Last week we had a rare event: HiRISE turned off! We call this safe mode, because it’s a safety measure built into the instrument’s software. Whenever any of the sensors starts going out of bounds, like temperatures or voltages, the instrument powers down to prevent damage to the electronics. In this case, one temperature sensor went over its upper limit of 35 degrees Celsius. It’s pretty disconcerting when something unexpected like this happens, but at least we know the instrument is protected.

We had the difficult detective job of figuring out what went wrong. It was clear early on that the instrument overheated, but we couldn’t figure out why. Our tool that predicts the temperatures (”HiTemp”) didn’t predict anything that hot. We didn’t take a really large image, which would heat us up (at least, nothing bigger than normal! ). The local operations team worked with the health & safety people, the spacecraft engineers at LMA, and some of the software developers at Ball Aerospace that originally designed HiRISE. Together we all investigated the problem.

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On Thursday, April 19, 2007 I presented “HiRISE: The People’s Camera” at the Prescott Public Library in Prescott, Arizona. The library and the Prescott Astronomy Club put together a wonderful sequence of talks and star parties as part of International Astronomy Week.

My presentation went well. For some reason I was especially nervous right before the talk, but immediately after I started my nervousness went away, most likely because my hosts and the audience were so receptive. I am not sure how many people attended, but the room was full. At the end of the presentation there were a lot of great questions from the audience, including basic questions about Mars, questions about our current understanding of Mars, questions about HiRISE and its capabilities, and questions about the future of space exploration. I put my foot in my mouth only once, when I referred to the Deep Space Network (DSN) as “antiquated”. A former JPL engineer in the audience politely and informatively corrected my word choice.

A couple weeks before the talk we snail mailed two color printouts of PSP_001336_1560 – “Delta in Eberswalde” – to Prescott for framing. One image is the entire black-and-white image with central color swath, and the other is a zoomed-in color subscene. During setup prior to the presentation, the frame shop delivered the images, and they had done a fantastic framing job! People were naturally drawn to the images before and after the presentation and I answered lots of questions about them.

I promised I would place the PowerPoint presentation online, and here it is. The PowerPoint presentation file is about 22 MB in size. I have notes in the notes section of the slides, including information about the images used as well as their URLs. I want to especially thank Stuart Heggie for allowing me to use his beautiful astrophotography image “Conjunction of Moon, Venus and Mars – Dec 1 2002“. His image helped me to make a point about the history of Mars observation.

Thank you to my hosts, including Meghan and Douglas, and everyone who attend a delicious pre-presentation pizza dinner, including the current and former presidents of the Prescott Astronomy Club and their spouses, the library’s Adult Services Director, and the talented graphic designer of many of their brochures and other materials (including a t-shirt I will take a picture of soon). The audience deserves my thanks because they had such great questions and were incredibly good-natured. Thank you, everyone!

We mention our automated pipelines a lot, so I might as well jump in and provide some more information about them, on top of what might already have been mentioned before. I will start with the first one – HiDog – in a moment, but first, let me introduce Watchdog.

You should know by now the route our data takes: from the HiRISE camera on MRO to storage to spacecraft radiation to the Deep Space Network radio telescopes here on Earth to the ground data system network to JPL in Pasadena, CA to the University of Arizona campus network to our servers in the HiRISE Operations Center. Our Watchdog software, well, watches the JPL servers for new HiRISE raw image data. When it sees a new raw channel file (2 channels per CCD, up to 14 CCDs per observation), Watchdog flags that file as ready to be downloaded by HiDog.

HiDog is the first automated pipeline. It wakes up every few minutes to see if the Watchdog has flagged any new files (basically, it is checking a sources table in our database). If there is nothing new in the sources table, then it goes back to sleep. If there is something new, HiDog wags its tail, rapidly downloads the file, checks to see if there are any gaps in the data, and then tells the next pipeline that a new image channel has arrived in Tucson, ready for further processing. Then, it checks to see if there are any more files ready for downloading, and goes back to sleep if there are not. Sweet dreams, little doggy.

Over and over again, 24 hours a day, 7 days a week, the Dogs are ready and waiting for the latest HiRISE data from Mars.

Next time…the EDRgen pipeline.

Some of you out there may be asking: what happens to a HiRISE image between the time that it is taken and the time that it is released to the public? Well, I’d like to give a summary here.

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We just received the telemetry to confirm that the HiRISE camera took its first picture!!! We all gathered around a screen projecting the telemetry data, and everyone cheered as the numbers came in. We’ll have to wait another ~6 hours or so to actually receive the image… The images go from the spacecraft to the DSN network, then to JPL, then to us.