Objectives of this Role:
Develop and advance new and existing solar remote-sensing spectroscopic and/or imaging instrumentation and missions in ultraviolet, X-rays, and other wavelengths.Develop and advance new and existing solar spectroscopic analysis and data processing techniques, especially multi-dimensional spectrospatial deconvolution and differential emission measure analysis.Contribute to development of new laboratory facilities and procedures for testing and calibration of solar remote-sensing instruments.Propose and lead new applied and fundamental research projects relevant to solar coronal and chromospheric plasma physics, including instrumentation and missions to advance related research. Daily and Monthly Responsibilities:
Engage in largely self-directed research and development activities in support of the position objectives.Develop new and compelling research concepts for eventual implementation, in solar physics or other related fields.Lead new proposals to governmental or other agencies to pursue funding in support of the position objectives, for the applicant and other relevant personnel.Participate in existing data analysis and instrumentation projects for solar coronal spectroscopy and imaging.Present progress and results within the project core development teams, at scientific conferences, and in peer-reviewed publications. Requirements:
Requires a PhD in Solar Physics, Astronomy/Astrophysics, Applied Physics, or related fields with relevant experience.3-5 years: Solar remote-sensing imaging and/or spectroscopic instrument development, including design, calibration, integration, and testing.3-5 years: Experience in solar physics data analysis, theory, and/or modeling, demonstrated via a strong track record of peer-reviewed publications, conference presentations, and key roles on successfully funded proposals.3-5 years: Specific experience in solar spectroscopic observations and data analysis, with emphasis on ultraviolet and X-rays, and multi-dimensional deconvolution.