Zobrazeno 1 - 10
of 14
pro vyhledávání: '"Donald Ngobeni"'
Publikováno v:
Physics, Vol 3, Iss 4, Pp 1190-1225 (2021)
Global modulation studies with comprehensive numerical models contribute meaningfully to the refinement of very local interstellar spectra (VLISs) for cosmic rays. Modulation of positrons and anti-protons are investigated to establish how the ratio o
Externí odkaz:
https://doaj.org/article/617f7dc607d5406ca9b43d25b305d579
Autor:
Alex Lenni, Mirko Boezio, Riccardo Munini, Nadir Marcelli, Marius Potgieter, Donald Ngobeni, Oscar Adriani, Giancarlo C. Barbarino, Galina A. Bazilevskaya, Roberto Bellotti, Edward A. Bogomolov, Massimo Bongi, Valter Bonvicini, Alessandro Bruno, Francesco Cafagna, Donatella Campana, Per Carlson, Marco Casolino, Guido Castellini, Cristian De Santis, Arkadiy M. Galper, Sergey V. Koldashov, Sergey Koldobskiy, Alexander N. Kvashnin, Alexey A. Leonov, Vitaly V. Malakhov, Laura Marcelli, Matteo Martucci, Andrey G. Mayorov, Wolfgang Menn, Matteo Mergé, Vladimir V. Mikhailov, Emiliano Mocchiutti, Alfonso Monaco, Nicola Mori, Giuseppe Osteria, Beatrice Panico, Paolo Papini, Mark Pearce, Piergiorgio Picozza, Marco Ricci, Sergio B. Ricciarini, Manfred Simon, Alessandro Sotgiu, Roberta Sparvoli, Piero Spillantini, Yuri I. Stozhkov, Andrea Vacchi, Elena Vannuccini, Gennady I. Vasilyev, Sergey A. Voronov, Yuri T. Yurkin, Gianluigi Zampa, Nicola Zampa
Publikováno v:
Proceedings of 27th European Cosmic Ray Symposium — PoS(ECRS).
Publikováno v:
Advances in Space Research. 68:2953-2962
Effects on galactic cosmic rays (GCRs) of several heliospheric factors during the minimum phases of the sunspot cycles are studied. Times of maximum GCR intensity are determined for the last five sunspot minima, including the present one, together wi
Publikováno v:
Bulletin of the Russian Academy of Sciences: Physics. 85:1179-1182
A study is performed of phases of solar cycle minima in sunspots, the heliosphere, and the intensity of Galactic cosmic rays (GCRs). Times of maximum GCR intensity in the minima of the last five cycles (including the current one), corresponding main
Autor:
Innocentia Ramokgaba, Donald Ngobeni, Mabedle Donald Ngobeni, Opm Aslam, Chris Ndiitwani, Marius Potgieter, Driaan Bisschoff
Publikováno v:
Proceedings of 37th International Cosmic Ray Conference — PoS(ICRC2021).
Autor:
Marius Potgieter, Driaan Bisschoff, Alex Lenni, Nadir Marcelli, Mirko Boezio, Mabedle Donald Ngobeni, Riccardo Munini, O. P. M. Aslam, Wolfgang Menn
The space-borne PAMELA experiment was launched on the 15th June 2006 on board the Russian satellite Resurs-DK1 from the Baikonur cosmodrome. From the beginning PAMELA performed high-precision measurements of cosmic rays over a wide energy range until
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e4108c43e901d7ad00fb5e96e8a23e7c
http://hdl.handle.net/11368/2995938
http://hdl.handle.net/11368/2995938
Autor:
O. P. M. Aslam, Mikhail Krainev, Marius Potgieter, Boris Gvozdevsky, Donald Ngobeni, Mikhail Kalinin
Publikováno v:
Proceedings of 37th International Cosmic Ray Conference — PoS(ICRC2021).
The exact two-dimensional (2D) transport equation (TPE) for galactic cosmic ray (GCR) intensity in the heliosphere averaged over longitude, derived by averaging the full three-dimensional (3D) steady-state TPE over longitude is considered. This exact
Autor:
Donald Ngobeni, Mikhail Krainev, Mikhail Kalinin, Marius Potgieter, O. P. M. Aslam, Boris Gvozdevsky
Publikováno v:
Proceedings of 37th International Cosmic Ray Conference — PoS(ICRC2021).
The conditions in the heliosphere are considered during the minimum phase of the sunspot cycle when the intensity of galactic cosmic rays (GCRs) attains its maximum at the Earth. These times of maximum GCR intensity are determined for the last five s
Autor:
O. P. M. Aslam, Donald Ngobeni, Mirko Boezio, Riccardo Munini, Marius Potgieter, Driaan Bisschoff, Alex Lenni, Nadir Marcelli
Publikováno v:
Proceedings of 37th International Cosmic Ray Conference — PoS(ICRC2021).
Time-dependent energy spectra of galactic cosmic rays (GCRs) carry fundamental information regarding their origin and propagation. When observed at the Earth, these spectra are significantly affected by the solar wind and the embedded solar magnetic
Autor:
Mabedle Donald Ngobeni, O.P.M Aslama, D. Bisschoffa, D.C Ndiitwania, M.S Potgieterc, M. Boeziod, N. Marcellie, R. Muninid, V.V Mikhailov, S.A Koldobskiyf
Publikováno v:
Proceedings of 37th International Cosmic Ray Conference — PoS(ICRC2021).
The global features of the modulation of galactic cosmic ray protons and helium nuclei are studied in the heliosphere from minimum to maximum solar activity with a comprehensive, three-dimensional drift model and compared to observations measured by