SS
Steven Sembay
University of Leicester
Research areas: Physics and Astronomy · Astronomy and Astrophysics · Solar and Space Plasma Dynamics · Ionosphere and magnetosphere dynamics · Astrophysical Phenomena and Observations
0000-0002-3700-9784
Employment
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University of Leicester Research Fellow1989 - Present
Education
Education history is unavailable.
Projects & Funding
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Continued Post Launch Support of XMM-Newton EPIC in the UK Science and Technology Facilities Council2009 - 2011
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Continued Post Launch Support of XMM-Newton EPIC in the UK Science and Technology Facilities Council2007 - 2009
Publications (30)
- Finding the Magnetopause Standoff Distance Using Soft X‐Ray Images: Application for the SMILE Mission Save
- Determining the Magnetopause Location With SMILE‐SXI Using a Constrained Solar Wind Independent SWCX Model Save
- The Soft X-ray Imager (SXI) on the SMILE Mission Save
- Determining the Subsolar Magnetopause Position Using CMEM Save
- Modeling the Magnetospheric 3D X‐Ray Emission From SWCX Using a Cusp‐Magnetosheath Emissivity Model Save
- Can XMM‐Newton Be Used to Track Compositional Changes in the Solar Wind? Save
- Can XMM-Newton be used to track compositional changes in the solar wind? Save
- Modeling Soft X‐Ray Emissions at the Dayside Magnetopause Save
- Dynamical Response of Solar Wind Charge Exchange Soft X-Ray Emission in Earth’s Magnetosphere to the Solar Wind Proton Flux Save
- The Relationship between Solar Wind Charge Exchange Soft X-ray Emission and the Tangent Direction of Magnetopause in an XMM–Newton Event Save
- Finding Magnetopause Standoff Distance Using a Soft X‐Ray Imager: 1. Magnetospheric Masking Save
- Finding Magnetopause Standoff Distance Using a Soft X‐ray Imager: 2. Methods to Analyze 2‐D X‐ray Images Save
- Finding Magnetopause Standoff Distance using a Soft X-ray Imager - Part 1: Magnetospheric masking Save
- Finding Magnetopause Standoff Distance using a Soft X-ray Imager - Part 2: Methods to Analyze 2-D X-ray Images Save
- Solar Wind Charge Exchange Soft X-Ray Emissions in the Magnetosphere during an Interplanetary Coronal Mass Ejection Compared to Its Driven Sheath Save
- Deriving the Magnetopause Position from the Soft X‐Ray Image by Using the Tangent Fitting Approach Save
- European Space Agency SMILE and Czech participation Save
- Design and implementation of electron diverters for lobster eye space-based X-ray optics Save
- Boundary Detection in Three Dimensions With Application to the SMILE Mission: The Effect of Model‐Fitting Noise Save
- Boundary Detection in Three Dimensions With Application to the SMILE Mission: The Effect of Photon Noise Save