Meet the Team: Michael Aye

Today we have the next installment of our Meet the Planet Four Team series, featuring Michael Aye from the Science Team.

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Name:  K.-Michael Aye

What is your current position and where/institution?

Postdoctoral Researcher at UCLA in Los Angeles, CA, Department of Earth, Planetary and Space Sciences 

Where are you originally from/where did you grow up?

I am from Germany, where I grew up approx 100 km northwest of Hamburg, near the North Sea.

What are your research interests/what do you work on?

  • Surface atmosphere interactions on Mars, creating visual phenomena that do not exist on Earth
  • Calibration of the Diviner radiometer instrument on-board the Lunar Reconnaissance Orbiter (LRO)
  • Automated image feature extraction using machine learning procedures

In 3 lines explain your PhD thesis?

I developed a calibration system for the photo-multiplier based cameras of the ground-based high energy gamma-ray telescope system H.E.S.S. This system was based on using nano-second short UV-laser pulses fluorescing a scintillator material and transporting that broader-band light through 50 m of fiber cables and have all this remote controllable. I finished up with installing and operating a LIDAR and radiometer to monitor the atmosphere status as required to cross-calibrate the observed gamma-ray flashes from the particle showers in the atmosphere.

Why are you interested in Mars?

Mars and Venus are the closest siblings of Earth and to understand their differences makes us understand Earth better (but I don’t like the multitude of Venusian chemistry that much.. yet ;) The lack of water on Mars really makes it a great lab for studying the interface between the surface and atmosphere because on Earth most of what we see is dominated by water-based erosion. On Mars, it’s the wind and amazing CO2 sublimation effects.

What is your favorite movie?

The Matrix

What is your favorite book?

I don’t have much time for reading anymore, but when I did, these books were big fun:

  • “Surely you’re joking, Mr. Feynman” (showing a bit too much hubris at times, but he was indeed a genius)
  • “Titan” from Steven Baxter (greatly informed S-F)
  • The robot novels of Isaac Asimov made me appreciate the complexity of connecting human language and interaction schemes to the operation of machines. It inevitably makes you think about the human consciousness definition as well. A must read for any S-F fan.

What is the song you currently can’t get out of your head?

“Get lucky” by Daft Punk

What three albums would you bring with you to a desert island?

  • “Love is the tender trap” by Stacey Kent. The most ingenious introduction to Jazz ever made. Soft, gentle, but with everything that ever was important for Jazz to make it less fringy but more popular. It was my intro to Jazz and I will never stop loving it. It has an absolute genius of a piano player as well.
  • “Gran Riserva” by dZihan & Kamien. Great electronic lounge for the long work nights. I basically wrote my PhD with it.
  • And now the surprise :) “Once more with feeling”, soundtrack to the musical episode of Buffy the Vampire slayer. Also a remnant of my PhD times, it shows the early genius of Joss Whedon to its fullest.

Favorite cocktail or beverage?

I wouldn’t be able to pick really favorites, but among them are Margaritas on hot days, Caipirinhas and Mojitos. And since my 4 year stay in good ol’ England, I really am loving ales of all kind.

A Summary of a P4 Summer

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At the end of August, Chuhong Mai  presented a summary and results from her undergrad summer research internship at the Institute of Astronomy Astrophysics, Academia Sinica working with Meg on Planet Four. You can learn more about Chuhong here.

Chuhong spent July and August in Taiwan working on map projecting HiRISE images and exploring frost features. She kindly agreed to share her final presentation talk slides (see below) and some text to describe each slide. Thanks Chuhong for all your help this Summer!

Final Pre_ASIAA2014 58Mars has a very thin atmosphere, 96% of which is . Every year, the two poles of Mars participate in the gas exchange of atmosphere. Since the south pole contains a lot of , it plays an significant role in Martian atmospheric dynamics.

Final Pre_ASIAA2014 59But what’s really interesting is we observe fans and blotches appear in early spring and disappear in summer each year on the south pole. Araneiform features or ‘spiders’, which are radial channels that converge in the center, often accompany those dark stuff.

Final Pre_ASIAA2014 60These features are everywhere from -70 to -87 deg. and not limited to the ‘cryptic region’ (low temperature because of dry ice, low albedo caused by translucent ice layer) as thought before. We use solar longitude (Ls) to measure time on Mars, these features appear from Ls 170 to Ls 300 typically.

Final Pre_ASIAA2014 61The basic idea of the formation of fans and blotches:

  1. In the southern winter, in the atmosphere tends to condensate and dust grains serve as condensation nuclei. They fall onto the ground with and thus are embedded in the slab ice later. In spring, they are heated by the sun and heat the surrounding ice subsequently. These ice sublimate and form bubbles which then sink through the ice layer.
  2. With bubbles accumulate in the bottom, pressure between ice layer and the ground increase, so the ice could break and then jets of gas, together with dust, come out.
  3. Due to local topography and wind, the jets form fan-shaped deposits.

The gas beneath the ice layer might carve the Mars surface and form ‘spiders’.

Final Pre_ASIAA2014 62With local wind, the deposits look like fans with orientation that can indicate the direction of wind. Without wind to blow down the material, the deposits become blotches.

Final Pre_ASIAA2014 63We now have a powerful instrument to study such features. The HiRISE camera on MRO has resolution as high as 0.25m per pixel and excellent SNR (100:1). So we can study sub-meter objects like boulders on Mars. It’s able to observe same locations at different time and thus show the evolution of the south pole. It has finished 4 seasons of observation. Season is 2006-2007, season 2 is 2008-2009, etc.

Final Pre_ASIAA2014 64This schematic show you what the focal plane of HIRISE is like. There are 10 RED CCDs, 2 NIR, 2 BG. So color images can be obtained in the middle of the focal plane. Note that there are overlaps between every 2 CCDs.

 

Final Pre_ASIAA2014 65Though we have large amount of data from HiRISE, computers are bad at recognize the features in it. Thus we invite citizens on Earth to help marking them on Planet Four. It is a project under Zooniverse. Users can use the tools in the classification interface to mark features’ sources and orientation.

Final Pre_ASIAA2014 66Some examples of cutouts on Planet Four.

 

 

Final Pre_ASIAA2014 67The cutouts are made from RGB, non-projected HiRISE products. Most people are able to make reasonable markings, and the clusters of people’s markings are recorded as pixel position. So we need to convert pixel position to latitude & longitude

 

. Final Pre_ASIAA2014 68We have 2 types of data but we only use the raw data (EDR). Only map projected products of Reduced data (RDR) have spacecraft information with them. As we actually need position information of non-projected products (they are where the Planet Four cutouts come from), we decided to reassemble mosaics using raw data.

 

Final Pre_ASIAA2014 69

The tool we used, ISIS, is a free, specialized, digital image processing software package developed by the USGS for NASA. It is able to process data from NASA and International spacecraft missions including HiRISE. With applications in ISIS, we could follow the whole process presented here.

Final Pre_ASIAA2014 70The schematic of the reduction process. We developed a pipeline of it.

 

Final Pre_ASIAA2014 71Now, we are able to grab position information of any point. By getting the central points of HiRISE images, we have the distribution of them in a polar view. By drawing the images’ outlines, we show the overlap of different HiRISE images, which were taken at different periods. Study on a point in the overlap region will give the time evolution of it.

Final Pre_ASIAA2014 72We can use these data to study fans with frost, which are common in early spring. The latest hypothesis is that the blue color is caused by a change in the structure of the ice caused the the fan particles sinking into the ice.  Yet there is little evidence of it.

Final Pre_ASIAA2014 73Firstly we need to review certain amount of cutouts with frost in it. The review pool is the cutouts tagged as ‘frost’ or ‘blue’… in Planet Four Talk. Though they are not all the cutouts with frost, but there are still a large amount and might contribute to revealing secrets of frost fans.

 

 

Final Pre_ASIAA2014 74While reviewing, we classified these frost fans, as shown in slides (18-20)

Final Pre_ASIAA2014 75

Final Pre_ASIAA2014 76

Final Pre_ASIAA2014 77By dividing them into different periods of time, we study how the fraction of each types change over time. It can be seen clearly that type ‘outside’ dominate all the time.

Final Pre_ASIAA2014 78Next, we combined several types of frost fans together and took a clearer look at how the locations of frost relative to fans change. We found that frosts only appear very early and then nearly all of them become outside of fans later.

Final Pre_ASIAA2014 79Another combining shows that frosts mainly lie in the same direction of fans, some in different directions appear early at the beginning.

Final Pre_ASIAA2014 80I picked 6 points of the 4 regions of interest for detailed study.

Final Pre_ASIAA2014 81Only point B is presented since it has beautiful overlap. The table shows how the type of frost fans changes over time. Font color represents the typical color of frost or fans at corresponding time. Final Pre_ASIAA2014 82This series of pictures are of the same region. At the very beginning, nothing’s there. Gradually, we can see some dark blue stuff appear around the vents. They then expand to the outside and become bright blue. After that they begin to disappear, and the whole surface becomes white soon, with dark cores left

Final Pre_ASIAA2014 83Another series show the similar process. Actually, we observe such process not just in B region. So we might have a general idea of frost evolution, as the slide shows. Interesting ‘dark rings’ are observed after frosts disappear in some places. It is the first time we see such features.

Final Pre_ASIAA2014 84This slide concludes my work in summer and work might do in the near future.

 

 

And the winner is….

A month ago, we asked for your help to decide which bit of the Martian South Pole  (Inca City, Ithaca, or Manhattan) the world would see first to mark the start of the new season of  HiRISE‘s  South Pole monitoring campaign. A big thank you to everyone who voted in the Season 5 Sneak Peek vote,  and many thanks to the HiRISE team and the Zooniverse team for their help as well.

The votes have been tallied and we have a winner. The winner is….

IncaCity

The breakdown in votes can be found below:

final_results

Inca City was the most popular choice. Inca City is known for its boulders. It will be exciting to see if there are already fans by the boulders after the early days of sunlight when the first HiRISE monitoring campaign image gets taken. Once the first observation of Inca City has been acquired and processed by the HiRISE team, it will be made ready for public release. We’ll let you know on the blog as soon as the Inca City observation has been made public.

This image is just a sneak peak of what is to come. We will have all of the South Pole Season 5 monitoring images to look forward to in the future on Planet Four, but in meantime while we wait for the Inca City’s first image, if you have some spare time today, mark seasonal fans and blotches to help us better understand the Martian climate at http://www.planetfour.org

An Introduction to HiRISE

Today we have a guest post from Chuhong Mai, an undergraduate student working on Planet Four this summer as part of the ASIAA Summer Student Program.

By now, you may have helped the Planet Four team classified hundreds of thousands of cutouts produced from HiRISE season 1 to 3 products, and you may have voted for a region target for HiRISE to be observe in season 5, however, but how well do you know about this camera that makes the whole Planet Four project possible? And that’s what this blog post is going to talk about.

The High Resolution Imaging Science Experiment (HiRISE) camera is carried on the Mars Reconnaissance Orbiter (MRO) spacecraft and since the spacecraft entered Mars orbit in 2006, HiRISE has produced a large amount of beautiful images in unprecedented detail. It was in a 2-year Primary Science Phase (PSP) during 2006 and 2007, corresponding to season 1 in Planet Four project. Later, it had two 2-year Extended Science Phases (ESP) in 2008-2009 (season 2) and 2010-2011 (season 3). HiRISE continues today to operate under an extended mission taking images of unprecedented detail. So if you notice the images’ names (not the cutouts’ names), you’ll find all of them begin with PSP or ESP, which indicates the mission phase HiRISE were in when a certain picture was taken. The rest of their names tell you some other information of HiRISE’s orbit.

The HiRISE camera mainly consists of a telescope with 50 cm diameter and a focal plane system right behind it. This plane might be one of the most important parts of HiRISE since 14 CCD detectors are installed on it, each with 2 separated output channels and 2048 pixels. 10 of these CCDs are for the Red band (RED0 to RED9), 2 are for the Infrared (IR) band (IR10, IR11) and the rest 2 are for the Blue-Green (BG) band (BG12, BG13). They overlap each other by around 48 pixels. Their positions are shown in Fig.1. So as you see, the red band will cover a much wider range (5.0-6.4 km wide) of Mars surface than the other two bands, but only RED4 and RED5, which locate at the center, can cooperate with IR and BG band to generate color products (1.0-1.3 km wide). The HiRISE team also use Time Delay Integration (TDI) to increase SNR (Signal-Noise Ratio). The basic idea of TDI is to image the same small patch of surface many times and add up together to improve SNR. Different numbers of TDI lines (8, 32, 64, 128) are used under different conditions. In addition, six pixel binning modes can be used to increase coverage and SNR, either. Click here to learn more about how binning works. On the whole, HiRISE is able to reach a high resolution: 0.25m/pixel with low SNR exceeding 100:1. This makes sub-meter surface study of Mars possible.

The three bands are selected to differentiate a broad classes of surface materials like bedrocks, frost or ice, sand, dust and other minerals and to avoid ambiguities between shades and different materials, which is often the case in grayscale products. Typically, frost and ice appear bright white and blue, sand and rocks appear bluer and darker, while the dust are the reddest material in these images. Therefore, with these bands combined together, a final color product you see are usually not a true-color images (like what you see through naked eyes), it is either an IRB product, which combines the 3 bands mentioned above, or a RGB product, which combines the Red, BG and synthetic blue band. The latter one is used by Planet Four to make cutouts for you, as RGB images usually do better in contrasting RED with BG color variations. Note again that these images are false-color products and the true Mars surface appear relatively bland and red. Sorry about that because how beautiful these cutouts are!

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Fig 1. Schematic of the focal plane system on HiRISE (from A.S. McEwen et al [Reference 2])

Fig 1. Schematic of the focal plane system on HiRISE (from A.S. McEwen et al [Reference 2])

 

References:

W. Alan Delamere, and 15 colleagues, 2009. Color imaging of Mars by the High Resolution Imaging Science Experiment (HiRISE). Icarus, 205, 38-52

Alfred S. McEwen, and 14 colleagues, 2007. Mars Reconnaissance Orbiter’s High Resolution Imaging Science Experiment (HiRISE). J. Geophys. Res., 112, E05S02

Update on the Season 5 Sneak Peak Vote

On August 1st, we announced a public vote in partnership with the HiRISE team. It is your chance to decide which of the 3 regions we have featured on Planet Four in the first half of this year  will have its first observation from the new HIRISE monitoring season prepared for public release by the HiRISE team.

P4voteregions

You can help determine which of one these 3 regions on the South Pole will have its first observation of the Season 5 HiRISE monitoring campaign prepared for public release.

Below is the breakdown of the tallied votes as they stand right now. Inca City has the lead with Ithaca trailing not that far behind in second. Manhattan is  a distant third.

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Cast your vote (as often as you like) until September 1st for Inca City, Ithaca, or Manhattan at www.planetfour.org/vote , and while you’re at it if you can spare some time, help map the seasonal fans and blotches today at www.planetfour.org

Meet the Planet Four Team: Brian Carstensen

Today we have the next installment of our Meet the Planet Four Team series, featuring Brian Carstensen from the Zooniverse development team.

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Name: Brian Carstensen

What is your current position and where/institution?

Front end web developer at the University of Oxford

Where are you originally from/where did you grow up?

I’m originally from Chicago.

In 3 lines explain what you do as part of the Zooniverse development team?

I used to build user interfaces for various projects.
Now I’m working on the UI for the new Zooniverse-as-a-platform infratructure.
I’m also taking on some graphic design responsibility for the new system.

What was your role in Planet Four?

I built the part of the site our volunteers interact with. The marking tools in Planet Four were actually the first prototype of the drawing library now used in most of the more recent Zooniverse projects.

Why do you find interesting about Mars?

I’m just waiting patiently for someone to start terraforming it so my great-great-great-etc. grandbabies can hang out there.

What is your favorite movie?

Primer (2004)

What is your favorite book?

Anathem by Neal Stephenson

What is the song you currently can’t get out of your head?

Ella Fitzgerald’s botched recording of Mack the Knife.

 What three albums would you bring with you to a desert island?

Six Demon Bag by Man Man
The Milk Eyed Mender by Joanna Newsom
Milo Goes to College by Descendent

Favorite cocktail or beverage?

Moscow mule!

The Sun is back!

 I wrote a post on my new blog showing how I go about finding out what’s currently going on at the southpole of Mars!
Sorry for the cross-linking, but there’s no way to show the nice IPython notebooks (combing text and code) in a clear and pretty format here in WordPress:

Planet Four at ZooCon 2014

Image Credit: Grant Miller

Image Credit: Grant Miller

The Zooniverse UK HQ hosted ZooCon 2014 this past Saturday at Oxford University with an afternoon inspired by Zooniverse projects. There was representation from science team members (physically and virtually) from many of the projects as well as some of the core Zooniverse team in attendance.

I was invited to give a talk at this year’s ZooCon virtually. I gave an update on Planet Four, and I talked about the progress the science team has been making towards the project’s first paper. You can find the recorded video below:

If you were at ZooCon or just watched the video and have questions, I’ve started a thread on Talk for further discussion.

There is also going to be a second ZooCon called ZooCon Portsmouth hosted at the University of Portsmouth. It will take place on September 13th. There will be some talks as well as an editathon to improve coverage of Citizen Science on Wikipedia. They have a schedule set for the day that you can check out. More details here (Like the Oxford event, tickets are free, but there is limited space at both the lecture hall and the pub) so do register.

Inca City, Ithaca, Manhattan: Which part of the Martian Arctic do you want to see first?

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Image credit: Adapted from Tanaka et al. (2014) ISSN 2329-132X http://pubs.usgs.gov/sim/3292/

Mars Reconnaissance Orbiter and the HiRISE camera will soon begin the 5th Season of the South Pole seasonal processes monitoring campaign, and now’s your chance to decide which region will have its first observation from the new season prepared for public release by the HiRISE team. Often these first images are striking, and though the Sun is low in the sky and close to the horizon, there may be active carbon dioxide jets present and already starting to create the first springtime fans and blotches!

Since January, we’ve been focusing on targets of interest from the Season 1 campaign asking you to help map fans and blotches in the areas nicknamed ‘Inca City‘, ‘Ithaca‘ (currently live on the site), and ‘Manhattan‘. To celebrate the start of the new monitoring season, Planet Four is partnering with the HiRISE team to organize a  public vote where you get the chance to decide which of these three regions you want to see first.

Voting will be open from August 1, 2014 9am GMT – September 1, 2014 9am GMT. We will be announcing the results on September 2nd. When the winning region’s first Season 5 observation is ready, we’ll post the image here on the blog.

Whether it be the boulders of Inca City, the fans of Ithaca, or the lace terrain of Manhattan that strikes your fancy, cast your vote today (as often as you like) at http://www.planetfour.org/vote.

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My Summer with Planet Four

Today we have a guest post from Chuhong Mai, an undergraduate student working on Planet Four this summer as part of the ASIAA Summer Student Program.

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As a summer student at ASIAA (Institute of Astronomy & Astrophysics at Academia Sinica), I am studying seasonal processes on the South Pole of Mars with Dr.Meg Schwamb. Well, we are quite aware that fans and blotches appear and disappear on the South Pole as the seasons change. Via HiRISE on MRO mission, we can obtain unprecedented details of them but also a large amount of unprocessed data. We hope to make good use of the data in order to have a better understanding of their physical processes, yearly evolution and influence on Mars climate.

Our first problem is the position. With all the markings you’ve made on these HiRISE cut-outs, we need to know the precise locations and thus the distribution of them. The way the images you see are Planet Four are processed we can’t directly add the spacecraft information needed to  calculate the latitude and longitude straight from the x and y positions from your markings. Instead I’ve written a pipeline using the Integrated Software for Imagers and Spectrometers (ISIS) to turn raw HiRISE data from Season 2 & 3  into pretty mosaics with the spacecraft information added. Now we are able to get the detailed greographic information of any point of interest. This means that the Planet Four team can now  measure the actual size and shape of these fans and blotches, as well as to project them on the true surface. Once we do the time series analysis, we can have a deep look on seasonal change.

In addition,  I’m also working on  ‘frost fans‘, which contain pretty blue or white stuff around or in the center of themselves. They are considered to possibly be the condensation of CO2 that come out of the vents,  but we actually have little knowledge of them. I’ll be examining images from Talk where volunteers have used hashtags to mark these features and seeing what I can learn about when and under what conditions these colored features appear. Perhaps the following study could reveal some clues to decode the puzzle.

Meet Chuhong

Name: Chuhong Mai

What is your current position and where/institution?

I am an undergraduate student in Sun Yat-sen University, Guangzhou, China. And now I am working as a summer student at the Institute of Astronomy & Astrophysics at Academia Sinica (ASIAA), Taiwan.

Where are you originally from/where did you grow up?

Jiangmen, Guangdong Province, China.

What are your research interests/what do you work on?

I am interested in the whole solar system, and solar systems beyond our own. For me they are places full of miracles and hopes. I’m curious about their origins, their histories and their future. Thus I work on planets, small bodies and planet formation.

Why are you interested in Mars?

Because of its mystery. I am a huge fan of science fiction, and Mars is always one of the most popular topics in sci-fi books and films. I like its red face and wonder what happened and is happening on it.

What is your favorite movie?

Contact, directed by Robert Zemeckis

What is your favorite book?

<The Three Body Problem> by Cixin LIu (It’s not a mathematics textbook but science fiction.)

What is the song you currently can’t get out of your head?

Valder Fields by Tamas Wells

What three albums would you bring with you to a desert island?

<A Plea en Vendredi> by Tamas Wells, <Europa> by Ron Korb, <A Wish to the Moon> by Joe Hisaishi.

Favorite cocktail or beverage?

Milk tea.

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