EUV Polarimetry for Solar Magnetic Field Studies

ORAU

Huntsville (AL)

On-site

USD 65,000 - 85,000

Full time

10 days ago

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Job summary

NASA's Postdoctoral Program at the Marshall Space Flight Center in Huntsville seeks a researcher to advance next‑generation EUV polarimetric instrumentation for solar heliophysics. The fellow will integrate theory, lab work, and calibration with experts in radiative transfer and detector development, potentially contributing to sounding rocket missions.

Applicants must hold a Doctoral Degree and be eligible to work in the United States; the project emphasizes innovation in EUV measurements and

Qualifications

  • Doctoral Degree required.
  • Eligibility under NASA postdoctoral program rules.
  • Experience with solar physics instrumentation is preferred.

Responsibilities

  • Develop EUV polarimetric instrumentation for solar observations.
  • Model polarization diagnostics and calibrate optical systems.
  • Collaborate with detector development and coatings teams.
  • Assist with mission concept development and lab validation.
  • Contribute to analysis of suborbital flight data.

Skills

Solar magnetism
Polarization theory
Optical coatings
EUV/X-ray instrumentation
Detector development
Programming and modeling
Image processing
Laboratory instrumentation

Education

Doctoral Degree

Job description

Organization

National Aeronautics and Space Administration (NASA)

Reference Code

0022-NPP-NOV26-MSFC-Heliophys

Description

The NASA Postdoctoral Program (NPP) offers unique research opportunities to highly-talented scientists to engage in ongoing NASA research projects at a NASA Center, NASA Headquarters, or at a NASA-affiliated research institute. These one- to three-year fellowships are competitive and are designed to advance NASA’s missions in space science, Earth science, aeronautics, space operations, exploration systems, and astrobiology.

Understanding how magnetic energy is transported and released in the upper solar atmosphere remains one of the fundamental challenges in heliophysics. While routine observations of the solar photosphere provide detailed measurements of surface magnetic fields, direct observations of magnetic fields in the chromosphere, transition region, and low corona remain extremely limited. These atmospheric layers govern coronal heating, the initiation of solar eruptions, and the evolution of space weather, yet their magnetic structure is largely inferred through modeling rather than direct measurement.

Recent advances in ultraviolet spectropolarimetry have demonstrated the scientific potential of polarization diagnostics for probing solar magnetic fields. Extending these techniques into the extreme ultraviolet (EUV) offers the opportunity to directly measure magnetic fields in hotter plasma at greater heights on the Earth-facing solar disk than is currently accessible. Achieving this capability, however, requires significant advances in EUV coatings, detector technology, instrument calibration, and forward modeling.

The selected postdoctoral fellow will contribute to the development of next-generation EUV polarimetric instrumentation intended to enable future observations of magnetic fields in the upper solar atmosphere. Research opportunities span theoretical modeling of polarization diagnostics, optical system design, multilayer coating development, calibration methodologies, laboratory validation, and mission concept development. The exact balance of these activities will be tailored to the interests and expertise of the selected candidate.

The candidate will also aid in coupling forward models of polarized EUV emission with practical instrument design to establish measurement requirements and optimize observational performance. This work will be performed in close collaboration with experts in solar radiative transfer, advanced coatings, detector development, and space instrumentation. Opportunities also exist to participate in laboratory characterization of EUV optical systems, development of calibration techniques for polarization-sensitive optics, and analysis of experimental measurements.

In addition to the primary research effort, the postdoctoral fellow will have opportunities to contribute to the development and scientific exploitation of NASA sounding rocket payloads. The Solar Physics and Astrophysics Branch at NASA Marshall Space Flight Center maintains an active suborbital research program encompassing high-resolution EUV and X-ray imaging, spectroscopy, detector development, and calibration activities. Depending on the fellow’s interests, participation may include instrument development, laboratory testing, mission operations, flight hardware integration, calibration campaigns, and scientific analysis of flight data from current and future sounding rocket investigations.

This position offers a unique opportunity to help establish EUV polarimetry as a new observational capability for heliophysics while participating in the complete lifecycle of space instrumentation from theoretical concept development and laboratory validation through suborbital flight demonstrations and future mission planning.

Field of Science

Heliophysics Science

Advisors

Genevieve Vigil

genevieve.d.vigil@nasa.gov

(360) 649-1607

Applications with citizens from Designated Countries will not be accepted at this time, unless they are Legal Permanent Residents of the United States. A complete list of Designated Countries can be found at: https://www.nasa.gov/oiir/export-control.

Eligibility
  • U.S. Citizens;
  • U.S. Lawful Permanent Residents (LPR);
  • Foreign Nationals eligible for an Exchange Visitor J-1 visa status; and,
  • Applicants for LPR, asylees, or refugees in the U.S. at the time of application with 1) a valid EAD card and 2) I-485 or I-589 forms in pending status
  • Degree: Doctoral Degree.
Preferred Expertise
  • Solar magnetism or radiative transfer
  • Polarization theory or spectropolarimetry
  • Optical system design or optical coatings
  • EUV/X-ray instrumentation
  • Scientific detector development
  • Scientific programming and numerical modeling
  • Image processing or data analysis
  • Laboratory instrumentation and experimental methods
Point of Contact

Mikeala

Questions about this opportunity?

Please email npp@orau.org

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