Tech Today: Measuring the Buzz, Hum, and Rattle

Tech Today: Measuring the Buzz, Hum, and Rattle

2 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater)

An array of microphones on the an airfield, with a sunrise in the background
The WirelessArray developed by Interdisciplinary Consulting Corporation (IC2), laid out here for a test flight at Langley Research Center, makes flight testing for drones quick and cost-effective.
Credit: NASA

Anyone who lives near an airport or is experiencing the emergence of a cicada brood can quickly identify the source of that ongoing noise. However, running tests to identify the noise created by a new drone or find pests in a field of crops requires a high-tech solution that maps sound.

With help from NASA, Interdisciplinary Consulting Corporation (IC2) introduced a new Wireless Array to do just that – anywhere, anytime. Airplanes undergo noise testing and require certification, so they don’t exceed the Federal Aviation Administration’s noise limits. Each small, saucer-shaped base, called a node, is equipped with an embedded microphone that measures the air pressure changes created by overhead sounds. For a large vehicle like an airplane, hundreds of these sensors, or microphone array, are laid out in a pattern on a runway to monitor the underside of the plane as it flies over.

Interested in making its flight tests more affordable, NASA’s Langley Research Center in Hampton, Virginia, supported the company with Small Business Innovation Research contracts and expert consulting.

“Each node contains a small computer system able to acquire and store data in memory on an SD card. It also has a small web server that allows the end user to start acquisition, stop recording, download files, check on the battery health, and more,” said Chip Patterson, vice president of IC2.

All it takes to operate an individual node or an extensive array is an off-the-shelf wireless access point and a standard laptop with IC2’s software application. The technology integrates into existing noise testing systems.

The microphone can easily be swapped for various other sensor types, like an acoustic sensor, making it possible to monitor animal noises that indicate health and well-being. An infrasonic sensor could measure the noise from supersonic aircraft, identifying the direction and arrival of a sonic boom.

This small, portable technology is finding its way into various projects and applications beyond aircraft testing. Working with an entomologist, IC2 will use acoustic data to listen for high-frequency insect sounds in agricultural settings. Discovering where insects feed on crops will allow farmers to intervene before they do too much damage while limiting pesticide use in those areas. With NASA’s help, IC2’s Wireless Array technology enables sound-based solutions in agriculture, aerospace, and beyond. 

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Andrew Wagner

NASA to Measure Moonquakes With Help From InSight Mars Mission

NASA to Measure Moonquakes With Help From InSight Mars Mission

6 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater)

The technology behind the two seismometers that make up NASA’s Farside Seismic Suite was used to detect more than a thousand Red Planet quakes.

The most sensitive instrument ever built to measure quakes and meteor strikes on other worlds is getting closer to its journey to the mysterious far side of the Moon. It’s one of two seismometers adapted for the lunar surface from instruments originally designed for NASA’s InSight Mars lander, which recorded more than 1,300 marsquakes before the mission’s conclusion in 2022.

Part of a payload called Farside Seismic Suite (FSS) that was recently assembled at NASA’s Jet Propulsion Laboratory in Southern California, the two seismometers are expected to arrive in 2026 at Schrödinger basin, a wide impact crater about 300 miles (500 kilometers) from the Moon’s South Pole. The self-sufficient, solar-powered suite has its own computer and communications equipment, plus the ability to protect itself from the extreme heat of lunar daytime and the frigid conditions of night.

Lunar Seismic Firsts

After being delivered to the surface by a lunar lander under NASA’s CLPS (Commercial Lunar Payload Services) initiative, the suite will return the agency’s first seismic data from the Moon since the last Apollo program seismometers were in operation nearly 50 years ago. Not only that, but it will also provide the first-ever seismic measurements from the Moon’s far side.

The Seismic Experiment for Interior Structure instrument (SEIS) aboard NASA’s Mars InSight is within the copper-colored hexagonal enclosure in this photo taken by a camera on the lander’s robotic arm on Dec. 4, 2018. The SEIS technology is being used on Farside Seismic Suite, bound for the Moon.
NASA/JPL-Caltech

Up to 30 times more sensitive than its Apollo predecessors, the suite will record the Moon’s seismic “background” vibration, which is driven by micrometeorites the size of small pebbles that pelt the surface. This will help NASA better understand the current impact environment as the agency prepares to send Artemis astronauts to explore the lunar surface.

Planetary scientists are eager to see what FSS tells them about the Moon’s internal activity and structure. What they learn will offer insights into how the Moon — as well as rocky planets like Mars and Earth — formed and evolved.

It will also answer a lingering question about moonquakes: Why did the Apollo instruments on the lunar near side detect little far-side seismic activity? One possible explanation is that something in the Moon’s deep structure essentially absorbs far-side quakes, making them harder for Apollo’s seismometers to have sensed. Another is that there are fewer quakes on the far side, which on the surface looks very different from the side that faces Earth.

“FSS will offer answers to questions we’ve been asking about the Moon for decades,” said Mark Panning, the FSS principal investigator at JPL and project scientist for InSight. “We cannot wait to start getting this data back.”

Mars-to-Moon Science

Farside Seismic Suite’s two complementary instruments were adapted from InSight designs to perform in lunar gravity — less than half that of Mars, which, in turn, is about a third of Earth’s. They’re packaged together with a battery, the computer, and electronics inside a cube structure that’s surrounded by insulation and an outer protective cube. Perched atop the lander, the suite will gather data continuously for at least 4½ months, operating through the long, cold lunar nights.

, Farside Seismic Suite’s inner cube
Seen here during assembly in November 2023, Farside Seismic Suite’s inner cube houses the NASA payload’s large battery (at rear) and its two seismometers. The gold, puck-shaped device holds the Short Period sensor, while the silver enclosure contains the Very Broadband seismometer.
NASA/JPL-Caltech

The Very Broadband seismometer, or VBB, is the most sensitive seismometer ever built for use in space exploration: It can detect ground motions smaller than the size of a single hydrogen atom. A fat cylinder about 5 inches (14 centimeters) in diameter, it measures up-and-down movement using a pendulum held in place by a spring. It was originally constructed as an emergency replacement instrument (a “flight spare”) for InSight by the French space agency, CNES (Centre National d’Études Spatiales).

Philippe Lognonné of Institut de Physique du Globe de Paris, the principal investigator for InSight’s seismometer, is an FSS co-investigator and VBB instrument lead. “We learned so much about Mars from this instrument, and now we are thrilled with the opportunity to turn that experience toward the mysteries of the Moon,” he said.

The suite’s smaller seismometer, called the Short Period sensor, or SP, was built by Kinemetrics in Pasadena, California, in collaboration with the University of Oxford and Imperial College, London. The puck-shaped device measures motion in three directions using sensors etched into a trio of square silicon chips each about 1 inch (25 millimeters) wide.

Assembled and Tested

The FSS payload came together at JPL over the last year. In recent weeks, it survived rigorous environmental testing in vacuum and extreme temperatures that simulate space, along with severe shaking that mimics the rocket’s motion during launch.

“The JPL team has been excited from the beginning that we’re going to the Moon with our French colleagues,” said JPL’s Ed Miller, FSS project manager and, like Panning and Lognonné, a veteran of the InSight mission. “We went to Mars together, and now we’ll be able to look up at the Moon and know we built something up there. It’ll make us so proud.”

More About the Mission

A division of Caltech in Pasadena, California, JPL manages, designed, assembled, and tested Farside Seismic Suite. The French space agency, CNES (Centre National d’Études Spatiales), and IPGP (Institut de Physique du Globe de Paris) provided the suite’s Very Broadband seismometer with support from Université Paris Cité and the CNRS (Centre National de la Recherche Scientifique). Imperial College, London and the University of Oxford collaborated to provide the Short Period sensor, managed by Kinemetrics in Pasadena. The University of Michigan provided the flight computer, power electronics, and associated software.

A selection of NASA’s PRISM (Payloads and Research Investigations on the Surface of the Moon), FSS is funded by the Exploration Science Strategy and Integration Office within the agency’s Science Mission Directorate. The Planetary Missions Program Office at NASA’s Marshall Space Flight Center provides program management. FSS will land on the Moon as part of an upcoming lunar delivery under NASA’s CLPS (Commercial Lunar Payload Services) initiative.

More information about FSS is at:

https://go.nasa.gov/FSS

News Media Contact

Melissa Pamer
Jet Propulsion Laboratory, Pasadena, Calif.
626-314-4928
melissa.pamer@jpl.nasa.gov

2024-074

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Anthony Greicius

Cargo Ship Departs, Two Rockets Near Launch During Busy Day on Station

Cargo Ship Departs, Two Rockets Near Launch During Busy Day on Station

May 28, 2024: International Space Station Configuration. Four spaceships are parked at the space station including the SpaceX Dragon Endeavour spacecraft, Northrop Grumman’s Cygnus space freighter, the Soyuz MS-25 crew ship, and the Progress 87 resupply ship.
May 28, 2024: International Space Station Configuration. Four spaceships are parked at the space station including the SpaceX Dragon Endeavour spacecraft, Northrop Grumman’s Cygnus space freighter, the Soyuz MS-25 crew ship, and the Progress 87 resupply ship.

A cargo ship departed the International Space Station on Tuesday leaving four spacecraft parked at the orbital lab. Meanwhile, as the Expedition 71 crew keeps up its advanced microgravity research two more spaceships are counting down to their missions to the orbital outpost in less than a week.

A trash-loaded Progress 86 cargo craft undocked from the space station’s Poisk module at 4:39 a.m. EDT on Tuesday. The Roscosmos resupply ship ended its six-month stay in space a few hours later when it reentered the Earth’s atmosphere for a safe, but fiery demise above the Pacific Ocean.

Meanwhile, two rockets are gearing up to launch more cargo and a new crew to the orbiting outpost by the end of the week. First, more than three tons of food, fuel, and supplies are scheduled to lift off aboard the Progress 88 spacecraft at 5:43 a.m. on Thursday from the Baikonur Cosmodrome in Kazakhstan. The resupply ship from Roscosmos will then orbit Earth for two days before its automated docking to Poisk at 7:47 a.m. on Saturday.

Cosmonauts Oleg Kononenko and Nikolai Chub trained on Tuesday for the arrival of the Progress 88. The duo practiced for the unlikely possibility of remotely controlling the spacecraft with the space station’s telerobotically operated rendezvous unit, or TORU. The device, located in the Zvezda service module, can send commands to control approaching Roscosmos’ spaceships and be used by cosmonauts to manually guide the vehicles to a docking if necessary.

Meanwhile, NASA astronauts Butch Wilmore and Suni Williams are preparing to depart Houston for Kennedy Space Center in Florida ahead of Boeing’s Crew Flight Test launch to the International Space Station. The experienced space duo is targeted to launch aboard Boeing’s Starliner spacecraft atop an Atlas V rocket from United Launch Alliance at 12:25 p.m. on Saturday. They will take a daylong trip around the planet before docking to the Harmony module’s forward port at 1:50 p.m. on Sunday.

NASA TV will broadcast both missions live on the NASA+ streaming service via the web or the NASA app. Launch and docking coverage also will air live on NASA Television, YouTube, and on the agency’s website. Learn how to stream NASA TV through a variety of platforms including social media.

Back in space, NASA Flight Engineer Tracy C. Dyson spent her day inspecting a treadmill and finalizing spacesuit work. She took turns with fellow NASA astronaut Jeanette Epps checking and cleaning components on the Tranquility module’s treadmill and photographing the condition of the exercise device for analysis. Next, Dyson joined NASA Flight Engineer Matthew Dominick in the Quest airlock and finished cleaning cooling loops inside a pair of spacesuits. Those suits are being readied for a trio of maintenance and science spacewalks planned for June.

NASA astronaut Mike Barratt spent most of his day supporting life science helping doctors understand how weightlessness affects biology. He started his day in the Kibo laboratory module configuring components on biology habitat hardware then installing the advanced gear on an artificial gravity generating incubator. Afterward, he participated in a vision test using a standard eye chart along with Dominick and Epps.

In the Roscosmos segment of the station, Kononenko and Chub worked on a pair of different experiments before their Progress 88 training session. Kononenko explored futuristic piloting techniques on a computer as Chub attached sensors to himself monitoring his heart activity and blood pressure. Flight Engineer Alexander Grebenkin started his day collecting station air samples for analysis before spending the rest of his shift on life support maintenance tasks.


Learn more about station activities by following the space station blog@space_station and @ISS_Research on X, as well as the ISS Facebook and ISS Instagram accounts.

Get weekly video highlights at: https://roundupreads.jsc.nasa.gov/videoupdate/

Get the latest from NASA delivered every week. Subscribe here: www.nasa.gov/subscribe

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Mark Garcia

Apollo 10 Ends Successfully

Apollo 10 Ends Successfully

In the middle of a deep blue ocean, choppy with small waves, are two rafts. On the left is a larger orange raft that surrounds the Apollo 10 spacecraft. The spacecraft is a rounded pyramid shape and is painted white. Two men in black wetsuits look on as astronaut Eugene A. Cernan emerges from the spacecraft. Two other astronauts dressed in white are already on the smaller orange raft on the right, along with another person in a black wetsuit.
NASA

Astronaut Eugene A. Cernan, lunar module pilot for the Apollo 10 mission, exits the spacecraft during recovery operations on May 26, 1969. He and the other two crew members already in the raft, Thomas P. Stafford (left) and John W. Young, were brought to the prime recovery ship, USS Princeton after splashdown.

The Apollo 10 mission was the first flight of a complete, crewed Apollo spacecraft to operate around the Moon. It encompassed all aspects of an actual crewed lunar landing, except the landing.

See more photos from the Apollo 10 mission.

Image Credit: NASA

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Monika Luabeya

Earth Science Information Partners Celebrate 25 Years of Collaboration

Earth Science Information Partners Celebrate 25 Years of Collaboration

13 min read

Earth Science Information Partners Celebrate 25 Years of Collaboration

Allison Mills, Earth Science Information Partners, allisonmills@esipfed.org
Susan Shingledecker, Earth Science Information Partners, susanshingledecker@esipfed.org

ESIP Photo 1
Photo 1. Photo of some of the in-person participants of the July 2023 ESIP Meeting. ESIP celebrated its twenty-fifth anniversary in 2023. Founded as a knowledge sharing space, the nonprofit has grown as a collaborative data hub.
Photo credit: Homer Horowitz/ Homer Horowitz Photography

Introduction

In 2023, the Earth Science Information Partners (ESIP) community celebrated 25 years since the nonprofit’s founding. Serving as a home for Earth science data and computing professionals, ESIP has evolved alongside the tools and vast expansion of Earth science data available now.

Building on the deep roots of collaboration that ground ESIP and honoring the 2023 Year of Open Science, the 2023 July ESIP Meeting’s theme focused on “Opening Doors to Open Science.” Open science is a collaborative culture enabled by technology that empowers the open sharing of data, information, and knowledge within the scientific community and the wider public to accelerate scientific research and understanding. This definition of open science comes from the 2021 article on the topic published in Earth and Space Science(To learn more about how open science is being implemented within the context of NASA’s Earth Science Division – see Open Source Science: The NASA Earth Science Perspective, in the September–October 2021 issue of The Earth Observer [Volume 33, Issue 5, pp. 5–9, 11].)

Participants from around the world gathered July 18–21, 2023, in Burlington, VT to explore this theme. One of the strengths of the ESIP community is how it brings people together from government agencies, academia, and industry to work toward common goals. Altogether, nearly 400 attendees from nearly as many institutions, spanning many technical domains and career stages, gathered for the 4-day meeting, which featured a hybrid format that allowed for both in-person participation and virtual access to all plenaries and breakout sessions. Some of the in-person attendees are shown in Photo 1.

This article begins with a brief section on the history and purpose of ESIP followed by a summary of the highlights from each day of the July 2023 meeting. 

History and Purpose of ESIP

ESIP was created in response to a National Research Council (NRC) review of the Earth Observing System Data and Information System (EOSDIS). (To learn more about EOSDIS, see Earth Science Data Operations: Acquiring, Distributing, and Delivering NASA Data for the Benefit of Society, in the March–April 2017 issue of The Earth Observer [Volume 29, Issue 2, pp. 4–18].) As NASA’s first Earth Observing System (EOS) missions were launching or preparing to launch, the NRC called on NASA to develop a new, distributed structure that would be operated and managed by the Earth science community and would include observation and research, application, and education data.

ESIP began with 24 NASA-funded partners, whose purpose was to experiment with and evolve methods to make Earth science data easy to preserve, locate, access, and use by a broad community encompassing research, education, and commercial interests. NASA adopted a deliberate and incremental approach in developing ESIP by starting with a limited set of prototype projects called ESIPs, representing both the research and applications development communities. These working prototype ESIP projects were joined by nine NASA distributed active archive centers (DAACs) to form the core of what was then known as the Federation of ESIPs and were responsible for creating its governing structures and the collaborative community it is today.

Although it started as a federation of partners connected due to a NASA mandate, ESIP has grown into an organization of organizations — and its membership has increased exponentially and diversified significantly. Today, there are more than 170 partner organizations – with room to grow. ESIP holds twice-annual meetings, which have run nonstop since 1998, and all past meeting material is available online. (To see an example of topics discussed at an early ESIP Federation meeting, see Meeting of the Federation of Earth Science Information Partners in the September–October 2001 issue of The Earth Observer [Volume 13, Issue 5, pp. 19–20, 26].)

ESIP also currently supports about 30 collaboration areas, which include 11 standing committees and numerous smaller clusters, or working groups. These committees and clusters conduct business both during and especially between meetings. ESIP also started the ESIP Lab, a microfunding initiative that supports learning objectives alongside technical skill-building. The establishment of an ESIP Community Fellows program has carved out a stronger foothold for early career professionals while the Awards, Endorsement, and programs offers knowledge sharing and recognition at all career stages.

ESIP still brings people together to work on complex Earth science issues — an important task that has not changed in over 25 years — but clearly the world is not the same as it was in 1998 when ESIP was established. This holds true for the hardware, software, remote sensing tools, and computing resources that have changed along with the people and communities who use them. In recognition of this, ESIP has developed a new mission and vision statements, and a new list of core values. A key moment in the 2023 July ESIP meeting (reported on below) was the revelation of these new statements, which were then refined during the meeting and voted on by the Board on July 17, 2023 — see ESIP Vision, Mission, and Core Value Statements below.

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ESIP Vision and Mission Statements and Core Values

Vision. We envision a world where data-driven solutions are a reality for all by making Earth science data actionable by all who need them anytime, anywhere.

Mission. To empower innovative use and stewardship of Earth science data to solve our planet’s greatest challenges.

Core Values. Integrity, inclusiveness, collaboration, openness, and curiosity.

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The new vision statement was intentionally worded to acknowledge how much power is at the fingertips of all data users. The new mission statement honors the depth of knowledge that is required to make data-driven decisions. Much like open science itself, there is a productive tension between wanting to make data as easy to use as possible while upholding the rigor of scientific standards.

All ESIP collaborations are open to everyone, whether an individual’s home institution is an ESIP partner or not.

Overview of the 2023 July ESIP Meeting

The 2023 July ESIP Meeting showcased how the attitudes, behaviors, connections, engagement, and responses of people to the natural environment as well as to agricultural and food systems – known as human dimensions – inform the ways the community tackles technical challenges and how important it is to gather, work together, and find inspiration. Summary highlights from the meeting follow – organized by day. All the meeting sessions were recorded and are available publicly through the ESIP YouTube channel. The reader is referred to these recordings to learn more about the topics mentioned here. 

The 2023 July ESIP meeting brought together 366 attendees – including 120 first-time participants. Through 4 plenaries and 44 breakout sessions, more than 100 organizers and speakers addressed the latest updates in Earth science data. Through the lens of open science, the community considered both the impact of the past 25 years of ESIP as well as how to move forward into the next quarter century. 

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Opening Doors – and Knocking Down Barriers – to Open Science

Throughout its history, ESIP meetings have brought together the most innovative thinkers and leaders around Earth observation data, forming a community dedicated to making Earth observations more discoverable, accessible, and useful to researchers, practitioners, policy makers, and the public. Openness is simply how work is done in ESIP.

Many participants are drawn to ESIP’s approach, because they find roadblocks to open collaboration and innovation elsewhere. While the ESIP community values the transparency and accountability that is fundamental to open science processes, ESIP participants also recognize the challenges in implementing those practices more broadly.

The 2023 July meeting was an excellent example. The “Opening Doors to Open Science” theme provided a space for participants to talk honestly about the institutional inertia, lack of incentives, and unintended consequences that hinder the open science approach. Often, the barriers are specific to particular domains, organizations, or roles. The ESIP meeting content explored such challenges – and solutions – for researchers, agencies, repositories, data managers, software developers, curriculum designers, and many other groups.

ESIP Sidebar Photo
Daniel Segessenman [ESIP Community Fellow] explains his poster at the Research Showcase in Burlington, VT.
Photo credit: Homer Horowitz
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DAY ONE

Susan Shingledecker [ESIP—Executive Director] gave the opening remarks and rallied the audience with interactive activities codesigned with Charley Haley [Way Foragers Consulting]. As a collaborative space, ESIP often breaks the norm of lecture-and-listen modes. The discussion and audience-driven talking points helped the community frame the week’s explorations of open science in Earth science data and computing.

Ken Casey [NOAA, National Center for Environmental Information (NCEI)—Deputy Chief of Data Stewardship and ESIP President 2021–2023] shared ESIP’s new mission, vision, and core values.

Kari Jordan [The Carpentries—Chief Executive Officer (CEO)] addressed the importance of authentic diversity and inclusion as a key function of open science. While she laid out systemic issues and barriers, her presentation focused mostly on action and solutions. She advised the ESIP community to use the organization’s core values and mission to continue opening doors to communities that have been historically left out of Science, Technology, Engineering, and Math (STEM) careers, leadership, and tech development.

The rest of the day was filled with rich, deep dives into many Earth science data and computing topics. Notable highlights include the hands-on, knowledge-sharing sessions led by the ESIP Cloud Computing Cluster, chaired by Aimee Barciauskas [Development Seed]. The sessions – from kerchunk tutorials to overviews of geospatial packages for the Python programming language, to lightning talks where speakers gave walkthroughs of tools used for cloud computing applications (e.g. GeoZarr, a geospatial extension to the Zarr specification for processing multidimensional arrays, or tensors, and storing and manipulating them on the cloud, and JupyterHub) – were often standing room only.

In addition to exploring technical tools, another breakout session motif centered around discussions on engaging stakeholders. One session featured Lesley-Ann Dupigny-Giroux [University of Vermont—State Climatologist], who spoke about climate preparedness for small communities, which was particularly relevant in light of the record-setting flooding that had taken place in Vermont just prior to the meeting. In another session, a team from NASA, including Grace Llewellyn [NASA/Jet Propulsion Laboratory—Software Engineer], Stephanie Schollaert Uz [NASA’s Goddard Space Flight Center (GSFC)—Applied Sciences Manager], and Jennifer Wei [GSFC—Scientist] alongside their collaborators Robert Gradeck [University of Pittsburgh], Mukul Sonwalkar [George Mason University], and Michiaki Tatsubori [IBM Research– Tokyo—Senior Technical Staff Member and Manager], focused on broader collaborations for natural disaster response. Several other sessions focused on specific end users in data centers, repositories, and universities.

DAY TWO

The second day of ESIP’s in-person meetings was nicknamed “Workshop Wednesday.” The day began with the ESIP Lab Plenary, followed by longer, in-depth sessions, and capped with the crowd-favorite Research Showcase Poster and Demo Reception.

Annie Burgess [ESIP—ESIP Lab Director] gave the opening remarks and welcomed Corine Farewell [University of Vermont Innovations] to share her perspective on open science and technology transfer. Many in the research community see the two at odds fundamentally – which the audience made clear during the question-and-answer session – but Farewell laid out how interactions between open science and technology transfer can open opportunities to tailor licensing and rollouts and to help ensure technology is shared and supported.

Scott Reinhard [New York Times—Graphics Editor] took the stage and showed a room full of data managers, researchers, and program directors just how powerful their work can be with the right color choice and analytical filtering for an audience’s intuitive ease – see Figure. As a data visualization expert, Reinhard laid out his creative process for making award-winning news graphics, built with data from sources such as the Moderate Resolution Imaging Spectroradiometer (MODIS) on NASA’s Terra and Aqua platforms, and from instruments on NASA–U.S. Geological Survey Landsat missions. His advice during the question-and-answer session was that “less is more.” He said sharing data with public audiences should be about meeting their needs with clarity and succinctness, which means removing ancillary data that is often included in more dense, scientific presentations.

ESIP Figure 1
Figure. This graphic shows an example of work by Scott Reinhard [New York Times], who uses national and state geospatial data to create data visualizations for broad audiences. This map depicts the Dixie Fire in California in 2021 and is shown in a newsprint layout.
Figure Credit: Scott Reinhard/New York Times

The rest of the day continued with community-led breakout sessions that dove into additional tools like OPeNDAP, Amazon Web Service’s SageMaker, and open data resources in NASA’s Earth Science Division. The day also featured a special plated lunch with presentations from ESIP Award winners. Falkenberg Awardees Angelia Seyfferth [University of Delaware] and Raskin Scholar Alexis Garretson [Tufts University] each shared their domain specialties, Seyfferth focusing on arsenic uptake in crops and Garretson on the ecology of mouse genomes.

In the afternoon, the ESIP Education Committee led the annual ESIP Teacher’s Workshop. The organizers brought together about a dozen instructors keen to learn more about Earth science data tools for use in their middle and high school classrooms. Every participant was given a solar eclipse kit, including eclipse glasses and lesson plans – see Photo 2.

The evening concluded with the Research Showcase, which featured 47 posters and demonstrations. This is a particularly important event for early career meeting attendees, including the ESIP Community Fellows.

ESIP Photo 2
Photo 2. The ESIP Teacher Workshop took participants outside to test the solar eclipse gear they will use in their classrooms.
Photo credit: Homer Horowitz

DAY THREE

While there was no plenary to start the day, breakout sessions continued throughout the morning and late afternoon. Covering artificial intelligence (AI) tools for wildfires, the United Nations Decade of Ocean Science for Sustainable Development (2021–2030), and the Ocean Decade, these ESIP sessions spanned the interdisciplinary breadth of the community. While many attendees have different backgrounds and career paths, it is the technical challenges and opportunities that bring everyone together.

A longer scheduled lunch break transitioned to the unconference, a space for on-the-fly and emergent discussions. Organizers pitched their mini-session ideas, the audience voted, then everyone split into discussion groups similar to organized coffee-break hallway chats. ESIP meeting feedback data shows that in-person attendees value time to integrate new knowledge and network; a short unconference has proven to be a productive way to encourage this.

Another key networking opportunity was the FUNding Friday microfunding competition. On Thursday night, participants gathered at a local eatery to ideate, write, and even draw their projects, which would be pitched the next morning.

DAY FOUR

While short, the final day of the ESIP meeting proved to be lively. The morning started with the FUNding Friday pitches and voting followed by the closing plenary and Partner Assembly Business meeting. The day concluded with the final breakout sessions, which highlighted the human and social aspects of implementing open science in an Earth data context. From the process of public comments to AI and large-language models, the breakouts illustrated how entangled human challenges are with technical and environmental ones.

Conclusion

Celebrating the organization’s twenty-fifth anniversary at the 2023 July ESIP Meeting tapped into the community’s deep roots while highlighting how much the gathering has grown and evolved. Over the next 25 years, the Earth sciences and its technology will continue to expand – and so will the user base.

To help make Earth science data and its tools accessible, ESIP is committed to making its meetings as open as possible. All ESIP meeting content is made freely available on the ESIP YouTube channel with no time limit.

In general, the ESIP community is open to all people interested in making Earth science data accessible and actionable. The community gathers twice each year in January and July, but the ESIP Collaboration Areas host monthly gatherings throughout the year. Additionally, the ESIP Lab offers seed funding for pilot projects.

Readers who wish to stay informed on the latest from ESIP, Earth science data community events, jobs, and resources are invited to subscribe to the weekly ESIP Update. The next ESIP meeting will take place in July 2024; watch the ESIP website and other social media for more details.

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