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Harnessing Supercomputers for Radio Astronomy Data Processing

Commercial supercomputers improve data processing for radio astronomy projects like GASKAP-H i.

Ian P. Kemp, Nickolas M. Pingel, Rowan Worth, Justin Wake, Daniel A. Mitchell, Stuart D. Midgely, Steven J. Tingay, James Dempsey, Helga Dénes, John M. Dickey, Steven J. Gibson, Kate E. Jameson, Callum Lynn, Yik Ki Ma, Antoine Marchal, Naomi M. McClure-Griffiths, Snežana Stanimirović, Jacco Th. van Loon

― 6 min read


Supercomputing in Radio Supercomputing in Radio Astronomy for radio astronomy projects. Revolutionary data processing methods
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Modern radio telescopes are Data-generating machines. They collect tons of information every second. The next generation of telescopes, like the Very Large Array and the Square Kilometre Array, is expected to generate up to 292 gigabytes of data every second. That's like trying to drink from a fire hose when all you want is a sip of water. Thankfully, Supercomputers have become more powerful and available, making it easier for astronomers to process this flood of data. In this article, we'll discuss a project that tested the use of commercial supercomputers to handle this data, specifically from the GASKAP-H i pilot surveys.

The Need for Supercomputing

Radio astronomy relies on high performance computing (HPC) because of the massive data volumes. The ASKAP telescope, for example, processes 3 gigabytes of data every second. Just imagine trying to sort through all that! As technology improves, so does the ability to handle these data deluges. While there were concerns years ago that future telescopes would outstrip available computing power, those worries have mainly disappeared. Now, many researchers are looking into commercial supercomputing options, which have become a viable alternative for Processing large datasets.

What is GASKAP-H i?

GASKAP-H i is a survey focused on studying neutral Hydrogen in the Milky Way and nearby Magellanic Clouds. It's like trying to understand the recipe for a delicious soup by examining each ingredient. The survey's goal is to get a close look at how hydrogen behaves in the cosmos, including how it moves and interacts with other gases. Picture trying to pick apart a fancy salad. This survey helps researchers understand the building blocks of stars and galaxies.

Setting Up the Experiment

The goal of this project was to see how well commercial supercomputers could handle the data from GASKAP-H i. We followed a straightforward four-step process that other researchers can use if they want to make the switch to commercial computing. This approach not only helped us process the data but also tuned our methods to improve cost and speed.

We started working on the data processing pipeline using WSClean, a software used for making images from the collected data. Our final aim was to create clear and accurate images for the science team working on GASKAP.

What Did We Find?

After diving into the data, we noticed some striking advantages and disadvantages of commercial supercomputing. The biggest perk was the immediate access to resources—no waiting in line! However, we also found that researchers needed to adjust their workflows to make the most of the new setup. It was like trying to fit a square peg into a round hole, but with a little help from the supercomputer's tech team, we managed to get everything running smoothly.

Data Collection and Processing

In the early stages, we collected calibrated data from the pilot surveys. The data was gathered over a series of observations capturing various areas in the Magellanic system. Each snapshot produced around 61 gigabytes of data, which is a lot when you have multiple fields to process!

Once we had the data, we used the supercomputer's resources to create images. Processing involved multiple steps, like downloading the data, adjusting visibility, and splitting channels for easier handling. Each step of the process required careful attention, just like when you're trying to assemble a complex puzzle.

The Hardware Behind the Magic

The supercomputer we used had a variety of nodes (essentially computers within the computer), each with impressive power. Some nodes had 64 cores, while others had even more memory for heavy tasks. This flexibility allowed us to run multiple jobs at once, which sped up our processing time significantly.

By using different types of nodes for different tasks, we could balance performance and cost effectively. It's like choosing the right tool for your workbench—using a hammer for nails but a screwdriver for screws.

Challenges Along the Way

Although we managed to achieve good results, it wasn't without its bumps in the road. One challenge was transferring the data from the main database to the supercomputer. To tackle this, we built a system that allowed us to “drip feed” the necessary visibility files, making the process smoother.

Additionally, we experimented with various software tools to see which worked best for our needs. This careful selection allowed us to speed up our workflow and improve the images produced in a shorter timeframe.

Optimizing Our Approach

With some trial and error, we optimized our software parameters and made changes to our workflow. By utilizing temporary storage and matching the number of processing threads to the number of cores, we were able to significantly cut down processing time. Imagine cooking a big meal; the more hands you have in the kitchen, the quicker everything gets done!

Results of Our Experiment

Once we fine-tuned everything, we produced impressive images from the data. The costs for processing were also reduced, making the entire operation more efficient. The final product not only met technical goals but also provided valuable images for the GASKAP-H i science team.

We processed multiple fields from the pilot survey, resulting in four image cubes that help researchers understand hydrogen in our universe. With the knowledge gained during the project, we created a resource estimate for future data processing, a bit like making a recipe for a favorite dish.

Lessons Learned

Throughout the project, we discovered various lessons that will benefit future researchers. One major takeaway was the importance of planning ahead. It’s crucial to consider how much code optimization will be necessary when moving to a new system. Like preparing for a big trip, the more you plan, the smoother the journey.

We also learned that having regular check-ins between astronomers and the tech support team is vital for overcoming obstacles. It’s just good teamwork—you know, like a well-oiled machine!

Conclusion: The Future of Commercial Supercomputing

This project showed that commercial supercomputing can effectively handle the demands of radio astronomy, especially with large datasets like those from GASKAP-H i. The combination of immediate resource access and flexible computing options makes it an attractive choice for researchers.

As we continue to push the boundaries of what's possible in astronomy, commercial supercomputing will likely play a larger role, helping scientists unlock the secrets of the universe one dataset at a time. So, next time you look up at the stars, remember that there's a whole world of data, supercomputers, and diligent researchers working to make sense of it all.

Original Source

Title: Processing of GASKAP-HI pilot survey data using a commercial supercomputer

Abstract: Modern radio telescopes generate large amounts of data, with the next generation Very Large Array (ngVLA) and the Square Kilometre Array (SKA) expected to feed up to 292 GB of visibilities per second to the science data processor (SDP). However, the continued exponential growth in the power of the world's largest supercomputers suggests that for the foreseeable future there will be sufficient capacity available to provide for astronomers' needs in processing 'science ready' products from the new generation of telescopes, with commercial platforms becoming an option for overflow capacity. The purpose of the current work is to trial the use of commercial high performance computing (HPC) for a large scale processing task in astronomy, in this case processing data from the GASKAP-HI pilot surveys. We delineate a four-step process which can be followed by other researchers wishing to port an existing workflow from a public facility to a commercial provider. We used the process to provide reference images for an ongoing upgrade to ASKAPSoft (the ASKAP SDP software), and to provide science images for the GASKAP collaboration, using the joint deconvolution capability of WSClean. We document the approach to optimising the pipeline to minimise cost and elapsed time at the commercial provider, and give a resource estimate for processing future full survey data. Finally we document advantages, disadvantages, and lessons learned from the project, which will aid other researchers aiming to use commercial supercomputing for radio astronomy imaging. We found the key advantage to be immediate access and high availability, and the main disadvantage to be the need for improved HPC knowledge to take best advantage of the facility.

Authors: Ian P. Kemp, Nickolas M. Pingel, Rowan Worth, Justin Wake, Daniel A. Mitchell, Stuart D. Midgely, Steven J. Tingay, James Dempsey, Helga Dénes, John M. Dickey, Steven J. Gibson, Kate E. Jameson, Callum Lynn, Yik Ki Ma, Antoine Marchal, Naomi M. McClure-Griffiths, Snežana Stanimirović, Jacco Th. van Loon

Last Update: 2024-12-04 00:00:00

Language: English

Source URL: https://arxiv.org/abs/2411.17118

Source PDF: https://arxiv.org/pdf/2411.17118

Licence: https://creativecommons.org/licenses/by/4.0/

Changes: This summary was created with assistance from AI and may have inaccuracies. For accurate information, please refer to the original source documents linked here.

Thank you to arxiv for use of its open access interoperability.

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