Retired Marshall engineer Erich Engler demonstrates antiquated calculation and design tools used in Apollo days.

Erich Engler Demonstrates Calculation Tools

Airborne NASA Radar Maps Mauna Loa Lava Changes in Hawaii

The world's largest active volcano – Hawaii's Mauna Loa – had been quiet for 38 years. But in 2022, the volcano began to stir, showing increased numbers of small earthquakes and subtle swelling of certain land surfaces in September. On November 27, fountains of lava began spurting from the mountain's Northeast Rift Zone and streams of molten rock flowed to the north. Ten days into the eruption, a NASA aircraft conducted its first flight over the erupting volcano. It carried NASA's Uninhabited Aerial Vehicle Synthetic Aperture Radar (UAVSAR) system, which was used to map the volcano's topography in fine detail with a Ka-band instrument called GLISTIN-A. Teams from NASA's Jet Propulsion Laboratory and the United States Geological Survey (USGS) used data from that sensor to map the thickness of those flows during a series of flights on December 7, 8, and 10. The map above shows the thickness of the lava flows during the flight on December 7, the day before USGS scientists noticed a significant decline in the pace of the eruption. A few days later, they declared the eruption had stopped. The map shows the thickness of the lava flows in the summit caldera, where the eruption began, and of lava flows on Mauna Loa's northeastern flank. The color variation from blue to orange indicates increasing lava flow thickness. A maximum thickness of roughly 25 meters (82 feet) is shown, though values exceeding 40 meters (131 feet) were observed in some areas. The thickening at the northern end of the flow is due to lava accumulating away from the vent, along with a flattening of the terrain at the saddle between the Mauna Loa and Mauna Kea volcanoes. By comparing to pre-eruption maps of this area's topography, including GLISTIN-A data collected in 2017, the USGS researchers were able to calculate the size and volume of the lava flow. Over the roughly 14-day eruption, Mauna Loa erupted more than 8.8 billion cubic feet (230 million cubic meters) along a lava flow that extended up to 16.5 miles (19.5 kilometers) from the vent, according to the USGS. The UAVSAR operates from a pod mounted beneath a crewed Gulfstream III jet from NASA's Armstrong Flight Research Center in California. Repeated topographic maps generated with each flight reveal the progression and thickening of lava with time – important information for scientific understanding of volcano processes and for emergency response. For the Mauna Loa science flights, the instrument suite featured an additional state-of-the-art imaging tool: the synthetic aperture radar-fusion optical short-wave infrared (SAR-Fusion Optical/SWIR) camera system. SAR-Fusion collects data over the same ground swath as GLISTIN-A to map land surface changes using optical/SWIR photogrammetry methods. GLISTIN-A was designed to provide all-weather, high-resolution surface topography not available through existing lidar or radar sensors. GLISTIN-A was originally demonstrated as a new radar technique for mapping ice surfaces. Science demonstration flights began in 2013 over alpine glaciers and sea ice in Alaska, and a floodplain in California. Its applications have since expanded to other areas, such as snow accumulation and volcano dynamics. The first time the instrument was deployed for volcano response was in 2018 during the three-month eruption of Kilauea. The success of that operation paved the way for deployment to Mauna Loa. https://photojournal.jpl.nasa.gov/catalog/PIA25526

New Earth-Observing Instrument Installed on the International Space Station

In January 2013, a new Earth-observing instrument was installed on the International Space Station (ISS). ISERV Pathfinder consists of a commercial camera, a telescope, and a pointing system, all positioned to look through the Earth-facing window of ISS’s Destiny module. ISERV Pathfinder is intended as an engineering exercise, with the long-term goal of developing a system for providing imagery to developing nations as they monitor natural disasters and environmental concerns. The image above is the “first light” from the new ISERV camera system, taken at 1:44 p.m. local time on February 16, 2013. It shows the Rio San Pablo as it empties into the Golfo de Montijo in Veraguas, Panama. It is an ecological transition zone, changing from agriculture and pastures to mangrove forests, swamps, and estuary systems. The area has been designated a protected area by the National Environmental Authority (ANAM) of Panama and is listed as a “wetland of international importance” under the Ramsar Convention. (Note that the image is rotated so that north is to the upper right.) “ISERV’s full potential is yet to be seen, but we hope it will really make a difference in people’s lives,” said principal investigator Burgess Howell of NASA’s Marshall Space Flight Center. “For example, if an earthen dam gives way in Bhutan, we want to be able to show officials where the bridge is out or where a road is washed out or a power substation is inundated. This kind of information is critical to focus and speed rescue efforts.” The instrument will be controlled from NASA Marshall in Huntsville, Alabama, in collaboration with researchers at hubs in Central America, East Africa, and the Hindu Kush–Himalaya region. They will rely on positioning software to know where the space station is at each moment and to calculate the next chance to view a particular area on the ground. If there's a good viewing opportunity, the SERVIR team will instruct the camera to take high-resolution photographs at 3 to 7 frames per second, totaling as many as 100 images per pass. With a resolution down to 3.2 meters (10 feet), it will be possible to spot fairly small details and objects. The current mission will test the limitations of Pathfinder and identify measures for improvements in a more permanent system. For instance, the engineering team is working to determine how the geometry of the ISS window affects the imagery; how much sunlight is needed to capture clear images; and how the atmosphere affects that clarity. This characterization phase will last several weeks to a few months. Eventually, ISERV should be made available to the natural hazards community and to basic research scientists. ISERV is short for ISS SERVIR Environmental Research and Visualization system. Together with the U.S. Agency for International Development, NASA runs the SERVIR program to provide satellite data, maps, and other tools to environmental decisionmakers in developing countries. (Servir is a Spanish word meaning “to serve.”) Learn more about the SERVIR program by clicking here: <a href="https://servirglobal.net/Global.aspx" rel="nofollow">servirglobal.net/Global.aspx</a> NASA image by Burgess Howell, SERVIR Global program. Caption by Dauna Coulter, NASA Marshall Space Flight Center, and Mike Carlowicz, NASA Earth Observatory. Instrument: ISS - ISERV Pathfinder Credit: <a href="http://www.earthobservatory.nasa.gov/" rel="nofollow"> NASA Earth Observatory</a> - <a href="http://1.usa.gov/12Aqmg9" rel="nofollow">1.usa.gov/12Aqmg9</a> <a href="http://www.nasa.gov/audience/formedia/features/MP_Photo_Guidelines.html" rel="nofollow">NASA image use policy.</a> <a href="http://www.nasa.gov/centers/goddard/home/index.html" rel="nofollow">NASA Goddard Space Flight Center</a> enables NASA’s mission through four scientific endeavors: Earth Science, Heliophysics, Solar System Exploration, and Astrophysics. Goddard plays a leading role in NASA’s accomplishments by contributing compelling scientific knowledge to advance the Agency’s mission. Follow us on <a href="http://twitter.com/NASA_GoddardPix" rel="nofollow">Twitter</a> Like us on <a href="http://www.facebook.com/pages/Greenbelt-MD/NASA-Goddard/395013845897?ref=tsd" rel="nofollow">Facebook</a> Find us on <a href="http://instagram.com/nasagoddard?vm=grid" rel="nofollow">Instagram</a>