Showing posts with label laser. Show all posts
Showing posts with label laser. Show all posts

Friday, June 1, 2012

Comparisons with the NASA ALVICE lidar are in Progress, so… Why Measure Water Vapour in the Upper Atmosphere?

The Crows have become Night Owls and put in a Herculean effort in the last couple weeks to prepare and begin measurements with our Network for the Detection of Atmospheric Composition Change (NDACC) colleagues from NASA’s Goddard Space Flight Center. The group we are collaborating with is led by Dr. Dave Whiteman and their lidar system is called ALVICE: Atmospheric Lidar for Validation, Interagency Collaboration and Education.



The NASA ALVICE trailer parked out at Western’s Environmental Science Research Facility. The building housing the PCL system is just to the left of the trailer.

The ALVICE system is mobile, meaning that it can be transported in a self-contained trailer. The system can measure water vapor mixing ratio, aerosol backscatter/extinction/depolarization and temperature in both daytime and nighttime. The ALVICE group is not just from NASA but includes students and faculty from Howard University in Washington DC, as well as collaborating scientists from Brazil and Bolivia.

The goal of our measurements over the next month is to compare our measurements to validate our system calibrations, by inter-comparisons, balloon measurements, calibration sources and satellites. The balloon measurements include regular weather balloons plus ozonesondes and frost point hygrometers, which are carried up by a balloon into the stratosphere to measure the small (a few ppmv) but important amount of water vapour present (1 ppmv means in a cubic litre of air in the lower stratosphere for every million air molecules there is 1 water vapour molecule). The PCL has been able to do these validation checks in the past in the lower and middle troposphere (the lower part of the atmosphere below about 12 km altitude) but has not had the ability to validate its measurements in the upper troposphere and lower stratosphere (the UTLS).

The UTLS is of great importance in large part due to water vapour, as water vapour is important in the chemistry of ozone. If the temperature changes in the troposphere it affects the amount of water vapour which can mix into the stratosphere and interact with ozone. Assessing this situation is complicated. Weather and climate are highly complex systems that are fully nonlinear, meaning that small changes to the system in one location can cause large feedbacks throughout the system. Weather is inherently highly variable, particular at middle latitudes. To make matters more complicated, humans have a significant affect on the already highly unstable natural cycle. The body of evidence shows we are in a period of rapid warming near the surface that is due to human activity, which appears to be having significant affects on the weather. To further complicate the affect of temperature change, for a significant period of time we released a large amount of chlorofluorocarbons into the lower atmosphere, which made there way into the stratosphere and caused unnaturally large ozone losses, particularly at the poles (e.g. polar ozone holes). Goals of the NDACC program include trying to understand these interactions be making long term measurements of water vapour, ozone and temperature.

An image from the International Space Station shows a pileus cloud forming over the Sarychev volcanic eruption in 2009 (from the Wikipedia page on Pileus Clouds).
In addition to affecting ozone chemistry, the UTLS is a region of important dynamical interactions between air in the stratosphere and troposphere The tropospheric air can contain natural and anthropogenic pollutants, which are carried into the stratosphere and distributed on a global-scale before falling back to the surface, a process called stratosphere-troposphere exchange. We used to imagine that the stratosphere and troposphere were separated by a rigid “lid”, (the temperature inversion which defines the tropopause). Dur­ing times of intense convection over cumulonimbus clouds a pileus cloud would occasionally be observed to form in the lower stratosphere, but otherwise dry, ozone-rich stratospheric air was separated from relatively moist, ozone-depleted tropospheric air. However, it is now known that when the speed of the jet stream intensifies in regions of surface cyclogenesis tropospheric folds can develop which can cause air to rapidly be exchanged between the upper troposphere and lower stratosphere.

It is just now being recognized another factor which can affect water vapour and ozone in the UTLS is due to forest fires. We are already at the start of what is appearing to be a extremely active fire season. A small number of these fires can develop into huge wildfires that can combine with severe thunderstorms, where vigorous convection is occurring. It was only recently appreciated that this convection can be so strong that smoke particles and carbon monoxide can be carried into the stratosphere and transported great distances. While initial reaction to this idea was met with some skepticism, measurements have clearly demonstrated this is the case. With global warming comes more forest fire activity, and pyroconvection may have significant implications on ozone and temperature change. There has been activity the last few days from fires out West that may bring some of this smoke over the London area.



Measurements of a smoke layer in the UTLS due to a fire in northern Saskatchewan (from Doucet, 2009).

I will post more updates as the campaign progresses. In fact I just heard we had a successfully FPH flight last night (though it looks like we would need a submarine to recover this one as it landed in Lake Ontario, drat!).

Monday, February 20, 2012

Why is this scientist smiling? Read the meter: 981mJ GREEN @ 30Hz. Game on! #lidar

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Well after a very long time the Crows are happy to report that we appear to have our laser issues resolved and we are hoping to be able to resume routine operations with our new transmitter. As the meter shows we are getting close to 1 J per pulse (@ 30 Hz) of green light from our new YAG. We were here before last March, but got stymied as the power quickly decayed. This problem appeared to be due to heat building up inside the system. Litron solved this problem by designing new covers with exhaust fans. There were also some internal times issues that appear to be resolved. We were also able to try our new beam expander, and it looks like we don't have any serious clipping issues (the beam was a bit larger than anticipated, but fixing the timing issues and changing lamps got us back to its nominal value).

Needless to see we are very happy and can get back to work, but without Crow Emily for a bit. She is up in Eureka working with the CANDAC CRL lidar system until April. We'll keep you posted on that.

See a few more snaps from the install here.

Thursday, February 16, 2012

Our rods have seen better days. #QuestFor1Jgreen

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Thursday, November 3, 2011

Lidar Open House featuring our #ICFAR friends. Nov 12. Come on out: @uwoscience @westernu @westernmustangs @uwogazette @cpsxnews #westernu

We're having an open house out at the new observatory. Come on out, the laser will be on and you can tour both our facility and ICFAR (Institute for Chemicals and Fuels from Alternative Resources) a centre at Western dedicated to developing new and environmentally friendly energy alternatives. Saturday, Nov 12, 5-8 pm.





Lidar_ICFAR_Open_House_Final.pdf
Download this file


Thursday, June 23, 2011

Crow Emily & @cpsxnews: Successful test of lunar analog rover to study #ImpactCratering #westernu



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Here's an article from Western News on what Crow Emily does in her "spare time" (Emily is shown on the right in the photo, correcting Prof Osinski rather than Prof Sica :-). The group remotely operated a rover that someday will collect lunar samples relating to impact cratering, including a laser ranging imager.

Saturday, March 12, 2011

Robin caught the first light of our new 1000mJ green beam into the night sky. Check it out here:




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Watch on Posterous


Long, long day (week!) but we got some light up into the sky! 1000 mJ @ 30 Hz (30 W) of green at 532 from our new Litron YAG. Well done Crows!



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Monday, March 7, 2011

Getting our green on at the PCL. Day 1 of the laser install. Check out first light here:




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Watch on Posterous


Starting to get some green light out of the new laser. This first flash of green was at "low" power (390 mW of green at 30 Hz). Check the afterglow on the camera, I though I burned out my phone's retinal display (more realistic, right, you are supposed to have a hole in your retina!).

Thursday, March 3, 2011

Why are we so happy? We didn’t tip over a 1 ton laser table! #westernu




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The profound-ess problem of the day: how to move our 1 ton laser table a couple feet forward as part of the new laser install? After MUCH looking around town, including every gadget AB Rental had to offer we founds some dollies at Canadian Tire made for moving a disabled car around. We were concerned the feet at the bottom of the table would punch right through them, but they held and we got the table in place in anticipation of Monday’s install. Much thanks to Peter D who is an expert with the jack! Amazing how much weight that 4x4 can bear.





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Watch on Posterous



Wednesday, March 2, 2011

Our New Nd:YAG laser has arrived! 1000 mJ/pulse @ 30Hz, 532 nm #westernu


Ohhh it has been a LOOONNNGGGG wait but the PCL has taken a big step towards getting back in action. Our new laser was trucked in today and Emily and Robin were there to meet it. Fortunately for them so were Caroline from the Western Environmental Field Station and several real nice folks from the ICFAR lab with strong backs and a forklift. As you can see in the picture they were certainly needed. I thought 2 people would be able to lift the laser head, but it was hard to get it on the table with 5! We are hoping to get it operational Monday and have our fingers crossed it will robustly meet its spec of 1000 mJ/pulse at 30 Hz in the green.


More to follow!

Bob



Monday, November 22, 2010

Cranes/large telescope/flying laser tables, movie of the Purple Crow Lidar's move to our new observatory online. Check it!

A summer of hard work and we have moved from the Delaware Observatory to our new facility, Echo Base. Our next step in the project is getting our new laser installed, which we hope to have done before year's end. We'll keep you posted!


[vimeo http://www.vimeo.com/17037859 w=500&h=283]