The Magnetic Field at the Inner Boundary of the Heliosphere Around Solar Minimum
Abstract STEREO A and B observations of the radial magnetic field between 1 January 2007 and 31 October 2008 show significant evidence that in the heliosphere, the ambient radial magnetic field component with any dynamic effects removed is uniformly distributed. Based on this monopolar nature of the...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Zhao, X. P. [verfasserIn] |
|---|
| Format: |
Artikel |
|---|---|
| Sprache: |
Englisch |
| Erschienen: |
2010 |
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| Schlagwörter: |
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| Anmerkung: |
© Springer Science+Business Media B.V. 2010 |
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| Übergeordnetes Werk: |
Enthalten in: Solar physics - Springer Netherlands, 1967, 266(2010), 2 vom: 28. Aug., Seite 379-390 |
|---|---|
| Übergeordnetes Werk: |
volume:266 ; year:2010 ; number:2 ; day:28 ; month:08 ; pages:379-390 |
| Links: |
|---|
| DOI / URN: |
10.1007/s11207-010-9618-0 |
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OLC2033607941 |
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| 520 | |a Abstract STEREO A and B observations of the radial magnetic field between 1 January 2007 and 31 October 2008 show significant evidence that in the heliosphere, the ambient radial magnetic field component with any dynamic effects removed is uniformly distributed. Based on this monopolar nature of the ambient heliospheric field we find that the surface beyond which the magnetic fields are in the monopolar configuration must be spherical, and this spherical surface can be defined as the inner boundary of the heliosphere that separates the monopole-dominated heliospheric magnetic field from the multipole-dominated coronal magnetic field. By using the radial variation of the coronal helmet streamers belts and the horizontal current – current sheet – source surface model we find that the spherical inner boundary of the heliosphere should be located around 14 solar radii near solar minimum phase. | ||
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10.1007/s11207-010-9618-0 doi (DE-627)OLC2033607941 (DE-He213)s11207-010-9618-0-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Zhao, X. P. verfasserin aut The Magnetic Field at the Inner Boundary of the Heliosphere Around Solar Minimum 2010 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media B.V. 2010 Abstract STEREO A and B observations of the radial magnetic field between 1 January 2007 and 31 October 2008 show significant evidence that in the heliosphere, the ambient radial magnetic field component with any dynamic effects removed is uniformly distributed. Based on this monopolar nature of the ambient heliospheric field we find that the surface beyond which the magnetic fields are in the monopolar configuration must be spherical, and this spherical surface can be defined as the inner boundary of the heliosphere that separates the monopole-dominated heliospheric magnetic field from the multipole-dominated coronal magnetic field. By using the radial variation of the coronal helmet streamers belts and the horizontal current – current sheet – source surface model we find that the spherical inner boundary of the heliosphere should be located around 14 solar radii near solar minimum phase. Heliosphere Heliospheric base Sun: corona Sun: magnetic field Hoeksema, J. T. aut Enthalten in Solar physics Springer Netherlands, 1967 266(2010), 2 vom: 28. Aug., Seite 379-390 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:266 year:2010 number:2 day:28 month:08 pages:379-390 https://doi.org/10.1007/s11207-010-9618-0 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 AR 266 2010 2 28 08 379-390 |
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10.1007/s11207-010-9618-0 doi (DE-627)OLC2033607941 (DE-He213)s11207-010-9618-0-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Zhao, X. P. verfasserin aut The Magnetic Field at the Inner Boundary of the Heliosphere Around Solar Minimum 2010 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media B.V. 2010 Abstract STEREO A and B observations of the radial magnetic field between 1 January 2007 and 31 October 2008 show significant evidence that in the heliosphere, the ambient radial magnetic field component with any dynamic effects removed is uniformly distributed. Based on this monopolar nature of the ambient heliospheric field we find that the surface beyond which the magnetic fields are in the monopolar configuration must be spherical, and this spherical surface can be defined as the inner boundary of the heliosphere that separates the monopole-dominated heliospheric magnetic field from the multipole-dominated coronal magnetic field. By using the radial variation of the coronal helmet streamers belts and the horizontal current – current sheet – source surface model we find that the spherical inner boundary of the heliosphere should be located around 14 solar radii near solar minimum phase. Heliosphere Heliospheric base Sun: corona Sun: magnetic field Hoeksema, J. T. aut Enthalten in Solar physics Springer Netherlands, 1967 266(2010), 2 vom: 28. Aug., Seite 379-390 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:266 year:2010 number:2 day:28 month:08 pages:379-390 https://doi.org/10.1007/s11207-010-9618-0 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 AR 266 2010 2 28 08 379-390 |
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10.1007/s11207-010-9618-0 doi (DE-627)OLC2033607941 (DE-He213)s11207-010-9618-0-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Zhao, X. P. verfasserin aut The Magnetic Field at the Inner Boundary of the Heliosphere Around Solar Minimum 2010 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media B.V. 2010 Abstract STEREO A and B observations of the radial magnetic field between 1 January 2007 and 31 October 2008 show significant evidence that in the heliosphere, the ambient radial magnetic field component with any dynamic effects removed is uniformly distributed. Based on this monopolar nature of the ambient heliospheric field we find that the surface beyond which the magnetic fields are in the monopolar configuration must be spherical, and this spherical surface can be defined as the inner boundary of the heliosphere that separates the monopole-dominated heliospheric magnetic field from the multipole-dominated coronal magnetic field. By using the radial variation of the coronal helmet streamers belts and the horizontal current – current sheet – source surface model we find that the spherical inner boundary of the heliosphere should be located around 14 solar radii near solar minimum phase. Heliosphere Heliospheric base Sun: corona Sun: magnetic field Hoeksema, J. T. aut Enthalten in Solar physics Springer Netherlands, 1967 266(2010), 2 vom: 28. Aug., Seite 379-390 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:266 year:2010 number:2 day:28 month:08 pages:379-390 https://doi.org/10.1007/s11207-010-9618-0 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 AR 266 2010 2 28 08 379-390 |
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10.1007/s11207-010-9618-0 doi (DE-627)OLC2033607941 (DE-He213)s11207-010-9618-0-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Zhao, X. P. verfasserin aut The Magnetic Field at the Inner Boundary of the Heliosphere Around Solar Minimum 2010 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media B.V. 2010 Abstract STEREO A and B observations of the radial magnetic field between 1 January 2007 and 31 October 2008 show significant evidence that in the heliosphere, the ambient radial magnetic field component with any dynamic effects removed is uniformly distributed. Based on this monopolar nature of the ambient heliospheric field we find that the surface beyond which the magnetic fields are in the monopolar configuration must be spherical, and this spherical surface can be defined as the inner boundary of the heliosphere that separates the monopole-dominated heliospheric magnetic field from the multipole-dominated coronal magnetic field. By using the radial variation of the coronal helmet streamers belts and the horizontal current – current sheet – source surface model we find that the spherical inner boundary of the heliosphere should be located around 14 solar radii near solar minimum phase. Heliosphere Heliospheric base Sun: corona Sun: magnetic field Hoeksema, J. T. aut Enthalten in Solar physics Springer Netherlands, 1967 266(2010), 2 vom: 28. Aug., Seite 379-390 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:266 year:2010 number:2 day:28 month:08 pages:379-390 https://doi.org/10.1007/s11207-010-9618-0 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 AR 266 2010 2 28 08 379-390 |
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10.1007/s11207-010-9618-0 doi (DE-627)OLC2033607941 (DE-He213)s11207-010-9618-0-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Zhao, X. P. verfasserin aut The Magnetic Field at the Inner Boundary of the Heliosphere Around Solar Minimum 2010 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media B.V. 2010 Abstract STEREO A and B observations of the radial magnetic field between 1 January 2007 and 31 October 2008 show significant evidence that in the heliosphere, the ambient radial magnetic field component with any dynamic effects removed is uniformly distributed. Based on this monopolar nature of the ambient heliospheric field we find that the surface beyond which the magnetic fields are in the monopolar configuration must be spherical, and this spherical surface can be defined as the inner boundary of the heliosphere that separates the monopole-dominated heliospheric magnetic field from the multipole-dominated coronal magnetic field. By using the radial variation of the coronal helmet streamers belts and the horizontal current – current sheet – source surface model we find that the spherical inner boundary of the heliosphere should be located around 14 solar radii near solar minimum phase. Heliosphere Heliospheric base Sun: corona Sun: magnetic field Hoeksema, J. T. aut Enthalten in Solar physics Springer Netherlands, 1967 266(2010), 2 vom: 28. Aug., Seite 379-390 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:266 year:2010 number:2 day:28 month:08 pages:379-390 https://doi.org/10.1007/s11207-010-9618-0 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 AR 266 2010 2 28 08 379-390 |
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Abstract STEREO A and B observations of the radial magnetic field between 1 January 2007 and 31 October 2008 show significant evidence that in the heliosphere, the ambient radial magnetic field component with any dynamic effects removed is uniformly distributed. Based on this monopolar nature of the ambient heliospheric field we find that the surface beyond which the magnetic fields are in the monopolar configuration must be spherical, and this spherical surface can be defined as the inner boundary of the heliosphere that separates the monopole-dominated heliospheric magnetic field from the multipole-dominated coronal magnetic field. By using the radial variation of the coronal helmet streamers belts and the horizontal current – current sheet – source surface model we find that the spherical inner boundary of the heliosphere should be located around 14 solar radii near solar minimum phase. © Springer Science+Business Media B.V. 2010 |
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Abstract STEREO A and B observations of the radial magnetic field between 1 January 2007 and 31 October 2008 show significant evidence that in the heliosphere, the ambient radial magnetic field component with any dynamic effects removed is uniformly distributed. Based on this monopolar nature of the ambient heliospheric field we find that the surface beyond which the magnetic fields are in the monopolar configuration must be spherical, and this spherical surface can be defined as the inner boundary of the heliosphere that separates the monopole-dominated heliospheric magnetic field from the multipole-dominated coronal magnetic field. By using the radial variation of the coronal helmet streamers belts and the horizontal current – current sheet – source surface model we find that the spherical inner boundary of the heliosphere should be located around 14 solar radii near solar minimum phase. © Springer Science+Business Media B.V. 2010 |
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Abstract STEREO A and B observations of the radial magnetic field between 1 January 2007 and 31 October 2008 show significant evidence that in the heliosphere, the ambient radial magnetic field component with any dynamic effects removed is uniformly distributed. Based on this monopolar nature of the ambient heliospheric field we find that the surface beyond which the magnetic fields are in the monopolar configuration must be spherical, and this spherical surface can be defined as the inner boundary of the heliosphere that separates the monopole-dominated heliospheric magnetic field from the multipole-dominated coronal magnetic field. By using the radial variation of the coronal helmet streamers belts and the horizontal current – current sheet – source surface model we find that the spherical inner boundary of the heliosphere should be located around 14 solar radii near solar minimum phase. © Springer Science+Business Media B.V. 2010 |
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<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a22002652 4500</leader><controlfield tag="001">OLC2033607941</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230504045844.0</controlfield><controlfield tag="007">tu</controlfield><controlfield tag="008">200819s2010 xx ||||| 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1007/s11207-010-9618-0</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)OLC2033607941</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-He213)s11207-010-9618-0-p</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rakwb</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">530</subfield><subfield code="q">VZ</subfield></datafield><datafield tag="084" ind1=" " ind2=" "><subfield code="a">16,12</subfield><subfield code="2">ssgn</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Zhao, X. P.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">The Magnetic Field at the Inner Boundary of the Heliosphere Around Solar Minimum</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2010</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">ohne Hilfsmittel zu benutzen</subfield><subfield code="b">n</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Band</subfield><subfield code="b">nc</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="500" ind1=" " ind2=" "><subfield code="a">© Springer Science+Business Media B.V. 2010</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract STEREO A and B observations of the radial magnetic field between 1 January 2007 and 31 October 2008 show significant evidence that in the heliosphere, the ambient radial magnetic field component with any dynamic effects removed is uniformly distributed. Based on this monopolar nature of the ambient heliospheric field we find that the surface beyond which the magnetic fields are in the monopolar configuration must be spherical, and this spherical surface can be defined as the inner boundary of the heliosphere that separates the monopole-dominated heliospheric magnetic field from the multipole-dominated coronal magnetic field. 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