Study of the 27 day variations in GCR fluxes during 2007–2008 based on PAMELA and ARINA observations

R Modzelewska, GA Bazilevskaya… - The Astrophysical …, 2020 - iopscience.iop.org
Using measurements from the PAMELA and ARINA spectrometers on board the Resurs-
DK1 satellite, we have examined the 27 day intensity variations in galactic cosmic ray (GCR) …

The 27-day cosmic ray intensity variations during solar minimum 23/24

R Modzelewska, MV Alania - Solar Physics, 2013 - Springer
We have studied the 27-day variations and their harmonics in Galactic cosmic ray (GCR)
intensity, solar wind velocity, and interplanetary magnetic field (IMF) components during the …

Study of short-term periodicities in the occurrence of Forbush decreases: wavelet analysis

YP Singh, Badruddin - Astrophysics and Space Science, 2024 - Springer
We utilized the Forbush decreases (magnitude> 1.5%) detected in cosmic ray neutron
monitor data during continuous five solar cycles, viz., 20, 21, 22, 23 and 24 (1965 to 2019) …

Hale cycle and long-term trend in variation of galactic cosmic rays related to solar rotation

A Gil, K Mursula - Astronomy & Astrophysics, 2017 - aanda.org
Context. Galactic cosmic ray (GCR) intensities around solar minimum times are modulated
by magnetic drifts that depend on the overall solar polarity. GCR intensities reach a higher …

Energy spectrum of the recurrent variation of galactic cosmic rays during the solar minimum of cycles 23/24

A Gil, MV Alania - solar physics, 2016 - Springer
The Sun during the recent epoch of solar activity operated in a different way than during the
last 60 years, being less active. We study temporal changes of the energy spectrum of the …

Theoretical and experimental studies of the rigidity spectrum of the 27-day variation of the galactic cosmic ray intensity in different epochs of solar activity

A Gil, MV Alania - Solar Physics, 2013 - Springer
We consider the recent, very exceptional, 11-year cycle (2003–2009) of solar activity and
confirm that the relative amplitude in rigidity spectrum, δD (R)/D (R), which can be …

Corotating solar wind structures and recurrent trains of enhanced diurnal variation in galactic cosmic rays

T Yeeram, D Ruffolo, A Sáiz, N Kamyan… - The Astrophysical …, 2014 - iopscience.iop.org
ABSTRACT Data from the Princess Sirindhorn Neutron Monitor at Doi Inthanon, Thailand,
with a vertical cutoff rigidity of 16.8 GV, were utilized to determine the diurnal anisotropy (DA) …

Fourth harmonic behaviour of the 27-day periodicity in galactic cosmic rays during different solar magnetic polarity intervals

PB Kotzé - Solar Physics, 2020 - Springer
Galactic cosmic rays as observed by the Hermanus and Jungfraujoch Neutron Monitors
between 1960 and 2018 have been analysed using various spectral analysis techniques …

Quasi-periodic changes in the 3D solar anisotropy of Galactic cosmic rays for 1965–2014

R Modzelewska, MV Alania - Astronomy & Astrophysics, 2018 - aanda.org
Aims. We study features of the 3D solar anisotropy of Galactic cosmic rays (GCR) for 1965−
2014 (almost five solar cycles, cycles 20− 24). We analyze the 27-day variations of the 2D …

Passage of the high-speed solar wind streams, their plasma/field properties, and resulting geomagnetic disturbances

F Mustajab - Advances in Space Research, 2017 - Elsevier
We study the geomagnetic disturbances and solar wind plasma/field properties during the
passage of High Speed Solar Wind Streams (HSS) emanating from the sun. We consider the …