A Statistical Analysis of Solar Wind Parameters and Geomagnetic Indices during the Solar Cycle 23

2015 ◽  
Vol 58 (2) ◽  
pp. 170-178
Author(s):  
SHEN Xiao-Fei ◽  
NI Bin-Bin ◽  
GU Xu-Dong ◽  
ZHOU Chen ◽  
LIU Yong ◽  
...  
Keyword(s):  
Solar Wind ◽  
Statistical Analysis ◽  
Solar Cycle ◽  
Geomagnetic Indices ◽  
Solar Cycle 23 ◽  
Solar Wind Parameters

Statistical analysis of solar wind parameters and geomagnetic indices during HILDCAA/HILDCAA ∗ occurrences between 1998 and 2007

2017 ◽  
Vol 60 (8) ◽  
pp. 1850-1865 ◽  
Author(s):  
Alan Prestes ◽  
Virginia Klausner ◽  
Arian Ojeda González ◽  
Silvio Leite Serra
Keyword(s):  
Solar Wind ◽  
Statistical Analysis ◽  
Geomagnetic Indices ◽  
Solar Wind Parameters

scholarly journals Wavelet Analysis on Solar Wind Parameters and Geomagnetic Indices

Solar Physics ◽  
2012 ◽  
Vol 280 (2) ◽  
pp. 623-640 ◽  
Author(s):  
C. Katsavrias ◽  
P. Preka-Papadema ◽  
X. Moussas
Keyword(s):  
Solar Wind ◽  
Wavelet Analysis ◽  
Geomagnetic Indices ◽  
Solar Wind Parameters

scholarly journals Extremely low geomagnetic activity during the recent deep solar cycle minimum

2011 ◽  
Vol 7 (S286) ◽  
pp. 200-209 ◽  
Author(s):  
E. Echer ◽  
B. T. Tsurutani ◽  
W. D. Gonzalez
Keyword(s):  
Solar Wind ◽  
Solar Cycle ◽  
Geomagnetic Activity ◽  
Solar Minimum ◽  
Solar Wind Speed ◽  
Sunspot Cycle ◽  
Cycle Minimum ◽  
Current Minimum ◽  
Solar Wind Parameters ◽  
Xix Century

AbstractThe recent solar minimum (2008-2009) was extreme in several aspects: the sunspot number, Rz, interplanetary magnetic field (IMF) magnitude Bo and solar wind speed Vsw were the lowest during the space era. Furthermore, the variance of the IMF southward Bz component was low. As a consequence of these exceedingly low solar wind parameters, there was a minimum in the energy transfer from solar wind to the magnetosphere, and the geomagnetic activity ap index reached extremely low levels. The minimum in geomagnetic activity was delayed in relation to sunspot cycle minimum. We compare the solar wind and geomagnetic activity observed in this recent minimum with previous solar cycle values during the space era (1964-2010). Moreover, the geomagnetic activity conditions during the current minimum are compared with long term variability during the period of available geomagnetic observations. The extremely low geomagnetic activity observed in this solar minimum was previously recorded only at the end of XIX century and at the beginning of the XX century, and this might be related to the Gleissberg (80-100 years) solar cycle.

scholarly journals Relationship between Solar Energetic Particles and Properties of Flares and CMEs: Statistical Analysis of Solar Cycle 23 Events

Solar Physics ◽  
2015 ◽  
Vol 290 (3) ◽  
pp. 841-874 ◽  
Author(s):  
M. Dierckxsens ◽  
K. Tziotziou ◽  
S. Dalla ◽  
I. Patsou ◽  
M. S. Marsh ◽  
...  
Keyword(s):  
Statistical Analysis ◽  
Solar Cycle ◽  
Energetic Particles ◽  
Solar Energetic Particles ◽  
Solar Cycle 23

Verifying the Relationship between Solar Neutrinos and Solar Wind for Solar Cycle 23

2019 ◽  
Vol 4 (1) ◽  
pp. 65-72
Author(s):  
Imad A. H. Al-Hayali ◽  
Wafaa H. A. Zaki ◽  
Shadan S. Salih
Keyword(s):  
Solar Wind ◽  
Solar Cycle ◽  
Solar Neutrinos ◽  
Solar Cycle 23 ◽  
The Relationship

Structure of solar-wind streams at the maximum of solar cycle 23

2005 ◽  
Vol 31 (8) ◽  
pp. 546-556 ◽  
Author(s):  
N. A. Lotova ◽  
K. V. Vladimirskii ◽  
V. N. Obridko ◽  
B. P. Filippov ◽  
O. A. Korelov
Keyword(s):  
Solar Wind ◽  
Solar Cycle ◽  
Solar Cycle 23
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