Notes from the Field

The Village

July 14th, 2022 by Alex Haughton

Alex Haughton is a graduate student in the Astrophysical and Planetary Sciences department at University of Colorado Boulder studying ultraviolet instrumentation with sounding rockets. His team has traveled to Equatorial Launch Australia’s Arnhem Space Center near Nhulunbuy, Australia to launch the Dual-channel Extreme Ultraviolet Continuum Experiment (DEUCE) Sounding Rocket and observe the stars Alpha Centauri A & B in extreme ultraviolet wavelengths.

It takes a village to send something to space.

Currently, the Suborbital Imaging Spectrograph for Transition region Irradiance from Nearby Exoplanet host stars (SISTINE) rocket payload is sitting on the launch pad ready to go.  As we wait for high winds to die down, I am reflecting on how many people it takes to get here.

SISTINE has a science team of four people in East Arnhem Land, but many others were left back at the lab in Colorado – mechanical and electrical engineers, technicians, graduate and undergraduate students. The payload itself consists of a telescope made by Nu-Tek in Maryland, special ultraviolet reflective coatings applied by NASA Goddard, a diffraction grating made by Horiba JY in France, and a microchannel plate detector made by Sensor Sciences in Berkely. If all those things sound like advanced technology that take a lot of people, work, and know how to make, it’s because they are.

And that’s just the science payload. There’s the minor matter of launching it into outer space. There are over 70 people here from NASROC (NASA Rockets), White Sands Missile Range, and NASA. These are people who can set up and operate the motors of a sounding rocket (the part that goes boom), people who can set up antennas to communicate with the rocket as it flies to and from space and monitor where it is, people who can point the rocket in the right direction when it gets there, people to pick up the rocket and bring it back when it comes back down, and people to manage all these other people. This blog post is facilitated by a NASA communications team sent to cover the launch (you can find some of their excellent work here).

Then there’s the local infrastructure. The launch site itself was built with a partnership between Equatorial Launch Australia and the Gumatj Corporation, the Indigenous owned and run corporation that manages the land on which the launch site was built. East Arnhem Land is beautiful, but densely populated it is not, and the influx of people requires places to stay, food to eat, vehicles to drive, and other resources that stretch the capabilities of the nearby town of Nhulunbuy (the area has responded admirably).

I feel like there’s a tendency to put a single face on scientific discovery or technical achievement. The Nobel Prizes certainly tend in this direction. Theoreticians of the past may have had fewer people supporting them, but modern scientific discoveries are built on the culmination of years, if not decades, of hard work by large teams of people, all of whom are critical to success.

Sometime in next few decades the astronomy community will begin detecting and analyzing atmospheric data from potentially habitable exoplanets. There’s a chance life signatures could be discovered. When this happens, the next two launches, along with a multitude of other projects, will have helped paved the way for that discovery. And these two launches, small potatoes compared to what it takes for even moderately sized space telescopes, take a village to succeed.


July 13th, 2022 by Alex Haughton

Alex Haughton is a graduate student in the Astrophysical and Planetary Sciences department at University of Colorado Boulder studying ultraviolet instrumentation with sounding rockets. His team has traveled to Equatorial Launch Australia’s Arnhem Space Center near Nhulunbuy, Australia to launch the Dual-channel Extreme Ultraviolet Continuum Experiment (DEUCE) Sounding Rocket and observe the stars Alpha Centauri A & B in extreme ultraviolet wavelengths.

This is a story about the color red. Oh sure, there are sounding rockets; there are telescopes with new technology for ultraviolet astronomy; there is cool science on stellar atmospheres; there is a new spaceport built in collaboration with the Indigenous community; there is the cast of colorful characters that it takes to get space science done. First and foremost, however, is the prevalent red that claims everything in East Arnhem Land, the area we have come to for our rocket launch.

Some say red is simply the color of the dirt here, but they underestimate what they are dealing with. This is so much more than any dirt could be. This is red. Since our arrival a week ago, we are slowly turning into red. When I walk outside, whether I crunch on gravel or plunk through a puddle, my feet turn into red. I walk inside, bringing the red with me, and the floor is now red. We drive to and from Nhulunbuy, the town about 30 minutes from our camp at the Gulkula Cultural Center, and the beat-up 2WD Toyota Hilux we have fondly named “Twobacca” is red. I open and shut Twobacca’s doors and my hand is red, and whatever I touch next will turn into red.

When things are dry, red takes the form of a dust that fills the air. We breathe red. Lately, as East Arnhem does its best impression of Ray Bradybury’s “The Long Rain,” the dust is replaced by something best described as paint. The surface of the Earth is a completely sticky red that seeps under doorjams, coats your trousers, and even climbs the walls.

East Arnhem Land has many inhabitants – Yolngu people, miners, scientists come to launch rockets, crocodiles, spiders, snakes, wallabies, and other beasties. But here red rules over all.

Interning at 40,000 Feet: The NASA Student Airborne Research Program Experience

January 20th, 2022 by McKenna Price-Patak, Jacob Schenthal, and Jacob Ramthun

Participants from NASA’s 2020-2021 Student Airborne Research Program pose in the hangar at Armstrong Flight Research Center in southern California. Photo by McKenna Price-Patak.

For students who want to take atmospheric science as literally as possible, it doesn’t get much better than flying in a NASA aircraft.

Each year, the Student Airborne Research Program (SARP) invites a team of rising college seniors to Armstrong Flight Research Center in Southern California to conduct research aboard NASA’s airborne science fleet. Each aircraft is equipped with instruments for land, ocean, and atmospheric research–enabling sample collection and imaging over the Earth’s surface. After operating the instruments in-flight, participants are then able to use the resulting data for their own individual research projects.

…as soon as they recover from the air sickness, of course.

Jacob Schenthal, who graduated from Vanderbilt University in 2021, was drawn to the NASA SARP program for its emphasis on independent, field-based research and multidisciplinary scientific teams. McKenna Price-Patak, a 2021 Tulane University grad, felt it was a rare opportunity for an undergraduate student to be responsible for an entire research project: from data collection to analysis and project development.

“I’ve always had interests in a variety of fields within Earth science, which is why I was excited about the multidisciplinary aspect of SARP,” Price-Patak said.

Both Schenthal and Price-Patak were placed with Dr. Donald Blake, conducting air sampling aboard the aircraft to study atmospheric pollution.

L-R: Jacob Schenthal, Donald Blake, and McKenna Price-Patak. Photo by McKenna Price-Patak.

Dr. Blake is kind of a big deal in the atmospheric science community. An atmospheric chemist at UC Irvine, Blake is half of the eponymous Rowland-Blake Group: the research lab whose other namesake, the late Dr. F. Sherwood Rowland, won a Nobel Prize in chemistry for identifying compounds responsible for Earth’s ozone hole. Today, Blake continues the lab’s work as a leading expert on the impacts of atmospheric chemistry and air pollution on human health, and has conducted NASA-sponsored airborne research for over 30 years.

“Dr. Blake is a phenomenal mentor and really helped me find a newfound interest in air quality research–which intersects directly with climate change and environmental justice: two of my other passions,” Schenthal said. As Price-Patak put it, “Don takes a genuine interest in each member of his group and their success. When my project took a last minute detour and had to be redone days before final presentations, Don sat with me on Zoom for hours a day helping me recover and create a project I was proud of.”

Air pollution visible in the skies above southern California. Photo by Jacob Schenthal.

Both Schenthal and Price-Patak were accepted into the SARP program in 2020. Unable to make the flights that year due to the COVID-19 pandemic, the program had to take a different approach. For the first time in SARP’s history, participants received air quality testing canisters in the mail to remotely collect initial data points.

“Although the program during summer 2020 was remote, it was exciting to take air samples to help measure emission impacts of the COVID-19 lockdowns,” Schenthal said.

“The way the program pivoted to a virtual environment was incredible,” Price-Patak said. “While we would’ve loved to be in person, we still had so much support from our research groups and mentors so we could successfully complete our projects in the short time frame.”

Schenthal’s project, titled Investigating Xylene and Toluene in Disadvantaged Communities Downwind of LAX, blended NASA’s airborne science data within an environmental justice framework. He examined how xylene and toluene–two airborne compounds that damage the nervous system with chronic exposure–are more common in disadvantaged communities near and around Los Angeles International Airport (LAX). Schenthal found that Inglewood, a predominantly Black and low-income community, experienced exposure levels for both compounds at 50 times the background level. Additionally, his project results indicated the compounds acted as tracers, meaning hundreds of other pollutants are also potentially travelling from LAX throughout these communities.

Price-Patak’s project, Dimethyl Sulfide (DMS) in the Imperial Valley and its impact on Sulfate Aerosol Loading, used data collected on SARP flights from 2014 to 2019 to locate sources of inland DMS. DMS is typically released from plankton in the ocean, and can turn into sulfate aerosols which can cause respiratory illness. Her research indicated there may be inland sources of DMS producing up to 10% of the sulfate aerosols in the Imperial Valley, an important agricultural region east of Los Angeles.

Jacob and McKenna collecting air samples aboard Armstrong Flight Research Center’s DC-8 aircraft. Photo by McKenna Price-Patak.

More than a year later, they got their chance to make the flight. In December 2021, fully-vaccinated participants from the 2020 and 2021 teams were finally able to take their projects airborne. Over the course of a week, the team participated in multiple flights over southern California aboard a DC-8 aircraft, taking samples adding to the program’s extensive record of air quality data.

By the end of the program, Price-Patak and Schenthal were able to rack up a combined 27 hours of flight time–and even experienced sitting in the cockpit for low approaches around Long Beach harbor!

According to Price-Patak, the value of the program comes not only from the work itself, but from the opportunity to connect with other early career scientists.

“Through SARP, I developed a new interest in atmospheric chemistry and connected with other students who have gone on to work as consultants with business firms, pursue PhDs, and everything else in between. Not only is the opportunity to conduct research through the program incredible, but the flights are truly a once in a lifetime experience. I would recommend any undergrad student with a STEM background to apply!”

“SARP has been an incredible experience, both personally and professionally. For me, it allowed me to explore my interest in air quality and environmental justice–all while engaging in field research and my independent research project,” Schenthal added.

Now, Schenthal and Price-Patak credit SARP in helping their careers take off–with both program alumni now working with NASA SERVIR at the University of Alabama in Huntsville (UAH).

A collaboration between NASA and USAID, SERVIR works with organizations around the world to design and implement satellite-based services supporting climate adaptation and natural resource management. Schenthal is the Regional Science Associate for SERVIR’s Mekong hub, while Price-Patak is a graduate research assistant for SERVIR-Hindu Kush-Himalaya while enrolled in UAH’s Master’s program in Earth science. And yes–both are still involved in air quality research. The application for SARP 2022 closes January 26th, and can be found here. Don’t hesitate to apply–and be prepared to pack your dramamine!

A NASA DC-8 aircraft sits on the tarmac at Edwards Air Force Base in Edwards, California. Photo by McKenna Price-Patak.

The CYGNSS constellation of 8 SmallSats was launched into low Earth orbit five years ago, on December 15, 2016. It began as a two year mission to study how well GPS signals reflected from the ocean surface can help us measure the winds in hurricanes and improve our ability to forecast them. Well, we’ve done that, but it turns out those reflected signals can tell us a lot more. One of the key reasons we’ve been able to learn about all the other applications is the extra time we’ve had on orbit, to make more measurements, study their sensitivity to other environmental parameters, construct new data products, and develop scientific uses for them. For that, I am sincerely grateful to the team of technicians, engineers and managers at the Southwest Research Institute and the Space Physics Research Lab who designed, built, tested and now operate the spacecraft, and to our partners at Surrey Satellite Technology Ltd. who designed and built the GPS receivers that take our science measurements. They were given a schedule, a budget and a two-year requirement for on-orbit operations. We got to orbit on time and under budget and here we are, five years later, still making high quality observations with each GPS receiver on every spacecraft at 100% duty cycle.  I am also very grateful to NASA for the support they have provided and for their willingness to expand the scope of CYGNSS science as we discover new, exciting and impactful things we can do with our mission.

One of the great things about operating 8 spacecraft with a 100% duty cycle is the frequency with which you can sample tropical cyclones throughout their entire life cycle. This is illustrated in the following figure, which shows when and how well CYGNSS sampled every major storm (Cat 3 or greater) from 2018 to 2020.

In the figure, the red lines are the track of each storm throughout its life cycle, the dots are when there was a CYGNSS overpass, and the color of the dot indicates how well we sampled the inner core of the storm. Every storm is sampled between one and three times a day, which helps monitor its development and capture sudden changes like rapid intensification. The impact our observations have on hurricane forecast skill is an active area of research by the CYGNSS science team. One recent example is work by researchers at the NOAA Hurricane Research Division that is highlighted in this figure.

Observing System Experiment results illustrate the reduction in Vmax error when CYGNSS obs are included as inputs to the HWRF forecast model, Source:

The figure shows the error in the operational forecast of maximum wind speed during Hurricane Michael’s rapid intensification, which occurred between 36 and 72 hours into the forecast (black line), and the reduced error that would have been present had CYGNSS observations been included (green line). The peak error is reduced from about 45 to 25 knots, or cut almost in half.

CYGNSS spends much less than 0.1% of its time over hurricanes but its radar receivers operate continuously. This enables many other uses of the data. Data products over ocean include near-surface wind speed and, from it, sea-to-air fluxes of latent and sensible heat. One new data product released in 2021 is the concentration of ocean microplastics, derived from the suppression of ocean surface roughness by surfactants acting as tracers of the microplastics. Time lapse microplastic concentration maps of Yangtze River outflow are shown in the following figure.

Microplastic concentration in the East China Sea averaged over different time intervals. (A) Annual average. One week averages over (B) 22–28 Jun 2017, (C) 27 Oct – 2 Nov 2017, (D) 2–8 Dec 2017. Short lived bursts of high microplastic concentration indicate river outflow. Source:

The upper left panel (A) in the figure shows the annual average microplastic concentration in the East China Sea near the mouth of the Yangtze. There is no obvious outflow signal. Panels (B)-(D) show the concentration averaged over individual weeks of the year in which there is a prominent outflow plume.

CYGNSS operates over both ocean and land, and the land reflections contain two important pieces of information. When standing water is not present in the measurement footprint to any significant degree, it is possible to retrieve near-surface soil moisture content. We can measure the global distribution of soil moisture several time per day and those data have been shown to significantly improve global land surface hydrology models <>.  When inland water bodies are present in the footprint, reflections from them tend to dominate the measurements. CYGNSS is then able to effectively map the extent of the water. One application of this capability is shown in the following figure of flood inundation across the island of Hispaniola as imaged by CYGNSS after Hurricane Isaias landfall.

Flood inundation in Santo Domingo due to Hurricane Isaias landfall is imaged by the change in GPS reflections observed by CYGNSS. Image credit: C. Chew, UCAR.

The “Delta” map shows the change in surface reflectivity from before to after landfall. The extensive flooding that occurred in the capital city of Santo Domingo is highlighted by bright yellow (high delta) areas.

Inland water body maps produced by CYGNSS have two distinct properties. One, which derives from the large number of satellites in the constellation, is their ability to be updated often. This allows them to capture sudden changes like flood events.  The other, which derives from the use of GPS signals that can penetrate through clouds, rain and vegetation canopies, is their ability to map wetland extent in heavily vegetated regions. One exciting new application of this capability is improved prediction of methane emission from wetlands. The accuracy of a global wetland methane emission model was evaluated when initialized by three different water masks. The results are shown in the following figure.

Wetland methane emission model comparison with three different water mask initializations. Source:

If a static water mask derived from Vis/IR imagers is used (SWAMPS blue curve in figure), seasonal variations in water extent are not represented and anomalous conditions associated with clouds and vegetation are misrepresented. If the model uses a dynamic rainfall map to better account for seasonal effects (ERA5 black curve), complications in the relationship between rainfall and wetland inundation are neglected. The best results are had using dynamic maps of wetland extent derived from CYGNSS observations (CYGNSS red curve) because they are based on direct, time varying measurements of the inundation that are insensitive to clouds and vegetation.

The first five years of on-orbit operation have produced valuable ocean wind observations for improved hurricane forecasting and have uncovered many new applications of the data away from hurricanes. We will continue to refine our measurements of winds, soil moisture and inland water bodies. And who knows what other new sensitivities we will uncover in the next five years?

Unraveling the Mysteries of Arctic Greening and Browning

October 5th, 2021 by Logan Berner and Patrick Burns (Northern Arizona University), and Roman Dial (Alaska Pacific University)

To better understand impacts of climate change on vegetation in the Alaskan Arctic, researchers will link long-term NASA satellite observations with ecological field data collected while trekking through the Brooks Range in northern Alaska. Photo by Roman Dial.

Following caribou and brown bear trails when possible, a small NASA-supported research team trekked 800 miles across Alaska’s Brooks Range last summer. With additional support from NSF, the Alaska Space Grant Program, and the Explorers Club/Discover, the research team is collecting extensive ecological field data that will be linked with satellite observations to better understand long-term changes in vegetation, including impacts of climate warming. The Arctic is warming nearly twice as rapidly as the rest of the planet and the impacts are becoming increasingly evident as glaciers melt, permafrost thaws, and tundra greens.

Arctic greening and browning

Earth-observing satellites have detected widespread increases in tundra greenness in the Arctic over the last four decades. The phenomena is caused, in part, by increases in vegetation growth as summers have become warmer and longer, and has been termed “Arctic greening.” On the other hand, satellite observations have also detected localized declines in tundra greenness attributed to surface flooding, extreme weather, and other disturbances. This has been termed “Arctic browning.” Satellite observations of greening and browning show that extensive changes are occurring in the Arctic, but much remains unclear about why specific regions have greened or browned in recent decades.

Earth-observing satellites have detected Arctic tundra becoming greener in recent decades as the growing seasons became warmer and longer. Landsat satellite observations indicate that about 22% of the Arctic became greener from 2000 to 2016, while 5% became browner. Adapted from Berner et al. (2020).
The team

To better understand recent greening and browning in northern Alaska, Professor Roman Dial’s team from Alaska Pacific University (APU) has been collecting extensive ecological observations while trekking throughout Alaska’s Brooks Range. For nearly forty years, Dial has studied and traversed the Alaskan wilderness, including nearly 2,000 miles by foot and packraft throughout the Brooks Range during the last three field seasons. For 11 days last summer, Dial’s team was joined by Dr. Logan Berner and Patrick Burns who are research ecologists from Northern Arizona University (NAU) and members of NASA’s Arctic-Boreal Vulnerability Experiment (ABoVE). While Dial is an expert in field ecology and wilderness travel, Berner and Burns are experts in satellite remote sensing and ecological informatics. By combining their expertise, these researchers hope to shed light on the extent, nature, and causes of vegetation changes during recent decades in the Brooks Range.

Pixel walking team (left to right) Logan Berner, Patrick Burns, Ben Weissenbach, Julia Ditto, Madeline Zietlow, Russell Wong. Photo by Roman Dial.
Trekking through the Brooks Range

The Brooks Range forms a natural barrier that separates the boreal forest of Alaska’s interior from the arctic tundra of Alaska’s North Slope. This mountain range includes the largest complex of protected wilderness in the United States, including 21,000,000 acres among the Arctic National Wildlife Refuge, Noatak National Preserve, and Gates of the Arctic National Park. Berner and Burns joined Dial’s research team as they trekked from the northern edge of boreal forest into the Noatak Wilderness where trees give way to thickets of shrubs, wetlands, and barren rocky ridges. During the course of 11 rain-soaked days, the team followed caribou and brown bear trails through verdant valley bottoms and over cloud-choked mountain passes as they traversed about 80 miles from the Ambler River to the Cutler River. While trekking, the researchers collected ecological field data to be linked with measurements of vegetation greenness from NASA Earth-observing satellites.

Route traveled by researchers during an 11-day segment of a summer-long trek through the western Brooks Range in northern Alaska. The orange route corresponds to off-trail foot travel, while the blue route corresponds to a combination of foot and raft travel. Image by Patrick Burns.

Roman, Logan, and Pat. Photo by Ben Weissenbach.

Photo by Roman Dial.

Ecological research often involves establishing field plots and then meticulously characterizing the composition and other attributes of the plant community in each field plot. Plot sampling provides valuable information, but the time consuming nature of the approach limits the spatial extent over which measurements can be made. Dial recognized that to better understand recent greening and browning, there is a need for more spatially extensive information on plant community composition than can be provided by field plots alone. He thus has pioneered an alternative approach that involves continuously documenting plant community composition and other attributes while trekking across the landscape. Termed “pixel-walking”, this approach harnesses the multifunctionality of smartphones to record and geolocate visual observations of vegetation composition and density for the overstory, midstory, and understory. While pixel-walking, researchers record a new observation every time they visually detect a change in vegetation composition or density at about a 30 meter spatial scale, corresponding to one pixel from the Landsat satellites. These spatially extensive field observations are thus collected with the explicit goal of being linked to decades of Landsat satellite observations.

Photo by Roman Dial.

Photo by Roman Dial.

Researchers record visual observations of plant community composition and density while “pixel-walking” through the Brooks Range in northern Alaska. Photo by Roman Dial.

During summer 2021, Dial’s research team pixel-walked over 800 miles from east to west through the Brooks Range, collecting data on vegetation composition for about 100,000 Landsat pixels. Over the coming year, Dial’s team will work with Berner, Burns, and Professor Scott Goetz (ABoVE Science Team Lead) at NAU to link these extensive field data with several decades of Landsat satellite observations provided by NASA. This collaboration will help unravel the mysteries of Arctic greening and browning by shedding light on where, how, and why plant communities changed in recent decades. NASA’s Earth-observing satellites provide long-term observations that are crucial for monitoring and understanding ongoing environmental changes in the rapidly-warming Arctic, especially when complemented by field data collected across large regions.

Boreal forest gives way to sparse tundra while heading north into the Brooks Range. Photo by Logan Berner.