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Biological Effects of Magnetic Storms and ELF Magnetic Fields [PDF]

open access: yesBiology, 2023
Magnetic fields are a constant and essential part of our environment. The main components of ambient magnetic fields are the constant part of the geomagnetic field, its fluctuations caused by magnetic storms, and man-made magnetic fields.
Ruslan M. Sarimov   +2 more
doaj   +2 more sources

Specific interplanetary conditions for CIR-, Sheath-, and ICME-induced geomagnetic storms obtained by double superposed epoch analysis [PDF]

open access: yesAnnales Geophysicae, 2010
A comparison of specific interplanetary conditions for 798 magnetic storms with Dst <−50 nT during 1976–2000 was made on the basis of the OMNI archive data.
Yu. I. Yermolaev   +3 more
doaj   +5 more sources

Study on the Thermospheric Density Distribution Pattern during Geomagnetic Activity

open access: yesApplied Sciences, 2023
The atmospheric density of the thermosphere is a fundamental parameter for spacecraft launch and orbit control. Under magnetic storm conditions, the thermospheric atmospheric density experiences significant fluctuations, which have a negative impact on ...
Lirong Yin   +6 more
doaj   +1 more source

Dynamics and spatio-temporal distribution of geomagnetic disturbances during periods of increased solar activity and magnetic storms [PDF]

open access: yesE3S Web of Conferences, 2020
A detailed spatio-temporal analysis of magnetic data was performed during the periods of magnetic storms on October 02, 2013 and September 27, 2019 based on measurements of the station network.
Mandrikova Oksana, Rodomanskay Anastasia
doaj   +1 more source

Relationship Between Relativistic Electron Events Magnetic Storms, and Magnetic Substorms [PDF]

open access: yesJournal of Astronomy and Space Sciences, 2003
This paper reports a statistical study on the relationship between relativistic electron events(REE), magnetic storms, and substorms. We have used magnetic storm events that occurred between 1996 and 1998, and have classified them into two groups, (i ...
Jung-A Hwang   +3 more
doaj   +1 more source

Variation of Magnetic Field (By , Bz) Polarity and Statistical Analysis of Solar Wind Parameters during the Magnetic Storm Period [PDF]

open access: yesJournal of Astronomy and Space Sciences, 2011
It is generally believed that the occurrence of a magnetic storm depends upon the solar wind conditions, particularly the southward interplanetary magnetic field (IMF) component. To understand the relationship between solar wind parameters and magnetic
Ga-Hee Moon
doaj   +1 more source

Seasonal variations in the occurrence of geomagnetic storms [PDF]

open access: yesAnnales Geophysicae, 1996
Seasonal variations in the onset of magnetic storms are investigated. For the purposes of this study storms have been defined as events in which Dst falls below –50 nT for at least four consecutive hours.
J. R. Taylor, M. Lester, T. K. Yeoman
doaj   +1 more source

Differences in the response to CME and CIR drivers of geomagnetic disturbances

open access: yesSolar-Terrestrial Physics, 2023
Utilizing 1-minute resolution data on the geomagnetic indices SYM-H, AE, solar wind parameters (velocity Vsw and density Np), and z-component Bz of the interplanetary magnetic field (IMF) during solar cycles 23 and 24, we have statistically analyzed the ...
Namuun B.   +3 more
doaj   +1 more source

Mercury's magnetospheric substorm and storm

open access: yes地球与行星物理论评, 2022
Magnetospheric substorms and magnetic storms are explosive energy storage and release processes occurring during the interactions between the solar wind and planetary magnetospheres. They are accompanied by complex plasma dynamics processes and they have
Jiutong Zhao, Weijie Sun, Qiugang Zong
doaj   +1 more source

ANALYSIS OF THE MAGNETIC STORMS CATALOG FOR MONITORING RADIO SOURCE FLUXE DATA WITH THE URAN-4 RADIO TELESCOPE IN THE ODESA MAGNETIC ANOMALY ZONE [PDF]

open access: yesRadio Physics and Radio Astronomy, 2020
Purpose: Compilation of a digital catalog of magnetic storms in the Odesa magnetic anomaly zone in order to find the reasons for possible changes in the radiation fluxes of cosmic radio sources, according to observations at the URAN-4 radio telescope.
L. I. Sobitnyak   +6 more
doaj   +1 more source

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