Inhaltsverzeichnis
Falls es irgendweche Rückfragen gibt, so schreibe man diese an esa@fsmpi.rwth-aachen.de!
If there are any additional questions, please send an email to esa@fsmpi.rwth-aachen.de!
Auf dieser Seite mögen sich alle Menschen eintragen, die beim Projekttag Physik 2013 (Freitag, der 11.10.) Experimente betreuen.
In this Wiki, all tutors who are helping at the „Projekttag Physik 2013“ (Friday, 11th of October) shall register.
Die gelb gehighlighteten Versuche sind dabei nur von Mitarbeitern aus dem Physikzentrum zu besetzen, da es sich hier um „gefährliche“ Versuche handelt, für die die Betreuer sinnvoller Weise Erfahrung oder sogar eine Unterweisung in die Nutzung der Materialien vorweisen können sollten.
The yellow highlighted experiments are somehow „dangerous“ and thus, shall only be overseen by „professionals“ from the RWTH physics department.
Schichtenplan / Time Slots
(Versuchsbeschreibungen s. unten.)
(Experiment descriptions see below)
Time | hole in coin (2 people wished), Room: 26 C 402 | interference with hair (2 people wished), Room: 26 C 401 | pendulum (2 people wished), Room 26 C 201 | balloon rocket, Room: 28 B 110 | water rocket Place: In the back of building 28, floor 1, main door (next to the big lecture hall) | gusher, Place: In front of building 28 (southern door, floor 0) | pinhole camera, Place: 26 C 1xx (one of the rooms) | bridge and ship, Room: MBP 026 | Band generator, Room: MBP 015 |
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11:00 - 11:30 | Jan-Michael Mol & Farshad Foroughi | Sebastian Mann & Patrick Bethke | Pascal und Andreas | Marvin Hübener & Patrick Niedziela | Christoph Gordalla | Johannes Hamann | Marion Funken | Emily Hofmann | Jan-Niklas Siekmann & Philip Kramer |
11:30 - 12:00 | Jan-Michael Mol & Farshad Foroughi | Sebastian Mann & Patrick Bethke | Pascal und Andreas | Marvin Hübener & Patrick Niedziela | Christoph Gordalla | Johannes Hamann | Toni Voebel & Sabrina Smyczek | Emily Hofmann | Jan-Niklas Siekmann & Philip Kramer |
12:00 - 12:30 | Eugen Kammerloher & Stefanie Tenberg | Sebastian Mann & Patrick Bethke | Pascal und Andreas | Christoph Gordalla | Lukas Klamt | Jonas Bitter-Davidts & Joel Pommerening | Toni Voebel & Sabrina Smyczek | Emily Hofmann | Jan-Niklas Siekmann & Philip Kramer |
12:30 - 13:00 | Eugen Kammerloher & Stefanie Tenberg | Sebastian Mann & Patrick Bethke | Jan-Niklas Siekmann & Philip Kramer | Christoph Gordalla | Lukas Klamt | Jonas Bitter-Davidts & Joel Pommerening | Toni Voebel & Sabrina Smyczek | Marvin Hübener & Patrick Niedziela | Max Beutelspacher |
13:00 - 13:30 | Pascal Cerfontaine & Jennifer Arps | Jan-Niklas Siekmann & Philip Kramer | Tobias Ziegler | Lukas Klamt | Jonas Bitter-Davidts & Joel Pommerening | Toni Voebel & Sabrina Smyczek | Marvin Hübener & Patrick Niedziela | Max Beutelspacher | |
13:30 - 14:00 | Pascal Cerfontaine & Jennifer Arps | Jan-Niklas Siekmann & Philip Kramer | Tobias Ziegler | Jonas Bitter-Davidts & Joel Pommerening | Adrian Hauffe-Waschbüsch & Marco Nüchel | Nikita Malyschkin | Max Beutelspacher | Manfred Ersfeld | |
14:00 - 14:30 | Jan Dauber & Pascal Kaienburg | Olga Faley | Jan-Niklas Siekmann & Philip Kramer | Tobias Ziegler | Jonas Bitter-Davidts & Joel Pommerening | Adrian Hauffe-Waschbüsch & Marco Nüchel | Nikita Malyschkin | Luisa Krückeberg | Manfred Ersfeld |
14:30 - 15:00 | Jan Dauber & Pascal Kaienburg | Olga Faley | Jan Burger, Thomas Billaudelle | Marvin Knol & Jan Düchting | Jonas Bitter-Davidts & Joel Pommerening | Adrian Hauffe-Waschbüsch & Marco Nüchel | Nikita Malyschkin | Luisa Krückeberg, Jana Ammersbach | Manfred Ersfeld |
15:00 - 15:30 | Arne Hollmann & Richard Neumann | Olga Faley | Jan Burger,Thomas Billaudelle | Marvin Knol & Jan Düchting | Luisa Krückeberg, Jana Ammersbach | Adrian Hauffe-Waschbüsch & Marco Nüchel | Sebastian Arnold | Tiziana von Witzleben | Manfred Ersfeld |
15:30 - 16:00 | Arne Hollmann & Richard Neumann | Olga Faley | Jan Burger,Thomas Billaudelle | Marvin Knol & Jan Düchting | Luisa Krückeberg, Jana Ammersbach | Adrian Hauffe-Waschbüsch & Marco Nüchel | Sebastian Arnold | Tiziana von Witzleben | Manfred Ersfeld |
Versuchsbeschreibungen / Experiment descriptions
Die anderen Versuchsbeschreibungen folgen.
The other descriptions are coming soon!
Hole in coin (Institute peole only)
The task here is, to get a tiny hole into a coin, without completely destructing it.
To do so, there is various stuff, which could be used.
The solution idea is to freeze a banana with the liquid nitrogen. (This must not be done by the students but by one of the tutors.) Then, the banana can be used as a hammer.
Then, a fixing pin can be sticked into a cork. Now, this can be used as „nail“.
With the banana-hammer, the pin-cork-nail can be used to get a tiny hole into the coin.
To confuse the students a little more, other stuff will be there.
The goal here is, to let the students think about creative solutions for this pretty uncommon probem in style of MacGyver.
There is no need for a final presentation of the „master solution“, because the students may also find no result, which is not too seldom in physics.
Interference with hair (Institute peole only)
The task of this experiment will be to measure the width $ d $ of tiny objects (like hairs) with a monochromatic laser of given wavelength $ \lambda $. To do this, one profits from the fact, that the position of the diffraction minima is the same as in a single-slit experiment whith a slit of the same width $ d $. (Indeed, the basic goal in this experiment is, to understand why.)
A simpe derivation of the corresponding formula $d\,\sin\theta_{n} = n\lambda$ (in Fraunhofer approximation) can be found here: http://en.wikipedia.org/wiki/Diffraction#Single-slit_diffraction
To see, why the minima are at the same positions, consider three systems. First, consider the singe-slit, which we will indicate by $ s $, second, consider the hair ($h$) and finally, consider a free system, where the light ray is propagating without any barrier ($f$).
Let us denote the light's amplitudes on the screen in system $i$ as $A_i(\theta)$. Then, by the principle of superposition,
$A_f(\theta)=A_s(\theta)+A_h(\theta)$.
Assuming the light ray's diameter to be smaller than the position of the first minimum (which can always be gained by moving the screen away from the laser), we have
$A_f(\theta\geq\theta_1)=0$,
because outside the ray, there must be a vanishing amplitude. This implies
$A_h(\theta\geq\theta_1)=-A_s(\theta\geq\theta_1)$.
As what we can see are not amplitudes but intensities $I_i\propto A_i^2$, we can take the square of this equation and get finally
$I_h(\theta\geq\theta_1)\propto I_s(\theta\geq\theta_1)$,
which implies, that the positions of the minima (and indeed, all other critical points) are the same.
This derivation shall be presented to the new students in approximately 5 minutes. If they ask, one should spend another 2 minutes to explain the minima formula for the single-slit.
But the most important thing is to make clear, that we cannot observe the amplitudes directly, but the intensities.
Pendulum
This experiment is probably the one with the biggest part of physics.
The task is to measure Earth's gravity constant $g$ in the usual constant approximation close to the surface.
To do this, the students shall use a pendulum, constructed by a string and some screw nuts.
This system can be approximately described by the differential equation of the harmonic oscillator (Which can be derived by a force ansatz [driving component of gravity] and a Taylor expansion $\sin\varphi\approx\varphi$):
$0=\ddot\varphi+\frac gl \varphi$,
where $\varphi$ is the angle coordinate and $l$ is the length of the pendulum. Of course, this description neglects friction and is ony valid in the usual small-angle approximation.
In this case, the angular frequency $\omega$ is given by
$\omega^2=\frac gl$
which leads to
$g=\omega^2 l$.
(This can for exampe be shown by inserting $\varphi(t)=\hat\varphi\sin{\left(\omega t+\phi\right)}$ into the differential equation.)
The students shall also think about the error on $g$. So, not only the previous part has to be discussed, but also the basic formula for the propagation of errors:
$\sigma_y^2=\sum\limits_i \left(\frac{\partial y}{\partial x_i}\right)^2\sigma_{x_i}^2$
There is no need to derive this formula, but one should present the derivation of the special case of relative errors.
Assuming $y=\prod\limits_i x_i^{\nu_i}$, we have (by the error propagation formula):
$\sigma_y^2=\sum\limits_i \left(\nu_i\cdot x_i^{\nu_i-1}\prod\limits_{j\neq i}x_j^{\nu_j}\right)^2\sigma_{x_i}^2$
Division by $y^2$ then yieds:
$\left(\frac{\sigma_y}y\right)^2=\sum\limits_i \left(\nu_i\cdot \frac{\sigma_{x_i}}{x_i}\right)^2$
With this in mind, the students shall estimate $g$ and $\sigma_g$ as precisely as possible and the shall also think on how to improve their measurement.
For example, a smaller amplitude $\hat\varphi$ leads to a better justification of the small-angle aproximation and measuring $N$ instead of one period reduces the error on the corresponding time $T_N$, which will be dominated by the reaction time of the person who controls the chronograph, by a factor of $\sim N$.
The students shall also think about any other effects that could disturb their measurement. (For example, the string wil not be perfecty rigid and thus, the length $l$ could vary a little bit. And there is also friction!) They shall try to quantify the errors and get a feeling for the dominant ones.
More on the topic can be found here: http://en.wikipedia.org/wiki/Pendulum
The presentation of the differential equation and the related quantities should not take more than 4 minutes. The error propagation formula and the derivation of the relative-error propagation formula could take another 3 minutes.
Balloon rocket
In this experiment, the challenge is, which studentgroup can build the best balloon rocket.
The idea is to bend a balloon to a straw which is fixed on a long cord. Who reaches the furthest point, wins.
The material, the students get, is:
- a balloon per group
- tape