most citedOn the relationship of the 27-day variations of the solar wind velocity and galactic cosmic ray intensity in minimum epoch of solar activity

25 citations · 76 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.SR2015★ 4 cited

Numerical methods for solution of the stochastic differential equations equivalent to the non-stationary Parker's transport equation

A. Wawrzynczak, R. Modzelewska, M. Kluczek

We derive the numerical schemes for the strong order integration of the set of the stochastic differential equations (SDEs) corresponding to the non-stationary Parker transport equ…

astro-ph.SR2015★ 10 cited

Stochastic approach to the numerical solution of the non-stationary Parker's transport equation

A. Wawrzynczak, R. Modzelewska, A. Gil

We present the newly developed stochastic model of the galactic cosmic ray (GCR) particles transport in the heliosphere. Mathematically Parker transport equation (PTE) describing n…

astro-ph.SR2015★ 2 cited

A stochastic method of solution of the Parker transport equation

A. Wawrzynczak, R. Modzelewska, A. Gil

We present the stochastic model of the galactic cosmic ray (GCR) particles transport in the heliosphere. Based on the solution of the Parker transport equation we developed models…

astro-ph.SR2015

Annual Variations of the Galactic Cosmic Ray Intensity and Seasonal Distribution of the Cloudless Days and Cloudless Nights in Abastumani (41.75oN, 42.82oE; Georgia): (1) experimental study and (2) theoretical modeling

M. V. Alania, G. G. Didebulidze, R. Modzelewska +2

We study a possible relationships between seasonal distributions of the visually observed cloudless days (CD) and cloudless nights (CN) at Abastumani Astrophysical Observatory (41.…

astro-ph.SR2015★ 3 cited

27-day variation of the GCR intensity based on corrected and uncorrected for geomagnetic disturbances data of neutron monitors

M. V. Alania, R. Modzelewska, A. Wawrzynczak +2

We study 27-day variations of the galactic cosmic ray (GCR) intensity for 2005- 2008 period of the solar cycle #23. We use neutron monitors (NMs) data corrected and uncorrected for…

astro-ph.SR2015★ 25 cited

On the relationship of the 27-day variations of the solar wind velocity and galactic cosmic ray intensity in minimum epoch of solar activity

M. V. Alania, R. Modzelewska, A. Wawrzynczak

We study the relationship of the 27-day variation of the galactic cosmic ray intensity with similar changes of the solar wind velocity and the interplanetary magnetic field based o…

astro-ph.SR2015★ 14 cited

Pecularities of cosmic ray modulation in the solar minimum 23/24

M. V. Alania, R. Modzelewska, A. Wawrzynczak

We study changes of the galactic cosmic ray (GCR) intensity for the ending period of the solar cycle 23 and the beginning of the solar cycle 24 using neutron monitors experimental…

astro-ph.SR2015★ 18 cited

Modeling and experimental study of the 27-day variation of galactic cosmic-ray intensity for a solar-wind velocity depending on heliolongitude

M. V. Alania, R. Modzelewska, A. Wawrzynczak

We develop a three dimensional (3-D) model of the 27-day variation of galactic cosmic ray (GCR) intensity with a spatial variation of the solar wind velocity. A consistent, diverge…