Remote Entry

My boyfriend’s apartment recently upgraded from metal keys to key fobs and I recently moved offices, retiring the old code for pressing my student card against a reader.  It got me thinking, how exactly do these devices work?  What is their security like?  Unfortunately, the internet understands “fob” as something completely different, however, I did find some interesting information regarding remote entries, such as to your car.

How remote entry works:  http://auto.howstuffworks.com/remote-entry2.htm
Reprogramming a remote (including how to use one remote for two cars): http://hackaday.com/2010/07/13/key-fob-programming/

Physics & Astronomy Colloquium – THURS. 26th January – DR. BLAINE CHRONIK, Western

Poster: http://www.physics.uwo.ca/colloquia/Colloquia%20Notices/2011_2012/CHRONIK%20Colloquium.pdf

 

The University of Western Ontario
DEPARTMENT OF PHYSICS AND ASTRONOMY

 

PHYSICS & ASTRONOMY COLLOQUIUM

 

Date:           Thursday, 26th January 2011
Time:          1:30 p.m.
Location:    Physics & Astronomy Seminar Room 22

 

Dr. Blaine Chronik
Physics & Astronomy Department
The University of Western Ontario

 

“Variable fields in MRI: progress, opportunities, and challenges”

 

ABSTRACT

 

Over the past 8 years or so, we have worked on Magnetic Resonance Imaging methods and technology which are distinguished because of their focus on the use of rapidly varying, strong magnetic fields.

Our approach has evolved, from what was purely “laboratory,” preclinical implementation, to our current efforts which focus on systems for use in clinical MR scanners.

In this talk, I will describe a new method of MRI in which we strive to produce very specific MR image contrast due to the presence of a chemical contrast-agent, only when that agent is bound to target molecules of interest. This represents a means to achieve contrast specificity in MRI that has not been previously available. The method is called “dreMR”: delta relaxation enhanced MR (reference: Magn Reson in Med, 61(4):796-8002 (2009)). This technique requires a major change to the MRI system architecture¾specifically, the ability to vary the main magnetic field strength as a function of time. I will review the concept behind the method, our preclinical technological implementation, and we will discuss the applicability of the method for human-scale subjects. Along the way, we will also review the wider range of MR system developments we’ve worked on, and some of our future projects.

Coffee & cookies will be provided.

Thinking – incorrectly – about waves

Last year I supervised Erin Kennedy’s honors thesis research. Erin plans to be a teacher, so she was interested in doing a thesis on physics education. Her project involved studying how well students understood some basic ideas about mechanical waves. Her guinea pigs were last year’s Physics 2110 and Physics 1502 classes, which I taught. She gave the second years a diagnostic test (developed by Wittmann as part of his 1998 PhD thesis at the University of Maryland) early in the course, and again at the end. She analyzed the results of the pre-test to see where students held misconceptions about wave physics, then designed and delivered lessons intended to help correct these misconceptions. The post-test was intended to show how well the students’ understanding improved as a result of the inspired teaching they received.

 

Wittmann had earlier used his diagnostic test on first-year students in the U.S. He (and earlier researchers) found that the students held a number of interesting misconceptions. For example, many students thought that if you flicked an stretched string harder, then the wave you produced would travel faster. (It won’t, by the way. The speed of the wave is a property of the string – it depends only on the mass density of the string and the tension, and doesn’t depend on the way the wave is produced. But you knew that.) Wittmann figured out that many students were taking ideas from their understanding of the motion of objects and incorrectly applying them to wave motion. In other words, students were trying to treat waves the same way they would treat a baseball: If you throw a ball harder, it moves faster. Therefore, if you hit the string harder, the wave will move faster. When I read Wittmann’s work, I was astounded by this. I had taught first-year physics, and waves in particular, many times, and I had never knowingly run across this way of thinking. Clearly students in the US must be a lot dumber than students in Canada!

 

Well, guess what Erin found? Our students are just as dumb as the US students. To be a bit more polite, our students held exactly the same misconceptions as those found in the previous studies. She did find that student understanding improved from first year to the end of the second year course, which is reassuring. In many cases, however, these misconceptions persisted even after the students had studied waves in first year, and then had a full course on oscillations and waves in second year! I confess I was surprised by this.

 

What I find really interesting, however, is that the same common misconceptions have been found in studies on students from the US, Canada, France, Australia, and Thailand. It seems that the misconceptions cannot be blamed on cultural factors or on a particular educational system. They are universal. I suspect the same is true of the common misconceptions that have been identified in other areas of mechanics. Why? Why would a kid from Thailand independently come up with the same wrong ideas about wave propagation as a kid from France? It must have something to do with the way our brains work, the way our minds try to make sense out of the world. It’s too bad that our brains evidently come up with something that’s not physics, but, to be fair, it took people as smart as Galileo and Newton to figure this stuff out in the first place!

Job Opportunity: Canada Research Chair in Exoplanets

The Department of Physics and Astronomy and the Centre for Planetary Science and Exploration at The University of Western Ontario, Canada, invite applications for a Tier 2 Canada Research Chair in the area of Exoplanets. The appointment will be at the rank of Assistant or Associate Professor, within the Department of Physics and Astronomy. The selected candidate will be nominated to a Tier 2 Canada Research Chair and appointment to the faculty position will not be conditional on the candidate being awarded the Canada Research Chair.

 

Expressions of interest are invited immediately. Consideration of applications will begin on February 15, 2012and the position will remain open until filled.

 

Full details of the announcement can be found here.

Extinction? Star Cluster ‘Death Rays’ #westernu

A recent article [http://www.newscientist.com/article/mg21328465.400-did-star-cluster-death-ray…] suggests that a blast of radiation from a nearby star cluster, specifically gamma rays, could be the cause of mass extinctions.

Gamma-Ray Bursts (GRBs) occur when a massive star explodes (supernova) or when 2 neutron stars merge. If a GRB occurred in a star cluster we can trace its position and speed to deduce whether it coincides with past extinction events [the European Space Agency’s Gaia star-mapper (2013) will determine the position and speed of star clusters].

The author calculated that at least 1 GRB has occurred within striking distance of the Earth in the last billion years.

 

Paper: arxiv.org/abs/1112.1792

 

What is the Schumann Cavity? #westernu

The Schumann cavity surrounds the Earth and exists between the surface and the bottom of the ionosphere (~80 km). Schumann resonances (SRs) are peaks in the extremely low frequency (ELF) portion of the Earth’s electromagnetic (EM) field. These resonances are excited by lightning discharges in the cavity.

This cavity resonates at about 7.83 Hz (fundamental) and experiences little attenuation. Other bodies in the Universe have their own SRs that require certain parameters to be satisfied:

1. A spherically-shaped body

2. Conducting lower and upper boundaries separated by an insulating medium

3. Source of excitation of EM waves in the ELF range

The most popular application of the SR would be that of wireless energy transmission (see Colorado Springs Experiment 1899). The idea revolves around the fact that there is an enormous amount of energy in this cavity that goes unused.

 

Jokes from the desk of a grad student: Vol 2 #westernu

Q: What is the simplest way to observe the optical Doppler effect?
A: Go out and look at cars. The lights of the ones approaching you are white, while the lights of the ones moving away from you are red.

“If there was no such thing as night the Sun would have run out twice as fast.”

Black holes are where God is dividing by zero.

After eating his first meal on the Moon, the astronaut reported, “The food was good, but the place lacked atmosphere.”

Why did Captain Kirk go into the ladies toilet?
To boldly go where no man has been before!

 

Electrons in Motion

By exciting nano-scaled silver with laser pulses that last for only femtoseconds (that’s 10^-15), a team of ressearchers at California Institute of Technology have been able to trace the energy individual electrons gain. The ability to map the electric fields around the structure, and the likely positions of the electrons, may translate to direct study of the interactions of particles, molecules, and even cells.