Members Can Post Anonymously On This Site
-
Similar Topics
-
By NASA
An artist’s concept of NASA’s Europa Clipper spacecraft. Credits: NASA/JPL-Caltech Lee esta nota de prensa en español aquí.
NASA will provide live coverage of prelaunch and launch activities for Europa Clipper, the agency’s mission to explore Jupiter’s icy moon Europa. NASA is targeting launch at 12:31 p.m. EDT Thursday, Oct. 10, on a SpaceX Falcon Heavy rocket from Launch Complex 39A at NASA’s Kennedy Space Center in Florida.
Beyond Earth, Jupiter’s moon Europa is considered one of the solar system’s most promising potentially habitable environments. After an approximately 1.8-billion-mile journey, Europa Clipper will enter orbit around Jupiter in April 2030, where the spacecraft will conduct a detailed survey of Europa to determine whether the icy world could have conditions suitable for life. Europa Clipper is the largest spacecraft NASA has ever developed for a planetary mission. It carries a suite of nine instruments along with a gravity experiment that will investigate an ocean beneath Europa’s surface, which scientists believe contains twice as much liquid water as Earth’s oceans.
For a schedule of live events and the platforms they’ll stream on, visit:
https://go.nasa.gov/europaclipperlive
The deadline for media accreditation for in-person coverage of this launch has passed. NASA’s media credentialing policy is available online. For questions about media accreditation, please email: ksc-media-accreditat@mail.nasa.gov.
NASA’s mission coverage is as follows (all times Eastern and subject to change based on real-time operations):
Tuesday, Oct. 8
1 p.m. – In-person, one-on-one interviews, open to media credentialed for this launch.
3:30 p.m. – NASA’s Europa Clipper science briefing with the following participants:
Gina DiBraccio, acting director, Planetary Science Division, NASA Headquarters Robert Pappalardo, project scientist, Europa Clipper, NASA JPL Haje Korth, deputy project scientist, Europa Clipper, Applied Physics Laboratory (APL) Cynthia Phillips, project staff scientist, Europa Clipper, NASA JPL Coverage of the science news conference will stream live on NASA+ and the agency’s website, Learn how to stream NASA content through a variety of platforms, including social media.
Media may ask questions in person and via phone. Limited auditorium space will be available for in-person participation. For the dial-in number and passcode, media should contact the NASA Kennedy newsroom no later than one hour before the start of the event at: ksc-newsroom@mail.nasa.gov.
Wednesday, Oct. 9
2 p.m. – NASA Social panel at NASA Kennedy with the following participants:
Kate Calvin, chief scientist and senior climate advisor, NASA Headquarters Caley Burke, Flight Design Analyst, NASA’s Launch Services Program Erin Leonard, project staff scientist, Europa Clipper, NASA JPL Juan Pablo León, systems testbed engineer, Europa Clipper, NASA JPL Elizabeth Turtle, principal investigator, Europa Imaging System instrument, Europa Clipper, APL The panel will stream live on NASA Kennedy’s YouTube, X, and Facebook accounts. Members of the public may ask questions online by posting to the YouTube, X, and Facebook live streams or using #AskNASA.
3:30 p.m. – NASA’s Europa Clipper prelaunch news conference (following completion of the Launch Readiness Review), with the following participants:
NASA Associate Administrator Jim Free Sandra Connelly, deputy associate administrator, Science Mission Directorate, NASA Headquarters Tim Dunn, launch director, NASA’s Launch Services Program Julianna Scheiman, director, NASA Science Missions, SpaceX Jordan Evans, project manager, Europa Clipper, NASA JPL Mike McAleenan, launch weather officer, 45th Weather Squadron, U.S. Space Force Coverage of the prelaunch news conference will stream live on NASA+, the agency’s website, the NASA app, and YouTube.
Media may ask questions in person and via phone. Limited auditorium space will be available for in-person participation. For the dial-in number and passcode, media should contact the NASA Kennedy newsroom no later than one hour before the start of the event at ksc-newsroom@mail.nasa.gov.
5:30 p.m. – NASA’s Europa Clipper rollout show. Coverage will stream live on NASA+, the agency’s website, the NASA app, and YouTube.
Thursday, Oct. 10
11:30 a.m. – NASA launch coverage in English begins on NASA+ and the agency’s website.
11:30 a.m. – NASA launch coverage in Spanish begins on NASA+, the agency’s website and NASA’s Spanish YouTube channel.
12:31 p.m. – Launch
Audio Only Coverage
Audio only of the news conferences and launch coverage will be carried on the NASA “V” circuits, which may be accessed by dialing 321-867-1220, -1240 or -7135. On launch day, “mission audio,” countdown activities without NASA+ media launch commentary, is carried on 321-867-7135.
Live Video Coverage Prior to Launch
NASA will provide a live video feed of Launch Complex 39A approximately 18 hours prior to the planned liftoff of the mission on the NASA Kennedy newsroom YouTube channel. The feed will be uninterrupted until the launch broadcast begins on NASA+.
NASA Website Launch Coverage
Launch day coverage of the mission will be available on the agency’s website. Coverage will include links to live streaming and blog updates beginning no earlier than 10 a.m., Oct. 10, as the countdown milestones occur. On-demand streaming video and photos of the launch will be available shortly after liftoff.
Follow countdown coverage on the Europa Clipper blog. For questions about countdown coverage, contact the Kennedy newsroom at 321-867-2468.
Para obtener información sobre cobertura en español en el Centro Espacial Kennedy o si desea solicitar entrevistas en español, comuníquese con Antonia Jaramillo: antonia.jaramillobotero@nasa.gov o Messod Bendayan: messod.c.bendayan@nasa.gov
Attend the Launch Virtually
Members of the public can register to attend this launch virtually. NASA’s virtual guest program for this mission also includes curated launch resources, notifications about related opportunities or changes, and a stamp for the NASA virtual guest passport following launch.
Watch, Engage on Social Media
Let people know you’re following the mission on X, Facebook, and Instagram by using the hashtags #EuropaClipper and #NASASocial. You can also stay connected by following and tagging these accounts:
X: @NASA, @EuropaClipper, @NASASolarSystem, @NASAJPL, @NASAKennedy, @NASA_LSP
Facebook: NASA, NASA’s Europa Clipper, NASA’s JPL, NASA’s Launch Services Program
Instagram: @NASA, @nasasolarsystem, @NASAKennedy, @NASAJPL
For more information about the mission, visit:
https://science.nasa.gov/mission/europa-clipper
-end-
Karen Fox / Molly Wasser
Headquarters, Washington
202-358-1600
karen.c.fox@nasa.gov / molly.l.wasser.nasa.gov
Leejay Lockhart
Kennedy Space Center, Florida
321-747-8310
leejay.lockhart@nasa.gov
Share
Details
Last Updated Oct 03, 2024 LocationKennedy Space Center Related Terms
Europa Clipper Europa Jupiter Jupiter Moons Missions View the full article
-
By NASA
5 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater)
NASA’s Psyche spacecraft is depicted receiving a laser signal from the Deep Space Optical Communications uplink ground station at JPL’s Table Mountain Facility in this artist’s concept. The DSOC experiment consists of an uplink and downlink station, plus a flight laser transceiver flying with Psyche.NASA/JPL-Caltech The Deep Space Optical Communications tech demo has completed several key milestones, culminating in sending a signal to Mars’ farthest distance from Earth.
NASA’s Deep Space Optical Communications technology demonstration broke yet another record for laser communications this summer by sending a laser signal from Earth to NASA’s Psyche spacecraft about 290 million miles (460 million kilometers) away. That’s the same distance between our planet and Mars when the two planets are farthest apart.
Soon after reaching that milestone on July 29, the technology demonstration concluded the first phase of its operations since launching aboard Psyche on Oct. 13, 2023.
“The milestone is significant. Laser communication requires a very high level of precision, and before we launched with Psyche, we didn’t know how much performance degradation we would see at our farthest distances,” said Meera Srinivasan, the project’s operations lead at NASA’s Jet Propulsion Laboratory in Southern California. “Now the techniques we use to track and point have been verified, confirming that optical communications can be a robust and transformative way to explore the solar system.”
Managed by JPL, the Deep Space Optical Communications experiment consists of a flight laser transceiver and two ground stations. Caltech’s historic 200-inch (5-meter) aperture Hale Telescope at Caltech’s Palomar Observatory in San Diego County, California, acts as the downlink station to which the laser transceiver sends its data from deep space. The Optical Communications Telescope Laboratory at JPL’s Table Mountain facility near Wrightwood, California, acts as the uplink station, capable of transmitting 7 kilowatts of laser power to send data to the transceiver.
This visualization shows Psyche’s position on July 29 when the uplink station for NASA’s Deep Space Optical Communications sent a laser signal about 290 million miles to the spacecraft. See an interactive version of the Psyche spacecraft in NASA’s Eyes on the Solar System.NASA/JPL-Caltech By transporting data at rates up to 100 times higher than radio frequencies, lasers can enable the transmission of complex scientific information as well as high-definition imagery and video, which are needed to support humanity’s next giant leap when astronauts travel to Mars and beyond.
As for the spacecraft, Psyche remains healthy and stable, using ion propulsion to accelerate toward a metal-rich asteroid in the main asteroid belt between Mars and Jupiter.
Exceeding Goals
The technology demonstration’s data is sent to and from Psyche as bits encoded in near-infrared light, which has a higher frequency than radio waves. That higher frequency enables more data to be packed into a transmission, allowing far higher rates of data transfer.
Even when Psyche was about 33 million miles (53 million kilometers) away — comparable to Mars’ closest approach to Earth — the technology demonstration could transmit data at the system’s maximum rate of 267 megabits per second. That bit rate is similar to broadband internet download speeds. As the spacecraft travels farther away, the rate at which it can send and receive data is reduced, as expected.
On June 24, when Psyche was about 240 million miles (390 million kilometers) from Earth — more than 2½ times the distance between our planet and the Sun — the project achieved a sustained downlink data rate of 6.25 megabits per second, with a maximum rate of 8.3 megabits per second. While this rate is significantly lower than the experiment’s maximum, it is far higher than what a radio frequency communications system using comparable power can achieve over that distance.
This Is a Test
The goal of Deep Space Optical Communications is to demonstrate technology that can reliably transmit data at higher speeds than other space communication technologies like radio frequency systems. In seeking to achieve this goal, the project had an opportunity to test unique data sets like art and high-definition video along with engineering data from the Psyche spacecraft. For example, one downlink included digital versions of Arizona State University’s “Psyche Inspired” artwork, images of the team’s pets, and a 45-second ultra-high-definition video that spoofs television test patterns from the previous century and depicts scenes from Earth and space.
This 45-second ultra-high-definition video was streamed via laser from deep space by NASA’s Deep Space Optical Communications technology demonstration on June 24, when the Psyche spacecraft was 240 million miles from Earth. NASA/JPL-Caltech The technology demonstration beamed the first ultra-high-definition video from space, featuring a cat named Taters, from the Psyche spacecraft to Earth on Dec. 11, 2023, from 19 million miles away. (Artwork, images, and videos were uploaded to Psyche and stored in its memory before launch.)
“A key goal for the system was to prove that the data-rate reduction was proportional to the inverse square of distance,” said Abi Biswas, the technology demonstration’s project technologist at JPL. “We met that goal and transferred huge quantities of test data to and from the Psyche spacecraft via laser.” Almost 11 terabits of data have been downlinked during the first phase of the demo.
The flight transceiver is powered down and will be powered back up on Nov. 4. That activity will prove that the flight hardware can operate for at least a year.
“We’ll power on the flight laser transceiver and do a short checkout of its functionality,” said Ken Andrews, project flight operations lead at JPL. “Once that’s achieved, we can look forward to operating the transceiver at its full design capabilities during our post-conjunction phase that starts later in the year.”
More About Deep Space Optical Communications
This demonstration is the latest in a series of optical communication experiments funded by the Space Technology Mission Directorate’s Technology Demonstration Missions Program managed at NASA’s Marshall Space Flight Center in Huntsville, Alabama, and the agency’s SCaN (Space Communications and Navigation) program within the Space Operations Mission Directorate. Development of the flight laser transceiver is supported by MIT Lincoln Laboratory, L3 Harris, CACI, First Mode, and Controlled Dynamics Inc. Fibertek, Coherent, Caltech Optical Observatories, and Dotfast support the ground systems. Some of the technology was developed through NASA’s Small Business Innovation Research program.
For more information about the laser communications demo, visit:
https://www.jpl.nasa.gov/missions/dsoc
NASA’s Optical Comms Demo Transmits Data Over 140 Million Miles The NASA Cat Video Explained 5 Things to Know About NASA’s Deep Space Optical Communications News Media Contacts
Ian J. O’Neill
Jet Propulsion Laboratory, Pasadena, Calif.
818-354-2649
ian.j.oneill@jpl.nasa.gov
2024-130
Share
Details
Last Updated Oct 03, 2024 Related Terms
Deep Space Optical Communications (DSOC) Jet Propulsion Laboratory Psyche Mission Space Communications & Navigation Program Space Operations Mission Directorate Space Technology Mission Directorate Tech Demo Missions Explore More
3 min read How NASA Astronauts Vote from Space Aboard International Space Station
Article 23 mins ago 2 min read The Science of the Perfect Cup for Coffee
Material research is behind the design of a temperature-regulating mug
Article 6 days ago 1 min read Let It Go: (After Latching) Challenge
Article 1 week ago Keep Exploring Discover Related Topics
Missions
Humans in Space
Climate Change
Solar System
View the full article
-
By NASA
Skywatching Home What’s Up: October 2024… Skywatching Skywatching Home Eclipses What’s Up Explore the Night Sky Night Sky Network More Tips and Guides FAQ Comets: Unpredictable, But Irresistible
A new comet is passing through the inner solar system! Time will tell if it’s the brightest of the year, once it appears in twilight after about October 14.
Skywatching Highlights
All month – Planet visibility report: Look for Venus low in the west just after sunset; Saturn can be seen toward the southeast as soon as it gets dark; Mars rises around midnight; and Jupiter rises in the first half of the night (rising earlier as the month goes on). October 2 – New moon October 11 – Europa is easily observable to one side of Jupiter by itself this morning using binoculars. October 14-31 – Comet C/2023 A3 (Tsuchinshan-ATLAS) becomes visible low in the west following sunset. If the comet’s tail is well-illuminated by sunlight, it could be visible to the unaided eye. The first week and a half (Oct. 14-24) is the best time to observe, using binoculars or a small telescope. October 13-14 – After dark both nights, look for the nearly full Moon with Saturn toward the southeast. October 17 – Full moon October 20 – The Moon rises near Jupiter, with the giant planet looking extremely bright. You should be able to find them low in the east after around 10 pm. October 23-24 – Early risers will be able to spot Mars together with the Moon, high overhead in the south both mornings. October 25 – Europa is easily observable to one side of Jupiter by itself this morning using binoculars. Transcript
What’s Up for October?
This month’s viewing tips for Venus, Saturn, Mars and Jupiter. When’s the best time to observe the destination of NASA’s next deep space mission? And how you can see a (potentially bright) comet this month?
And watch our video ’till the end for photos of highlights from last month’s skies.
Sky chart showing Mars near the Moon on October 23. The pair appear quite high overhead, along with Jupiter. NASA/JPL-Caltech Up first, we look at the visibility of the planets in October. Look for Venus low in the west just after sunset. It’s setting by the time the sky is fully dark. Saturn is visible toward the southeast as soon as it gets dark out, and sets by dawn. Mars rises around midnight all month. By dawn it has climbed quite high into the south-southeastern sky, appearing together with Jupiter. Now, Jupiter is rising in the first half of the night. In early October you’ll find it high in the south as dawn approaches, and later in the month it’s progressed farther over to the west before sunrise.
And, speaking of Jupiter, NASA plans to launch its latest solar system exploration mission to one of the giant planet’s moons this month. Europa Clipper is slated to blast off as early as October 10th. It’s thought that Europa holds an enormous ocean of salty liquid water beneath its icy surface. That makes this the first mission dedicated to studying an ocean world beyond Earth. Europa Clipper is designed to help us understand whether this icy moon could support some form of life, and along the way it’ll teach us more about the conditions that make a world habitable.
Now, if you’ve ever pointed binoculars or a telescope at Jupiter, you know the thrill of seeing the little star-like points of light next to it that are its four large moons, which were first observed by Galileo in 1610.
There are two mornings in October, the 11th and the 25th, when you can most easily observe Europa. These are times when the moon is at its greatest separation from the planet as seen from here on Earth, and it’s all by itself to one side of Jupiter. So be sure to have your own peek at Jupiter’s moon Europa this month, as a new NASA mission begins its journey to explore an ocean in the sky.
Now a look at Moon and planet pair-ups for October. On the 13th and 14th after dark, look for the nearly full Moon with Saturn toward the southeast. Then on the evening of October 20th, the Moon rises near Jupiter, with the giant planet looking extremely bright.
You should be able to find them low in the east after around 10 pm that night. Then, in the morning of Oct. 23rd and 24th, early risers will be able to spot Mars together with the Moon, high overhead in the south.
Sky chart showing the location of Comet C/2023 A3 between Oct. 14 and Oct 24 following sunset. The comet climbs higher each evening, but also grows fainter. NASA/JPL-Caltech October offers a chance to observe what could be the brightest comet of the year. Earlier this year we got a look at Comet 12P, which was visible with binoculars but not super bright. Now another of these ancient and icy dust balls is streaking through our neighborhood on an 80,000-year orbit from the distant reaches of the Oort Cloud. The comet, known as C/2023 A3, aka Tsuchinshan-ATLAS, is currently speeding through the inner solar system. It passed its closest to the Sun in late September, and will be at its closest to Earth on October 13th. And after that time, through the end of the month, will be the best time to look for it. This is when the comet will become visible low in the western sky beginning during twilight.
It will quickly rise higher each subsequent evening, making it easier to observe, but it’ll also be getting a little fainter each night. As with all comets, predictions for how bright it could get are uncertain. If the comet’s tail is brilliantly illuminated by the Sun, predictions show that it could become bright enough to see with the unaided eye. But comets have a way of surprising us, so we’ll just have to wait and see.
Your best shot at seeing it will be from around October 14th through the 24th, with binoculars or a small telescope, and a reasonably clear view toward the west. So good luck, and clear skies, comet hunters!
Watch our video for views of what some of the highlights we told you about in last month’s video actually looked like.
The phases of the Moon for October 2024. NASA/JPL-Caltech And here are the phases of the Moon for October. Stay up to date on all of NASA’s missions exploring the solar system and beyond at science.nasa.gov. I’m Preston Dyches from NASA’s Jet Propulsion Laboratory, and that’s What’s Up for this month.
Keep Exploring Discover More Topics From NASA
Skywatching
Skywatching FAQ
Frequently asked questions about skywatching, answered by NASA.
What’s Up
Explore the Night Sky
View the full article
-
By NASA
9 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater)
The Oceans group, from the 2024 Student Airborne Research Program (SARP) West Coast cohort, poses in front of the natural sciences building at UC Irvine, during their final presentations on August 13, 2024. NASA Ames/Milan Loiacono Faculty Advisor: Dr. Henry Houskeeper, Woods Hole Oceanographic Institute
Graduate Mentor: Lori Berberian, University of California, Los Angeles
Lori Berberian, Graduate Mentor
Lori Berberian graduate student mentor for the 2024 SARP West Oceans group, provides an introduction for each of the group members and shares behind-the scenes moments from the internship.
Emory Gaddis
Leveraging High Resolution PlanetScope Imagery to Quantify oil slick Spatiotemporal Variability in the Santa Barbara Channel
Emory Gaddis, Colgate University
Located within the Santa Barbara Channel of California, Coal Oil Point is one of the world’s largest hydrocarbon seep fields. The area’s natural hydrocarbon seepage and oil production have sustained both scientific interest and commercial activity for decades. Historically, indigenous peoples in the region utilized the naturally occurring tar for waterproofing baskets, establishing early evidence of the natural presence of hydrocarbons long before modern oil extraction began. Gaseous hydrocarbons are released from the marine floor through the process of seeping, wherein a buildup of reservoir pressure relative to hydrostatic pressure causes bubbles, oily bubbles, and droplets to rise to the surface. This hydrocarbon seepage is a significant source of Methane CH4—a major greenhouse gas––emissions into the atmosphere. Current limitations of optical remote sensing of oil presence and absence in the ocean leverage geometrical as well as biogeochemical factors and include changes in observed sun glint, sea surface damping, and wind roughening due to changes in surface oil concentrations. We leverage high-resolution (3m) surface reflectance observations obtained from PlanetScope to construct a time series of oil slick surface area spanning 2017 to 2023 within the Coal Oil Point seep field. Our initial methods are based on manual annotations performed within ArcGIS-Pro. We assess potential relationships between wind speed and oil slick surface area to support a sensitivity analysis of our time series. Correcting for confounding outside factors (e.g., wind speed) that modify oil slick surface area improves determination of oil slick surface area and helps test for changes in natural seepage rates and whether anthropogenic activities, such as oil drilling, alter natural oil seepage. Future investigations into oil slick chemical properties and assessing how natural seepage impacts marine and atmospheric environments (e.g., surface oil releases methane into the atmosphere) can help to inform the science of optimizing oil extraction locations.
Rachel Emery
Investigating Airborne LiDAR Retrievals of an Emergent South African Macroalgae
Rachel Emery, The University of Oklahoma
Right now, the world is facing an unprecedented biodiversity crisis, with areas of high biodiversity at the greatest risk of species extinction. One of these biodiversity hotspots, the Western Cape Province of South Africa, features one of the world’s largest unique marine ecosystems due to the extensive growth of canopy forming kelps, such as Macrocystis and Ecklonia, which provide three-dimensional structure important for fostering biodiversity and productivity. Canopy-forming kelps face increasing threats by marine heatwaves and pollution related to climate change and local water quality perturbation. Though these ecosystems can be monitored using traditional field surveying methods, remote sensing via airborne and satellite observations support improved spatial coverage and resample rates, plus extensive historical continuity for tracking multidecadal scale changes. Passive remote sensing observations—such as those derived using observations from NASA’s Airborne Visible-Infrared Imaging Spectrometer – Next Generation (AVIRIS-NG) —provide high resolution, hyperspectral imagery of oceanic environments anticipated to help characterize community dynamics and quantify macroalga physiological change. Active remote sensing observations, e.g., Light Detection and Ranging (LiDAR), are less understood in terms of applications to marine ecosystems, but are anticipated to support novel observations of vertical structure not supported using passive aquatic remote sensing. Here we investigate the potential to observe an emergent canopy-forming macroalgae (i.e., Ecklonia, which can extend more than a decimeter above the ocean’s surface) using NASA’s Land, Vegetation, and Ice sensor (LVIS), which confers decimeter-scale vertical resolution. We validate LVIS observations using matchup observations from AVIRIS-NG imagery to test whether LiDAR remote sensing can improve monitoring of emergent kelps in key biodiversity regions such as the Western Cape.
Brayden Lipscomb
Vertical structure of the aquatic light field based on half a century of oceanographic records from the southern California Current
Brayden Lipscomb, West Virginia University
Understanding the optical properties of marine ecosystems is crucial for improving models related to oceanic productivity. Models relating satellite observations to oceanic productivity or subsurface (e.g., benthic) light availability often suffer from uncertainties in parameterizing vertical structure and deriving columnar parameters from surface observations. The most accurate models use in situ station data, minimizing assumptions such as atmospheric optical thickness or water column structure. For example, improved accuracy of satellite primary productivity models has previously been demonstrated by incorporating information on vertical structure obtained from gliders and floats. We analyze vertical profiles in photosynthetically available radiation (PAR) obtained during routine surveys of the southern California Current system by the California Cooperative Oceanic Fisheries Investigation (CalCOFI). We find that depths of 1% and 10% light availability show coherent log-linear relationships with attenuation measured near surface (i.e., within the first 10 m), despite vertical variability in water column constituent concentrations and instrumentation challenges related to sensitivity, self-shading, and ship adjacency. Our results suggest that subsurface optical properties can be more reliably parameterized from near-surface measurements than previously understood.
Dominic Bentley
Comparing SWOT and PACE Satellite Observations to Assess Modification of Phytoplankton Biomass and Assemblage by North Atlantic Ocean Eddies
Dominic Bentley, Pennsylvania State University
Upwelling is the shoaling of the nutricline, thermocline, and isopycnals due to advection by eddies of the surface ocean layer. This shoaling effect leads to an increase in the productivity of algal blooms in a given body of water. Mesoscale to deformation scale eddy circulation modulates productivity based on latitude, season, direction, and other physical factors. However, many processes governing the effects of eddies on the ocean microbial environment remain unknown due to limitations in observations linking eddy strength and direction with productivity and ocean biogeochemistry. Currently, satellites are the only ocean observing system that allows for broad spatial coverage with high resample rates, albeit with limitations due to cloud obstructions (including storms that may stimulate productivity) and to observations being limited to the near-surface. A persisting knowledge gap in oceanography stems from limitations in the spatial resolution of observations resolving submesoscale dynamics. The recent launch of the Surface Water and Ocean Topography (SWOT) mission in December of 2022 supports observations of upper-ocean circulation with increased resolution relative to legacy missions (e.g. TOPEX/Poseidon, Jason-1, OSTM/Jason-2). Meanwhile, the launch of the Plankton, Aerosol, Cloud, ocean Ecosystem (PACE) satellite in February of 2024 is anticipated to improve knowledge of ocean microbial ecosystem dynamics. We match up SWOT observations of sea surface height (SSH) anomalies—informative parameters of eddy vorticity—with PACE observations of surface phytoplankton biomass and community composition to relate the distribution of phytoplankton biomass and assemblage structure to oceanic eddies in the North Atlantic. We observe higher concentrations of Chlorophyll a (Chla) within SSH minima indicating the stimulation of phytoplankton productivity by cyclonic features associated with upwelling-driven nutrient inputs.
Abigail Heiser
Assessing EMIT observations of harmful algae in the Salton Sea
Abigail Heiser, University of Wisconsin- Madison
In 1905, flooding from the Colorado River gave rise to what would become California’s largest lake, the Salton Sea. Today, the majority of its inflow is sourced from agricultural runoff, which is rich in fertilizers and pollutants, leading to elevated lake nutrient levels that fuel harmful algal blooms (HAB) events. Increasingly frequent HAB events pose ecological, environmental, economic, and health risks to the region by degrading water quality and introducing environmental toxins. Using NASA’s Earth Surface Mineral Dust Source Investigation (EMIT) imaging spectrometer we apply two hyperspectral aquatic remote sensing algorithms; cyanobacteria index (CI) and scattering line height (SLH). These algorithms detect and characterize spatiotemporal variability of cyanobacteria, a key HAB taxa. Originally designed to study atmospheric mineral dust, EMIT’s data products provide novel opportunities for detailed aquatic characterizations with both high spatial and high spectral resolution. Adding aquatic capabilities for EMIT would introduce a novel and cost-effective tool for monitoring and studying the drivers and timing of HAB onset, to improve our understanding of environmental dynamics.
Emma Iacono
Reassessing multidecadal trends in Water Clarity for the central and southern California Current System
Emma Iacono, North Carolina State University
Over the past several decades, the world has witnessed a steady rise in average global temperatures, a clear indication of the escalating effects of climate change. In 1990, Andrew Bakun hypothesized that unequal warming of sea and land surface temperatures would increase pressure gradients and lead to rising rates of alongshore upwelling within Eastern Boundary Currents, including the California Current System (CCS). An anticipated increase in upwelling-favorable winds would have profound implications for the productivity of the CCS, wherein upwelled waters supply nutrient injections that sustain and fuel coastal ocean phytoplankton stocks. Increasing upwelling, therefore, is anticipated to increase the turbidity of the upper ocean, corresponding with greater phytoplankton concentrations. Historical observations of turbidity are supported by observations obtained using a Secchi Disk, i.e., an opaque white instrument lowered into the water column. Observations of Secchi depth—or the depth at which light reflected from the Secchi Disk is no longer visible from the surface—provide a quantification of light penetration into the euphotic zone. The shoaling, or shallowing, of Secchi disk depths was previously reported for inshore, transition, and offshore waters of the central and southern CCS for historical observations spanning 1969 – 2007. Here, we reassess Secchi disk depths during the subsequent period spanning 2007 to 2021 and test for more recent changes in water clarity. Additionally, we evaluate the seasonality and spatial patterns of Secchi disk trends to test for potential changes to oceanic microbial ecology. Indications of long-term trends in some of the coastal domains assessed were found. Generally, our findings suggest a reversal of the trends previously reported. In particular, increases in water clarity likely associated with a recent marine heatwave (MHW) may be responsible for recent changes in Secchi disk depth observations, illustrating the importance of MHW events for modifying the CCS microbial ecosystem.
Click here watch the Atmospheric Aerosols Group presentations.
Click here watch the Terrestrial Ecology Group presentations.
Click here watch the Whole Air Sampling (WAS) Group presentations.
Return to 2024 SARP West Closeout Share
Details
Last Updated Sep 25, 2024 Related Terms
General View the full article
-
By NASA
10 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater)
The Whole Air Sampling (WAS) group, from the 2024 Student Airborne Research Program (SARP) West Coast cohort, poses in front of the natural sciences building at UC Irvine, during their final presentations on August 13, 2024. NASA Ames/Milan Loiacono Faculty Advisor: Dr. Donald Blake, University of California, Irvine
Graduate Mentor: Katherine Paredero, Georgia Institute of Technology
Katherine Paredero, Graduate Mentor
Katherine Paredero, graduate student mentor for the 2024 SARP West Whole Air Sampling (WAS) group, provides an introduction for each of the group members and shares behind-the scenes moments from the internship.
Mikaela Vaughn
Urban Planning Initiative: Investigation of Isoprene Emissions by Tree Species in the LA Basin
Mikaela Vaughn, Virginia Commonwealth University
Elevated ozone concentrations have been a concern in Southern California for decades. The interaction between volatile organic compounds (VOC) and nitrous oxides (𝑁𝑂!) in the presence of sunlight leads to enhanced formation of tropospheric ozone (𝑂”) and secondary organic aerosols (SOA). This can lead to increased health hazards, exposing humans to aerosols that can enter and be absorbed by the lungs, as well as a warming effect caused by ozone’s role as a greenhouse gas in the lower levels of the atmosphere. This study will focus on a VOC that is of particular interest, isoprene, which has an atmospheric lifetime of one hour, making it highly reactive in the presence of the hydroxyl radical (OH) and resulting in rapid ozone formation. Isoprene is a biogenic volatile organic compound (BVOC) emitted by vegetation as a byproduct of photosynthesis. This BVOC has been overlooked but should be investigated further because of its potential to form large sums of ozone. In this study the reactivity of isoprene with OH dominated ozone formation as compared to other VOCs. Ambient isoprene concentrations were measured aboard NASA’s airborne science laboratory (King Air B200) along with whole air sampling canisters. Additionally, isoprene emissions of varying tree species, with one to three samples per type, were compared to propose certain trees to plant in urban areas. Results indicated that Northern Red Oaks and the Palms family emitted the most isoprene out of the nineteen species documented. The species with the lowest observed isoprene emissions was the Palo Verde and the Joshua trees. The difference in isoprene emissions between the Northern Red Oak and Joshua trees is approximately by a factor of 45. These observations show the significance of considering isoprene emissions when selecting tree species to plant in the LA Basin to combat tropospheric ozone formation.
Joshua Lozano
VOC Composition and Ozone Formation Potential Observed Over Long Beach, California
Joshua Lozano, Sonoma State University
Volatile organic compounds (VOCs), when released into the atmosphere, undergo chemical reactions in the presence of sunlight that can generate tropospheric ozone, which can have various health effects. We can gauge this ozone formation by multiplying the observed mixing ratios of VOCs by their respective rate constants (with respect to OH radicals). The OH radical reacts very quickly in the atmosphere and accounts for a large sum of ozone formation from VOCs as a result, giving us an idea of the ozone formation potential (OFP) for each VOC. In this study, we investigate observed mixing ratios of VOCs in order to estimate their contribution to OFP over Long Beach, California. The observed species of VOCs with the highest mixing ratios differs from the observed species with the highest OFP, which highlights that higher mixing ratios of certain VOCs in the atmosphere do not necessarily equate to a higher contribution to ozone formation. This underscores the importance of understanding mixing ratios of VOC species and their reaction rates with OH to gauge impacts on ozone formation. In the summer there were significantly lower VOC concentrations compared to the winter, which was expected because of differences in boundary layer height within the seasons. Additionally, a decrease in average mixing ratios was observed between the summer of 2014 and the summer of 2022. A similar trend was observed in OFP, but by a much smaller factor. This may indicate that even though overall VOC emissions are decreasing in Long Beach, the species that dominate in recent years have a higher OFP. This research provides a more comprehensive view of how VOCs contribute to air quality issues across different seasons and over time, stressing the need for targeted strategies to mitigate ozone pollution based on current and accurate VOC composition and reactivity.
Sean Breslin
Investigating Enhanced Methane and Ethane Emissions over the Long Beach Airport
Sean Breslin, University of Delaware
As climate change continues to worsen, the investigation and tracking of greenhouse gas emissions has become increasingly important. Methane, the second most impactful greenhouse gas, has accounted for over 20% of planetary warming since preindustrial times. Methane emissions primarily originate from biogenic and thermogenic sources, such as dairy farms and natural gas extraction. Ethane, an abundant hydrocarbon emitted from biomass burning and natural gas, contributes to the formation of tropospheric ozone. The data for this project was collected in December 2021 and June 2022 aboard the DC-8 aircraft, where whole air samples were taken during low approaches to find potential sources of methane and ethane emissions. Analysis of these samples using gas chromatography revealed a noticeable increase in methane and ethane concentrations over Long Beach Airport, an area surrounded by numerous plugged oil and gas wells extracting crude oil and natural gas. In this study, we observe that methane and ethane concentrations were lower in the summer and higher in the winter, which can be primarily attributed to seasonal variations in the Atmospheric Boundary Layer height. Our results show that in both summer and winter campaigns, the ratio of these two gases over the airport was approximately 0.03, indicating that for every 100 methane molecules, there are 3 ethane molecules. This work identifies methane and ethane hotspots and provides a critical analysis on potential fugitive emission sources in the Long Beach area. These results emphasize a need to perform in depth analyses on potential point sources of greenhouse gas emissions in the Long Beach area.
Katherine Skeen
Investigating Elevated Levels of Toluene during Winter in the Imperial Valley
Katherine Skeen, University of North Carolina at Charlotte
The Imperial County in Southern California experiences pollutants that do not meet the National Ambient Air Quality Standards, and as a result, residents are suffering from adverse health effects. Volatile organic compounds (VOCs) are compounds with a high vapor pressure at room temperature. They are readily emitted into the atmosphere and form ground level ozone. Toluene is a VOC and exposure poses significant health risks, including neurological and respiratory effects. This study aims to use airborne data to investigate areas with high toluene concentrations and investigate potential source. Flights over the Imperial Valley were conducted in the B200 King Air. Whole air canisters were used to collect ambient air samples from outside the plane. These Whole Air Canisters were put through the UCI Rowland Blake Lab’s gas chromatograph mass spectrometer, which identifies different gasses and quantifies their concentrations. Elevated values of toluene were found in the winter as compared to the summer in the Imperial Valley, with the town of Brawley having the most elevated amounts in the air. Excel and QGIS were utilized to analyze data trends. Additionally, a backward trajectory calculated using the NOAA HYSPLIT model revealed the general air flow on days exhibiting high toluene concentrations. Here we suggest Long Beach may be a source of enhanced toluene levels in Brawley. Both areas exhibited enhanced levels of toluene with slightly lower concentrations observed in Brawley. We additionally observed other VOCs commonly emitted in urban areas, and saw a similar decrease in gasses from Long Beach to Brawley. This trend may indicate transport of toluene from Long Beach to Brawley. Further research could be done to investigate the potential for other regions that may contribute to high toluene concentrations in Brawley. My study contributes valuable insights to the poor air quality in the Imperial Valley, providing a foundation for future studies on how residents are specifically being affected.
Ella Erskine
Characterizing Volatile Organic Compound (VOC) Emissions from Surface Expressions of the Salton Sea Geothermal System (SSGS)
Ella Erskine, Tufts University
At the southeastern end of the Salton Sea, surface expressions of an active geothermal system are emitting an assemblage of potentially toxic and tropospheric ozone-forming gasses. Gas measurements were taken from ~1 to 8 ft tall mud cones, called gryphons, in the Davis-Schrimpf seep field (~50,000 ft2). The gaseous compounds emitted from the gryphons were collected using whole air sampling canisters. The canisters were then sent to the Rowland-Blake laboratory for analysis using gas chromatography techniques. Samples from June of 2022, 2023, and 2024 were utilized for a time-series analysis of VOC distribution. Originally, an emission makeup similar to petroleum was expected, as it has previously been found in some of the seeps. It is thought that hydrothermal fluid can rapidly mature organic matter into hydrothermal petroleum, so it is logical that the emission makeup could be similar. However, unexpectedly high levels of the VOC benzene were recorded, unlike concentrations generally observed in crude oil emissions. This may indicate a difference between the two sources in regard to their formation process or parent material composition. A possible cause of the elevated benzene could be its relatively high aqueous solubility compared to other hydrocarbons, which could allow it to be more readily incorporated into the hydrothermal fluid. Since the gryphons attract almost daily visitors, it is important to quantify their human health effects. Benzene harms the bone marrow, which can result in anemia. It is also a carcinogen. Additionally, benzene can react with the OH radical to form ozone, an additional health hazard. Future studies should revisit the Davis-Schrimpf field to continue the time series analysis and collect samples of the water seeps. Additionally, drone and ground studies should be conducted in the geothermal power plant adjacent to the gryphons to determine if benzene is being emitted from drilling activities.
Amelia Brown
Airborne and Ground-Based Analysis of Los Angeles County Landfill Gas Emissions
Amelia Brown, Hamilton College
California has the highest number of landfills of any individual US state. These landfills are concentrated in densely populated areas of California, especially within the Los Angeles metropolitan area. Landfills produce three main byproducts: heat, leachate, and landfill gas (LFG). LFG is primarily composed of methane (CH₄) and carbon dioxide (CO₂), with small concentrations of volatile organic compounds (VOCs) and other trace gases. The CH4 and CO2 components of LFG are well documented, but the VOCs and trace gases in LFG remain underexplored. This study investigates the emission of trace gases from four landfills in Los Angeles County, with a particular focus on substances known to have high Ozone Depletion Potentials (ODPs) and Global Warming Potentials (GWPs). The four landfills sampled were Chiquita Canyon Landfill, Lopez Canyon Landfill, Sunshine Canyon Landfill, and Toyon Canyon Landfill. Airborne samples were taken above the four landfills and ground samples were taken at Lopez Canyon as this was the only site accessible by our research team. The substances of interest were chlorofluorocarbons (CFCs), hydrochlorofluorocarbons (HCFCs), hydrofluorocarbons (HFCs), and halons. Airborne CH4 and CO2 measurements over the four landfills were obtained using the Picarro instrument onboard NASA’s B-200 aircraft. Ground samples were collected using whole air sampling canisters and were analyzed to determine the concentrations of these gases. The analytical approach for the ground samples combined Gas Chromatography-Mass Spectrometry (GCMS) with Flame Ionization Detection (FID) and Mass Selective Detection (MSD), providing a comprehensive profile of the emitted compounds. Findings reveal elevated levels of substances with high ODP and GWP, which were banned under the Montreal Protocol of 1987 and its subsequent amendments due to their contributions to stratospheric ozone depletion and climate change. These results underscore the importance of monitoring and mitigating landfill gas emissions, particularly for those containing potent greenhouse gases and ozone-depleting substances.
Click here watch the Atmospheric Aerosols Group presentations.
Click here watch the Terrestrial Ecology Group presentations.
Click here watch the Ocean Group presentations.
Return to 2024 SARP West Closeout Share
Details
Last Updated Sep 25, 2024 Related Terms
General 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.