Akamai Maui Short Course AO Demonstration Activity Wiki
Basic Outline:
This 3-4 hour activity will take place at the end of theAkamai
Maui Short Course. There will be ~15 students who have just completed
several activities, including: Camera Obscura & Sun Shadows, Lenses &
Refraction, Build-a-Telescope and Color-Light-&-Spectra, as well as a
Haleakala & AEOS tour and the "High-Tech Investigations" activity.The 2007
schedule is here. The activity will have an outline like this:
Activity Outline:
1.) Motivator Talk ~10min
A talk to set the context - why is AO important. Show lots of pretty pictures
and animations. Discuss how images can be "sharpened". Show stars twinkling and
some pre-post images but do not show any block diagrams, don't use any
key-words and don't give instrument details.
2.) A Teaser on the AO Demonstrator ~10min
Show the AO demonstrator as a system - show them open and closed loop. Show how
an image gets sharpened. Don't touch anything really, just point and talk -
creating an interest.
3.) The Three Workstations ~2hrs
Wavefront "Aberration" (how do aberrations work?)
Wavefront "Sensing" (how do we quantify the distortion?)
Wavefront "Correcting" (how do we fix the distortion?).
There will be 3 groups of roughly 5 students. Each group will do each station,
but the final station will be the "specialty" for presentation. 30min, 30min,
45min. There will be small breaks between stations to give the students time to
organize their thoughts both to themselves and each other. Writing in their
notebooks is encouraged.
4.) Poster Presentations
~15min. Students specialize in their third station and prepare a poster placing
their station into the full AO context.
5.) Presentations
~20min. Student groups present their posters on their station to a facilitator
panel with the rest of the class as audience; feedback provided on presentation
skills
5.) Synthesis Talk
~20min. A summary talk of how the AO system works.
[My comments in color -- Scott]
OK So I see the outline. Here's how I see it (I realize this is a repeat of the same info...)
Introduction ~10min
AO Workbench Teaser starter ~10min
Split into 3 groups ~couple minutes
Station 1 ~30min
Break and rotate ~5min
Station 2 ~30min
Break and rotate ~5min
Station 3 ~45min
Poster preparation ~15min
Poster presentations ~20min
Something may be missing here. In your "Evidence" it
seems like you're looking for block-diagram, "systems thinking" understanding
of an overall AO system, but I don't really see that emerging yet. What do you
think about having the students do another rotation, maybe 5 minutes per
station, to go back over things after they've seen their peers presentations,
and somehow help them assemble the full block diagram of an AO system? There
would need to be some kind of new prompt here, a new task you're assigning
them, not sure the wording, but something like: "Now how would you explain an
entire AO system? What level of detail? What might you draw?"
What do you think about providing them with some kind of very-minimal block diagram, to give them a little structure to get started?
What about they do the extra ~15min of rotation and then they convene as a whole group at the AO workbench to work out this block diagram communally? (I could see an argument for doing it in smaller groups or individually too, just throwing the idea out there.) So this might take a total of 15-30min total.
Synthesis ~20min
TOTAL time: about 3hrs 40 minutes including the new suggested part.
STUDENT BACKGROUND:
Students will mostly be from engineering and going to school in Hawaii
This will be the last activity for the course
Students will have some prior lab experience
Students are very group-oriented
An intentional effort should be made to ensure that the activity environment is encouraging of female students to contribute as much as the male students
This is the end of the week when students will have been conditioned to certain attitudes about inquiry -- like that it's ok to manipulate all the materials. This may be relevant for the wavefront sensing station.
Students will have dealt with the ray nature of light but not so much its wave properties (yes, there is a spectroscopy day but we're really not dwelling on the dual nature of light). More on this below.
GOALS:
Content:
wavefronts, phase conjugation, tilt of a wavefront = changes in focal point,
there are many different kinds & types of aberrations.
Light behaves like waves... Well... at the "wavefront" sensing station they'll use a raybox, emphasizing the ray nature of light and visualizing a concept that's perpindicular to the wavefront. I don't think the concept of the wavefront will emerge on its own. It would be fair to introduce it in the introduction somehow but it doesn't really fit the pretty-pictures-with-AO theme that's currently planned there. Ideas?
There is a continuous feedback mechanism between the wavefront sensor and the deformable mirror
Phase Conjunction is needed for the deformable mirror to correct the aberrated wavefront. Again it would be good to think about these concepts like "phase" that the students aren't really going to see. I think what they'll take away from the Correction station is that the correction has to un-do whatever has been done. That may mean "phase conjugation" to an expert, but...
The incident angle of incoming wavefronts can be measured by the displacement of foci on the image plane from an array of lenses
Aberrations can be chaaracterized by their scale and time-dependence
Process:
breaking a complex system into simple components, identify tradeoffs, use
feedback & control mechanisms, communication & summary (synthesis),
apply recently acquired knowledge.
Students will find through experimentation that there is a trade-off between the strength of a signal and the amount of distortion
Students will formulate hypotheses before each experiment to guage their prior understanding of the phenomena and compared it to the understanding they possess during synthesis
Students will communicate their results to both one another and to the facilitators
Students will apply knowledge as apllicable from their prior activities,
especially those on leses and refraction.
Nature of Science:
Complex systems are built by combining simple components & ideas, use &
make creative solutions by combining and adapting existing technology to new
situations.
Attitude:
confidence and comfortable handling expensive & complicated machinery,
no-fear of black boxes, excitement.
Operationalized Goals:
Manipulate the wave-like behavior of light by applying corrections to aberrated
wavefronts (at a pupil).Same comments. Does it harm
anything for them to say that they are manipulating bundles of rays (which the
rayboxes will illustrate for them)? When do we expect the term "wavefront" to
come up? (I notice it is assumed as vocabulary in some of the station
descriptions below.)
Gain confidence in using high-end technology by breaking down a complex system
into simple components (WF aberration, sensing, correcting).
Gain experience and confidence in testing unknown technology by using simple
aberrators to find and exceed the limitations of the AO demonstrator.
Articulate the effects and consequences of different aberrations on an image
and express how these differences motivate and affect system design (AO needs
high time & spatial-freq response).
Use recently acquired knowledge (lenses) and basic technology (lenslet array)
to describe & measure complex phenomena (tilted & aberrated
wavefronts).
Articulate a method of wavefront tip-tilt measurement using spot position
(express the inversion of the WF sensing activity - spot position = wf tilt
just as wf tilt = spot position).Same
comments.
Note that these are not comments about whether you all know what you're talking about --- of course you do. I'm just trying to see it from the students' perspective. There are multiple correct ways to talk about these same issues and I think the language that the students will have is related to rays and geometric optics. For instance, other ways without mentioning the wavefront we could say that the lenses at the Shack-Hartmann station change incident ray angles into image positions. We could say the same thing using Fourier transform language (a lens just Fourier transforms angles to positions and positions to angles). Or we could talk about phase and wavefronts. Any thoughts?
EVIDENCE:
Block Diagrams of the full AO system-- This is the part that I think could use some support.
Varying solutions to the wave correction with lists of advantages and disadvantages to each solution-- How can we have the materials around to suggest other solutions? Something to think about.
Demonstrating the inverted shape of the correcting mirror with the aberrating mirror
Plot relationship between the tilt of the incident light and the offset of the wave detector
FACILITATION:
Leading questions when necessary
Lab notebook checks
The synthesis review panel (having students defend their conclusions before the facilitators)
Prompt sheets instead of worksheets.
Also: "An intentional effort should be made to ensure that the activity environment is encouraging of female students to contribute as much as the male students"
============Detailed Descriptions & Notes======
General comments about the station descriptions.
Sarah has done a really nice job of being quite detailed and having 2 concrete plans for 30- and 45-minute rotations. The other two stations should be this well-planned-out.
(Of course I have comments on her plans too, but the level of detail is really good.)
The focus is to teach interns how to get up to speed on a project quickly and
to be able to test the limitations of a "black-box". In the beginning of the
session, tell them that they will confront equipment or techniques in their
internships that they are unfamiliar with. They will have to play with the
equipment, learn how it works and get an idea of it's capability. This should
be outlined in the intro discussion.
The 3 Stations in Detail:
Light Distortion (Mark)
Concept:
Light passing through a medium can become distorted before entering an optical system, resulting in a "poor quality" image. This image can be "corrected" by the AO system, but this correction has its limitations based on the scale size and time variability of the distortion.
Overview:
This station allows the students to manipulate the light distortions entering the AO system. The main point of the exercise is to familiarize the students with scale- and time-variable distortions, and how those can or cannot be corrected by the AO system. The students will also have an opportunity to manipulate the field-of-view of the output image by swapping sets of columnating lenses. The students should walk away with an understanding of: 1) What properties make up a "good quality" image, 2) The process of testing extreme conditions to determine the limitations of an unfamiliar system, 3) The different ways in which a medium can distort an image, both static and time-variable, and 4) How to manipulate the input into a system and monitor the output so that a "black box" can be tested.
Materials:
Distortions: The distorting materials will be pre-fashioned to be easily exchangable within the optical path, able to be held steady with minimal vibrations if desired, and have a wide variety of distorion scales. A rig should also be made to swing or rotate the media in a regular manner for time-variable testing. If it can be done practically, gaseous and/or liquid mediums should also be available to emphasize the role of the atmosphere in distorting incoming light from space.
Prompt Sheet: Prompt sheets are to contain leading questions to be worded in a way that points the students toward specific avenues of experimentation without making the answer obvious beforehand. Some points for the sheet may include: 1) A list of all the materials available for the students to work with, 2) Encouragement to define how they know if the AO system is correcting an image... correctly, 3) Suggestions of what types of data should be recorded, 4) Challenges to discern the relationships between the scale and time variation of the media with the image quality, 5) A request for the students to quantify the limitations of the AO system as best they can
Lab Notebooks: Facilitators are to check the students notebooks on occasion, primarily as a means of determining where the students are conceptually without necessarily having to disturb the students themselves. Anything written in response to the prompt sheet should also end up expressed in the notebooks.
Facilitation:
30-min rotations:
0 min: Quick verbal intro to station and emphasize which materials are available for experimentation
0-10 min: Let them "play around" with no interference
10 min: Quick check to see if the students are recording their observations, and if they are defining what a "good image" is
15 min: If they do not do so on their own motivation, facilitators should encourage the students to shift, spin, or otherwise disturb the media to induce time-dependent distortions.
20 min: If they havn't done so yet, encourage the students to test the extremes of the distortions and see how the AO responds
25 min: Check to see of the students are recording the relationships and limitations they are finding
Additions for final 45-min rotation:
30 min: If they have not done so already, encourage the students to experiment with the field-of-view, and whether changing ti can improve the image quality in spite of the distorions
35 min: Ask students to try and explain how the media are distorting the image given what they know from the distortion detection station, as well as what might cause the limitations of the AO system based on their experience at the distortion correction stationAn idea: "at the last station you were at, you bent the mirror yourself to correct the image. Is there someone doing that in this system? If not, how is it done here? what might be the limitations of that setup?"
If there is time to do so, this is when the students would be
allowed to see the "guts" of the AO system
Wavefront Sensing (Sonnett)
The purpose of this station is to allow students to realize ways in which we
detect and quantify wavefront distortion. This station does *not* handle how to
correct for these distortions...
================================================================
Initial set-up: Three to four ray boxes will already be aligned with each other
so that every wavefront is parallel to the box onto which the rays project. An
equal number of lenses will be placed in front of the ray boxes at varying
angles, so that they roughly focus the light rays onto the side of the box.
Graph paper and tape or pushpins will be set aside, but not actually placed on
the side of the box. The students should have their lab notebooks, pencils, and
calculators if they think they'll need them. I think this design also calls for
a small poster board with the synthesis questions on them (which won't be
revealed until the synthesis), so that I don't have to take time verbally
posing them... Also, if possible, I'd like to have some different lenses set
aside for the 45-minute group so they can play with them after their
synthesis.
================================================================
30 minute shack-hartman activity (group of 5):
0 min) Begin with a task-oriented statement: "Using these ray boxes, lenses,
and other materials available here, you can make a model of how an AO system
senses and quantifies exactly what is happening to an image."
1 min) have the students play with the set-up.
6 min) 5 minutes into the activity, if they haven't figured out that you can't
change the ray boxes or the lenses, then prompt them with the following
questions: -- what do the ray boxes represent in a real-world situation?
-- what do the lenses represent?
-- what does the grid represent?
-- what do the ray boxes represent?
If they still don't get it a minute later, then tell them that the ray boxes
and lenses have to remain fixed. Over the next 15 minutes, the facilitator
(that's me!) should be going around, briefly inquiring about what they've
written in their notes. A good way to check the success of their progress is to
make sure they place the graph paper against the side of the box and to look
for the beginnings of a table or plot.
You could use your judgment on other groups, and instead
of asking a series of directed questions, you could ask for a more open-ended
explanation, then use these questions only to fill in gaps (or to suggest
things that need to go in their notebooks). This comment applies to both the 30
and 45 minute versions. What do you think?
21 min) synthesis: pose all these questions, ask them to write answers down in
their notebooks, then share them in a group (if time is short, we'll just have
each person answer one question).
-- how do you think we detect distortions in the real-world situation?
-- can you brainstorm any ideas on how to correct for this distortion (i.e.,
what's the next step)?
-- can you think of any limitations or special considerations within this
set-up?
-- what do you think are the main differences between this model and the actual
component of the AO system?
================================================================
45 minute activity (group of 5):
0 min) Begin with a task-oriented statement: "Using these ray boxes, lenses,
and other materials available here, you can make a model of how an AO system
senses and quantifies exactly what is happening to an image."
1 min) have the students play with the set-up.
6 min) 5 minutes into the activity, if they haven't figured out that you can't
change the ray boxes or the lenses, then prompt them with the following
questions: -- what do the ray boxes represent in a real-world situation?
-- what do the lenses represent?
-- what does the grid represent?
-- what do the ray boxes represent?
If they still don't get it a minute later, then tell them that the ray boxes
and lenses have to remain fixed. Over the next 15 minutes, the facilitator
(that's me!) should be going around, briefly inquiring about what they've
written in their notes. A good way to check the success of their progress is to
make sure they place the graph paper against the side of the box and to look
for the beginnings of a table or plot.
21 min) synthesis: pose all these questions, ask them to write answers down in
their notebooks, then share them in a group (if time is short, we'll just have
each person answer one question).
-- how do you think we detect distortions in the real-world situation?
-- can you brainstorm any ideas on how to correct for this distortion (i.e.,
what's the next step)?
-- can you think of any limitations or special considerations within this
set-up?
-- what do you think are the main differences between this model and the actual
component of the AO system?
At the end of the questions, ask for further comments/questions, and then ask
the students to think about how they would want to present the results of their
investigation.
31 min) allow the students to go back to the station and play more, hopefully
fleshing out their tables and plots. If possible, I can let them play with
different lenses (diverging, mixed focal lengths, etc.). Facilitation should be
similar to before the synthesis, this with an emphasis on how they want to
present results. The idea is to get them thinking about their posters and what
they'll need when writing them.
Wavefront Correcting (Dave)
This station makes use of the "bendy mirror". A Fresnel lens is put on a table
top to make a collimated beam from a lamp (with an F cardboard cutout). This
collimated beam goes on to an "aberrator" - a mirror bent in a simple parabola.
This aberrator is "hidden" in a cardboard box so the students can only see that
the aberrator is a warped mirror. This beam is then bounced off a flat mirror,
focused, re-collimated, and refocused on to a screen. The way to un-do the
aberration is to put in another bendy mirror in the shape of a parabola in
place of the flat mirror. The activity goes like this - first, the aberrator is
bypassed by placing a flat mirror in front. The students are shown the image of
the F. The bypass mirror is then removed and the image gets fuzzy. The students
are told to "fix" the image. They are told to not touch the lamp, first lens,
or aberrator. The instructions are left vague enough that they should confront
various "fixes". They have access to an image plane and can "stop the beam
down" and remove some of the aberration at the cost of a dimmer image.
The last time this station was done (45min), the students all instantly started
moving the lenses around. This time we would like them to see the "stopping the
beam" solution. With 15min remaining, if the group has not discovered this
solution, some facilitation should be used. We would like to hear something
like "we can block some of the light and the image gets sharper, but it gets
fainter too". Students will be encouraged to write down their observations
frequently. We would like to see them get the concept of phase-conjugation -
the aberrator and bendy-mirror parabola shapes match.
How can we draw out students' thinking in this station?
Usually they try lots of things and make quick decisions about what is and
isn't "working" but how can we get them to articulate what "working"
is?
I think there needs to be a clear statement at the beginning of the station
about recording experiments in their lab books. Leaving a record of what they
did and what they observed is critical for us and them. Perhaps facilitation
can be avoided by making a statement at the beginning of the workstation saying
"Make sure to record all observations in your notebooks. What fix did you try?
What does the image look like before and after you try something? Record that
data in your notebooks".
Facilitation Notes
As facilitator, are there ways you can help/support
students without giving anything away? What paths have you seen and how would
you like to respond to them? How can we support the alternate, pinhole
path?
There are several facilitation problems that might happen here. Typically, the
students immediately start playing with the Fresnel lenses. This is a good
thing.... However, we've shaved off some time from this activity and there are
a few concerns. One is that students finish too early and another is that they
finish too late. Scenario one: They go straight for the bendy mirror and will
figure the station out inside 5 minutes (or they cheat and look inside the
aberrator to see that the mirror is bent. Facilitation scenarios: 1) they
actually get the solution before you can prevent or distract them. There are
other solutions (stopping the beam down). Ask the students: "Can you find
another way to sharpen the image?". Hopefully, they will find the "stopping the
beam" solution using the other materials. 2) With roughly 10 minutes to go, if
they haven't found the bendy mirror solution, the facilitator should come in
and suggest something....
Aberrator Issue - the mirror doesn't have independent actuators. It's more like
a drum-head than an actual DM. Only mild lenses will be nicely correctable. One
can also "trick" the mirror by inserting a mild (-500mm FL) lens to force the
DM to take on a half-stroke defocus mode. This will allow more complex shapes
to be attained by the DM. Instead of a translation stage for constant-velocity,
we will use a post on a rail. The DM doesn't have good time response (10Hz?) so
that simple plastics or lenses on a movable mount will be sufficient to
overload the capabilities of the demonstrator.
Poster Prep Session Notes:
We're going to transition from the stations to the posters in the following
way: Each group will have ~20 min to make a poster on their station to present
to the group. The first 5 minutes of the session will be a "walk-around" where
the students go revisit the other stations. The prompt will be "Explain your
station and how it fits in to an AO system" to the group. The point being that
a 3-block diagram of (Aberration-Detection-Correction) should show up on their
poster somewhere. A thinking tool that may/should be shown during the "walk
around" is that of a simple telescope with two blocks - light comes in, one
block (mirror) collects and focuses light, another block (ccd/film) records
that light. The main reason for focusing on this is the goal: "To break a
complex system into simple interacting parts." This is the only activity of the
AMSC that addresses the complexity. **one issue - Mark - how exactly is this
going to work with your station. Do you foresee any problem with your station
being "the atmosphere"? Think the kids will pick up on that idea ok?
What Good Posters Look Like:
Bendy Mirror: There should be a block diagram highlighting the "correction"
function of this station. We'd like to see a ray trace of the station (with the
aberrator bypass in place) showing how there are places where there are images
and other collimated places. The goal is to get the students to show that there
are different solutions - bendy mirror and stopping the beam. The other major
concept is that the "aberrator" and "corrector" have the same shape. This
should be shown somewhere on the poster. Throughout the station and poster prep
sessions students will be encouraged to draw out the ray-trace of the station.
This will be a common theme for all stations. The ray-trace on the poster
should be taken directly from their notebooks.
Detection station: The goals here would be for the students to understand
what's happening to the rays in this set-up, what each component does, and give
a stab at the bigger picture (i.e., what each component represents and maybe
what happens next in the process). To get these concepts manifested, we
should look for a detailed ray diagram showing all three subcomponents (the ray
box, lenses, and detection surface). It would also be nice to see a either
drawing of what the detector looks like under different lens configurations or
a plot to a similar effect. More importantly, however, there should be a table
or bulleted list with descriptions of each subcomponent including what it does,
what are its limitations, and what it might represent (more here?).
Poster Sharing Session Notes:
2008-11-22
2008-10-23
2008-10-21
2008-10-05
2008-09-27
2008-09-26
2008-09-11
2008-09-04
2008-09-02
2008-08-28
2008-08-27
2008-08-26
2008-08-22
2008-08-21
2008-08-13
2008-08-12
2008-08-07