Members Can Post Anonymously On This Site
Preparing for Euclid’s first images: from puzzling data to dazzling views
-
Similar Topics
-
By NASA
4 min read
NASA Atmospheric Wave-Studying Mission Releases Data from First 3,000 Orbits
Following the 3,000th orbit of NASA’s AWE (Atmospheric Waves Experiment) aboard the International Space Station, researchers publicly released the mission’s first trove of scientific data, crucial to investigate how and why subtle changes in Earth’s atmosphere cause disturbances, as well as how these atmospheric disturbances impact technological systems on the ground and in space.
“We’ve released the first 3,000 orbits of data collected by the AWE instrument in space and transmitted back to Earth,” said Ludger Scherliess, principal investigator for the mission and physics professor at Utah State University. “This is a view of atmospheric gravity waves never captured before.”
Available online, the data release contains more than five million individual images of nighttime airglow and atmospheric gravity wave observations collected by the instrument’s four cameras, as well as derived temperature and airglow intensity swaths of the ambient air and the waves.
This image shows AWE data combined from two of the instrument’s passes over the United States. The red and orange wave-structures show increases in brightness (or radiance) in infrared light produced by airglow in Earth’s atmosphere. NASA/AWE/Ludger Scherliess “AWE is providing incredible images and data to further understand what we only first observed less than a decade ago,” said Esayas Shume, AWE program scientist at NASA Headquarters in Washington. “We are thrilled to share this influential data set with the larger scientific community and look forward to what will be discovered.”
Members of the AWE science team gather in the mission control room at Utah State University to view data collected by the mapping instrument mounted on the outside of the International Space Station. SDL/Allison Bills Atmospheric gravity waves occur naturally in Earth’s atmosphere and are formed by Earth’s weather and topography. Scientists have studied the enigmatic phenomena for years, but mainly from a few select sites on Earth’s surface.
“With data from AWE, we can now begin near-global measurements and studies of the waves and their energy and momentum on scales from tens to hundreds and even thousands of kilometers,” Scherliess said. “This opens a whole new chapter in this field of research.”
Data from AWE will also provide insight into how terrestrial and space weather interactions affect satellite communications, and navigation, and tracking.
“We’ve become very dependent on satellites for applications we use every day, including GPS navigation,” Scherliess said. “AWE is an attempt to bring science about atmospheric gravity waves into focus, and to use that information to better predict space weather that can disrupt satellite communications. We will work closely with our collaborators to better understand how these observed gravity waves impact space weather.”
AWE’s principal investigator, Ludger Scherliess, briefs collaborators of initial analysis of early AWE data. Information from the NASA-funded mission is helping scientists better understand how weather on Earth affects weather in space. SDL/Allison Bills The tuba-shaped AWE instrument, known as the Advanced Mesospheric Temperature Mapper or AMTM, consists of four identical telescopes. It is mounted to the exterior of the International Space Station, where it has a view of Earth.
As the space station orbits Earth, the AMTM’s telescopes capture 7,000-mile-long swaths of the planet’s surface, recording images of atmospheric gravity waves as they move from the lower atmosphere into space. The AMTM measures and records the brightness of light at specific wavelengths, which can be used to create air and wave temperature maps. These maps can reveal the energy of these waves and how they are moving through the atmosphere.
To analyze the data and make it publicly available, AWE researchers and students at USU developed new software to tackle challenges that had never been encountered before.
“Reflections from clouds and the ground can obscure some of the images, and we want to make sure the data provide clear, precise images of the power transported by the waves,” Scherliess said. “We also need to make sure the images coming from the four separate AWE telescopes on the mapper are aligned correctly. Further, we need to ensure stray light reflections coming off the solar panels of the space station, along with moonlight and city lights, are not masking the observations.”
As the scientists move forward with the mission, they’ll investigate how gravity wave activity changes with seasons around the globe. Scherliess looks forward to seeing how the global science community will use the AWE observations.
“Data collected through this mission provides unprecedented insight into the role of weather on the ground on space weather,” he said.
AWE is led by Utah State University in Logan, Utah, and it is managed by the Explorers Program Office at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. Utah State University’s Space Dynamics Laboratory built the AWE instrument and provides the mission operations center.
By Mary-Ann Muffoletto
Utah State University, Logan, UT
NASA Media Contact: Sarah Frazier
Share
Details
Last Updated Mar 14, 2025 Related Terms
Heliophysics Heliophysics Division Ionosphere Mesosphere Science Mission Directorate The Sun Uncategorized Explore More
2 min read Hubble Sees a Spiral and a Star
Article
7 hours ago
5 min read NASA’s Record-Shattering, Theory-Breaking MMS Mission Turns 10
Article
2 days ago
4 min read Discovery Alert: ‘Super-Earth’ Swings from Super-Heated to Super-Chill
Article
3 days ago
Keep Exploring Discover More Topics From NASA
Missions
Humans in Space
Climate Change
Solar System
View the full article
-
By NASA
Earth (ESD) Earth Explore Explore Earth Science Climate Change Air Quality Science in Action Multimedia Image Collections Videos Data For Researchers About Us 6 Min Read NASA Data Supports Everglades Restoration
Mangroves blanket roughly 600 square miles of South Florida’s coastal terrain. This dense grove — one of the largest in the world — is the ecological backbone of the Everglades system. This story is the second installment of a series on NASA’s mission to measure greenhouse gases in Florida’s mangrove ecosystem. Read the first part here.
Along the southernmost rim of the Florida Peninsula, the arching prop roots of red mangroves line the coast. Where they dip below the water’s surface, fish lay their eggs, using the protection from predators that the trees provide. Among their branches, wading birds like the great blue heron and the roseate spoonbill find rookeries to rear their young. The tangled matrix of roots collects organic matter and ocean-bound sediments, adding little by little to the coastline and shielding inland biology from the erosive force of the sea.
In these ways, mangroves are equal parts products and engineers of their environment. But their ecological value extends far beyond the coastline.
Tropical wetlands absorb carbon dioxide (CO2) from the atmosphere with impressive efficiency. Current estimates suggest they sequester carbon dioxide 10 times faster and store up to five times more carbon than old-growth forests. But as part of the ever-changing line between land and sea, coastal wetlands are vulnerable to disturbances like sea level rise, hurricanes, and changes in ocean salinity. As these threats intensify, Florida’s wetlands — and their role as a critical sink for carbon dioxide — face an uncertain future.
A new data product developed by NASA-funded researchers will help monitor from space the changing relationship between coastal wetlands and atmospheric carbon. It will deliver daily measurements of gaseous flux — the rate at which gas is exchanged between the planet’s surface and atmosphere. The goal is to improve local and global estimates of carbon dioxide levels and help stakeholders evaluate wetland restoration efforts.
NASA measures carbon dioxide from ground, air and space
At SRS-6, an eddy covariance tower measures carbon dioxide and methane flux among a dense grove of red, black, and white mangroves. (The term eddy covariance refers to the statistical technique used to calculate gaseous flux based on the meteorological and scalar atmospheric data collected by the flux towers.) Credits: NASA / Nathan Marder In the Everglades, flux measurements have historically relied on data from a handful of “flux towers.” The first of these towers was erected in June 2003, not far from the edge of Shark River at a research site known as SRS-6. A short walk from the riverbank, across a snaking path of rain-weathered, wooden planks, sits a small platform where the tower is anchored to the forest floor. Nearly 65 feet above the platform, a suite of instruments continuously measures wind velocity, temperature, humidity, and concentrations of atmospheric gases. These measurements are used to quantify the amount of carbon dioxide that wetland vegetation removes from the atmosphere — and the amount of methane released.
“Hundreds of research papers have come from this site,” said David Lagomasino, a professor of coastal ecology at East Carolina University. The abundance of research born from SRS-6 underscores its scientific value. But the BlueFlux campaign is committed to detailing flux across a much larger area — to fill in the gaps between the towers.
A true-color image of South Florida captured by the MODIS instrument aboard NASA’s Terra satellite. The area of Earth’s surface that the instrument’s sensors can “see” at one time — its swath — has a width of roughly 1,448 miles. Areas where primary BlueFlux fieldwork deployments occurred are marked with red triangles. NASA/ Nathan Marder Part of NASA’s new greenhouse-gas product is a machine-learning model that estimates gaseous flux using observations made by the Moderate Resolution Imaging Spectroradiometer (MODIS) instruments on NASA’s Aqua and Terra satellites. The MODIS instruments capture images and data of South Florida every one to two days, measuring the wavelength of sunlight reflected by the planet’s surface to produce a dataset called surface spectral reflectance.
Different surfaces — like water, vegetation, sand, or decaying organic matter — reflect different wavelengths of light. With the help of some advanced statistical algorithms, modelers can use these measurements to generate a grid of real-time flux data.
To help ensure the satellite-based model is making accurate predictions, researchers compare its outputs to measurements made on the ground. But with only a handful of flux towers in the region, ground-based flux data can be hard to come by.
To augment existing datasets, NASA researchers use a relatively new airborne technique for measuring flux. Since April 2022, NASA’s airborne science team has conducted 34 flights equipped with a payload known colloquially as “CARAFE,” short for the CARbon Airborne Flux Experiment. The CARAFE instrument measures concentrations of methane, carbon dioxide, and water vapor, generating readings that researchers combine with information about the plane’s speed and orientation to estimate rates of gaseous flux at fixed points along each flight’s path.
“This is one of the first times an instrument like this has flown over a mangrove forest anywhere in the world,” said Lola Fatoyinbo, a forest ecologist at NASA’s Goddard Space Flight Center in Greenbelt, Maryland.
Erin Delaria, a research scientist at the University of Maryland, monitors live, in-flight readings made by the CARbon Airborne Flux Experiment (CARAFE), the instrument package responsible for measuring atmospheric levels of carbon dioxide, methane, and water vapor concentrations above the wetland landscape. These data — along with information like the plane’s speed, flight path, and humidity levels — allow researchers to calculate flux at fixed points along the flight’s path. NASA/ Nathan Marder Early findings from space-based flux data confirm that, in addition to acting as a sink of carbon dioxide, tropical wetlands are a significant source of methane — a greenhouse gas that traps heat roughly 80 times more efficiently than carbon dioxide. In fact, researchers estimate that Florida’s entire wetland expanse produces enough methane to offset the benefits of wetland carbon removal by about 5%.
“There are also significant differences in fluxes between healthy mangroves and degraded ones,” Fatoyinbo said. In areas where mangrove forests are suffering, say after a major hurricane, “you end up with more greenhouse gases in the atmosphere.” As wetland ecology responds to intensifying natural and human pressures, the data product will help researchers precisely monitor the impact of ecological changes on global carbon dioxide and methane levels.
‘We need this reliable science’
The Everglades today are roughly half their original size — primarily the result of a century’s worth of uninterrupted land development and wetland drainage projects. It’s difficult to quantify the impact of wetland losses at this scale. Florida’s tropical wetlands aren’t just an important reminder of the beauty and richness of the state’s natural history. They’re also a critical reservoir of atmospheric carbon and a source of drinking water for millions of South Florida residents.
“We know how valuable the wetlands are, but we need this reliable science to help translate their benefits into something that can reach people and policymakers,” said Steve Davis, chief science officer for the Everglades Foundation, a non-profit organization in Miami-Dade County that provides scientific research and advocacy in an effort to protect and restore the Everglades.
As new policies and infrastructure are designed to support Everglades restoration, researchers hope NASA’s daily flux product will help local officials evaluate their restoration efforts in real time — and adjust the course as needed.
The prototype of the product, called Daily Flux Predictions for South Florida, is slated for release this year and will be available through NASA’s Oak Ridge National Laboratory (ORNL) Distributed Active Archive Center (DAAC).
By Nathan Marder
NASA’s Goddard Space Flight Center, Greenbelt, Maryland
About the Author
Nathan Marder
Share
Details
Last Updated Mar 14, 2025 Location Goddard Space Flight Center Related Terms
Earth Climate Change Earth’s Atmosphere Greenhouse Gases Explore More
8 min read NASA Researchers Study Coastal Wetlands, Champions of Carbon Capture
In the Florida Everglades, NASA’s BlueFlux Campaign investigates the relationship between tropical wetlands and greenhouse…
Article
23 hours ago
5 min read NASA’s Record-Shattering, Theory-Breaking MMS Mission Turns 10
Article
2 days ago
2 min read 2025 Aviation Weather Mission: Civil Air Patrol Cadets Help Scientists Study the Atmosphere with GLOBE Clouds
Article
1 week ago
Keep Exploring Discover More Topics From NASA
Missions
Humans in Space
Climate Change
Solar System
View the full article
-
By European Space Agency
Week in images: 10-14 March 2025
Discover our week through the lens
View the full article
-
By European Space Agency
Video: 01:08:00 Watch the replay of our Hera mission Mars flyby event. On 12 March 2025, ESA’s Hera mission came to within 5000 km of the surface of the red planet and 300 km of Mars’s more distant and enigmatic moon Deimos. During this flyby, Hera performed observations of both Mars and the city-sized Deimos. Hera then needed to swing its High Gain Antenna back to Earth to transmit its data home. On Thursday, 13 March, these images were premiered by Hera’s science team from ESA’s ESOC mission control centre in Darmstadt, Germany, explaining what they reveal, during our public webcast starting at 11:50 CET. The team was joined by ESA astronaut Alexander Gerst and renowned science fiction writer Andy Weir, author of The Martian and Project Hail Mary, as well as a surprise special guest!
View the full article
-
By NASA
4 Min Read NASA Cameras on Blue Ghost Capture First-of-its-Kind Moon Landing Footage
This compressed, resolution-limited video features a preliminary sequence of the Blue Ghost final descent and landing that NASA researchers stitched together from SCALPSS 1.1’s four short-focal-length cameras, which were capturing photos at 8 frames per second. Altitude data is approximate. Credits: NASA/Olivia Tyrrell A team at NASA’s Langley Research Center in Hampton, Virginia, has captured first-of-its-kind imagery of a lunar lander’s engine plumes interacting with the Moon’s surface, a key piece of data as trips to the Moon increase in the coming years under the agency’s Artemis campaign.
The Stereo Cameras for Lunar-Plume Surface Studies (SCALPSS) 1.1 instrument took the images during the descent and successful soft landing of Firefly Aerospace’s Blue Ghost lunar lander on the Moon’s Mare Crisium region on March 2, as part of NASA’s Commercial Lunar Payload Services (CLPS) initiative.
To view this video please enable JavaScript, and consider upgrading to a web browser that supports HTML5 video
This compressed, resolution-limited video features a preliminary sequence of the Blue Ghost final descent and landing that NASA researchers stitched together from SCALPSS 1.1’s four short-focal-length cameras, which were capturing photos at 8 frames per second. Altitude data is approximate.NASA/Olivia Tyrrell The compressed, resolution-limited video features a preliminary sequence that NASA researchers stitched together from SCALPSS 1.1’s four short-focal-length cameras, which were capturing photos at 8 frames per second during the descent and landing.
The sequence, using approximate altitude data, begins roughly 91 feet (28 meters) above the surface. The descent images show evidence that the onset of the interaction between Blue Ghost’s reaction control thruster plumes and the surface begins at roughly 49 feet (15 meters). As the descent continues, the interaction becomes increasingly complex, with the plumes vigorously kicking up the lunar dust, soil and rocks — collectively known as regolith. After touchdown, the thrusters shut off and the dust settles. The lander levels a bit and the lunar terrain beneath and immediately around it becomes visible.
Although the data is still preliminary, the 3000-plus images we captured appear to contain exactly the type of information we were hoping for…
Rob Maddock
SCALPSS project manager
“Although the data is still preliminary, the 3000-plus images we captured appear to contain exactly the type of information we were hoping for in order to better understand plume-surface interaction and learn how to accurately model the phenomenon based on the number, size, thrust and configuration of the engines,” said Rob Maddock, SCALPSS project manager. “The data is vital to reducing risk in the design and operation of future lunar landers as well as surface infrastructure that may be in the vicinity. We have an absolutely amazing team of scientists and engineers, and I couldn’t be prouder of each and every one of them.”
As trips to the Moon increase and the number of payloads touching down in proximity to one another grows, scientists and engineers need to accurately predict the effects of landings. Data from SCALPSS will better inform future robotic and crewed Moon landings.
The SCALPSS 1.1 technology includes six cameras in all, four short focal length and two long focal length. The long-focal-length cameras allowed the instrument to begin taking images at a higher altitude, prior to the onset of the plume-surface interaction, to provide a more accurate before-and-after comparison of the surface. Using a technique called stereo photogrammetry, the team will later combine the overlapping images – one set from the long-focal-length cameras, another from the short focal length – to create 3D digital elevation maps of the surface.
This animation shows the arrangement of the six SCALPSS 1.1 cameras and the instrument’s data storage unit. The cameras are integrated around the base of the Blue Ghost lander. Credit: NASA/Advanced Concepts Lab The instrument is still operating on the Moon and as the light and shadows move during the long lunar day, it will see more surface details under and immediately around the lander. The team also hopes to capture images during the transition to lunar night to observe how the dust responds to the change.
“The successful SCALPSS operation is a key step in gathering fundamental knowledge about landing and operating on the Moon, and this technology is already providing data that could inform future missions,” said Michelle Munk, SCALPSS principal investigator.
The successful SCALPSS operation is a key step in gathering fundamental knowledge about landing and operating on the Moon, and this technology is already providing data that could inform future missions
Michelle Munk
SCALPSS principal investigator
It will take the team several months to fully process the data from the Blue Ghost landing. They plan to issue raw images from SCALPSS 1.1 publicly through NASA’s Planetary Data System within six months.
The team is already preparing for its next flight on Blue Origin’s Blue Moon lander, scheduled to launch later this year. The next version of SCALPSS is undergoing thermal vacuum testing at NASA Langley ahead of a late-March delivery to Blue Origin.
The SCALPSS 1.1 project is funded by the Space Technology Mission Directorate’s Game Changing Development program.
NASA is working with several American companies to deliver science and technology to the lunar surface under the CLPS initiative. Through this opportunity, various companies from a select group of vendors bid on delivering payloads for NASA including everything from payload integration and operations, to launching from Earth and landing on the surface of the Moon.
About the Author
Joe Atkinson
Public Affairs Officer, NASA Langley Research Center
Share
Details
Last Updated Mar 13, 2025 Related Terms
General Explore More
4 min read Five Facts About NASA’s Moon Bound Technology
Article 2 weeks ago 6 min read Ten NASA Science, Tech Instruments Flying to Moon on Firefly Lander
Article 2 months ago 3 min read Electrodynamic Dust Shield Heading to Moon on Firefly Lander
Article 2 months ago Keep Exploring Discover More Topics From NASA
Missions
Humans in Space
Climate Change
Solar System
View the full article
-
-
Check out these Videos
Recommended Posts
Join the conversation
You can post now and register later. If you have an account, sign in now to post with your account.
Note: Your post will require moderator approval before it will be visible.