Galactic Cosmic Ray Decreases Associated With Non-Interacting Magnetic Clouds in the 23 Rd Solar Cycle

Proceedings of the International Astronomical Union - United Kingdom
doi 10.1017/s1743921313011654
Full Text
Abstract

Available in full text

Date
Authors
Publisher

Cambridge University Press (CUP)

Related search

The Behaviour of Galactic Cosmic-Ray Intensity During Solar Activity Cycle 24

Solar Physics
AstrophysicsAstronomyPlanetary ScienceSpace
2019English

Exceptionally Strong Variation of Galactic Cosmic Ray Intensity at Solar Rotation Period After the Maximum of Solar Cycle 2

2016English

Hale Cycle in Solar-Rotation Related Recurrence of Galactic Cosmic Rays

2017English

The Interaction of Cosmic Rays With Galactic Center Molecular Clouds

2019English

Amplification of Galactic Magnetic Fields by the Cosmic-Ray-Driven Dynamo

Astrophysical Journal
AstrophysicsAstronomyPlanetary ScienceSpace
2004English

The Variations of Solar Magnetic Networks Over the Solar Cycle 23

Proceedings of the International Astronomical Union
AstrophysicsAstronomyPlanetary ScienceSpace
2012English

Cosmic‐Ray History and Its Implications for Galactic Magnetic Fields

Astrophysical Journal
AstrophysicsAstronomyPlanetary ScienceSpace
2003English

Solar Cycle Variation of Cosmic Ray Intensity Along With Interplanetary and Solar Wind Plasma Parameters

Latvian Journal of Physics and Technical Sciences
EngineeringAstronomyPhysics
2008English

On the Connection of Gamma Rays From Supernova Remnants Interacting With Molecular Clouds and Cosmic Ray Ionization Measured

2016English

Amanote Research

Note-taking for researchers

Follow Amanote

© 2024 Amaplex Software S.P.R.L. All rights reserved.

Privacy PolicyRefund Policy