Analytical and numerical modelling of magnetic flux rope structures in the heliosphere
About the role
This project will focus on the development of analytical and numerical models of magnetic flux rope structures in the heliosphere. It involves studying:
- Deformations due to self-interaction or external factors like the coronal magnetic field or solar wind variations.
- Structural changes such as expansion or changes in magnetic twist.
- Stability conditions and constraints.
- Model configurations for comparison with real-world in-situ magnetic field measurements.
Responsibilities
Theoretical approaches developed within this program will be validated using in-situ or remote imaging data from current missions such as Parker Solar Probe or STEREO.
Requirements
To apply, candidates must have completed a Doctoral Degree and meet eligibility criteria including being a U.S. Citizen, U.S. LPR, Foreign National eligible for J-1 visa, or applicants for LPR, asylees, or refugees with valid EAD cards and pending I-485 or I-589 forms.
Qualifications
A strong background in physics, particularly in heliophysics, is required. Experience with numerical simulations and analytical methods is preferred.
Skills
Proficiency in Python, MATLAB, or similar programming languages is essential. Knowledge of heliophysics and magnetic field dynamics is crucial.
Benefits
The NASA Postdoctoral Program offers unique research opportunities at NASA Centers, Headquarters, or affiliated institutes. Fellowships are competitive and support one to three years of research.
Pay
The salary range for this position is $70,000 - $100,000 per year, depending on qualifications and experience.
Schedule
The schedule is flexible and tailored to the needs of the project and the individual researcher.
Note: Please visit the NASA Postdoctoral Program website for detailed application instructions and requirements.