Jack Brooks – Iowa State University

In gamma-ray astronomy, the ability to combine data from multiple observatories that sample different regions of the gamma-ray spectrum is crucial to understanding processes–such as particle acceleration and diffusion–that take place in and around astrophysical phenomena. Ground-based gamma-ray observatories therefore provide an important complement to NASA’s Fermi Gamma-Ray Space Telescope (FGST).

In particle astrophysics, extended maximum likelihood methods, which can be used to derive the fractional contributions as well as spatial and spectral parameters of multiple data components with different astrophysical origins, also provide a natural framework for combining data from multiple observatories. Such techniques are already the standard approach for analyzing data from the FGST. Our research seeks to address the problems that arise when applying the technique of binned extended maximum likelihoods to data procured for ground-based gamma-ray astronomy. These problems stem from the fact that gamma-ray astronomy data spaces are largely dominated not by gamma-rays, but by cosmic rays. The large uncertainties associated with Monte Carlo models of cosmic ray background in conjunction with the low uncertainties of gamma-ray models result in a data space comprising regions of high uncertainty and other regions of low uncertainty. A data space of this form introduces serious mathematical issues for present maximum likelihood methods. Our objective is to run a series of tests that emulate this problematic scenario in order to better understand the statistical considerations that must be made for maximum likelihood analysis of gamma-ray data.

Mallory Weber – University of Iowa

X-ray science can shed light on key physics, probing how black holes behave, how they influence galactic evolution, and how massive stars shape their environments through powerful winds. Observations at these wavelengths require sending technology above the Earth’s atmosphere, where the desired signals are not absorbed. This makes CubeSats and SmallSats important tools for conducting X-ray science, providing low cost access to space for focused experiments. However, these missions require efficient, moderately sized X-ray detectors at low costs in order to perform their target science. My group is examining the performance of commercial CMOS sensors for use in soft X-ray observations and their potential as low-cost alternatives to CCD sensors.

We have shown that the CMOS performance is on par with CCDs currently in use in several major spacecraft, and their readout rates and operable temperatures are more favorable. My research focuses on measuring the quantum efficiency (QE) of the CMOS sensor, which will inform us upon the sensitivity of the instrument. I will develop a test bed in a specialized vacuum chamber equipped with an X-ray source that will allow us to make preliminary measurements at different X-ray wavelengths to determine the QE. Additionally, we plan to eventually further these measurements during a test campaign at the Advanced Light Source, an X-ray synchrotron facility.

James Neal – Drake University

While space flight is a crucial and exciting part of NASA’s mission, it can inflict a significant blow to one’s physiology. The intense vibration of an aircraft rattles the brain, resulting in changes on the cellular, molecular, and even cognitive level. Studies have demonstrated that helicopter pilots enduring chronic, low-level vibrations are more vulnerable to central nervous system (CNS) degeneration. Furthermore, mild traumatic brain injuries (mTBIs) can mimic neurodegenerative conditions such as Alzheimer’s and Parkinson’s Disease in their molecular and cognitive manifestation. Therefore, it is critical to the safety of astronauts to better understand the CNS effects of the vibrations endured during space flight.

Our lab employs a mouse model of mTBI on cognition and neurodegeneration. We test mice that have had mTBIs in different cognitive and behavioral dimensions, including an operant conditioning paradigm that assays working memory, attention, and decision-making. We then examine biomarkers of neurodegeneration in the prefrontal cortex, striatum, and hippocampus. A previous study conducted in our lab has highlighted a potential neuroprotective role of female sex hormones following mTBIs. We hope to expand this research to specifically investigate the repetitive vibrational injuries endured during spaceflight to inform safety procedures and possible neuroprotective interventions and treatments for traumatic brain injuries.

Adam Haroon – Iowa State University

As Urban Air Mobility (UAM) emerges as a transformative transportation solution, ensuring equitable access and community acceptance becomes paramount for successful integration into urban environments. Current UAM development often overlooks community needs and may exacerbate transportation inequities if not carefully designed. This project addresses the critical gap between advanced autonomous air transportation technology and inclusive urban planning by developing machine learning frameworks that prioritize both safety and social equity in UAM system design.

Our research employs a multi-faceted approach combining deep reinforcement learning policies with hybrid LSTM-Graph Neural Network architectures to enable safe, efficient multi-agent UAV collision avoidance in complex urban airspaces. Using real-world data from Austin, Texas, we are creating robust simulation environments that model realistic UAM operations while developing equitable algorithms for airspace management. The project includes optimization of vertiport placement through Monte Carlo tree search methods and the creation of VertiCAP, an innovative planning tool that integrates community input into UAM infrastructure design decisions.

The research will produce scalable algorithms capable of managing high-density UAM traffic while ensuring equitable access across diverse urban communities. By incorporating community-driven design principles, the project aims to prevent the digital divide from extending into aerial transportation, ensuring that UAM benefits all urban residents rather than creating new forms of transportation inequality. The VertiCAP tool will provide municipalities with data-driven insights for inclusive vertiport placement and operational planning.

This project directly supports NASA ARMD’s Strategic Thrusts by advancing autonomous collision avoidance systems (Thrust 6), enabling safe vertical lift vehicle integration (Thrust 4), developing scalable airspace management for global operations (Thrust 1), and creating real-time safety assurance capabilities (Thrust 5). Our work provides NASA with foundational technologies for next-generation aviation infrastructure while pioneering community-centered approaches essential for sustainable and equitable aviation transformation in urban environments.

Owenn Hermann – Kennedy Space Center

Describe what you did during your internship:

 

Did you achieve your goals?

 

Describe positive lessons learned:

 

Describe negative lessons learned:

 

What was the impact of this internship?

 

Luke Post – Langley Research Center

Student in lab equipment showing off internship project.

Describe what you did during your internship:

I started by investigating whether electroding the flax-based composite samples was necessary for accurate dielectric measurements which entailed creating a mask for uniform electrodes, and then thermal evaporating gold and sputtering silver on them. After that testing was complete, I moved to the main goal of my spring here which was characterizing the effect of moisture on the dielectric constant of the composites. For that study another intern and I made a humidity chamber by developing a bubbling system and exposed all of the samples to increased levels of humidity. I then took capacitance measurements on those samples every morning and calculated the dielectric constant. Doing that, I was able to find a line that fit the moisture level versus dielectric constant plot so we should be able to figure out how much moisture is in these composites by their dielectric constant. While I was doing that, I was also using an inkjet printer to print frequency selective surfaces (FSSs) in silver and attempting to find the optimal sintering conditions that resulted in the lowest resistivity of the printed structure. I then used those printed structures to detect moisture inside of the biocomposite samples based on the change in the frequency response of the samples when there was no moisture present. I also started preliminary work on using those same FSSs to test for strain within the material by looking at the shifted resonant frequency of the FSS when the composites were under a load.

Did you achieve your goals?

Yes, I did achieve my goals. For the dielectric measurements, I was able to classify a baseline dielectric constant for all three different composites and create a fitted curve that related to their moisture content vs dielectric constant. I also figured out that electroding of the samples was unnecessary for our experiment. Then for the moisture testing, I, along with one of my mentors, discovered that 1 uL of water was able to be detected when placed behind the flax/Rilsan sample, and we have preliminary results for strain testing on a milled FSS but nothing yet for the FSSs on the flax composites.

Describe positive lessons learned:

I learned how to effectively conduct research, how to better report my findings, and how to write a technical report for journals and conferences. I also gained in experience in how to effectively work in a team research setting.

Describe negative lessons learned:

The only negative I can think of is that sometimes layoffs happen and during my time in the internship, there was a lot of unease about what was going to happen.

What was the impact of this internship?

This internship has shown me how much I truly love research. It has challenged me in a way that I don’t get to see in school with real world problems and has allowed me to work on projects that have the potential to change the world. It has made me sure of the fact that I desire to continue school beyond my bachelors and aim for a PhD so that I can continue to do this kind of research when I graduate. It has also cemented my desire to work in the aerospace industry long term. The aerospace industry brings unique challenges to the table every day due to our minimal understanding of everything that goes on in space which I love. Getting to see all of the mind-blowing work that goes on at Langley certainly redefined portions of my goals and confirmed other aspects.

Joshua Laird – University of Iowa

I use a combination of novel and published fossil occurrence data to investigate ecological changes in marine paleocommunities during intense ecosystem changes in the Ordovician Period (~487–443 million years ago) of Earth’s history. My work focuses on trilobites, an extinct group of marine arthropods, and how they distributed themselves across different habitat types during the prolonged ecosystem restructuring of the Ordovician Radiation, as well as their response to the more abrupt end-Ordovician mass extinction. The fossil record contains many examples of climate change-induced mass extinction events, but only a few are associated with the transition from an “icehouse” to an “ice-free” world. The end-Ordovician event is one such instance and therefore can provide useful context for the ongoing biodiversity crisis and associated ecosystem changes.

My research has two primary aims. First, I am investigating the reorganization of trilobite communities across depth-related habitat types in response to the climate change-driven end-Ordovician mass extinction, which eliminated over 50% of global trilobite diversity at higher taxonomic levels. Within-habitat (alpha) species diversity remained unaffected by the extinction event, which suggests that a dissimilarity component of diversity may have been altered. I am investigating the between-habitat (beta) diversity response of trilobites to determine if local (alpha) diversity was maintained by reducing taxonomic dissimilarity among habitat types. Additionally, I am examining the habitat associations of taxonomic lineages that survived, and did not survive, the extinction event to assess if habitat preference, or changes to it over time, was linked to extinction likelihood.

Initial results from Laurentia (most of present-day North America) support a decline in between-habitat dissimilarity following the end-Ordovician mass extinction. This mechanism appears to have at least partially maintained local diversities, potentially buffering against wider ecosystem changes in the wake of the extinction. Ongoing research will determine if this reorganization was unique to Laurentia and if the pattern holds up to additional examination.

John Momberg – University of Iowa

Be stars are a type of star that rotate so rapidly that the centrifugal force causes their equators to bulge outward. If they rotate fast enough, they can eject material into an orbiting disk. To form such a disk, these stars must be spinning near their critical velocity (the speed where the centrifugal force at the equator throwing material outwards balances the force of gravity pulling material inwards). However, spectroscopic observations of Be stars show that they are only rotating at about 70% critical, which isn’t fast enough to eject material into orbit and create the disks we see. These observations have assumed that the stars rotate as solid bodies. The goal of my project is to investigate whether differential rotation along the surface (meaning that different parts of the surface rotate at different rates) could explain why spectroscopic observations might underestimate the true rotation rate. To test this, I have calculated the shape and rotation rate of a rotating star and used a library of spectral data to simulate the total spectra produced by the star. I have successfully applied this method to a few test cases, such as an ellipsoid-shaped star, and verified that the effects of rotation on the resulting spectra match my expectations. I plan on applying this method to a differentially rotating star to see what effects the differential rotation has on the spectra. 

Kenneth Buffo – University of Iowa

The Astrophysics Division of NASA’s SMD emphasizes the development of precision X-ray optics to study the hot X-ray emitting plasma associated with faint celestial sources. Additionally, modern diffraction-limited storage rings and X-ray free-electron laser beamlines have enabled extremely bright and coherent X-ray beams that require precisely shaped optics focus these beamlines so as to not degrade their performance. This research project will mature the readiness of adjustable X-ray optics for use in astronomy and X-ray beamlines. This technology will enable the production of thin mirrors without compromising their focusing capability. These mirrors employ a set of discrete, thin-film piezoelectric actuators that when supplied a set of voltages induce a deterministic figure change to the mirror. This can correct for a variety of distortions and improve mirror angular resolution. This project will include designing an electronic control system and optical alignment configuration to test adjustable mirrors of different geometries and actuator materials. Interferometry will be used to measure the surface correctability of these mirrors on the scale of nanometers. Different optimization techniques will be explored to understand how to better calculate the voltages necessary to induce figure changes that yields the best angular resolution.

Gage MacLin – University of Iowa

This work focuses on advancing the integration of autonomous aircraft into civilian airspace, a key component of NASA’s Urban Air Mobility (UAM) initiative. Previously, I developed a cooperative planning and control framework that ensures collision avoidance and energy-efficient autonomous flight using optimal control and formal safety guarantees. This framework provides mathematically rigorous methods for generating safe trajectories in constrained and dynamic environments. Building on this foundation, I am now investigating how neural networks can enhance trajectory generation by improving adaptability to dynamic airspace conditions. Traditional optimal control methods, while effective, often face computational challenges when applied in real-time. By integrating data-driven techniques, I aim to develop a framework that enables computationally efficient trajectory generation for autonomous aircraft in complex environments.