Solar Intranetwork Magnetic Elements: Flux Distributions
The current study aims at quantifying the flux distributions of solar intranetwork (IN) magnetic field based on the data taken in four quiet and two enhanced network areas with the Narrow-band Filter Imager of the Solar Optical Telescope on board the Hinode satellite. More than 14000 IN elements and...
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| Published in | Solar physics Vol. 283; no. 2; pp. 273 - 282 |
|---|---|
| Main Authors | , , |
| Format | Journal Article |
| Language | English |
| Published |
Dordrecht
Springer Netherlands
01.04.2013
Springer Nature B.V |
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| Abstract | The current study aims at quantifying the flux distributions of solar intranetwork (IN) magnetic field based on the data taken in four quiet and two enhanced network areas with the Narrow-band Filter Imager of the Solar Optical Telescope on board the
Hinode
satellite. More than 14000 IN elements and 3000 NT elements were visually identified. They exhibit a flux distribution function with a peak at 1 – 3×10
16
Mx (maxwell) and 2 – 3×10
17
Mx, respectively. We found that the IN elements contribute approximately to 52 % of the total flux and an average flux density of 12.4 gauss of the quiet region at any given time. By taking the lifetime of IN elements of about 3 min (Zhou
et al.
,
Solar Phys.
267
, 63,
2010
) into account, the IN fields are estimated to have total contributions to the solar magnetic flux up to 3.8×10
26
Mx per day. No fundamental distinction can be identified in IN fields between the quiet and enhanced network areas. |
|---|---|
| AbstractList | The current study aims at quantifying the flux distributions of solar intranetwork (IN) magnetic field based on the data taken in four quiet and two enhanced network areas with the Narrow-band Filter Imager of the Solar Optical Telescope on board the Hinode satellite. More than 14000Â IN elements and 3000Â NT elements were visually identified. They exhibit a flux distribution function with a peak at 1â[euro][per thousand]â[euro]"â[euro][per thousand]3Ã--10^sup 16^Â Mx (maxwell) and 2â[euro][per thousand]â[euro]"â[euro][per thousand]3Ã--10^sup 17^Â Mx, respectively. We found that the IN elements contribute approximately to 52Â % of the total flux and an average flux density of 12.4 gauss of the quiet region at any given time. By taking the lifetime of IN elements of about 3 min (Zhou et al., Solar Phys. 267, 63, 2010 ) into account, the IN fields are estimated to have total contributions to the solar magnetic flux up to 3.8Ã--10^sup 26^ Mx per day. No fundamental distinction can be identified in IN fields between the quiet and enhanced network areas.[PUBLICATION ABSTRACT] The current study aims at quantifying the flux distributions of solar intranetwork (IN) magnetic field based on the data taken in four quiet and two enhanced network areas with the Narrow-band Filter Imager of the Solar Optical Telescope on board the Hinode satellite. More than 14000 IN elements and 3000 NT elements were visually identified. They exhibit a flux distribution function with a peak at 1 – 3×10 16 Mx (maxwell) and 2 – 3×10 17 Mx, respectively. We found that the IN elements contribute approximately to 52 % of the total flux and an average flux density of 12.4 gauss of the quiet region at any given time. By taking the lifetime of IN elements of about 3 min (Zhou et al. , Solar Phys. 267 , 63, 2010 ) into account, the IN fields are estimated to have total contributions to the solar magnetic flux up to 3.8×10 26 Mx per day. No fundamental distinction can be identified in IN fields between the quiet and enhanced network areas. |
| Author | Jin, Chunlan Wang, Jingxiu Zhou, Guiping |
| Author_xml | – sequence: 1 givenname: Guiping surname: Zhou fullname: Zhou, Guiping email: gpzhou@nao.cas.cn organization: Key Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of Sciences – sequence: 2 givenname: Jingxiu surname: Wang fullname: Wang, Jingxiu organization: Key Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of Sciences – sequence: 3 givenname: Chunlan surname: Jin fullname: Jin, Chunlan organization: Key Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of Sciences |
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| References_xml | – reference: ShimizuT.NagataS.TsunetaS.TarbellT.EdwardsC.ShineR.Solar Phys.20082492212008SoPh..249..221S10.1007/s11207-007-9053-z – reference: JinC.L.WangJ.X.XieZ.X.Solar Phys.2012280512012SoPh..280...51J10.1007/s11207-012-0050-5 – reference: HartjB.KneerF.Astron. Astrophys.20023852642002A&A...385..264H10.1051/0004-6361:20020081 – reference: Trujillo BuenoJ.ShchukinaN.Asensio RamosA.Nature20044303262004Natur.430..326T10.1038/nature02669 – reference: ParkerE.N.Astrophys. J.19913727191991ApJ...372..719P10.1086/170015 – reference: ZhouG.P.WangJ.X.JinC.L.Solar Phys.2010267632010SoPh..267...63Z10.1007/s11207-010-9641-1 – reference: TsunetaS.IchimotoK.KatsukawaY.NagataS.OtsuboM.ShimizuT.Solar Phys.20082491672008SoPh..249..167T10.1007/s11207-008-9174-z – reference: VöglerA.ShelyagS.SchüsslerM.CattaneoF.EmonetT.LindeT.Astron. Astrophys.20054293352005A&A...429..335V10.1051/0004-6361:20041507 – reference: Domínguez CerdeñaI.Sánchez AlmeidaJ.KneerF.Astrophys. 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| Snippet | The current study aims at quantifying the flux distributions of solar intranetwork (IN) magnetic field based on the data taken in four quiet and two enhanced... |
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| SubjectTerms | Astrophysics and Astroparticles Atmospheric Sciences Fluctuations Magnetic fields Physics Physics and Astronomy Solar physics Space Exploration and Astronautics Space Sciences (including Extraterrestrial Physics Sun |
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| Title | Solar Intranetwork Magnetic Elements: Flux Distributions |
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