Interstellar mapping and acceleration probe (IMAP): A new NASA mission
Abstract The Interstellar Mapping and Acceleration Probe (IMAP) is a revolutionary mission
that simultaneously investigates two of the most important overarching issues in …
that simultaneously investigates two of the most important overarching issues in …
The structure of the large-scale heliosphere as seen by current models
J Kleimann, K Dialynas, F Fraternale, A Galli… - Space science …, 2022 - Springer
This review summarizes the current state of research aiming at a description of the global
heliosphere using both analytical and numerical modeling efforts, particularly in view of the …
heliosphere using both analytical and numerical modeling efforts, particularly in view of the …
The habitability of proxima centauri bI. irradiation, rotation and volatile inventory from formation to the present
Proxima b is a planet with a minimum mass of 1.3M⊕ orbiting within the habitable zone (HZ)
of Proxima Centauri, a very low-mass, active star and the Sun's closest neighbor. Here we …
of Proxima Centauri, a very low-mass, active star and the Sun's closest neighbor. Here we …
Seven years of imaging the global heliosphere with IBEX
DJ McComas, EJ Zirnstein, M Bzowski… - The Astrophysical …, 2017 - iopscience.iop.org
Abstract The Interstellar Boundary Explorer (IBEX) has now operated in space for 7 years
and returned nearly continuous observations that have led to scientific discoveries and …
and returned nearly continuous observations that have led to scientific discoveries and …
Oblique and rippled heliosphere structures from the Interstellar Boundary Explorer
Past analysis has shown that the heliosphere structure can be deduced from correlations
between long-scale solar wind pressure evolution and energetic neutral atom emissions …
between long-scale solar wind pressure evolution and energetic neutral atom emissions …
Local interstellar magnetic field determined from the Interstellar Boundary Explorer ribbon
The solar wind emanating from the Sun interacts with the local interstellar medium (LISM),
forming the heliosphere. Hydrogen energetic neutral atoms (ENAs) produced by the solar …
forming the heliosphere. Hydrogen energetic neutral atoms (ENAs) produced by the solar …
Sun–heliosphere observation-based ionization rates model
JM Sokół, DJ McComas, M Bzowski… - The Astrophysical …, 2020 - iopscience.iop.org
The solar wind (SW) and the extreme ultraviolet (EUV) radiation modulate fluxes of
interstellar and heliospheric particles inside the heliosphere both in time and in space …
interstellar and heliospheric particles inside the heliosphere both in time and in space …
A new 3D solar wind speed and density model based on interplanetary scintillation
C Porowski, M Bzowski… - The Astrophysical Journal …, 2022 - iopscience.iop.org
The solar wind (SW) is an outflow of the solar coronal plasma, which expands
supersonically throughout the heliosphere. SW particles interact by charge exchange with …
supersonically throughout the heliosphere. SW particles interact by charge exchange with …
Interstellar neutrals, pickup ions, and energetic neutral atoms throughout the heliosphere: present theory and modeling overview
Abstract Interstellar neutrals (ISNs), pick-up ions (PUIs), and energetic neutral atoms (ENAs)
are fundamental constituents of the heliosphere and its interaction with the neighboring …
are fundamental constituents of the heliosphere and its interaction with the neighboring …
IBEX: the first five years (2009–2013)
DJ McComas, F Allegrini, M Bzowski… - The Astrophysical …, 2014 - iopscience.iop.org
ABSTRACT The Interstellar Boundary Explorer (IBEX) returned its first five years of scientific
observations from 2009 to 2013. In this study, we examine, validate, initially analyze, and …
observations from 2009 to 2013. In this study, we examine, validate, initially analyze, and …