Jennifer Carter

University of Leicester

United Kingdom

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Articles (17)

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2025

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2025

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2022

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2022

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2022

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2022

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2022

Collaborators (12)

Andrey Samsonov

University College London

UNITED KINGDOM

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C. Forsyth

UNITED KINGDOM

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Maria-Theresia Walach

University of Lancaster

UNITED KINGDOM

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Dimitra Koutroumpa

CNRS Délégation Ile-de-France Sud

FRANCE

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Kjellmar Oksavik

Professor (100%)

University of Bergen

NORWAY

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G. E. Bower

UNITED KINGDOM

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Tom Elsden

University of Glasgow

UNITED KINGDOM

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Liang Zhao

University of Michigan

UNITED STATES

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Susan Lepri

University of Michigan

UNITED STATES

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Graziella Branduardi-Raymont

University College London

UNITED KINGDOM

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Timothy Yeoman

Professor

University of Leicester

UNITED KINGDOM

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Sudeshna Boro Saikia

Tenure-track Assistant Professor

Universität Wien

AUSTRIA

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Jennifer Carter

Research Interests

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Articles (17)

Empirical Functions for Highly Charged Ion Abundances in Solar Wind Charge Exchange Models: Addressing Post‐2011 ACE Data Limitations

A Holistic Approach to the SMILE Mission and SMILE Public Engagement

Determining the Subsolar Magnetopause Position Using CMEM

Modeling the Magnetospheric 3D X‐Ray Emission From SWCX Using a Cusp‐Magnetosheath Emissivity Model

X-ray detection of astrospheres around three main-sequence stars and their mass-loss rates

The exosphere of Mars can be tracked by a high-spectral resolution telescope, such as the Line Emission Mapper

Can XMM‐Newton Be Used to Track Compositional Changes in the Solar Wind?

Multi-instrument observations of the effects of a solar wind pressure pulse on the high latitude ionosphere

Dynamical Response of Solar Wind Charge Exchange Soft X-Ray Emission in Earth’s Magnetosphere to the Solar Wind Proton Flux

The Relationship between Solar Wind Charge Exchange Soft X-ray Emission and the Tangent Direction of Magnetopause in an XMM–Newton Event

Mean Energy Flux, Associated Derived Height‐Integrated Conductances, and Field‐Aligned Current Magnitudes Evolve Differently During a Substorm

Finding Magnetopause Standoff Distance Using a Soft X‐Ray Imager: 1. Magnetospheric Masking

Finding Magnetopause Standoff Distance Using a Soft X‐ray Imager: 2. Methods to Analyze 2‐D X‐ray Images

Solar Wind Charge Exchange Soft X-Ray Emissions in the Magnetosphere during an Interplanetary Coronal Mass Ejection Compared to Its Driven Sheath

Solar Minimum Exospheric Neutral Density Near the Subsolar Magnetopause Estimated From the XMM Soft X‐Ray Observations on 12 November 2008

Influence of Off‐Sun‐Earth Line Distance on the Accuracy of L1 Solar Wind Monitoring

Lobe Reconnection and Cusp‐Aligned Auroral Arcs

Collaborators (12)

Andrey Samsonov

C. Forsyth

Maria-Theresia Walach

Dimitra Koutroumpa

Kjellmar Oksavik

G. E. Bower

Tom Elsden

Liang Zhao

Susan Lepri

Graziella Branduardi-Raymont

Timothy Yeoman

Sudeshna Boro Saikia

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