Standard

Reconstruction of the IMF polarity using midlatitude geomagnetic observations in the nineteenth century. / Vokhmyanin, M.V.; Ponyavin, D.I.

в: JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Том 121, 2016.

Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование

Harvard

Vokhmyanin, MV & Ponyavin, DI 2016, 'Reconstruction of the IMF polarity using midlatitude geomagnetic observations in the nineteenth century', JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Том. 121. https://doi.org/10.1002/2016JA023138

APA

Vokhmyanin, M. V., & Ponyavin, D. I. (2016). Reconstruction of the IMF polarity using midlatitude geomagnetic observations in the nineteenth century. JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 121. https://doi.org/10.1002/2016JA023138

Vancouver

Vokhmyanin MV, Ponyavin DI. Reconstruction of the IMF polarity using midlatitude geomagnetic observations in the nineteenth century. JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS. 2016;121. https://doi.org/10.1002/2016JA023138

Author

Vokhmyanin, M.V. ; Ponyavin, D.I. / Reconstruction of the IMF polarity using midlatitude geomagnetic observations in the nineteenth century. в: JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS. 2016 ; Том 121.

BibTeX

@article{c888aeefb6524f40b3676372f7f386c4,
title = "Reconstruction of the IMF polarity using midlatitude geomagnetic observations in the nineteenth century",
abstract = "The interplanetary magnetic field (IMF) By component affects the configuration of field-aligned currents (FAC) whose geomagnetic response is observed from high to low latitudes. The ground magnetic perturbations induced by FACs are opposite on the dawn and dusk sides and depend upon the IMF By polarity. Based on the multilinear regression analysis, we show that this effect is presented at the mid-latitude observatories, Niemegk and Arti, in the X and Y components of the geomagnetic field. This allows us to infer the IMF sector structure from the old geomagnetic records made at Ekaterinburg and Potsdam since 1850 and 1890, respectively. Geomagnetic data from various stations provide proxies of the IMF polarity which coincide for the most part of the 19th and 20th centuries. This supports their reliabilities and makes them suitable for studying the large-scale IMF sector structure in the past.",
keywords = "Interplanetary Magnetic Field, Geomagnetic variations, IMF polarity, IMF reconstruction, Long-term",
author = "M.V. Vokhmyanin and D.I. Ponyavin",
year = "2016",
doi = "10.1002/2016JA023138",
language = "English",
volume = "121",
journal = "Journal of Geophysical Research: Biogeosciences",
issn = "0148-0227",
publisher = "American Geophysical Union",

}

RIS

TY - JOUR

T1 - Reconstruction of the IMF polarity using midlatitude geomagnetic observations in the nineteenth century

AU - Vokhmyanin, M.V.

AU - Ponyavin, D.I.

PY - 2016

Y1 - 2016

N2 - The interplanetary magnetic field (IMF) By component affects the configuration of field-aligned currents (FAC) whose geomagnetic response is observed from high to low latitudes. The ground magnetic perturbations induced by FACs are opposite on the dawn and dusk sides and depend upon the IMF By polarity. Based on the multilinear regression analysis, we show that this effect is presented at the mid-latitude observatories, Niemegk and Arti, in the X and Y components of the geomagnetic field. This allows us to infer the IMF sector structure from the old geomagnetic records made at Ekaterinburg and Potsdam since 1850 and 1890, respectively. Geomagnetic data from various stations provide proxies of the IMF polarity which coincide for the most part of the 19th and 20th centuries. This supports their reliabilities and makes them suitable for studying the large-scale IMF sector structure in the past.

AB - The interplanetary magnetic field (IMF) By component affects the configuration of field-aligned currents (FAC) whose geomagnetic response is observed from high to low latitudes. The ground magnetic perturbations induced by FACs are opposite on the dawn and dusk sides and depend upon the IMF By polarity. Based on the multilinear regression analysis, we show that this effect is presented at the mid-latitude observatories, Niemegk and Arti, in the X and Y components of the geomagnetic field. This allows us to infer the IMF sector structure from the old geomagnetic records made at Ekaterinburg and Potsdam since 1850 and 1890, respectively. Geomagnetic data from various stations provide proxies of the IMF polarity which coincide for the most part of the 19th and 20th centuries. This supports their reliabilities and makes them suitable for studying the large-scale IMF sector structure in the past.

KW - Interplanetary Magnetic Field

KW - Geomagnetic variations

KW - IMF polarity

KW - IMF reconstruction

KW - Long-term

U2 - 10.1002/2016JA023138

DO - 10.1002/2016JA023138

M3 - Article

VL - 121

JO - Journal of Geophysical Research: Biogeosciences

JF - Journal of Geophysical Research: Biogeosciences

SN - 0148-0227

ER -

ID: 7617316