Abstract The Lunar Environment heliospheric X-ray Imager (LEXI) is a wide field-of-view soft
X-ray telescope developed to study solar wind-magnetosphere coupling. LEXI is part of the …

Imaging is one of the essential techniques to observe astronomical structures. While
analyzing the observed images, it is a challenge in many scientific fields to reconstruct the 3 …

The Earth's magnetosheath and cusps are the sources of soft X‐rays. In the accompanying
paper (Part 1) and this paper, we discuss the methods of finding the magnetopause position …

The magnetopause standoff distance characterizes global magnetospheric compression
and deformation in response to changes in the solar wind dynamic pressure and …

The study of solar wind charge exchange (SWCX) emission is vital to both the X-ray
astrophysics and heliophysics communities. SWCX emission contaminates all astrophysical …

The Solar wind Magnetosphere Ionosphere Link Explorer (SMILE) is an ESA-CAS joint
mission. Primary goals are investigating the dynamic response of the Earth's …

Soft X‐ray imaging is a new method used to observe the structure of the Earth's
magnetosphere. Reconstruction of the Earth's three‐dimensional (3‐D) magnetospheric …

Jupiter has the most complex and energetic radiation belts in our Solar System and one of
the most challenging space environments to measure and characterize in-depth. Their …

We present an initial assessment of using tomography on single‐spacecraft images to
reconstruct 3D X‐ray emissions from the Earth's magnetosheath. 3D structures in the Earth's …

Interactions between solar wind ions and neutral hydrogen atoms in Earth's exosphere can
lead to the emission of soft X‐rays. Upcoming missions such as SMILE and LEXI aim to use …