Results 21 to 30 of about 35,714 (290)

Active Regions and the Interplanetary Magnetic Field [PDF]

open access: yesSymposium - International Astronomical Union, 1968
The relation of solar active regions to the large-scale sector structure of the interplanetary field is discussed. In the winter of 1963–64 (observed by the satellite IMP-1) the plage density was greatest in the leading portion of the sectors and lesser in the trailing portion of the sectors. The boundaries of the sectors (places at which the direction
John M. Wilcox   +2 more
openaire   +1 more source

Correlation Between Monthly Cumulative Auroral Electrojet Indices, DST Index and Interplanetary Electric Field During Magnetic Storms [PDF]

open access: yesJournal of Astronomy and Space Sciences, 2005
Magnetospheric substorms occur frequently during magnetic storms, suggesting that the two phenomena are closely associated. We can investigate the relation between magnetospheric substorms and magnetic storms by examining the correlation between AE and ...
Yoon-Kyung Park   +2 more
doaj   +1 more source

Geoeffectiveness of Interplanetary Alfvén Waves. I. Magnetopause Magnetic Reconnection and Directly Driven Substorms

open access: yesThe Astrophysical Journal, 2023
In particular during the descending phase of the solar cycle, Alfvén waves in the high-speed solar wind streams are a major form of interplanetary disturbances.
Lei Dai   +8 more
doaj   +1 more source

Lessons from a career in space physics

open access: yesFrontiers in Astronomy and Space Sciences, 2022
Frameworks for describing magnetospheric substorms are as good as the data on which they are based. While disturbances in the ionosphere are well described by existing data bases, the plasma and field data acquired by satellites in the magnetosphere are ...
Gordon Rostoker
doaj   +1 more source

Solar Rotational Oscillation and Its Subharmonics in Solar Wind Plasma Field, Geomagnetic, and Cosmic Ray Intensity Indicator in the Solar Cycle 24/25 Minimum

open access: yesEarth and Space Science, 2020
To study synodic period and its subharmonics, we have utilized hourly average data of solar wind plasma field, geomagnetic index, and galactic cosmic ray intensity along with 5 min average data of selected solar wind field parameters during the recent ...
Y. P. Singh
doaj   +1 more source

Analysis of cosmic ray dynamics and ionospheric parameters during increased solar activity and magnetic storms [PDF]

open access: yesE3S Web of Conferences, 2019
Based on the ground station data, the paper investigates the dynamics of space rays and ionospheric parameters during strong and moderate magnetic storms 2018.
Mandrikova Oksana   +2 more
doaj   +1 more source

Revised time-of-flight calculations for high-latitude geomagnetic pulsations using a realistic magnetospheric magnetic field model [PDF]

open access: yes, 2005
We present a simple time-of-flight analysis of Alfvén pulsations standing on closed terrestrial magnetic field lines. The technique employed in this study in order to calculate the characteristic period of such oscillations builds upon earlier time-of ...
Waters, C. L.   +2 more
core   +1 more source

32. Interplanetary magnetic field [PDF]

open access: yesSymposium - International Astronomical Union, 1958
The magnetic field outside the sun (interplanetary magnetic field) is certainly far from a dipole field. A model of it has recently been suggested (Tellus,8, 1, 1956). This model is in agreement with cosmic ray and magnetic storm data and reconcilable with the coronal ray structure. Some possibilities to check the model are discussed.
openaire   +1 more source

Magnetospheric access for solar protons during the January 2005 SEP event

open access: yesJournal of Space Weather and Space Climate, 2018
The early phase of the extraordinary solar energetic particle 20 January, 2005 event having the highest peak flux of any SEP in the past 50 years of protons with energies > 100 MeV is studied.
Kalegaev Vladimir V.   +3 more
doaj   +1 more source

Propagation of low frequency geomagnetic field fluctuations in Antarctica: comparison between two polar cap stations [PDF]

open access: yesAnnales Geophysicae, 2007
We conduct a statistical analysis of the coherence and phase difference of low frequency geomagnetic fluctuations between two Antarctic stations, Mario Zucchelli Station (geographic coordinates: 74.7° S, 164.1° E; corrected geomagnetic ...
L. Santarelli, S. Lepidi, L. Cafarella
doaj   +1 more source

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