Comparison of heliospheric conditions near the earth during four recent solar maxima

A. V. Dmitriev; I. S. Veselovsky; A. V. Suvorova

doi:10.1016/j.asr.2004.06.018

Comparison of heliospheric conditions near the earth during four recent solar maxima

A. V. Dmitriev, I. S. Veselovsky, A. V. Suvorova

太空科學與工程學系

研究成果: 雜誌貢獻 › 期刊論文 › 同行評審

5 引文斯高帕斯（Scopus）

摘要

Statistical properties of the daily averaged values of the solar activity (sunspot numbers, total solar irradiance and 10.7 cm radio emission indices), the solar wind plasma and the interplanetary magnetic field parameters near the Earth's orbit are investigated for a period from 1964 to 2002 covering the maxima of four solar cycles from 20th to 23rd. Running half-year averages show significant solar cycle variations in the solar activity indices but only marginal and insignificant changes in comparison with background fluctuations for heliospheric bulk plasma and magnetic field parameters. The current 23rd cycle maximum is weaker than 21st and 22nd maxima, but slightly stronger than 20th cycle in most of solar and heliospheric manifestations.

原文	???core.languages.en_GB???
頁（從 - 到）	2339-2344
頁數	6
期刊	Advances in Space Research
卷	36
發行號	12
DOIs	https://doi.org/10.1016/j.asr.2004.06.018
出版狀態	已出版 - 2005

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10.1016/j.asr.2004.06.018

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title = "Comparison of heliospheric conditions near the earth during four recent solar maxima",

abstract = "Statistical properties of the daily averaged values of the solar activity (sunspot numbers, total solar irradiance and 10.7 cm radio emission indices), the solar wind plasma and the interplanetary magnetic field parameters near the Earth's orbit are investigated for a period from 1964 to 2002 covering the maxima of four solar cycles from 20th to 23rd. Running half-year averages show significant solar cycle variations in the solar activity indices but only marginal and insignificant changes in comparison with background fluctuations for heliospheric bulk plasma and magnetic field parameters. The current 23rd cycle maximum is weaker than 21st and 22nd maxima, but slightly stronger than 20th cycle in most of solar and heliospheric manifestations.",

keywords = "Earth heliospheric conditions, Interplanetary magnetic field, Solar activity, Solar maxima, Solar wind, Space weather",

author = "Dmitriev, {A. V.} and Veselovsky, {I. S.} and Suvorova, {A. V.}",

note = "Funding Information: This work is supported by the Grants NSC-91-2811-M-008-010, RFBR 01-02-16579 and 00-15-96623, INTAS-ESA 99-00727, INTAS 00-752, the Programs “Universities of Russia” and “Astronomia”. The authors are grateful to the referees for their comments on the paper. ",

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doi = "10.1016/j.asr.2004.06.018",

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volume = "36",

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TY - JOUR

T1 - Comparison of heliospheric conditions near the earth during four recent solar maxima

AU - Dmitriev, A. V.

AU - Veselovsky, I. S.

AU - Suvorova, A. V.

N1 - Funding Information: This work is supported by the Grants NSC-91-2811-M-008-010, RFBR 01-02-16579 and 00-15-96623, INTAS-ESA 99-00727, INTAS 00-752, the Programs “Universities of Russia” and “Astronomia”. The authors are grateful to the referees for their comments on the paper.

PY - 2005

Y1 - 2005

N2 - Statistical properties of the daily averaged values of the solar activity (sunspot numbers, total solar irradiance and 10.7 cm radio emission indices), the solar wind plasma and the interplanetary magnetic field parameters near the Earth's orbit are investigated for a period from 1964 to 2002 covering the maxima of four solar cycles from 20th to 23rd. Running half-year averages show significant solar cycle variations in the solar activity indices but only marginal and insignificant changes in comparison with background fluctuations for heliospheric bulk plasma and magnetic field parameters. The current 23rd cycle maximum is weaker than 21st and 22nd maxima, but slightly stronger than 20th cycle in most of solar and heliospheric manifestations.

AB - Statistical properties of the daily averaged values of the solar activity (sunspot numbers, total solar irradiance and 10.7 cm radio emission indices), the solar wind plasma and the interplanetary magnetic field parameters near the Earth's orbit are investigated for a period from 1964 to 2002 covering the maxima of four solar cycles from 20th to 23rd. Running half-year averages show significant solar cycle variations in the solar activity indices but only marginal and insignificant changes in comparison with background fluctuations for heliospheric bulk plasma and magnetic field parameters. The current 23rd cycle maximum is weaker than 21st and 22nd maxima, but slightly stronger than 20th cycle in most of solar and heliospheric manifestations.

KW - Earth heliospheric conditions

KW - Interplanetary magnetic field

KW - Solar activity

KW - Solar maxima

KW - Solar wind

KW - Space weather

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U2 - 10.1016/j.asr.2004.06.018

DO - 10.1016/j.asr.2004.06.018

M3 - 期刊論文

AN - SCOPUS:28044457212

SN - 0273-1177

VL - 36

SP - 2339

EP - 2344

JO - Advances in Space Research

JF - Advances in Space Research

IS - 12

ER -

Comparison of heliospheric conditions near the earth during four recent solar maxima

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