The Sun's net radiative output varies on timescales of minutes to gigayears. Direct
measurements of the total solar irradiance (TSI) show changes in the spatially-and spectrally …

We have studied long-term variations of galactic cosmic-ray (GCR) intensity in relation to the
sunspot number (SSN) during the most recent solar cycles. This study analyses the time lag …

A perspective is given of the solar modulation of galactic cosmic rays in the heliosphere
during the extraordinary quiet solar minimum period from 2006 to 2009. This is done in the …

Neutron monitors provide continuous measurements of secondary nucleonic particles
produced in the atmosphere by the primary cosmic rays and form the main tool to study the …

Simultaneous and continuous observations of galactic cosmic-ray electrons (e−) and
positrons (e+) from the PAMELA and AMS02 space experiments are most suitable for …

Galactic cosmic rays (GCRs) are energetic, charged particles coming from outside the solar
system. These particles encounter an outward-moving turbulent solar wind with cyclic …

A numerical model for the solar modulation of cosmic rays, based on the solution of a set of
stochastic differential equations (SDEs), is used to illustrate the effects of modifying the …

After a prolonged and deep solar minimum at the end of Cycle 23, the current Solar Cycle 24
is one of the lowest cycles. These two periods of deep minimum and mini-maximum are …

All the evolution of the scientific knowledge about Cosmic Rays (CRs) in the 20 th century
leads to the following statement: Cosmic Rays constitutes a time and spatial variable flux of …

Based on the monthly sunspot numbers (SSNs), the solar-flare index (SFI), grouped solar
flares (GSFs), the tilt angle of heliospheric current sheet (HCS), and cosmic-ray intensity …