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Anomalous Component of Cosmic Rays
The anomalous component of cosmic rays (ACR) in the heliosphere (Fig. 5.1) was discovered in the early 1970s from spacecraft measurements. The ACR...
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Anomalous Cosmic Rays and Heliospheric Energetic Particles
We present a review of Anomalous Cosmic Rays (ACRs), including the history of their discovery and recent insights into their acceleration and...
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Galactic Cosmic Rays Throughout the Heliosphere and in the Very Local Interstellar Medium
We review recent observations and modeling developments on the subject of galactic cosmic rays through the heliosphere and in the Very Local...
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Theory of Cosmic Ray Transport in the Heliosphere
Modelling the transport of cosmic rays (CRs) in the heliosphere represents a global challenge in the field of heliophysics, in that such a study, if...
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Method for Detecting Anomalous Changes in the Speed of Arrival of Cosmic Rays to the Earth Using Machine Learning
An automated method for detecting anomalous changes in the speed of arrival of galactic cosmic rays to the Earth is proposed. The method is based on...
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Transport of Particles in the Heliosphere
To date, it is well established that the heliosphere is filled with charged particles of various origins (solar wind and solar cosmic rays, GCR,...
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Low-energy cosmic rays: regulators of the dense interstellar medium
Low-energy cosmic rays (up to the GeV energy domain) play a crucial role in the physics and chemistry of the densest phase of the interstellar...
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Course 7: Cosmic Rays and Particle Acceleration at Astrophysical Shocks
The acceleration of particles in the vicinity of astrophysical shocks has become the main paradigm in astrophysics for the production of cosmic rays...
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Studies of Heliospheric Modulation of Cosmic Rays at ShICRA SB RAS and Prospects of Their Further Development
AbstractThe paper presents the results of the staff of ShICRA SB RAS on cosmic ray research over the past two decades. A brief description of the...
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Observations of the Outer Heliosphere, Heliosheath, and Interstellar Medium
The Voyager spacecraft have left the heliosphere and entered the interstellar medium, making the first observations of the termination shock,...
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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...
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Inhomogeneity in the Local ISM and Its Relation to the Heliosphere
This paper reviews past research and new studies underway of the local interstellar environment and its changing influence on the heliosphere. The...
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The Structure of the Large-Scale Heliosphere as Seen by Current Models
This review summarizes the current state of research aiming at a description of the global heliosphere using both analytical and numerical modeling...
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Interplanetary Disturbances
The Sun emits the variable solar wind which interacts with the very local interstellar medium to form the heliosphere. Hence variations in solar...
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Turbulence in the Outer Heliosphere
The solar wind (SW) and local interstellar medium (LISM) are turbulent media. Their interaction is governed by complex physical processes and creates...
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Cosmic Radioactivity and Galactic Chemical Evolution
The description of the tempo-spatial evolution of the composition of cosmic gas on galactic scales is called ‘modelling galactic chemical evolution’....
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The Structure of the Global Heliosphere as Seen by In-Situ Ions from the Voyagers and Remotely Sensed ENAs from Cassini
The exploration of interplanetary space and our solar bubble, the heliosphere, has made a big leap over the past two decades, due to the...
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Future Exploration of the Outer Heliosphere and Very Local Interstellar Medium by Interstellar Probe
A detailed overview of the knowledge gaps in our understanding of the heliospheric interaction with the largely unexplored Very Local Interstellar...
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Cosmic Radioactivity and Galactic Chemical Evolution
The description of the tempo-spatial evolution of the composition of cosmic gas on galactic scales is called ‘modelling galactic chemical evolution’....
