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The world's most remote island, where moai stand and stare at the stars, will experience an annular solar eclipse on Oct. 2, 2024. For one eclipse-chaser, it's unmissable.

Why ordinary people will follow orders to the point of hurting others remains a critical question for scientists—though some answers have emerged

We have known that water ice exists on the Moon since 1998. These large deposits are found in the permanently shadowed craters around the polar region. The challenge is how to get it since shadowed craters are not the best place for solar powered vehicles to operate. A team of engineers have identified a design for an ice-mining vehicle powered by americium-241. With a half-life of 432 years, this element is an ideal power source for a vehicle to operate in the dark for several decades. 

Ice in the polar regions of the Moon is of vital importance for our future space explorations, not just lunar visits but as we stretch our legs in the Solar System. Its thought to be ancient material deposited by comets or formed by interactions with solar wind. It is expensive to take materials to the Moon so harvesting on site is far more efficient. Ice on the Moon can provide drinking water, oxygen for breaking and even hydrogen for rocket fuel. Surveys suggest something in the region of 600 billion kilograms of ice deposited at the lunar poles. 

Exposed water ice (green or blue dots) in lunar polar regions and temperature. Credit: Shuai Li

The challenge facing future lunar harvesting missions is that operations in the permanently  shadowed regions (or PSRs as they have been called) cannot be powered by solar panels as is often the case. The environment is cold too, in the region of 40K, that’s -233?C and at those temperatures special power considerations are required. 

A team of researchers have been exploring the use of Radioisotope Power Systems (RPS) to provide thermal and electrical power systems. These power systems have been used before during deep space missions for example Voyager and New Horizons. They work by generating electricity using the heat that is released from the natural decay of a radioactive isotope usually plutonium-238.

Artist rendition of Voyager 1 entering interstellar space. (Credit: NASA/JPL-Caltech)

The team led by Marzio Mazzotti from the University of Leicester have explored an ice-mining rover using power generated by the radio activate decay fo Americium-241. It has a half-life of 432 years which means it takes 432 years for half of a sample of Americium to decay. During this time, half of the atoms in the substance will transform into a different element. Using this power source will provide a stable power supply for an ice-mining rover in the darkness of the lunar polar craters for decades.

Apollo 17 commander Eugene Cernan with the lunar rover in December 1972, in the moon’s Taurus-Littrow valley. Credit: NASA

Using a radioisotope power system is not new however the team came upon the idea that the excess heat that is not used can be used to thermally mine ice from samples of lunar material. The rover would be fitted with a sublimation plate that would turn any ice deposits into a gas which would be collected in a cold trap.

The team developed a model of its Thermal Management System and tested it for icy regolith (the fine dusty lunar surface) material with a water ice content of 0-10 vol %. Their simulations showed that it is possible to mine ice using thermal techniques in the PSR of the Moon using an RPS (I had to really concentrate writing that sentence!) powered lunar rover. 

Source : Ice-Mining Lunar Rover using Americium-241 Radioisotope Power Systems

The post A New Rover Design Could Crawl Across the Moon for Decades Harvesting Water appeared first on Universe Today.

An office in the Pentagon investigated UFOs—and the paranormal—over a decade ago, segueing into a long saga leading to Congressional hearings and breathless news stories today. But the real story looks more like former defense officials pushing their personal mythology, rather than any cover-up of aliens

A distant planet should have been consumed when its star expanded to become a red giant, perhaps offering insights into planetary migration

A distant planet should have been consumed when its star expanded to become a red giant, perhaps offering insights into planetary migration

Only 2 astronauts will launch to the ISS Sept. 26 with SpaceX instead of the planned 4. We spoke with the crew before the big change was made.

Earth will get a "new moon" this weekend when, on Sunday (Sept. 29), it captures the asteroid 2024 PT5, claiming it as a very temporary "mini-moon."

For northern hemisphere dwellers, September's Full Moon was

Spanning light-years, this

Radar images have captured snowman-shaped 2024 ON asteroid tumbling through space.

A flurry of studies has found microplastics in nearly every organ in the human body, from the brain to the testicles. But very few have revealed whether these tiny bits of plastic impact our health

A flurry of studies has found microplastics in nearly every organ in the human body, from the brain to the testicles. But very few have revealed whether these tiny bits of plastic impact our health

Japan launched the IGS-Radar 8 spy satellite early Thursday morning (Sept. 26), on the second-to-last mission of the nation's venerable H-2A rocket.

DNA and genealogical evidence reveal, for the first time, the identity of cannibalised remains recovered from the Franklin expedition

DNA and genealogical evidence reveal, for the first time, the identity of cannibalised remains recovered from the Franklin expedition

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.

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Details Last Updated Sep 25, 2024 Related Terms

• General

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 (

10 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater) The Terrestrial Ecology 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 12, 2024. NASA Ames/Milan Loiacono

Faculty Advisor: Dr. Dan Sousa, San Diego State University

Graduate Mentor: Megan Ward-Baranyay, San Diego State University

Megan Ward-Baranyay, Graduate Mentor Megan Ward Baranyay, graduate student mentor for the 2024 SARP West Land group, provides an introduction for each of the group members and shares behind-the scenes moments from the internship.

Gerrit Hoving Predicting Ammonia Plume Presence at Feedlots in the San Joaquin Valley from VSWIR Spectroscopy of the Land Surface

Gerrit Hoving, Carleton College

Industrial-scale livestock farms, or Concentrated Animal Feeding Operations (CAFOs), are a major source of air pollutants including ammonia, methane, and hydrogen sulfide. Ammonia in particular is a major contributor to rural air pollution that is released from the breakdown of livestock effluent. Mitigating regional air pollution through improved waste management practices is only possible if emissions can be accurately monitored. However, ammonia is challenging to measure directly due to its short atmospheric lifetime and lack of VSWIR spectral signature. Here we investigate the potential for spectroscopic

imaging of the CAFO land surface to predict the presence of detectable ammonia emissions. Data from the Hyperspectral Thermal Emission Spectrometer (HyTES) instrument were found to clearly identify plumes of ammonia emitted by specific feedlots. Plume presence or absence was then tied to pixel-level reflectance spectra from the Earth Surface Mineral Dust Source (EMIT) instrument. Random forest classification models were found to predict ammonia plume presence/absence from VSWIR reflectance alone with an accuracy in the range of 70% to 80%. Our conclusions are limited by the limited number of

feedlots overflown by HyTES (n=96), the time gap between HyTES and EMIT data, and potential difficulty in comparing feedlots in different regions. While only tested over a modest area, our results suggest that ammonia plume presence/absence may be

predictable on the basis of surface features identifiable from VSWIR reflectance alone. Further investigation could focus on more comprehensive model validation, including characterization of the land surface processes and spectral signatures associated with feedlot surfaces with and without observable ammonia plumes. If generalizable, these results suggest that EMIT data may in some circumstances be used to predict the presence of ammonia emission plumes at feedlots in other areas, potentially enabling broader accounting of feedlot ammonia emissions.

Benjamin Marshburn Burn to Bloom: Assessing the Impact of Coastal Wildfires on Phytoplankton Dynamics in California

Benjamin Marshburn, California Polytechnic State University- San Luis Obispo

California is experiencing rising temperatures as well as increased frequency and length of drought conditions due to anthropogenic climate change. Wildfires are an intrinsic component of California and its Mediterranean ecosystems. However, this change in natural wildfire behavior increases the risk to ecosystems including soil erosion, poor plant regrowth, and ash/nutrient runoff that leads to the ocean. Previous work has attributed phytoplankton blooms in the coastal ocean to runoff from wildfires. This study aims to quantify the extent to which the concentration of chlorophyll-a, an indicator of phytoplankton abundance, can be predicted by wildfire parameters in coastal California and to evaluate which parameters are the most important predictors. Due to climatic variation in California we split the coast into three regions, northern, central and southern, and analyzed three fires from each area. For each fire, the stream length connecting the most severely burned area and the ocean was derived from analysis of a digital elevation model acquired by the Shuttle Radar Topography Mission. Additionally, differenced Normalized Burn Ratio (dNBR) was used to analyze burn severity for each fire. The change in chlorophyll-a levels before and after each fire from the impacted coastal area were evaluated using the Moderate Resolution Imaging Spectroradiometer (MODIS) on NASA’s Aqua satellite. The Random Forest Regression machine learning model did not strongly predict the difference in chlorophyll-a from the fire parameters. However, our moderate R2 value (0.36) shows promising avenues for future work, including investigating post-fire chlorophyll-a after the first significant rain event, as well as the impact of wind-blown ash on coastal chlorophyll-a concentrations.

Hannah Samuelson Species-specific Impact on Maximum Fire Temperature in Prescribed Burns at Sedgwick Reserve

Hannah Samuelson, University of St. Thomas

Fuel load plays a key role in determining severity (change in biomass), intensity (temperature), and frequency (length in time) of wildfires and prescribed fires. Fuel loads can vary in fuel conditions, like moisture content, amount, and flammability of the fuel, and are affected by species type and climatic conditions. Moreover, the difference in the chemical composition of plant species can affect its flammability. Anecdotal evidence from firefighters claim that Purple Sage burns hotter than other shrubs. Here we focus on two shrub species and two tree species that are broadly representative of California foothills; Blue Oak (Quercus douglasii), Coast Live Oak (Quercus agrifolia), Purple Sage (Salvia leucophylla), and California Sagebrush (Artemisia californica), and aim to understand species-specific proclivity to burn with higher or lower severity and intensity. In fall of 2023, a prescribed fire was conducted at Sedgwick Reserve in Santa Barbara County, CA. Field data collection included maximum temperature point measurements with metal pyrometers, the change in 3D vegetation structure using UAV LiDAR, and orthomosaic images for species identification. Radial buffers were created around the locations of the metal pyrometers and used to evaluate the spatial distribution of species, which were verified through field-observed species identification. The relationship between dominant overstory species, change in biomass, and maximum fire temperature was investigated. Preliminary results suggest that Purple Sage produced the highest maximum fire temperatures. Additionally, preliminary results showed both tree species, Blue Oak and Coast Live Oak, exhibit similar biomass change at low maximum fire temperatures. This investigation confirmed the firefighters’ anecdotal evidence on the relationship between species and their wildfire dynamics. The results have the potential to refine fire spread models and ultimately land management practices, improving the protection of humans and infrastructure while preventing habitat destruction from wildfires.

Angelina Harris Quantifying the Influence of Soil Type, Slope, and Aspect on Live Fuel Load in Sedgwick Reserve

Angelina Harris, William & Mary

The severity and increasing frequency of California wildfires requires investigation of factors that characterize pre-fire landscapes to improve approaches to wildland management and predict the spread of wildfire. Quantifying the relationship between soil type and fuel load could improve existing efforts to map both overall quantity and composition of live fuel for fire spread models which may assist in preventative wildfire measures and potentially active firefighting work. The southwest corner of Sedgwick Reserve, Santa Barbara County, CA hosts two dominant soil types that broadly represent soil variability in the area. The more northerly soil unit is a Chamise shaly loam, and the more southerly soil unit is a Shedd silty clay loam. The Chamise series has a mixed texture, abundant in clay with a significant amount of rock fragments (> 35%) composing its texture while the Shedd series has a fine texture dominated by silt-sized particles. Topography, specifically slope and aspect, plays a significant role in formation and characteristics of soil due to influence on erosion and deposition and sun exposure, respectively. This research aims to explore the relationship between soil type and topography and quantify their influence on live fuel using a Canopy Height Model (CHM) derived from airborne LiDAR collected on 11/04/2020 with a point density of 10.19 pts/m2. The LiDAR-based CHM was filtered to separate trees (> 2 m) and shrubs (.07 – 2 m). A Random Forest Regressor was used to investigate the relationship between soil type, slope, and aspect to identify which variable is the best predictor of canopy height. Preliminary results suggested that soil type and aspect were the most important variables to determine canopy height (variable importance of .50 and .41, respectively). Further studies investigating quantity and composition of live fuel load focusing on additional soil units within Sedgwick Reserve are encouraged.

Emily Rogers From Canopy to Chemistry: Exploring the Relationship Between Vegetation Phenology and Isoprene Emission

Emily Rogers, Bellarmine University

Isoprene (2-methyl-1,3-butadiene) represents the most abundant non-methane biogenic volatile organic compound in the troposphere, with annual emissions almost equal to those of methane. Depending on the chemical environment, this effective thermoregulator and reactive oxygen species scavenger participates in photochemical reactions to produce climate pollutants and toxins such as ozone and secondary organic aerosols. Previous studies have revealed strong connections between isoprene emission and photosynthesis as its precursors are formed during the Calvin Cycle. This raises questions as to whether the periodic biological events of plants, collectively known as vegetation phenology, influences tropospheric isoprene quantities. In this study, we investigate the influence of vegetation phenology on isoprene emission in Southern California by comparing photosynthetic activity and the spatial distribution of the isoprene oxidation product, formaldehyde, for regions dominated by plants of two different physiologies: high altitude woodlands and coastal shrublands. We interrogate the annual phenology of these regions using high resolution solar-induced chlorophyll fluorescence (SIF) estimates from the Orbiting Carbon Observatory-2 (OCO-2) satellite, and formaldehyde vertical column measurements from the recently activated Tropospheric Emissions: Monitoring of Pollution (TEMPO) geostationary satellite. We explore the seasonal trends in both formaldehyde formation and SIF as well as their bivariate relationship. Preliminary results indicate both heightened formaldehyde emission and heightened SIF during summer months relative to winter months, with a comparatively stronger correlation between the two metrics during the fall. Our findings will provide insight toward the response of plants to variations in their environment which directly influence chemical systems in the air. Whereas VOCs hold a great potential for environmental and anthropological harm if emitted in excess, it is crucial to understand the factors involved in their formation. As such, we hope that our findings provide information relevant to the development of air pollution mitigation strategies.

Sydney Kent Keeping it Fresh(water): Understanding the Influence of Surface Mineralogy on Groundwater Quality within Volcanic Aquifer Systems

Sydney Kent, Miami University

Geology plays a key role in determining the chemical profile of groundwater through weathering and erosion, leading to minerals entering the groundwater. The Columbia Plateau, a geologic region that resides within the Pacific Northwest volcanic aquifer system, is known to have water management issues due to groundwater extraction for agriculture. Decreases in groundwater levels can lead to higher concentrations of rock-originated minerals, so the relationship between basaltic geology and well water quality is particularly important in these systems. This research aims to assess the extent in which the basaltic surface mineralogy of the Columbia Plateau impacts predetermined health benchmarks pertaining to trace elements, radionuclides, and nutrients. NASA’s Earth Surface Mineral Dust Source Investigation (EMIT) instrument, a spaceborne imaging spectrometer on the International Space Station, was used to map surface minerals within and among distinct regions of the Columbia Plateau. Some basalt aquifers have uranium that decays to radon-222, a mineral that can be toxic when consumed, as well as lithium, which is commonly found during volcanic eruptions. Preliminary findings showed that where basalt and its secondary minerals were identified with EMIT, chlorite and calcite, well data also indicated raised levels of lithium and radon-222. The relationship between EMIT mineral maps and water quality data indicated that EMIT can potentially be used to identify basalt aquifer systems that may be at risk of poor water quality. Results from this study can be used to enact more personalized water purification methods in areas with water quality issues and individuals with private wells can be more informed about the hazards present in their water.

Click here watch the Atmospheric Aerosols Group presentations.

Click here watch the Ocean Group presentations.

Click here watch the Whole Air Sampling (WAS) Group presentations.

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Details Last Updated Sep 25, 2024 Related Terms

• General

9 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater) The Atmospheric Aerosols 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 12, 2024. NASA Ames/Milan Loiacono

Faculty Advisors: Dr. Andreas Beyersdorf, California State University, San Bernardino & Dr. Ann Marie Carlton, University of California

Graduate Mentor: Madison Landi, University of California, Irvine

Madison Landi, Graduate Mentor Madison Landi, graduate student mentor for the 2024 SARP Aerosols group, provides an introduction for each of the group members and shares behind-the scenes moments from the internship.

Maya Niyogi A Comparative Analysis of Tropospheric NO2: Evaluating TEMPO Satellite Data Against Airborne Measurements

Maya Niyogi, Johns Hopkins University

Nitrogen dioxide (NO2) plays a major role in atmospheric chemical reactions; the inorganic compound both contributes to tropospheric ozone production and reacts with volatile organic compounds to create health-hazardous particulate matter. The presence of NO2 in the atmosphere is largely due to anthropogenic activity, making NO2 at the forefront of policy decisions and scientific monitoring. The Tropospheric Emissions: Monitoring of Pollution (TEMPO) satellite launched in 2023 with the goal of monitoring pollution across North America. The publicly-accessible data became available for use in May 2024, however parts of the data remain unvalidated and in beta, creating a need for an in situ validation of its data products. Here we analyze TEMPO’s tropospheric NO2 measurements and compare them to aloft NO2 measurements collected during the NASA Student Airborne Research Project (SARP) 2024 airborne campaign. Six of the campaign flights recording NO2 performed a vertical spiral, providing vertical column data that was adjusted to ambient conditions for comparison against the corresponding TEMPO values. Statistical analyses indicate we have reasonable evidence to conclude that TEMPO satellite data and the flight-collected data record similar values. This research fills a critical knowledge gap through the utilization of aloft NO2 measurements to validate NASA’s newly-launched TEMPO satellite. It is expected that future users of TEMPO data can apply these results to better inform project creation and research.

Benjamin Wells Investigating the Atmospheric Burden of Black Carbon Over the Past Decade in the Los Angeles Basin

Benjamin Wells, San Diego State University

Black Carbon is a primary aerosol emitted directly into the atmosphere as a result of biomass burning and incomplete combustion of fossil fuels. During the pre-industrial revolution, the main source of black carbon was natural sources whereas currently, the main source is anthropogenic activities. When black carbon is released into the atmosphere, it is a dominant absorber of solar radiation and leads to a significant warming effect on Earth’s climate. In addition to its harmful effects associated with climate change, ambient black carbon inhalation is correlated with adverse health effects such as respiratory and cardiovascular disease, cancer, and premature mortality. In this study, we analyze aloft black carbon measurements in 2016 and 2024 acquired on NASA SARP research flights and compare these concentrations to black carbon measurements taken during the 2010 CalNex field campaign. Both field campaigns flew similar flight paths over the Los Angeles basin allowing us to conduct a critical comparative analysis on vertical and spatial profiles of the atmospheric burden of black carbon over the past 14 years. During the CalNEX study, mass concentrations of black carbon ranged from 0.02 μg/m3 to 0.531 μg/m3, meanwhile 2024 SARP measurements demonstrate concentrations as elevated as 7.83 μg/m3 within the same region. Moreover, similar flight paths conducted during SARP 2024 and 2016 allow for further analysis of aloft black carbon concentrations over a period of time. The results of this study examines and analyzes the changing spatial and temporal characteristics of black carbon throughout the years, leading to an increase of adverse effects on both the climate and public health.

Devin Keith Tracking Methane and Aerosols in relation to Health Effects in the San Joaquin Valley

Devin Keith, Mount Holyoke College

The San Joaquin Valley (SJV) is located in central California and is one of the most productive agricultural regions in the country for dairy, nuts, and berries, producing more than half of California’s $42 billion output. Due to the SJV’s close proximity to the Sierra Nevada Mountain Range to the East and predominantly Easterly winds, air pollution often accumulates because it is trapped by the geography. Significant chemical constituents of trapped particulate matter are ammonium (NH4), chloride (Cl), sulfate (SO4), nitrate (NO3), black carbon, and organic carbon. The particle size measured in this study is less than 1 micron in diameter, and due to their size, can easily penetrate the respiratory tract leading to adverse health effects such as: asthma, chronic obstructive pulmonary disease, and cardiovascular disease. We employ airborne data collected during the SARP 2024 mission onboard NASA’s P-3 research plane to observe spatial and temporal trends of NH4, Cl, SO4, NO3, and black carbon. Further, we analyze measurements from SARP 2016 flights and compare the atmospheric burden of pollution in the SJV across time. To investigate observations in the context of the public health impacts, we utilize data collected by the California Office of Environmental Health Hazards Assessment and find asthma and cardiovascular disease rates are higher in the SJV hotspots identified here. Per capita health impacts are greater than other California regions such as Los Angeles and San Francisco. The SJV exhibits higher rates of poverty than other communities, which may reveal an environmental justice issue that is difficult to explicitly quantify especially where measurements are sparse.

Lily Lyons Investigating the Effects of Aerosols on Photosynthesis Using Satellite Imaging

Lily Lyons, Brandeis University

Aerosols in the atmosphere can affect the way sunlight travels to the ground by absorbing or scattering light. Sunlight is a critical component in plant photosynthesis, and the way light scatters affects productivity for vegetation and plant growth. When plants absorb sunlight, the chlorophyll in their leaves releases the excess energy as infrared light, which can be measured from space via satellite. To better understand how aerosol loading in the atmosphere affects plant photosynthesis, this study examines locations in Yosemite, Sequoia, Garrett, and Talladega national forests, and compares aerosol optical depth (AOD), normalized difference vegetation index (NDVI), and solar induced fluorescence (SIF) in these areas. Yosemite and Sequoia act as proxies for the old growth sequoia grove ecosystems, and Talladega and Garrett act as proxies for the Appalachian mixed mesophytic forest ecosystem. Our results show that within 2015-2020 during July, SIF and NDVI levels are significantly greater in mixed mesophytic forests than in sequoia groves. Using linear regression plots, we determined the correlation between SIF, NDVI and AOD to be weak in the given locations. Greater SIF in mixed mesophytic forests could suggest that the presence of a prominent and biodiverse understory is positive for the overall primary productivity of an ecosystem. This study is a good starting point for analyzing diverse ecosystems using SIF, NDVI and satellite data as proxies for photosynthesis, and broadening the scope of biomes examined for their SIF. Furthermore, it highlights the need for further investigation of aerosol impact on the trajectory and amount of sunlight that reaches certain plants.

Ryleigh Czajkowski Validating the Performance of CMAQ in Simulating the Vertical Distribution of Trace Gases

Ryleigh Czajkowski, South Dakota School of Mines and Technology

Air quality modeling simulates atmospheric processes and air pollutant transport to better understand gas-and particle-phase interactions in the atmosphere. The Environmental Protection Agency’s (EPA) Community Multiscale Air Quality (CMAQ) model couples meteorological, emission, and chemical transport predictions to simulate air pollution from local to hemispheric scales. CMAQ provides scientists and regulatory agencies with important assistance in air quality management, policy enactment, atmospheric research, and creating public health advisories. Recently, a new update to CMAQ (v5.4) was released, utilizing new chemistry mechanisms and incorporating a new atmospheric chemistry model. This study evaluates the performance of the latest model update by analyzing multiple time series of vertical distributions of formaldehyde (CH2O) and methane (CH4) in the Los Angeles Basin and Central Valley regions of California. It compares data from aloft measurements taken during NASA SARP 2017 flights with model predictions to evaluate accuracy. Our study analyzes CMAQ’s capabilities in capturing the vertical dispersion of CH2O and CH4 in different regions, offering insights into the effectiveness of CMAQ for air quality management and the analysis of trace and greenhouse gas dynamics. Using NASA airborne data, this research utilizes a diversified data set to validate the model, providing a more comprehensive evaluation of its capabilities, and thus providing valuable insight into future developments of CMAQ.

Alison Thieberg Estimating Aerosol Optical Properties Using Mie Theory and Analyzing Their Impact on Radiative Forcing in California

Alison Thieberg, Emory University

Anthropogenic aerosols, unlike greenhouse gasses, provide a net cooling effect to the Earth’s surface. Particles suspended in the atmosphere have the ability to scatter incoming solar radiation, preventing that radiation from heating up the surface. These aerosols like black carbon, ammonium nitrate, ammonium sulfate, and organics are byproducts of both natural and anthropogenic activities. Measuring radiative forcing as a result of these aerosols over time can provide insight on how anthropogenic industries are altering our Earth’s temperature. This study analyzes the changes in radiative forcing from aerosols in central and southern California using data collected from NASA SARP flights from 2016-2024. Aerosol size, composition, and single scattering albedo were used to estimate the aerosol characteristics and to calculate the aerosols’ radiative forcing efficiency. Our results show that aerosols are found to have less of a cooling effect over time when looking at the change in radiative forcing in California from 2016 to 2024. When narrowing in on specific geographic regions, we observe the same trends in the Central Valley with the area becoming warmer as a result of aerosols. However, more southern regions like Los Angeles and the Inland Empire have become cooler from aerosols during this time period. The overall decrease in the cooling effect of California’s aerosols could indicate that the average size of particulates is changing or that the aerosol composition could be shifting to a greater concentration of absorbing aerosols rather than scattering aerosols. This study shows how aerosols influence radiative forcing and their subsequent impacts across regions in California from multiple years.

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