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SAGE III/ISS Team Announces the Second Official Release of V5.2 Science Data Products

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The SAGE III/ISS Team is proud to announce the second official release of SAGE III/ISS products (V5.2) that are suitable for use in both validation and research studies for the data products as described in the Data Product User’s Guide (DPUG). The nominal monthly release of new SAGE III/ISS events will be processed only with V5.2 algorithm starting with March 2021. Version 5.1 remains publicly available for events from June 2017 through February 2021. This statement applies to SAGE III/ISS Version 5.2 Solar Level 1B, Solar Level 2, and Lunar Level 2 data products. The SAGE III/ISS Team recommends using Version 5.2 instead of Version 5.1 because of the modifications and improvements mentioned below.

Vertical profiles of ozone, nitrogen dioxide (NO2), and water vapor (H2O) concentrations, as well as multi-wavelength aerosol extinction coefficient, are included in the solar Level 2 data product files. Three ozone profiles are available in this release of the solar products: a UV based mesospheric product (i.e., “Ozone_Mes” in the product files) and two Chappuis-based products. One Chappuis-based product uses a spectrally-focused fitting retrieval (i.e., “Ozone_MLR”) while the other uses a broad-spectrum retrieval scheme that is similar to that of SAGE II (i.e., “Ozone_AO3”). Composite ozone and retrieved temperature/pressure products are not included in the V5.2 data set. Vertical profiles of ozone, nitrogen dioxide (NO2), and nitrogen trioxide (NO3) concentrations are included in the lunar Level 2 product files. Chlorine Dioxide (OClO) from lunar occultation is not included in this release. The channel wavelengths used in solar and lunar retrievals are available in the Data Product User’s Guide (DPUG).

Version 5.2 improvements and bug fixes recovered 311 more solar events (increase of 1.0%) compared to v5.1; 104 more lunar events (increase of 4.3%) compared to v5.1; improvements and the number of water vapor profiles withheld by QA was reduced from 570 (v5.1) to 30 (v5.2).

Reader Software:

Both IDL and Python reader software are available to access the products in the native format and a Python reader is available for the HDF format. The product formats have changed slightly, so the new readers are required for this release. Readers for previous versions of SAGE III data are not compatible with this version. However, the new IDL and Python data readers are backwards compatible with the previous version of the data product, in both formats.

Data Access Methods:

Direct Data Download

Earthdata Search

For questions regarding data usage, please ask us on the Earthdata Forum

Related URLS: https://asdc.larc.nasa.gov/project/SAGE%20III-ISS

Enhanced Stratospheric Aerosols from Fukutoku-Okanoba Eruption

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Did you know active volcanoes lie beneath the ocean’s surface? The Stratospheric Aerosol and Gas Experiment (SAGE) III on the International Space Station (ISS) instrument spotted remnants of the Fukutoku-Okanoba undersea volcanic eruption in Earth’s stratosphere.

Fukutoku-Okanoba erupted vigorously in the Philippine Sea on Aug. 13, 2021. Although the volcano’s summit is approximately 80 feet under water, the powerful eruption was still forceful enough to send ash and sulfate aerosol particles high above the sea’s surface and well up into the lower stratosphere at an altitude of approximately 16 km. While SAGE III was not measuring in the immediate vicinity to capture data at the time of the eruption, SAGE III observations passed through the same latitude one week later, and measurements discerned a new aerosol layer in the lower stratosphere.

These are important observations for SAGE III to make, because they help scientists understand global climate change better. Stratospheric aerosols such as these act to cool the Earth’s surface by reflecting sunlight back to space.

It is worth noting that sulfate aerosols don’t blast straight from the mouth of an underwater volcano into the stratosphere. Sulfuric dioxide from the volcano reacts with water to form sulfuric acid, which then condenses into the sulfate droplets spotted by SAGE III.

The map below illustrates the geographic area of the late August 2021 SAGE III measurements.

The data plot below shows the clear spike in aerosols right above the tropopause (dotted line) from the eruption of Fukutoku-Okanoba. Although this was a comparably small eruption in relation to some in the historical record, multiple minor and moderate eruptions causing aerosol enhancements in the stratosphere have a cumulative effect. The result has been shown to be important when studying past changes in Earth’s climate, as well as predicting future changes.

Higher in the stratosphere around 23 km, SAGE III also saw an enhanced layer of aerosols remaining from the eruption of the La Soufrière volcano in April 2021.

The SAGE III team continues to examine the evolution of these volcanic disturbances in the stratosphere as the instrument samples the tropics/sub-tropics in the coming months.

Summer Interns Successfully Accomplish Science and Engineering Projects for SAGE III Mission

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While the COVID 19 pandemic caused another summer of virtual internships, it didn’t stop students from across the country from furthering their education and professional experience with NASA.

With over 1,000 applicants to the mission’s internship program, the Stratospheric Aerosol and Gas Experiment (SAGE) III team at Langley Research Center in Hampton, VA selected a team of six student interns to work on a variety of science and engineering projects during the 10-week summer session.

Maggie Zheng, a rising senior at the Massachusetts Institute of Technology (MIT) studying aerospace engineering, worked with the SAGE III science validation team on the code base and documentation for a new automated Quick Look tool of SAGE III’s atmospheric ozone and water vapor measurements. Typically, there is a period of two months between SAGE III collecting data and when that data is released to the public. Zheng’s development of a Quick Look tool will allow the SAGE III team to examine data before this post-processing period.

“The Quick Look tool will give scientists insights from our data on current events and will allow SAGE III data to contribute to ongoing conversations in the scientific community,” said Zheng.

Zheng will be further working with the SAGE III team on this project during the fall session of NASA internships.

SAGE III intern Thomas Nicewicz attended NASA’s Boeing Orbital Flight Test-2 Launch in August 2021 and toured some of Kennedy Space Center’s facilities such as the Vehicle Assembly Building (VAB).

Thomas Nicewicz, a student at Washington and Jefferson College, worked to improve the coordinate transformation from the Disturbance Monitoring Package (DMP) to the Sensor Assembly (SA) on the SAGE III instrument. The coordinate transformation is needed to map small changes in attitude seen by the DMP to the SA and improves the team’s knowledge of SAGE III’s pointing.

In honor of National Interns Day, Nicewicz was randomly selected by the NASA internship program to attend the Boeing Orbital Flight Test-2 launch at NASA’s Kennedy Space Center in Florida with interns from across the agency. This uncrewed mission tested the end-to-end capabilities of the Starliner spacecraft and Atlas V rocket from launch to docking to a return to Earth in the desert of the western United States. Interns were able to view the launch to the International Space Station (ISS) from the coast of Cape Canaveral and tour some of the center’s iconic facilities.

Anya Lomsadze, a junior at Yale University studying Statistics and Data Science and Energy Studies, completed a project to study the low aerosol extinction values in the SAGE III data set. Lomsadze created a software tool that automates identifying and modeling low aerosol values in the data set and identifies how reliable SAGE’s measurements are at these low values. Her analysis points to a possible detection limit of the SAGE III instrument for measuring low aerosol values in the lower altitudes of the stratosphere.

“Through working on this project, collaborating with the other SAGE interns, and attending SAGE mission meetings, I learned about everything from atmospheric chemistry to collaborative code development to how ISS dockings can impact data collection. I’ve learned invaluable lessons this summer at Langley about the scientific process, collaboration, and lifelong learning that I am excited to apply in school, work, and life,” said Lomsadze.

Did you know that high school students can apply to the NASA internship program? Sophia Steven, a rising high school senior at Peak to Peak Charter School in Lafayette, Colorado joined the SAGE III internship team this summer. She created a user-friendly interface for extracting SAGE III science data from the database on the SAGE-PRIME data processing server. Based on a user’s requests, the interface can query the SAGE III database and return a collection containing the user’s specific data request, as well as a plot of the returned data all using Python.

Liam Hunsberger, a rising senior at Purdue University studying Applied Physics and Planetary Science, worked on a solution to better process limb scattering events measured by the SAGE III instrument. To process a limb scattering event, the raw data is retrieved, relevant telemetry is extracted, and a dataset is built for each limb event from the spectral data. Through the existing software, this process is done manually. Hunsberger worked to automate the process in Python by completing a script that can batch process multiple science events, and also created a functionality to continually search for and process events.

Michael Villordon, a senior at the University of Texas at Dallas majoring in computer science, worked on the Aerosol Classification Machine Learning project. The goal of Villordon’s project was to create a process that could automatically identify if any given point in a SAGE III data profile contained clouds via machine learning. Clouds often interfere with SAGE III measurements and are physically and chemically distinct from other atmospheric aerosols. An automated process to filter or to identify clouds can ultimately improve the quality of the data set and analyses using those data. Villordon’s work advanced the machine learning algorithm to make this process faster, more efficient, and highly extensible within a Python framework.

Although the SAGE III team of interns did not physically gather in person this summer, they still found the virtual internship experience to be rewarding.

“I was able to meet often with my mentors and collaborate with the other SAGE III interns virtually through Microsoft Teams and Git. I really appreciated how much time the mentors spent in training us in skills that will be useful to us later in our careers as well. And of course, I also loved getting to know the mentors and interns a bit outside of trainings and work,” said Zheng.

The NASA internship program wouldn’t be successful without the team of mentors across the agency that dedicate their time to support, educate, and train interns each year.

“The comprehensive training modules developed by the SAGE III/ISS mentors equip interns with skills and knowledge to put into practice wherever their careers take them, maybe even as future NASA employees. These are skills interns often do not have exposure to in their college careers, but are very beneficial in both the academic and professional environments,” said Dr. Charles Hill, lead SAGE III/ISS mentor.

The LaRC team of mentors hosted a couple of “Fireside Chats” to socialize with the SAGE interns, and even held a virtual Bob Ross painting night.

SAGE III interns and mentors display their finished art after enjoying a virtual Bob Ross painting lesson.

The innovation, hard work, and dedication of the SAGE III summer internship team will continue to support and benefit the Langley mission team for the foreseeable future.

To apply for the next session of NASA internships, please visit intern.nasa.gov.

Studying Earth’s Stratospheric Water Vapor

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What does water vapor have in common with Sisyphus, the mythological Greek character cursed to roll a rock uphill only to have it roll back down again? Water is continuously cycling on Earth between bodies of water such as oceans, lakes and rivers, land surfaces, and in the atmosphere. When water warms and evaporates from the Earth’s surface it becomes gaseous in the form of water vapor, H2O. As water vapor rises into the atmosphere, it cools and can condense into clouds which can produce rain or snow bringing water back to the Earth’s surface. And the cycle begins again.

Water vapor is also an important component in Earth’s evolving climate system. As a major greenhouse gas – a gas that traps heat – water vapor absorbs heat produced by Earth’s surface and the shining Sun. The water molecules then emit that heat back to Earth’s surface which can increase the temperature. This relationship between an increase in water vapor in the atmosphere contributing to warming temperatures, and warmer temperatures causing an increase in water vapor is called a positive feedback loop.

Although water vapor in the stratosphere is only a few molecules per million air molecules, this positive feedback relationship between water vapor and temperature is important as scientists study to better understand how much this impacts Earth’s changing climate.

In addition to measuring stratospheric ozone and aerosols, the Stratospheric Aerosol and Gas Experiment (SAGE) III instrument on the International Space Station (ISS) measures trace gases including water vapor. Unlike many other science data instruments, SAGE III provides a very precise and highly accurate measurement of water vapor in the upper troposphere and throughout the stratosphere.

Other satellite-based instruments, such as the Microwave Limb Sounder (MLS) on NASA’s Aura and the High-Altitude Lidar Observatory (HALO), measure atmospheric water vapor in the upper troposphere and stratosphere. SAGE III uses the solar occultation technique, which is unique, in that it can take more precise measurements covering vertical layers of atmosphere.

“Because SAGE III provides such a high accuracy data set, we can look at different levels of the atmosphere in more detail than ever before. We can see every kilometer in the vertical profiles of data,” said Mijeong Park, Project Scientist at the National Center for Atmospheric Research in Boulder, CO.

In partnership with the National Center for Atmospheric Research (NCAR), the National Oceanic and Atmospheric Administration (NOAA), and the Jet Propulsion Laboratory (JPL), the SAGE III team at NASA’s Langley Research Center in Hampton, Virginia released initial analyses of the SAGE III water vapor data version 5.1 in the paper “Near-Global Variability of Stratospheric Water Vapor Observed by SAGE III/ISS.”

Throughout the paper, the SAGE III version 5.1 water vapor data are validated against MLS version 5 retrievals and show overall first-rate agreement between the two data sets. The relatively young SAGE III/ISS dataset is recording water vapor seasonal variability that agrees well with MLS from the tropopause through the middle stratosphere (∼16–30 km).

By looking at SAGE III data between 2017 and 2020, scientists were given some insight into the year-to-year variability of H2O during boreal summer monsoon season. A monsoon is a seasonal change in wind and rain patterns observed in certain parts of the world, including North America.

“By looking at multiple years of data, we can understand how much water vapor is going into the stratosphere through the summer monsoon circulation each year,” said Park.

In the figure above, SAGE III (a and c) is compared to MLS (b and d) for August 2017 (top) and January 2018 (bottom). In August of 2017, SAGE III H2O showed that water vapor over the North American monsoon region was relatively higher than over the Asian monsoon region. While the SAGE III instrument takes about one month to cover the latitude range ∼60N–60S, scientists have found that this monthly sampling captures more localized values of water vapor in the lower stratosphere.

Although the summer monsoon season varies year by year, SAGE’s ability to detect the interannual variability of stratospheric water vapor during monsoon season helps scientists better understand how changes in water vapor are contributing to Earth’s climate.

Scientists are also able to study relative humidity (RH) with SAGE III’s water vapor data. Relative humidity tells us how much water vapor is in the air, relative to how much water vapor the air could hold at a given temperature. As air temperatures rise, warmer air can hold more water vapor increasing the saturation point. Cold air can hold less water vapor.

The RH-temperature relationships captured by SAGE III agree with the near-tropopause data derived from high-resolution Upper Troposphere/Lower Stratosphere (UTLS) aircraft measurements, which enhances the science community’s confidence in the quality of the SAGE III data set.

“The SAGE III data can be used for more detailed studies of relative humidity distribution and its variability because of the accuracy. It will also help scientists to better simulate our climate using global climate models,” said Park.

While SAGE III will continue to measure water vapor from ISS over the coming years, a longer record of water vapor data is needed.

“It is very important to have a continuous measurement of water vapor anywhere on Earth. There are many ways to measure water vapor, by satellite, like SAGE, by airplane, or by ground-based instruments. There is only one continuous water vapor record of 30-plus years from balloon measurements in Boulder, Colorado. Satellite missions have limited lifetimes. We need continuous measurements of water vapor to really understand how water vapor affects our climate,” said Park.

Using SAGE III water vapor data collected from June 2017 – February 2021, the visualization illustrates the transport of water vapor in Earth’s stratosphere at various altitudes and latitudes. In the equatorial region, notable masses of dry air (blue/green colors) are seen rising upward from the tropopause, the transition point between the troposphere and stratosphere denoted by the grey dashed line, through the lower to mid-stratosphere. The orbit of the International Space Station enables SAGE III to observe the southern mid-latitudes, tropics and northern mid-latitudes every month, with the exception of July and December when data is confined to the mid-latitudes.
Credits: Mijeong Park/National Center for Atmospheric Research

New SAGE III Science Team Members Selected

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NASA’s Science Mission Directorate has selected proposals for the solicited SAGE III on ISS Science Team program. The individuals selected for this team, from a variety of diverse institutions, will conduct studies using the data from the SAGE III instrument to help better understand the composition of Earth’s atmosphere and how it’s evolving. These ten individuals, selected by competitive solicitation, will provide data analysis and independent validation, limb scatter retrieval algorithm development and adaptation, assessments of atmospheric composition, studies of clouds and aerosols, contributions to modeling efforts, and multi-sensor data product development. You can find descriptions of each member’s proposed work here.

SAGE III/ISS Science Team Members:

Peter Bernath/Old Dominion University
Mian Chin/Goddard Space Flight Center
Sean Davis/Office of Oceanic and Atmospheric Research, Boulder
Glenn Jaross/Goddard Space Flight Center
Lars Kalnajs/University of Colorado, Boulder
Travis Knepp/Langley Research Center
Katherine Emma Knowland/Universities Space Research Association, Columbia
Stanley Sander/Jet Propulsion Laboratory
Jean-Paul Vernier/National Institute of Aerospace Associates
Hsiang-Jui (Ray) Wang/Georgia Institute of Technology
Jun Wang/University of Iowa, Iowa City

SAGE III Carries on Critical Measurements of Stratospheric Aerosols and Ozone

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On the fourth anniversary of its first-light measurements, we are taking a look at some of the critical data collected by NASA’s Stratospheric Aerosol and Gas Experiment III (SAGE III) aboard the International Space Station. Launched to the station in February 2017, SAGE III is the most recent in a series of SAGE instruments that have measured stratospheric gases and aerosols from space. The SAGE family of instruments started in 1979 and is one of NASA’s longest-running Earth-observing programs.

Data from SAGE II helped confirm human-driven changes to the ozone layer, which contributed to the 1987 Montreal Protocol that banned some of the most destructive industrially-produced ozone-depleting chemicals. Stratospheric ozone acts as a sunscreen for the Earth, filtering out harmful solar radiation by absorbing some of the Sun’s ultraviolet rays, providing people, animals and plants some protection from that harmful radiation.

This latest SAGE III instrument is helping scientists monitor the recovery of ozone resulting from the reduction in emissions of ozone-depleting substances called for under the Montreal Protocol. SAGE III has also measured the intrusion of aerosols into the stratosphere from intense wildfires in Australia and California, and from volcanic eruptions. Those aerosols, which can remain in the stratosphere for months or even years, can lead to variability in the climate record. Water vapor, a potent greenhouse gas that can be lofted into the stratosphere by extreme storms, is also visible to SAGE III. Though it’s normal to have some water vapor in the stratosphere, using SAGE data, scientists can better understand how year-to-year changes in tropical weather affect the amount of water vapor in regions of the stratosphere influenced by the tropical weather circulation.

SAGE III makes measurements using solar and lunar occultation, a technique that involves looking at light from the Sun or Moon as it passes through Earth’s atmosphere at the edge, or limb, of the planet. The SAGE III payload on the space station is managed by NASA’s Langley Research Center in Hampton, Virginia and was developed in partnership with the European Space Agency, Ball Aerospace Technology Corporation, and NASA’s Johnson Space Center in Houston.

Credits:
Allison McMahon (SSAI): Producer
Haley Reed (ADNET): Producer
David Flittner (NASA/LaRC): Scientist
Marilee Roell (NASA/LaRC): Scientist
Jamie Nehrir (NASA/LaRC): Engineer
Kevin Leavor (SSAI): Scientist
NASA’s Goddard Space Flight Center Conceptual Image Lab
NASA’s Scientific Visualization Studio

SAGE III Sees California Wildfire Effects in Stratosphere

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Wildfires have been burning across the state of California since August 2020. As the fires continue to rage, NASA Earth science missions have observed increased numbers of airborne particles known as aerosols across the country.

Different types of aerosols scatter or absorb sunlight to varying degrees, depending on their size, type and location. While most aerosols reflect sunlight, dark colored soot particles from fires absorb sunlight, warming Earth’s atmosphere, and shading the surface below it. When smoke from large wildfire events enters the stratosphere, these competing warming and cooling effects on the atmosphere can contribute to variability in the climate record.

In September and October, the Stratospheric Aerosol and Gas Experiment III (SAGE III) instrument aboard the International Space Station observed smoke from the ongoing wildfires using solar occultation, a measurement technique that involves looking at light from the Sun as it passes through Earth’s atmosphere at the edge, or limb, of the planet. The initial observation was made over the Eastern United States, but additional instances of increased stratospheric aerosols were observed south of California in the succeeding days. SAGE III observations show a significant increase in stratospheric aerosols when compared to data from July.

In September and October, SAGE III was clearly seeing smoke in the stratosphere from the California wildfires, and continuing to see smoke from the Australian bushfires. The red, orange, and yellow colors above the tropopause line, which separates the troposphere from the stratosphere, indicates increased levels of aerosols. Credits: NASA

Aerosols that reach the troposphere, the lowest layer of Earth’s atmosphere where most of the life on the surface exists, only remain for about a week because rain cleanses them from the air. Stratospheric aerosols can stick around for months or even years.

SAGE III measures stratospheric aerosols at nine wavelengths. The multi-wavelength data of SAGE III is unique, providing important clues to aerosol type. SAGE III data from September and October suggests the aerosols were larger than in previous months. Variation in size of the aerosol particles can also suggest a change in composition.

“Based on the context, the larger particles seen in the SAGE III/ISS data are most likely carbonaceous, or soot,” said David Flittner, SAGE III project scientist at NASA’s Langley Research Center in Hampton, Virginia.

SAGE III observations of the wildfires are supported by additional satellite and human observations. Aircraft observations of the California Creek Fire from the National Weather Service suggested convection pushed smoke to just over 9 miles (15 km) into the air, which was also observed by SAGE.

“SAGE III provides highly accurate and precise observations of aerosol properties that bridge and contextualize measurements from other instruments,” said Flittner.

This event marks yet another instance of intense fires lofting tremendous amounts of heat and moisture high into Earth’s atmosphere, creating dangerous smoke-infused clouds that resemble thunderstorms. The SAGE III instrument is still observing the stratospheric effects of the Australian fires that occurred in late 2019 and early 2020. NASA Earth scientists are tracking the frequency of these stratosphere-penetrating phenomena, also known as pyrocumulus events, and comparing them to the SAGE II instrument historical record.

 

 

20 Years of Observing Earth from the International Space Station

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After 20 years of continuous human presence, the International Space Station (ISS) has provided 241 visitors with an extraordinary view of Earth from outer space — one they have shared with the rest of the world.

Astronaut photography, formally called Crew Earth Observations (CEO), has resulted in more than 3.5 million photographs of the ever-changing blue planet. But camera-wielding astronauts are not the only ones looking down at Earth from their perch in the sky. An impressive suite of Earth Science instruments have also visited the station to capture vast amounts of data about our planet.

However, space aboard the station itself is limited, and the spots are highly coveted. Instruments go through a rigorous approval process and cycle through every couple of years, turning the station into a virtual swiss-army knife of interchangeable remote sensing tools. An especially comprehensive suite of Earth observing instruments are currently aboard the station, with two more approved and several more proposing to become future ISS instruments.

These instruments complement one another to provide a more complete picture of Earth systems, according to William Stefanov, branch chief for the Exploration Science Office at NASA’s Johnson Space Center, and principal investigator for the Crew Earth Observations Facility on the International Space Station. “That’s why it’s serendipitously great that all of these instruments are on the International Space Station and functioning simultaneously,” Stefanov said.

ECOSTRESS

The human crew came in especially handy for the Ecosystem Spaceborne Thermal Radiometer Experiment on Space Station (ECOSTRESS) instrument, which records the temperature of plants on Earth’s surface by measuring the heat they give off. The instrument required the addition of Wi-Fi modules to transmit its data to the station, which in turn required astronauts to conduct a spacewalk to install them.

Since then, ECOSTRESS has provided new insights into the relationship between plant temperatures and water usage. It can identify plant stress down to an individual farmer’s field, when intervention and water management may still be possible to save crops.

Principal investigator Simon Hook says scientists have only just begun to scratch the surface of how the instrument can be used based on its frequent and high-resolution temperature measurements. There is work underway to use the temperature data to observe wildfires, droughts, volcanoes and heat waves, or even to identify heat patterns within urban cities.

GEDI

From fields to forests, another plant-focused instrument is the Global Ecosystem Dynamics Investigation (GEDI). Using lidar—a method of bouncing a laser off the planet and measuring how long it takes the signal to return—GEDI is creating a record of the three-dimensional structure world’s tropical and temperate forests so that Earth’s tree canopies can be mapped and tracked over time.

The vertical structure of forests, which is essentially the height of the trees and how their leaves and branches are arranged vertically, can help determine how much carbon storage is lost from deforestation or gained from growing forests. GEDI principal investigator Ralph Dubayah, professor of Geographical Sciences at the University of Maryland, College Park, says this is the biggest uncertainty we have about the global carbon cycle, and why there is so much attention put on understanding how deforestation and tree growth contribute to atmospheric carbon dioxide concentrations. GEDI is a collaborative effort between NASA and UMD.

To supply its high-power laser, GEDI takes advantage of the massive solar panels on the station. “Right now on the International Space Station we have an amazing confluence of instruments that together are able to observe ecosystem function, structure and plant composition,” Dubayah said. “And it was entirely made possible because we have this incredible science platform in the ISS.”

LIS

Being high above the clouds also makes the station a good platform for observing the weather. NASA’s Lightning Imaging Sensor (LIS) records the time, energy output and locations of lightning events around the world in the lower atmosphere. It can provide information on when storms are growing or decaying, thereby helping to improve weather forecasting models and aircraft/spacecraft safety precautions.

It complements the Geostationary Lightning Mapper (GLM) aboard the Geostationary Operational Environmental Satellite (GOES-16), which is a collaboration between NASA, the National Atmospheric and Oceanic Administration (NOAA) and industry partners, and the European Space Agency’s (ESA) monitoring of thunderstorms and upper atmosphere lightning events through the Atmosphere Space Interaction Monitor (ASIM) instrument which is on the ISS.

The data from ASIM and LIS are both able to capture the impacts of dust storms, pollution, fires, and volcanic eruptions on cloud formation and electrification. This is just one example of how ESA, and other international agencies including the German Aerospace Center (DLR) and the Japan Aerospace Exploration Agency (JAXA), are also helping advance a global understanding of our planet through ISS-instruments with Earth observations of their own.

OCO-3

Several instruments currently aboard the station are not the first of their kind. As the name might suggest, the Orbiting Carbon Observatory-3 (OCO-3) is a third iteration instrument for long-term monitoring of atmospheric carbon dioxide distributions around the globe, complementing long-term ground-based observations. It provides insights into regional carbon sources and sinks and monitors changes in the carbon cycle linked to human activity.

Together with GEDI and ECOSTRESS, OCO-3 contributes to a more complete picture of terrestrial ecosystems. While its predecessor, the OCO-2 satellite, followed a polar orbit, OCO-3’s path aboard the station offers a denser data set for areas with large carbon fluxes, including Earth’s most biologically diverse regions like the Amazon rainforest.

The orbit also allows measurements at different times of day, which especially benefits ECOSTRESS and OCO-3 as plants and their contribution to the carbon cycle fluctuate with time of day due to variations in sun, temperature and water availability.

SAGE III

Like OCO-3, the Stratospheric Aerosol and Gas Experiment (SAGE) III, is a third-generation instrument. The successive SAGE instruments have provided an ongoing record of Earth’s upper atmospheric water vapor, aerosol and ozone – which make up the protective “sunscreen” layer for the planet.

The Stratospheric Aerosol and Gas Experiment (SAGE) III’s line of sight from the International Space Station provides a view of the aerosols and gases present in Earth’s atmosphere by taking advantage of the sunlight traveling through a slice of the atmosphere. Credits: NASA

When sunlight passes through the upper atmosphere, its unique mixture of particulates and gases create the picturesque colors of spectacular sunsets and sunrises. To replicate a sunset or sunrise view from the space station, SAGE III looks at Earth from a side angle, capturing a similar view of the atmosphere on its edge as someone watching the sunset from the ground. But from its vantage point of space, SAGE III can view the entirety of these atmospheric layers according to project scientist Dave Flittner, and sees 15 sunrises and sunsets every day.

Science manager Marilee Roell says the longevity of these observations has been crucial to monitoring and maintaining the protective ozone layer in the upper atmosphere. SAGE II closely monitored the past ozone decline from common aerosols in hair sprays and fire retardants that degraded the layer, and its data informed the Montreal Protocol Treaty, which phased out the use of these damaging chemicals.

“It’s one of the biggest success stories of science informing policy,” said Roell. “And not only is this a premier science instrument, but it’s also on the International Space Station—a crewed platform. We are kind of getting the best of both science and getting to be a part of the human spaceflight program in a peripheral way.”

TSIS-1

Additional atmospheric measurements of the sun come from the Total and Spectral Solar Irradiance Sensor (TSIS-1) – which is actually made of two instruments: the Total Irradiance Monitor (TIM) and Spectral Irradiance Monitor (SIM).

TSIS-1 continues the work of NASA’s Solar Radiation and Climate Experiment satellite by measuring the amount of sunlight that reaches Earth, and how it is distributed in wavelength.

These measurements of solar energy, along with model-based calculations of its absorption and reflection by Earth’s atmosphere and surface, provide insights into the sun’s influence on climate, the ozone layer, atmospheric circulation, and ecosystems. The data are critical inputs for modeling of Earth’s climate and atmospheric systems.

COMING SOON: EMIT & CLARREO-PF

There is still more to learn about Earth, and new instruments which can further contribute to our understanding like the Climate Absolute Radiance and Refractivity Observatory (CLARREO) Pathfinder and the Earth Surface Mineral Dust Source Investigation (EMIT) are already scheduled to reach the station within the next couple of years.

The CLARREO Pathfinder will measure sunlight reflected off Earth, and take direct measurements of the Sun, with unparalleled accuracy. The data can then help calibrate other sensors starting in 2021. EMIT is scheduled to launch the following year in 2022 to map dust-source regions on Earth’s surface and assess the impact of dust on the warming and cooling of the atmosphere.

“It’s been really satisfying to see the range of things we have had on the space station,” said Stefanov. From imaging systems to lasers and radars, and more recently hyperspectral instruments Stefanov believes that the limit to what they can do in the future is really only limited by what scientists and engineers are able to design and the number of instrument ports available.

“There will be opportunities for new sensors to go up to the station,” he said. “And I think it will continue to develop as a very useful remote sensing platform for Earth observations going forward.”

Lara Streiff
NASA’s Earth Science News Team

SAGE III Interns Successfully Complete Virtual Internship Program

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NASA offers a variety of internship opportunities to thousands of students across the country throughout the year. The 2020 internship program looked very different due to COVID-19. While interns were not able to be physically on-site at NASA centers, they were able to work virtually from home and gain the same professional experience.

Despite the many challenges that came with the COVID-19 pandemic, the Stratospheric Aerosol and Gas Experiment (SAGE) III on the International Space Station (ISS) team at NASA Langley Research Center in Hampton, VA was able to host a team of five student interns. The group of interns worked on various atmospheric science, mathematics and engineering projects during their 10-week virtual internship with the SAGE III mission team.

Laila Howar, a senior at George Mason University majoring in Atmospheric Science and Computer Science, worked on a project to solve the long-standing uncertainty in differentiating between clouds and aerosols. Her approach involved a supervised machine learning approach where she compared different classifiers and performed hyper-parameter optimization, as well as cross-validation, to assess the performance of the models.

“My work on SAGE III ties together everything for my future career aspirations,” said Howar. “The other interns and I can all say that our mentors have made this such an unforgettable experience for us. They provided us with countless learning opportunities and gave us the opportunity to get to know their fellow associates through shadowing.”

The SAGE III team sent the group of interns to the virtual SciPy conference which allows participants to showcase Python projects, learn from other user and developers, and collaborate together on code development.

For Ney-Ling Navarro, who virtually worked her NASA internship from Puerto Rico, the SciPy conference aligned well with her internship project and gave her an opportunity to learn more in the field of computer science. Ney-Ling worked on the Multiplicative Extended Kalman Filter (MEKF) code cleanup. Her updates fell into two categories: addressing open GitHub tickets for Python updates and updating and streamlining existing Jupyter notebooks to improve their usability.

To stay socially connected throughout the internship, SAGE III mentors hosted daily virtual coffee breaks and multiple “fireside” chats where mentors would discuss any topic of the intern group’s choosing. The group even got together for a virtual Bob Ross painting night!

The agency also connected interns across all centers through a series of online lectures on work going on across the agency, as well as virtual tours and intern meetups.

“I would say that this is not the experience I expected from a virtual internship. The amount of effort that the SAGE III team and NASA has put in to make this a great experience has done just that,” said Howar.

While COVID-19 may have changed the location of their internships, the SAGE III interns were resilient and successfully adapted to the virtual environment and using platforms such as Microsoft Teams.

“I learned over the course of my internship to arrive to virtual meetings early in case new software needed to be installed and to be ready to connect online in multiple ways in case the network was rough,” said SAGE III intern Preston Robinette.

The work that the SAGE interns completed during their internships continues to support the efforts of the mission team. A big thank you to Laila, Ney-Ling, Alexas, Preston, and Kate for all of the outstanding work and time dedicated to the SAGE III/ISS mission!

ROSES-20 Amendment 34: New Opportunity: SAGE III/ISS Science Team Added to ROSES-2020

By Uncategorized

A.50 SAGE III/ISS Science Team seeks proposals for members of the SAGE III Science Team. Proposals are sought in six topical areas that appear below. The first five areas are presented in no particular priority order, while the sixth topic, Independent validation, is deemed of somewhat lower priority:

· Assessing Long-term Changes in Atmospheric Composition
· Aerosol and Cloud Studies
· Data Analysis and Modeling Efforts Using SAGE Data Sets
· Multi-sensor Data Product Development
· Limb Scatter Retrieval Algorithm Development or Adaptation
· Independent Validation

In addition to proposals for SAGE III/ISS Science Team membership, there is also the opportunity to propose for the position as Team Leader for the SAGE III/ISS Science Team.

Amendment 34 announces a new opportunity: SAGE III/ISS Science Team has been added to ROSES-2020 as A.50. Notices of intent are requested by September 18, 2020, and proposals are due November 6, 2020.

On or about June 16, 2020, this Amendment to the NASA Research Announcement “Research Opportunities in Space and Earth Sciences (ROSES) 2020” (NNH20ZDA001N) will be posted on the NASA research opportunity homepage at: http://solicitation.nasaprs.com/ROSES2020 and will appear on SARA’s ROSES blog at: https://science.nasa.gov/researchers/sara/grant-solicitations/roses-2020/.

More information on science data processing may be found here under the “Data Access” tab.

Questions concerning A.50 SAGE III/ISS Science Team may be directed to Richard Eckman, who may be reached at richard.s.eckman@nasa.gov.

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Space Station Live: Wise Eye in the Sky

 

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SAGE III Promo

 

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NASA X Episode I: SAGE III Monitoring Earth

 

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SAGE III Integration and Test Timelapse

 

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Space Station Live: Studying Earth’s Sunscreen

 

SAGE III Sun Look Test Video

SAGE III Sunlook Test

 

NASA Launchpad: SAGE III/ISS

NASA Launchpad: SAGE III/ISS

 

NASA Real World: Ozone

NASA Real World: Good Ozone, Bad Ozone

 

NASA's Our World: Sunsets

NASA’s Our World: Sunsets and Atmosphere

 

SAGE III/ISS Overview Video

SAGE III/ISS Overview Video

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Mission Brochure

 

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SAGE III/ISS Fact Sheet

 

The SAGE Legacy's Next Chapter: SAGE III on the International Space Station

SAGE Earth Observer Article

 

SAGE III International Collaboration

SAGE III/ISS International Collaboration

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