Can We Stop the Zombie Apocalypse?

06.18.13 0 Comments

posted by: Thomas Yemc

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How are we going to stop Contagion if it hits?  Why do flocks of birds move in the way that they do?  How do we stop the population growth that seems to be shooting out of control?  What is the best strategy to stop the zombie apocalypse?!

Any of these questions can be answered by use of a simulation program called NetLogo.  At NDQC this summer, a group of high school students and teachers are attempting to find answers to some of these questions.  By running simulations on this program, students are able to test certain variables on these situations to examine what the important variables are.  In a Contagion simulation (screenshot below), the student can change how contagious a disease is to watch the effect on how it spreads.  In a bird flocking simulation (screenshot above), the student can examine the effects of a hawk flying through the flock might have.  In a zombie apocalypse simulation the student can change whether or not the military can use nuclear power to destroy the zombies.

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There are a multitude of possibilities to research with or just to play around with.  Take a look at the program for yourself…

NDQC Biocomplexity Website

Running a Few Simulations

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Summer at ND QuarkNet

06.18.13 0 Comments

posted by: Thomas Yemc

Expect great things from the Notre Dame QuarkNet Center (NDQC) this summer as a group of  professors, teachers, and high school students embark on research in the field of particle physics.  A series of seven specific research projects are to be conducted over the next few weeks.  I will be attempting to track the progress of these projects by taking photos and writing blog posts on any important happenings.  Below I have written a brief overview of each of the seven projects and their goals for the summer.

Biocomplexity:

In this first project, the students and teachers will be examining simulations of certain events that may be experienced in our own lives as well as events like a zombie apocalypse that may be a bit less common.  They will use a computer program called NetLogo which models events like this giving the user the ability to change certain variables and observe how the changing of that variable may affect the outcome. Events that can be looked at include spreading of a disease through a population, flocking of birds in the sky, protein binding, blood clotting, myxobacterium movement, and others.  Below is a screenshot of a sheep/wolf simulation like one may see when they use NetLogo.

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Cosmic Ray Detectors (CRDs):

This project will be examining the cosmic rays that come shooting in from space and examine properties of the muons that are detected.  This project focuses on detecting the muons and separating them from anything else that the detector might pick up.  A muon is like an oversized electron and they can be detected by placing a series of ray detector paddles one on top of the other.  Only the muons can make it through the detector far enough to be counted by all four detector paddles.

CMS Upgrade:

The CMS Upgrade project is focused on testing and building parts to be used in an upgrade done on the CERN Large Hadron Collider (LHC) in Switzerland.  This upgrade is to be done on the Compact Muon Solenoid (CMS) detector (pictured below) in a few years as physicists look to advance their knowledge in particle physics.  The CMS is one of four particle detectors in the collider.    The LHC has the ability to fire protons at incredibly fast speeds to do things such as recreating energy densities of the Big Bang.  The students and teachers on this project will be testing certain parts and pieces to be added to the detector to see what works best.  This project will be a very hands on project with some potentially very important results that hopefully will end up being used in the LHC.  The LHC currently includes over 500 components designed and constructed in part by high school teachers and students at NDQC.

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CMS Data:

The CMS Data group will be working on the CMS detector at CERN as well but they will be looking at the current data that has been released.  The Data group will try to look at the data that has been released and make it accessible.  The students and teachers will change certain graph plots to attempt to find meaning in it all.  They have available hundreds of thousands of plots to use in gaining insight into the physics of the LHC.

DVT:

The Digital Visualization Theatre (DVT) is the digital planetarium located in the Jordan Hall of Science at Notre Dame.  The job of the DVT group is to continue to write and produce a show in the digital planetarium for the general public on the LHC and its detectors.  The main focus on this project will be constructing all of the animation that is necessary for the show to happen.  Using a Hollywood level animation program (Lightwave), students and teachers will have to build everything themselves on the computer and then make it all into a show for the planetarium.  This will be no easy task, however, as some of the more complicated pieces to the show may take hours to complete.

Astrophysics:

The astrophysics project, as the name states, will primarily be studying the sky and stars.  One thing they will do is observe solar flares on the Sun which are a source of many strong cosmic rays.  They will be working on the roof of the Jordan Hall of Science with different telescopes primarily when it is dark out to take pictures of many different astronomical happenings in space.  They can expect to see some incredibly extraordinary events through the telescopes.  The students and teachers will collect their data late into the nighttime hours.  Then they will be able to analyze their pictures in the morning back in the lab and make observations based on what they saw the night before.

Project GRAND:

The study of Gamma Ray Astrophysics at Notre Dame (GRAND) is conducted in a large field off campus (below).  It is a series of sixty four cosmic ray detectors much like the ones that I talked about earlier.  The detectors function the same way as the CRDs in that they are stacked on top of each other and detect muons.   These particular detectors differ, however, in that they are much larger than the small cosmic ray detectors that will be used in the lab.  Each detector is housed in a building that looks a bit like an enlarged doghouse.  A key part to this project will be simply keeping the experiment running by doing maintenance on the detectors when needed.   The students and teachers also will look at the data, which is collected 24/7, and draw conclusions based on the muons that are detected.

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Summer Art Camp opportunity for middle schoolers

06.12.13 0 Comments

posted by: Tom Loughran

Here we pass along this announcement, flyer and registration form from the Notre Dame Center for Art and Culture.

To download the registration form immediately below, just find and click the “slideshare” button to the lower left of the frame; on the top of that slideshare page, find and click the “save” button, as illustrated on the screengrab further below.

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One Book, One Michiana science activities

04.10.13 Comments Off

posted by: Tom Loughran

Come rally around the Saint Joseph’s County Public Library’s One Book, One Michiana effort by supporting these science activities this month. What a great idea!

(Click the Full Screen button on the lower right corner of this slideshare document to get a closer view.)

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Spring into Science and Engineering

04.05.13 Comments Off

posted by: Tom Loughran

Coming this Spring are two excellent opportunities for student participation in Science and Engineering. The Exoplanet Masterclass is for high school students; the National Robotics Week event is open to the general public.

Errata: An earlier version of this post incorrectly reported both dates.

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Listening more carefully to echoes of the Big Bang

04.03.13 Comments Off

posted by: Tom Loughran

Maybe you’ve seen the picture: the best image we have of the cosmic microwave background radiation, from the Planck mission. This newest image of the oldest things is creating a bit of stir. It’s important to know something about why.

Cosmic microwave background radiation is the observable limit of the light that is emitted from the big bang. For most of us this has an unfamiliar ring, but it’s not so hard to grasp. When we catch a glimpse of the sun, light has just traveled the ~93 million miles to reach us, which took about 8 minutes. As we look further out–to the nearest star, say–it takes light longer (about four years) to cover the distance. But it turns out that the space over which that light is traveling is actually stretching: we know this from watching the chemical signatures in the light, which shift with distance in just the way that sound waves stretch (and seem lower in pitch) when their source (say, an ambulance) is moving away from us. Our speeding away from the source makes the wavelength of light more red when we detect it, just as sound waves seem lower when their source is fleeing; we call this change in light “red shift.” The upper limit of red-shifted light is from the oldest, furthest-away sources. These sources–like points on opposite ends of a balloon while it is being blow up–are fleeing every other point on the balloon most rapidly, and are stretched into longer wavelengths, in the microwave region.

This oldest, most red-shifted light from the big bang is the cosmic microwave background radiation. And it’s not behaving quite as the standard model of cosmology–what most scientists accept as pretty well established–predicted that it would. In many ways, that’s a bit misleading: it behaves as expected in a great many respects. But not in all. Watch the short video below to find out more. And stay tuned: Planck is still taking data, and what it has already delivered has stirred a flurry of scientific activity. It’s worth stretching a bit to follow the conversation.

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Expanding Horizons for middle school girls on April 27

04.02.13 Comments Off

posted by: Tom Loughran


The St. Joseph Valley Local Section of American Chemical Society has given a donation to provide scholarships to cover the cost of the conference for girls who indicate on the registration form that their main interest is in chemistry or earth sciences. The scholarships are available on a first come, first serve basis.

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Images from the 2013 Forum (that you can actually see)

03.08.13 Comments Off

posted by: Tom Loughran

Our sixth annual Collaborating for Education and Research Forum was held on February 23, 2013 in Jordan Hall of Science on the campus of the University of Notre Dame. Over 140 attendees participated in the event. Thanks to all involved. Below is the “raw data” from our photographer. We had some technical difficulties in an earlier attempt to share them here; these seem to now be resolved:)

Images courtesy of Matt Cashore, University of Notre Dame.

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All God’s children should code

02.28.13 1 Comment

posted by: Tom Loughran

I got to Code for South Bend on Saturday…or rather, I got to the presentation on the projects they undertook that day. It was a fantastic experience. I had spent six hours earlier in the day listening to some of the best ideas around for promoting STEM education in Michiana. By the end of my time at Code for South Bend, it was clearer to me than ever that even the best of our typical conversations about STEM education are overlooking a hugely important element that is crucial to Michiana’s future. Kids need to code. Take 10 minutes to watch this very fine defense of that claim.

Want to learn to code, but don’t know where to start? Consider starting here, at Code Academy. See my first mistake and first success, below. There are many free resources beyond this one, but I’d start here if you’re starting from scratch. (You can move on to Scratch, a free and easy-to-use program, later:)

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Here’s work that one local High School student has done with MATLAB, very early on in the learning process. (He had already learned to code in another language, Java, and was only just a month or so into learning MATLAB.) Very plainly, he’s learning to tell the computer what he wants it to do. For those really interested, his code is here.

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Got tech? Code for the Bend.

02.18.13 Comments Off

posted by: Tom Loughran

This fantastic event, scheduled for this Saturday, February 23, conflicts with our Collaborating for Research and Education Forum. But if you have the time and the spark, consider attending. Register for Code for South Bend here. Even if you have more interest than technical aptitude, there are projects here for you, including the writing of a South Bend-area wiki.

If you are attending the Forum, consider joining the Code for South Bend event (as I will) for the concluding presentation of projects at 5:00 pm. Hope to see you there!

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