz Sadiq is an Associate Producer for QUEST on KQED Television.

Julien Guy: supernova cosmologistI’m sitting in the airport right now, passing time as I wait for my flight back to SFO. Looking at the clock now, I see that my jet lag future does not bode well. I awoke at 5:00 AM here and nearly 11 hours later feel like the day is over, yet it is only 7:50 AM in CA.

I spent the last week at a conference in the Italian Alps with about 200 skier/cosmologists. Mornings were spent in the conference hall watching 15 or 25 minute presentations. Afternoons were for the slopes. Evenings were back in the conference hall.

The conference started with supernova talks - I was fourth on the list. Being in the field, I had heard most of the results that were presented in the other talks. Ditto the other attendees’ perspectives on my talk. However, there were some new and very promising results from the Supernova Factory.

The supernova factory is a LBNL-based research group that focuses on “nearby supernovae”. By nearby, I mean only a few hundred million light years away. These supernovae occur in galaxies that are distant enough to be free of the gravity of the Milky Way and our neighboring galaxies but close enough to observe with smaller telescopes.

The supernovae observed by the SN factory are very bright compared to the supernovae I observe with the Hubble Space Telescope. The supernovae are bright enough to make very precise measurements at each wavelength of the supernova spectrum. Just like my earlier post on spectroscopy, the supernova light is imaged after passing through a prism. These images provide very detailed information about the molecules and atoms that are present in the supernova explosion.

The spectroscopic observations also tell us how one supernova may differ from another. The small variations in type Ia supernovae have been a mystery for quite some time. If we can learn the causes of these variations, these supernovae could be come even more useful for measuring distances in space.

There are several models and theories to explain the differences, but none has been extensively tested. A large number of bright nearby supernovae is required to test these models. Hopefully, a project like the supernova factory will provide that sample. In this conference, they only showed a handful of supernovae. All but one of these supernovae was well-behaved, fitting our current models. The last one differed enormously from the others, but the detailed spectroscopic observations lent evidence as to why this may be the case. The data is still being examined, but I am encouraged by the progress necessary if supernovae are to be used to explain the cosmology of our universe.

The presentations over the next five days covered a very large range of topics. Some conference attendees presented ideas that had never occurred to me. One that I found very interesting was an experiment to model the orbital paths of stars around the black hole at the center of the Milky Way. For those patient enough to watch these stars for 15 years, it should be possible to measure the properties of gravity and the black hole itself by looking for deviations in the stars orbits from our current models.

While the talks were very interesting and well-attended, I can’t help but comment on the other important side of this conference. That would of course be the skiing. The Europeans really have it right - they chose the site and the schedule with the perfect balance for leisure time. We were only ten miles from the tallest mountain in Europe, within site of the Matterhorn, had perfect snow all week, and had just enough time to enjoy it. I even had a chance to practice my amateur photography on the slopes. Now the next challenge will be to organize a conference in Tahiti!

Kyle S. Dawson is engaged in post-doctorate studies of distant supernovae and development of a proposed space-based telescope at Lawrence Berkeley National Laboratory.