Solar Multipolar Moments: an up-to-date Pedagogical Approach. Implications for Stellar Properties. Part I: an Analytical Overview (TUTORIAL)

J. P. Rozelot; A. G. Kosovichev; A. Kilcik; S. Sahin; Y. Xu; J. Javaraiah; K. Georgieva; A. Özgüҫ

Solar Multipolar Moments: an up-to-date Pedagogical Approach. Implications for Stellar Properties. Part I: an Analytical Overview (TUTORIAL)

J. P. Rozelot, A. G. Kosovichev, A. Kilcik, S. Sahin, Y. Xu, J. Javaraiah, K. Georgieva, A. Özgüҫ

Research output: Contribution to journal › Conference article › peer-review

Abstract

Solar gravitational multipolar moments have not been yet extensively analyzed. However, they are at the crossroads of solar physics, solar astrometry, celestial mechanics and General Relativity. Their values reflect the physics of solar models: non-rigid rotation, solar latitudinal rotation, solar- core properties, solar-cycle variations and structure evolution. Their temporal variations are still often neglected; they are yet an essential aspect for constraining solar-cycle modeling or solar-evolution theories. They induced planet-planet inclinations in multitransiting systems gravitating in the neighboring of a star, leading to key issues future studies. This paper is devoted to an analytical analysis; a second part will address an helioseismology analysis.

Original language	English (US)
Pages (from-to)	1-24
Number of pages	24
Journal	Workshop Solar Influences on the Magnetosphere, Ionosphere and Atmosphere
State	Published - 2020
Event	12th Workshop on Solar Influences on the Magnetosphere, Ionosphere and Atmosphere, 2020 - Primorsko, Bulgaria Duration: Jun 3 2020 → Jun 7 2020

All Science Journal Classification (ASJC) codes

Earth and Planetary Sciences (miscellaneous)
Atmospheric Science
Geophysics
Space and Planetary Science

Cite this

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title = "Solar Multipolar Moments: an up-to-date Pedagogical Approach. Implications for Stellar Properties. Part I: an Analytical Overview (TUTORIAL)",

abstract = "Solar gravitational multipolar moments have not been yet extensively analyzed. However, they are at the crossroads of solar physics, solar astrometry, celestial mechanics and General Relativity. Their values reflect the physics of solar models: non-rigid rotation, solar latitudinal rotation, solar- core properties, solar-cycle variations and structure evolution. Their temporal variations are still often neglected; they are yet an essential aspect for constraining solar-cycle modeling or solar-evolution theories. They induced planet-planet inclinations in multitransiting systems gravitating in the neighboring of a star, leading to key issues future studies. This paper is devoted to an analytical analysis; a second part will address an helioseismology analysis.",

author = "Rozelot, {J. P.} and Kosovichev, {A. G.} and A. Kilcik and S. Sahin and Y. Xu and J. Javaraiah and K. Georgieva and A. {\"O}zg{\"u}ҫ",

note = "Publisher Copyright: {\textcopyright} 2020, Space Research and Technologies Institute, Bulgarian Academy of Sciences. All rights reserved.; 12th Workshop on Solar Influences on the Magnetosphere, Ionosphere and Atmosphere, 2020 ; Conference date: 03-06-2020 Through 07-06-2020",

year = "2020",

language = "English (US)",

pages = "1--24",

journal = "Workshop Solar Influences on the Magnetosphere, Ionosphere and Atmosphere",

issn = "2367-7570",

publisher = "Space Research and Technologies Institute, Bulgarian Academy of Sciences",

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TY - JOUR

T1 - Solar Multipolar Moments

T2 - 12th Workshop on Solar Influences on the Magnetosphere, Ionosphere and Atmosphere, 2020

AU - Rozelot, J. P.

AU - Kosovichev, A. G.

AU - Kilcik, A.

AU - Sahin, S.

AU - Xu, Y.

AU - Javaraiah, J.

AU - Georgieva, K.

AU - Özgüҫ, A.

PY - 2020

Y1 - 2020

N2 - Solar gravitational multipolar moments have not been yet extensively analyzed. However, they are at the crossroads of solar physics, solar astrometry, celestial mechanics and General Relativity. Their values reflect the physics of solar models: non-rigid rotation, solar latitudinal rotation, solar- core properties, solar-cycle variations and structure evolution. Their temporal variations are still often neglected; they are yet an essential aspect for constraining solar-cycle modeling or solar-evolution theories. They induced planet-planet inclinations in multitransiting systems gravitating in the neighboring of a star, leading to key issues future studies. This paper is devoted to an analytical analysis; a second part will address an helioseismology analysis.

AB - Solar gravitational multipolar moments have not been yet extensively analyzed. However, they are at the crossroads of solar physics, solar astrometry, celestial mechanics and General Relativity. Their values reflect the physics of solar models: non-rigid rotation, solar latitudinal rotation, solar- core properties, solar-cycle variations and structure evolution. Their temporal variations are still often neglected; they are yet an essential aspect for constraining solar-cycle modeling or solar-evolution theories. They induced planet-planet inclinations in multitransiting systems gravitating in the neighboring of a star, leading to key issues future studies. This paper is devoted to an analytical analysis; a second part will address an helioseismology analysis.

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M3 - Conference article

AN - SCOPUS:85216250208

SN - 2367-7570

SP - 1

EP - 24

JO - Workshop Solar Influences on the Magnetosphere, Ionosphere and Atmosphere

JF - Workshop Solar Influences on the Magnetosphere, Ionosphere and Atmosphere

Y2 - 3 June 2020 through 7 June 2020

ER -

Solar Multipolar Moments: an up-to-date Pedagogical Approach. Implications for Stellar Properties. Part I: an Analytical Overview (TUTORIAL)

Abstract

All Science Journal Classification (ASJC) codes

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