The evolution of vector magnetic field associated with major flares in NOAA AR10656

Shuo Wang; Yuanyong Deng; Rajmal Jain; Vasyl Yurchyshyn; Haimin Wang; Yuanyuan Liu; Zhiliang Yang

doi:10.1007/s12036-008-0007-0

The evolution of vector magnetic field associated with major flares in NOAA AR10656

Shuo Wang, Yuanyong Deng, Rajmal Jain, Vasyl Yurchyshyn, Haimin Wang, Yuanyuan Liu, Zhiliang Yang

Research output: Contribution to journal › Article › peer-review

Abstract

In this paper, we study the evolution of vector magnetic field of AR 10656 by using the observations of Huairou Solar Observing Station (HSOS, China) and Big Bear Solar Observatory (BBSO, USA). The magnetic flux emergence and cancellation, and thus, magnetic nonpotential changes, are associated with the major flares in this active region. Compared with some other super-active regions, the evolution of magnetic morphologies and non-potentialities are relatively gradual, and thus the energy transportation and release are relatively slow. This gradual process may result in the recurrent flares of AR 10656.

Original language	English (US)
Pages (from-to)	57-61
Number of pages	5
Journal	Journal of Astrophysics and Astronomy
Volume	29
Issue number	1-2
DOIs	https://doi.org/10.1007/s12036-008-0007-0
State	Published - 2008

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics
Space and Planetary Science

Keywords

Evolution
Flares
Magnetic field

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10.1007/s12036-008-0007-0

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title = "The evolution of vector magnetic field associated with major flares in NOAA AR10656",

abstract = "In this paper, we study the evolution of vector magnetic field of AR 10656 by using the observations of Huairou Solar Observing Station (HSOS, China) and Big Bear Solar Observatory (BBSO, USA). The magnetic flux emergence and cancellation, and thus, magnetic nonpotential changes, are associated with the major flares in this active region. Compared with some other super-active regions, the evolution of magnetic morphologies and non-potentialities are relatively gradual, and thus the energy transportation and release are relatively slow. This gradual process may result in the recurrent flares of AR 10656.",

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author = "Shuo Wang and Yuanyong Deng and Rajmal Jain and Vasyl Yurchyshyn and Haimin Wang and Yuanyuan Liu and Zhiliang Yang",

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language = "English (US)",

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T1 - The evolution of vector magnetic field associated with major flares in NOAA AR10656

AU - Wang, Shuo

AU - Deng, Yuanyong

AU - Jain, Rajmal

AU - Yurchyshyn, Vasyl

AU - Wang, Haimin

AU - Liu, Yuanyuan

AU - Yang, Zhiliang

PY - 2008

Y1 - 2008

N2 - In this paper, we study the evolution of vector magnetic field of AR 10656 by using the observations of Huairou Solar Observing Station (HSOS, China) and Big Bear Solar Observatory (BBSO, USA). The magnetic flux emergence and cancellation, and thus, magnetic nonpotential changes, are associated with the major flares in this active region. Compared with some other super-active regions, the evolution of magnetic morphologies and non-potentialities are relatively gradual, and thus the energy transportation and release are relatively slow. This gradual process may result in the recurrent flares of AR 10656.

AB - In this paper, we study the evolution of vector magnetic field of AR 10656 by using the observations of Huairou Solar Observing Station (HSOS, China) and Big Bear Solar Observatory (BBSO, USA). The magnetic flux emergence and cancellation, and thus, magnetic nonpotential changes, are associated with the major flares in this active region. Compared with some other super-active regions, the evolution of magnetic morphologies and non-potentialities are relatively gradual, and thus the energy transportation and release are relatively slow. This gradual process may result in the recurrent flares of AR 10656.

KW - Evolution

KW - Flares

KW - Magnetic field

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JF - Journal of Astrophysics and Astronomy

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The evolution of vector magnetic field associated with major flares in NOAA AR10656

Abstract

All Science Journal Classification (ASJC) codes

Keywords

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