3.9 Article

Long-term variations of solar magnetic fields derived from geomagnetic data

Journal

GEOMAGNETISM AND AERONOMY
Volume 53, Issue 7, Pages 852-856

Publisher

MAIK NAUKA/INTERPERIODICA/SPRINGER
DOI: 10.1134/S0016793213070062

Keywords

-

Ask authors/readers for more resources

There are limited homogeneous instrumental observations of the sunspot magnetic fields, but the Earth is a sort of a probe reacting to interplanetary disturbances which are manifestation of the solar magnetic fields. We find correlations between some parameters of geomagnetic activity (the geomagnetic activity flooraEurothe minimum value under which the geomagnetic activity cannot fall in a sunspot cycle, and the rate of increase of the geomagnetic activity with increasing sunspot number), and sunspot magnetic fields (the sunspot magnetic field in the cycle minimum, and the rate of increase of the sunspot magnetic field from cycle minimum to cycle maximum). Based on these correlations we are able to reconstruct the sunspot magnetic fields in sunspot minima and maxima since sunspot cycle 9 (mid 19th century).

Authors

I am an author on this paper
Click your name to claim this paper and add it to your profile.

Reviews

Primary Rating

3.9
Not enough ratings

Secondary Ratings

Novelty
-
Significance
-
Scientific rigor
-
Rate this paper

Recommended

Article Geochemistry & Geophysics

Analysis of Oscillatory Modes of the Magnetic Field of Solar Facular Formations

P. V. Strekalova, Yu. A. Nagovitsyn, V. V. Smirnova

GEOMAGNETISM AND AERONOMY (2018)

Article Geochemistry & Geophysics

Reconstruction of the Production Rate of Cosmogenic 14C in the Earth's Atmosphere for 17000-5000 BC

I. V. Kudryavtsev, D. M. Volobuev, V. A. Dergachev, Yu. A. Nagovitsyn, M. G. Ogurtsov

GEOMAGNETISM AND AERONOMY (2018)

Article Astronomy & Astrophysics

Refinement of the Gnevyshev-Waldmeier Rule Based on a 140-Year Series of Observations

Yu. A. Nagovitsyn, V. G. Ivanov, N. N. Skorbezh

ASTRONOMY LETTERS-A JOURNAL OF ASTRONOMY AND SPACE ASTROPHYSICS (2019)

Article Astronomy & Astrophysics

The effect of telescope aperture, scattered light and human vision on early measurements of sunspot and group numbers

Nina V. Karachik, Alexei A. Pevtsov, Yury A. Nagovitsyn

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2019)

Article Astronomy & Astrophysics

Features of the Gnevyshev-Waldmeier Rule for Various Lifetimes and Areas of Sunspot Groups

Yu. A. Nagovitsyn, V. G. Ivanov, A. A. Osipova

ASTRONOMY LETTERS-A JOURNAL OF ASTRONOMY AND SPACE ASTROPHYSICS (2019)

Article Astronomy & Astrophysics

Variations of interplanetary magnetic field on various long time-scales

Yury A. Nagovitsyn, Aleksandra A. Osipova

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2020)

Article Astronomy & Astrophysics

Tilt angle and lifetime of sunspot groups

Yury A. Nagovitsyn, Aleksandra A. Osipova, Alexei A. Pevtsov

Summary: The study revealed that the tilt angles of solar active regions exhibit non-linear changes with latitude, with significant differences between large long-living groups and small short-living groups. This implies potential differences in the physical properties and formation mechanisms of the two populations of solar groups.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2021)

Article Astronomy & Astrophysics

Generative Indices of Sunspot Solar Activity: 145-Year Composite Series

Y. A. Nagovitsyn, A. A. Osipova, E. Y. Nagovitsyna

Summary: Traditional indices describe solar activity while generative indices aim to describe the productivity of the solar dynamo by focusing on maximum magnetic region areas. This study compiles a unified 145-year series of generative indices using sunspot group data from two archives, revealing a 50-year variation in several indices and a potential additional secular cycle on the Sun.

SOLAR PHYSICS (2021)

Article Astronomy & Astrophysics

Average annual total sunspot area in the last 410 yr: the most probable values and limits of their uncertainties

Yury A. Nagovitsyn, Aleksandra A. Osipova

Summary: The aim of this work is to establish a long (410-yr) series of average annual total sunspot areas and analyze the relationship and periodicity between different sunspot indices for reconstruction.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2021)

Review Astronomy & Astrophysics

Long-term studies of photospheric magnetic fields on the Sun

Alexei A. Pevtsov, Luca Bertello, Yury A. Nagovitsyn, Andrey G. Tlatov, Valery V. Pipin

Summary: This study reviews the history of solar magnetic field observations and emphasizes the importance of historical data in detecting and understanding long-term trends in solar activity. Research demonstrates the value of historical data through studies of active region tilt and magnetic field evolution, revealing that the magnetic properties of sunspots have remained consistent over the past century.

JOURNAL OF SPACE WEATHER AND SPACE CLIMATE (2021)

Article Astronomy & Astrophysics

Duffing Oscillator Model of Solar Cycles

Yury A. Nagovitsyn, Alexei A. Pevtsov

ASTROPHYSICAL JOURNAL LETTERS (2020)

Article Geochemistry & Geophysics

Solar Activity from the Mid-Second Millennium BC to the First Millennium AD Based on Radiocarbon Data

V. A. Dergachev, I. Kudryavtseva, Yu A. Nagovitsyn

GEOMAGNETISM AND AERONOMY (2019)

Article Geochemistry & Geophysics

The Gnevyshev-Ohl Rule and Two Sunspot Group Populations

Yu. A. Nagovitsyn, A. A. Osipova

GEOMAGNETISM AND AERONOMY (2018)

Article Geochemistry & Geophysics

Some Features of the Two Sunspot Group Populations' Properties

Yu. A. Nagovitsyn, A. A. Pevtsov, A. A. Osipova, V. G. Ivanov

GEOMAGNETISM AND AERONOMY (2018)

Article Astronomy & Astrophysics

Bi-lognormal Distribution of Sunspot Group Areas

Yury A. Nagovitsyn, Alexei A. Pevtsov

Summary: The study analyzed the distribution of sunspot areas based on observational data, introducing a precision randomization method to account for measurement uncertainties. It confirmed the presence of two distinct components in the distribution of sunspots and showed that the area distribution can be described by the sum of two lognormal distributions. Additionally, it demonstrated a correlation between the area of main spots and the total area of sunspot groups.

ASTROPHYSICAL JOURNAL (2021)

No Data Available