Bittersweet: The End of A Professional Service Term

I have mentioned many times on this blog that I feel that performing service to my profession is just as important as the research and public outreach that I do; in a way, this is a form of professional outreach.

I have had the uncommon honor to serve on the American Physical Society (APS) Council and then, half way into my four-year term, I was elected to serve on their Executive Board.  I have met many new colleagues whom I would have never met otherwise since we don't work in the same field of physics.  Even better, some of them have become friends (good enough friends that I will even discuss my Impostor Syndrome issue with them - I wrote a whole post about this).

As far as contributing to the profession, I have had the opportunity to work extensively on strategic planning for the next decade of the society and represented young physicists' concerns on many issues.  Even more than that, I am now able to better understand the workings of my professional society, understand the concerns of physicists who work in industry, outside of the United States, etc. and learn more about the politics (inside and outside of physics) that make research happen (or not).

My term comes to a close (on both the Council and the Executive Board) at the end of this year and I have just traveled back from my last meetings in Salt Lake City, UT.  I am sad about not getting to meet the new people who will be elected to replace all of us rotating off this year (I do recognize if we never left, there would be no new people!).  A big relief to me is that I won't have to travel so much - if you serve on the Council, that is 2 trips a year and then if you serve on the Executive Board that is an additional 3 trips (or 4 trips next year).  Since I HATE to travel, this will mean more nights in my own bed <contented sigh>.

The view from my hotel room in Salt Lake City.  This is facing Temple Square and the LDS temple is visible between the 2 red-orange buildings.

If you are reading this and are not a physicist (I hope some of you aren't since it is for you that I really write this blog), I hope that I have given you a little peek into the physics community outside of LIGO.  If you are a physicist, I urge you to consider expanding whatever service work you do to the APS, AAPT, OSA, etc.  It can be a lot of work, but I would definitely do it all over again.  Of course, service isn't all work (just mostly):

Wine tasting during the APS Executive Board Retreat, Santa Barbara, CA (Photo: Ken Cole)

Special thanks to Ken Cole for permission to use his picture of me (above).  Ken is the APS Special Assistant to the Executive Officer (and has done a great job a wrangling me these last years) and is also a gifted photographer.  You can view more of his photos here.

Using Astronomy to Teach Physics Workshop and AAPT Summer Meeting

I've just returned from a week long trip to Nebraska for 2 conferences, one in Lincoln and the other in Omaha.

Using Astronomy to Teach Physics Workshop:

The Lincoln trip was for a special workshop on Using Astronomy to Teach Physics (UATP).  The goal of this workshop is to bring educators in physics and astronomy together, share the information on the state-of-the-art science projects in their fields and then breakout into small groups to identify ways to bring this frontier science into the undergraduate physics curriculum.  I put together a professional poster (see my post on the different types of posters for more information on scientific posters) on the educational work done in the Science Education Center (SEC) at LIGO, both locally and nationally as part of the LIGO Scientific Collaboration's Education and Public Outreach (EPO) group [this group has just announced its partnership with the 2012 US Science & Engineering Festival].  (I will put a link to this post as soon as it becomes publicly viewable.) While I was making this poster, I found pictures of all of the SEC staff and myself engaging students and the public in some way.  For my picture, I found one that I adore (which is shocking since I hate nearly all pictures of myself) that shows me talking to school students while giving a tour of the LIGO control room:

I found this workshop particularly interesting for 2 reasons: 1) there were talks on the different frontier astronomy projects to make sure everyone in attendance at least had a working knowledge of what the state-of-the-art is and 2) there were breakout sessions where groups who were interested in similar goals met to discuss actionable ways to incorporate the new astronomy into the undergraduate physics curriculum.  My big project that I am now working on as a direct consequence of this is a document I intend to publish in the American Journal of Physics on connections between the basic physics concepts taught in the undergraduate physics courses and the technology that makes LIGO possible.  For example:

LIGO is looking for gravitational waves that will change the length of its 4 km arms less than 1/1000th the diameter of a proton (that's 0.000000000000000001 meters).  At this length scale, one must consider the effects of quantum mechanics.  So, here's the issue: the thermal vibration of the atoms in the mirrors used in LIGO is going to be much bigger than the "big" gravitational wave cited above.  How can LIGO possibly hope ever detect gravitational waves distinctly from this thermal mirror vibration?  (The 'no math' answer is at the end of this post.)  

After publication of this document, I am thinking about approaching LIGO's EPO group to propose that we create a web site to support this kind of effort.  Basically, I would like to take the document apart and use it to make a skeleton for the web site.  Then, any time a LIGO member has a homework question, activity, etc. that they use in their classroom, they can contribute that content to the site so that anyone who is interested can also use that content.

AAPT Summer Meeting:

After 3 days in Lincoln, I then went to the American Association of Physics Teachers (AAPT) Summer Meeting in Omaha.  There I got to make new friends in the Physics Instructional Resource Association (PIRA) and we did something together just about every night (which, if you know me, is remarkable since I am the type to hole up in my hotel room during down time).  I also co-presented an invited talk on LIGO outreach using demonstrations with my colleague Kathy Holt.  Demonstrations are really at the core of the outreach we so since we do demonstrations with teachers and give them the tools they need to take those demonstrations back to their classrooms, we do demonstrations during public open houses and there is often a demonstration or two when we work with student field trips.  It was great doing this talk with Kathy since the combination of our backgrounds (she was a teacher before working at LIGO) give different and useful perspectives on what we do in the SEC.

Then, besides going to other talks, I also had some academic service obligations.  I believe that I have mentioned that I am on the APS Forum on Education (FEd) Executive Committee.  Even though the AAPT is not affiliated with the APS, they work together closely since they both serve physicists but with different focus.  Because of this, the AAPT Executive Board meets with the APS FEd Exec. Comm. to coordinate efforts and we had a good lunch meeting this year.  I am also on the AAPT Committee on Graduate Education in Physics and this committee also met to make plan for the upcoming AAPT Meetings and to discuss the broader impact activities we are undertaking.

In past blog posts, I have included pictures of the city I happened to travel to as seen from my hotel window (see Long Beach, Milwaukee, Anaheim).  The view out of my window was a horrible view of a parking lot and another hotel.  Fortunately, the view from my colleague's room was much better (she got a room in the main hotel for the conference and I didn't since I waited too long to make my reservations).  So, here is the view of Omaha from the window:

OH!  One more thing...  When I was flying from Omaha (whose airport in actually in Iowa), the north terminal of airport of evacuated for a "suspicious package".  Luckily for me, I was flying out of the south terminal.  Once I got home, I found out that the hours long closing was due to someone's physics classroom apparatus that got TSA's panties in a bunch (it went through security as a carry-on).  I suppose it's good that they were awake enough to think something suspicious but what concerns me is that it is almost a certainty that the same thing was carried on the plane to get to the meeting at all.  I guess it wasn't as threatening then :) 

Answer to the quantum mechanics question posed above (highlight text below to uncover the answer):

The thermal vibration of the mirror's atoms would indeed make it impossible to measure a gravitational wave only if the laser was so well focused as to only shine on the area of a few of the mirror's surface atoms.  Fortunately, that is not the case in LIGO!  The beam spot on the mirror is about 10 cm (4 inches) in diameter.  In that area, there are MANY surface atoms that are vibrating.  By observing this large area, LIGO effectively averages over the vibration of all of the atoms that the light falls on yielding a zero net motion.  Thus, LIGO works just fine!

Professional Service

Sorry about the slow posting this week!  I've been busy getting ready for a trip and Thanksgiving.  By themselves, they aren't that bad but I still need to get my regular work done so I've been trying to get ahead on that.  Hence, I haven't been on the blog as much as I'd like.

In my "About Me" section, I mention the 3 main parts of being an academic: research, teaching and service.  I've already talked about my research and teaching, so let me tell you a little about professional service.

Service covers basically any activity that enriches your profession but doesn't come in the form of teaching or performing research in whatever it is you do.  This could be sitting on a committee that helps ensure that the working environment is comfortable or you can serve the larger community through professional societies.  For physicists, the main professional society is the American Physical Society (APS) but I am also a member of the American Association of Physics Teachers (AAPT) and the American Astronomical Society (AAS).

This week, I am traveling to the APS Board and Council Meetings.  I sit on the APS Council as the representative of the Forum on Graduate Student Affairs (FGSA).  The Council is the legal decision making body of the APS and we vote on everything from general statements, to journal subscription rates.  Councilors are elected to the Board after 2 years (of a 4 year term) on the Council.  The Board does more behind the scenes discussions on matters before they are brought to the Council for a vote.  The Board meets 5 times a year and the Council twice (luckily for me, 2 of the Board Meetings happen the day before the Council meetings).  I will be sure to post later this week on what happens at these meetings.

Service is often seen as thankless work.  In many ways, it is.  That is one of the reasons I try to find ways to serve that I personally feel are fulfilling; that way even if no one notices the work I do, I still feel good about it.  Serving on the APS Board and Council is not only fulfilling, but I also feel deeply honored since I was elected by my peers to these posts.

Photo by Ken Cole, APS

The picture above shows Gay Stewart (University of Arkansas), Stefan Zollner (now of the New Mexico State University), and me at the LaserFest gala event that was held at the Smithsonian National Museum of American History on February 12th this year.  All of us are on the APS Council and were invited to represent the APS.  For me, this was a night when being nerdy was cool!  I got to mingle with several Nobel Prize winners.  This photo really doesn't show the extent that the Smithsonian went to for this gala.  You can read more about it and see great pictures here.  This is definitely a time when service was not thankless!

Conference Calls and a Poster

Conference Calls

When you work with scientists from around the world, you end up on a lot of phone meetings.  Today (and every Wednesday) I had two. 

The first one was the "Burst" data analysis call and I drew the short straw and got to take the minutes of the meeting.  I am not someone who is good with names (I once had a class of 4 students and I messed their names up all that time - I knew each person well, I just forgot their label); now imagine that you only have a voice to go on.  This is not my strong point but it wasn't too bad today.  We discussed what needs to be done now that our latest science data run is over to complete our analysis looking for gravitational waves.

The second call was with people I collaborate with at Penn State to keep the MATLAB library of software that has been written for various LIGO purposes available and up to date.  That doesn't mean that we write it all (I have only written some of it), but we work with the program authors to make sure that their work makes gets into the hands of the other scientists to use.  Right now we are working on taking some of the programs that have been written to perform utility functions (like checking to see if a time is in daylight savings or doing calculations on where a star was at any given time) and pulling them together into a general toolbox.  Creating a toolbox like this will help keep duplication of effort to a minimum (that is, to keep people from repeatedly reinventing the wheel) and help insure that users are getting the correct values from these basic utilities.  We are right in the middle of going through this pool of computer programs to make sure that they are documented well and up to date.

Poster

Last year, I had the honor and privilege of working with the APS to create a poster on gravitational waves.  It was a wonderful experience getting to be someone who communicated the science of LIGO to the public and I learned much from the APS editors on how to express concepts in more understandable ways.  I wrote way too much content for the poster with the idea that it is better to have too much and cut it down, than to not have enough and have to create more content later.  The side benefit to this is the full version of the text that I wrote was then adapted for the science pages on the ligo.org site!

The poster as premiered by the APS at the joint APS/AAPT Meeting in Washington, DC this past February.  LIGO also arranged to have the posters included with the November issue of the AAPT magazine "The Physics Teacher" and to have the posters mailed to every physics department in the US.  I was thrilled!  So, now I am starting to spot the poster in the wild.

A few days ago, a friends of mine who is now at the Coastal Carolina University sent me a picture of it hanging outside his office:

I also just got my November issue of "The Physics Teacher" and it was so cool to get a copy of the poster in my mail box!

If you would like to get a FREE copy, you can request it (or another great poster on the top 10 reasons to study physics) from the APS here.

Sorry for getting so giddy about this!  This is just one of those things that make your day and remind you why you get out of bed in the morning.  :)

Busy Last Week: SESAPS Meeting and LaserFest Teachers' Day

Sorry for the lack of posts but I have been completely knackered after the events of last week:


SESAPS Meeting @ LSU

The American Physical Society (APS) has regional section meetings across the country and the end of last week saw the Southeast Section Meeting of the APS Meeting at LSU.  Since Initial LIGO was decommissioned a few days before, LIGO opened up a few of its vacuum chambers to the SESAPS attendees to show off the optics that were contained within.  This was indeed a rare opportunity as the chambers are only opened in between science runs AND only when there was crucial work to be done on specific components.  I work on site and I have only ever gotten to see inside a few of the chambers before.

Over 100 (and I believe I am being conservative) guests visited LIGO on Thursday afternoon and toured the Science Education Center, control room and LVEA (Laser Vacuum Equipment Area, otherwise known as the corner of the LIGO detector where all the neat stuff is).

Above is the inside of HAM6 (Horizontal Access Module - it has a table inside in instead of hanging the equipment from the top of the chamber) which is the output of the LIGO detector.  The taller piece of equipment on the table is the Output Mode Cleaner (OMC) which will help insure that the laser light has optimal intensity and phase to be used to detect gravitational waves (you can read a more detailed description of this kind of mode cleaner here).

This is what is inside of BSC1 (Beam Splitter Chamber - the kind of chamber where the equipment is hung from the top of the chamber).  This mirror (which looks like glass, but the front surface has a transparent light purple coating to make it reflective to infrared light which is what our laser is) is called ITMY (Intermediate Test Mass on the Y [south] arm).  (Test mass is our complicated way of saying mirror.)  This mirror sits just after the corner beam splitter of LIGO to intercept the light returning from the end mirror to bounce it back to the end mirror - this bouncing happens about 100 times before the light gets past the ITM to recombine with the light coming from the X arm and go to the output (which you just saw in the previous picture).

This is a picture of me and my husband, Derek (who is an engineer at LIGO).  The bright light you see shining from the left is the spot light that is illuminating ITMY.  This isn't the best picture, but I just had to have a picture of us in front of this mirror before they closed the chamber up - which is exactly what they did just after this picture was taken!


LaserFest Teachers' Day
 

I've been talking lately about the workshop I've been planning for middle/high school teachers of physical science and physics.  Since 2010 is the 50th anniversary of the invention of the laser, this year is also LaserFest.  To that end, the professional societies whose research have benefited from lasers all got together to sponsor LaserFest and to promote the educational outreach of lasers.  Since the SESAPS Meeting was taking place at LSU with physicists from all over the region, I decided it would be great to organize a LaserFest Teachers' Day to focus on the classroom kits the APS is distributing for free to teachers and to invite the meeting physicists to have lunch with the teachers and chat about what they do.

Organizing this event was quite the journey.  The first thing that needed to be done was to find the funding for the event (even if the kits are free from the APS, there are costs for food, recruiting and other miscellaneous supplies) which was supplied by the APS Forum on Education, the American Association of Physics Teachers (AAPT) and the Optical Society of America (OSA).  Then I needed to recruit teachers from the surrounding areas.  I was lucky here since I work with the LIGO Science Education Center and was able to advertise this event through their contact who also helped to spread the word.  Then there is making sure that the supplies arrive in time, contracting catering for the event, making sure that the teachers know when and where to be and insuring that you have all the incidental supplies that are needed (e.g. the kits contain everything a teacher would need except things they should already have like scissors and tape - but I needed to make sure that we had those for the workshop).  I know that none of these things sound like a lot, but this reminded me a lot of the last days before my wedding when all the details needed to fall into place at the same time.

The day started at 9 am with breakfast followed by a wonderful talk by Dr. Ken Schafer who introduced us to the basic concepts that make a laser work, their history and their applications.  We then proceeded to the first of the 4 activities in the 2009 PhysicsQuest kit (which included a laser pointer, and LED light, polarizers, glow-in-the-dark vinyl and colored light filters).  At noon, we broke for lunch and chatting with some of the physicists visiting for the SESAPS Meeting.  The rest of the afternoon saw us working through the remaining 3 activities and the day concluded at about 3 pm.

The picture above is some of the teachers hard at work doing the laser activity where we measured the width of our hair by measuring the diffraction pattern made by shining the laser on the hair.  That explains why the teacher on the left is giving herself a hair cut!

The APS has put together a useful page on arranging a Teachers' Day of your own - see it here.

I know that there are many people out there with poor opinions of our education system and the teachers within it, but I was truly inspired by these teachers who attended this workshop on their own time and without pay so that they can learn how to do these activities and take them back into their classrooms.  These teachers definitely went above and beyond to better themselves and their students!