JC
Jennifer Carter
University of Leicester, European Space Astronomy Centre, University of Bristol, National Physical Laboratory
Research areas: Earth and Planetary Sciences · Space and Planetary Science · Solar and Space Plasma Dynamics · Ionosphere and magnetosphere dynamics · Lightning and Electromagnetic Phenomena
0000-0002-0981-2895
Employment
- 2005 - Present
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European Space Astronomy Centre Young Graduate Trainee2004 - 2005
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National Physical Laboratory Research Scientist2003 - 2004
Education
- 2007 - 2011
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University of Bristol MSci Physics with Astrophysics First Class Honours1998 - 2002
Projects & Funding
Projects & funding information is unavailable.
Publications (114)
- How accurately can we find the magnetopause standoff distance using SMILE SXI? Save
- Progress of the SMILE Modeling Working Group Save
- Finding the Magnetopause Standoff Distance Using Soft X‐Ray Images: Application for the SMILE Mission Save
- Elfen: a mission to measure the heavy ion composition of the Earth’s magnetosphere Save
- Resolving magnetosheath jet responses in soft X-ray images Save
- Determining the Magnetopause Location With SMILE‐SXI Using a Constrained Solar Wind Independent SWCX Model Save
- Ionospheric currents and auroral signatures during successive earthward bursty bulk flows and dipolarization: a 7 December 2023 case study Save
- Spectral Properties of Solar Wind Charge Exchange from Earth’s Magnetospheric Boundaries: MHD and Test Particle Simulations Save
- Jupiter's X‐ray Aurorae. A High Signal Spectral Analysis of the 0.24–1.40 keV Energy Range Save
- Jupiter's X-ray Aurorae. A high signal spectral analysis of the 1.60 keV to 7.00 keV energy range Save
- The Soft X-ray Imager (SXI) on the SMILE Mission Save
- Geoeffectivity of Solar Wind Heavy Ions Save
- Jupiter's X-ray Aurorae. A high signal spectral analysis of the 0.24 to 1.40 keV energy range Save
- A Holistic Approach to the SMILE Mission and SMILE Public Engagement Save
- Determining the Subsolar Magnetopause Position Using CMEM Save
- Empirical Functions for Highly Charged Ion Abundances in Solar Wind Charge Exchange Models: Addressing Post‐2011 ACE Data Limitations Save
- Modeling the Magnetospheric 3D X‐Ray Emission From SWCX Using a Cusp‐Magnetosheath Emissivity Model Save
- Empirical Functions for Highly Charged Ion Abundances in Solar Wind Charge Exchange Models: Addressing Post-2011 ACE Data Limitations Save
- Exospheric neutral density at the 10 RE subsolar point during solar maximum: estimates from XMM soft X-ray observations Save
- SMILE SXI can be used to track solar wind composition Save