Evidences to the pulse like origin of double spicules based on Hinode/SOT observations
Abstract We analyze the time series of Hα line obtained from Hinode/SOT on the solar limb. The wavelet analysis shows that there are nice correlations between dynamical properties of the two parts of a double spicule. The dominant periods for height variations are estimated ∼90 and ∼180 s. The lengt...
Ausführliche Beschreibung
Autor*in: |
Ebadi, H. [verfasserIn] |
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Artikel |
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Sprache: |
Englisch |
Erschienen: |
2013 |
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Anmerkung: |
© Springer Science+Business Media Dordrecht 2013 |
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Übergeordnetes Werk: |
Enthalten in: Astrophysics and space science - Springer Netherlands, 1968, 348(2013), 1 vom: 24. Juli, Seite 11-15 |
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Übergeordnetes Werk: |
volume:348 ; year:2013 ; number:1 ; day:24 ; month:07 ; pages:11-15 |
Links: |
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DOI / URN: |
10.1007/s10509-013-1559-2 |
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Katalog-ID: |
OLC2066271101 |
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10.1007/s10509-013-1559-2 doi (DE-627)OLC2066271101 (DE-He213)s10509-013-1559-2-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Ebadi, H. verfasserin aut Evidences to the pulse like origin of double spicules based on Hinode/SOT observations 2013 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media Dordrecht 2013 Abstract We analyze the time series of Hα line obtained from Hinode/SOT on the solar limb. The wavelet analysis shows that there are nice correlations between dynamical properties of the two parts of a double spicule. The dominant periods for height variations are estimated ∼90 and ∼180 s. The length of two parts of the spicule oscillates with the period of around ∼180 s. The mean distance between two parts of the spicule has a periodical treatment with the period of ∼90 s. Our results show that the strong pulses may lead to the quasi periodic rising of chromospheric plasma into the lower corona in the form of spicules. The periodicity may result from the nonlinear wake behind the pulse in the stratified atmosphere. Sun: spicules Spicule formation Double spicules Enthalten in Astrophysics and space science Springer Netherlands, 1968 348(2013), 1 vom: 24. Juli, Seite 11-15 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:348 year:2013 number:1 day:24 month:07 pages:11-15 https://doi.org/10.1007/s10509-013-1559-2 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2279 GBV_ILN_4012 AR 348 2013 1 24 07 11-15 |
spelling |
10.1007/s10509-013-1559-2 doi (DE-627)OLC2066271101 (DE-He213)s10509-013-1559-2-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Ebadi, H. verfasserin aut Evidences to the pulse like origin of double spicules based on Hinode/SOT observations 2013 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media Dordrecht 2013 Abstract We analyze the time series of Hα line obtained from Hinode/SOT on the solar limb. The wavelet analysis shows that there are nice correlations between dynamical properties of the two parts of a double spicule. The dominant periods for height variations are estimated ∼90 and ∼180 s. The length of two parts of the spicule oscillates with the period of around ∼180 s. The mean distance between two parts of the spicule has a periodical treatment with the period of ∼90 s. Our results show that the strong pulses may lead to the quasi periodic rising of chromospheric plasma into the lower corona in the form of spicules. The periodicity may result from the nonlinear wake behind the pulse in the stratified atmosphere. Sun: spicules Spicule formation Double spicules Enthalten in Astrophysics and space science Springer Netherlands, 1968 348(2013), 1 vom: 24. Juli, Seite 11-15 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:348 year:2013 number:1 day:24 month:07 pages:11-15 https://doi.org/10.1007/s10509-013-1559-2 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2279 GBV_ILN_4012 AR 348 2013 1 24 07 11-15 |
allfields_unstemmed |
10.1007/s10509-013-1559-2 doi (DE-627)OLC2066271101 (DE-He213)s10509-013-1559-2-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Ebadi, H. verfasserin aut Evidences to the pulse like origin of double spicules based on Hinode/SOT observations 2013 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media Dordrecht 2013 Abstract We analyze the time series of Hα line obtained from Hinode/SOT on the solar limb. The wavelet analysis shows that there are nice correlations between dynamical properties of the two parts of a double spicule. The dominant periods for height variations are estimated ∼90 and ∼180 s. The length of two parts of the spicule oscillates with the period of around ∼180 s. The mean distance between two parts of the spicule has a periodical treatment with the period of ∼90 s. Our results show that the strong pulses may lead to the quasi periodic rising of chromospheric plasma into the lower corona in the form of spicules. The periodicity may result from the nonlinear wake behind the pulse in the stratified atmosphere. Sun: spicules Spicule formation Double spicules Enthalten in Astrophysics and space science Springer Netherlands, 1968 348(2013), 1 vom: 24. Juli, Seite 11-15 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:348 year:2013 number:1 day:24 month:07 pages:11-15 https://doi.org/10.1007/s10509-013-1559-2 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2279 GBV_ILN_4012 AR 348 2013 1 24 07 11-15 |
allfieldsGer |
10.1007/s10509-013-1559-2 doi (DE-627)OLC2066271101 (DE-He213)s10509-013-1559-2-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Ebadi, H. verfasserin aut Evidences to the pulse like origin of double spicules based on Hinode/SOT observations 2013 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media Dordrecht 2013 Abstract We analyze the time series of Hα line obtained from Hinode/SOT on the solar limb. The wavelet analysis shows that there are nice correlations between dynamical properties of the two parts of a double spicule. The dominant periods for height variations are estimated ∼90 and ∼180 s. The length of two parts of the spicule oscillates with the period of around ∼180 s. The mean distance between two parts of the spicule has a periodical treatment with the period of ∼90 s. Our results show that the strong pulses may lead to the quasi periodic rising of chromospheric plasma into the lower corona in the form of spicules. The periodicity may result from the nonlinear wake behind the pulse in the stratified atmosphere. Sun: spicules Spicule formation Double spicules Enthalten in Astrophysics and space science Springer Netherlands, 1968 348(2013), 1 vom: 24. Juli, Seite 11-15 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:348 year:2013 number:1 day:24 month:07 pages:11-15 https://doi.org/10.1007/s10509-013-1559-2 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2279 GBV_ILN_4012 AR 348 2013 1 24 07 11-15 |
allfieldsSound |
10.1007/s10509-013-1559-2 doi (DE-627)OLC2066271101 (DE-He213)s10509-013-1559-2-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Ebadi, H. verfasserin aut Evidences to the pulse like origin of double spicules based on Hinode/SOT observations 2013 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media Dordrecht 2013 Abstract We analyze the time series of Hα line obtained from Hinode/SOT on the solar limb. The wavelet analysis shows that there are nice correlations between dynamical properties of the two parts of a double spicule. The dominant periods for height variations are estimated ∼90 and ∼180 s. The length of two parts of the spicule oscillates with the period of around ∼180 s. The mean distance between two parts of the spicule has a periodical treatment with the period of ∼90 s. Our results show that the strong pulses may lead to the quasi periodic rising of chromospheric plasma into the lower corona in the form of spicules. The periodicity may result from the nonlinear wake behind the pulse in the stratified atmosphere. Sun: spicules Spicule formation Double spicules Enthalten in Astrophysics and space science Springer Netherlands, 1968 348(2013), 1 vom: 24. Juli, Seite 11-15 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:348 year:2013 number:1 day:24 month:07 pages:11-15 https://doi.org/10.1007/s10509-013-1559-2 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2279 GBV_ILN_4012 AR 348 2013 1 24 07 11-15 |
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Abstract We analyze the time series of Hα line obtained from Hinode/SOT on the solar limb. The wavelet analysis shows that there are nice correlations between dynamical properties of the two parts of a double spicule. The dominant periods for height variations are estimated ∼90 and ∼180 s. The length of two parts of the spicule oscillates with the period of around ∼180 s. The mean distance between two parts of the spicule has a periodical treatment with the period of ∼90 s. Our results show that the strong pulses may lead to the quasi periodic rising of chromospheric plasma into the lower corona in the form of spicules. The periodicity may result from the nonlinear wake behind the pulse in the stratified atmosphere. © Springer Science+Business Media Dordrecht 2013 |
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Abstract We analyze the time series of Hα line obtained from Hinode/SOT on the solar limb. The wavelet analysis shows that there are nice correlations between dynamical properties of the two parts of a double spicule. The dominant periods for height variations are estimated ∼90 and ∼180 s. The length of two parts of the spicule oscillates with the period of around ∼180 s. The mean distance between two parts of the spicule has a periodical treatment with the period of ∼90 s. Our results show that the strong pulses may lead to the quasi periodic rising of chromospheric plasma into the lower corona in the form of spicules. The periodicity may result from the nonlinear wake behind the pulse in the stratified atmosphere. © Springer Science+Business Media Dordrecht 2013 |
abstract_unstemmed |
Abstract We analyze the time series of Hα line obtained from Hinode/SOT on the solar limb. The wavelet analysis shows that there are nice correlations between dynamical properties of the two parts of a double spicule. The dominant periods for height variations are estimated ∼90 and ∼180 s. The length of two parts of the spicule oscillates with the period of around ∼180 s. The mean distance between two parts of the spicule has a periodical treatment with the period of ∼90 s. Our results show that the strong pulses may lead to the quasi periodic rising of chromospheric plasma into the lower corona in the form of spicules. The periodicity may result from the nonlinear wake behind the pulse in the stratified atmosphere. © Springer Science+Business Media Dordrecht 2013 |
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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">OLC2066271101</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230502213741.0</controlfield><controlfield tag="007">tu</controlfield><controlfield tag="008">200820s2013 xx ||||| 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1007/s10509-013-1559-2</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)OLC2066271101</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-He213)s10509-013-1559-2-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">520</subfield><subfield code="a">530</subfield><subfield code="a">620</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">Ebadi, H.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Evidences to the pulse like origin of double spicules based on Hinode/SOT observations</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2013</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 Dordrecht 2013</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract We analyze the time series of Hα line obtained from Hinode/SOT on the solar limb. The wavelet analysis shows that there are nice correlations between dynamical properties of the two parts of a double spicule. The dominant periods for height variations are estimated ∼90 and ∼180 s. The length of two parts of the spicule oscillates with the period of around ∼180 s. The mean distance between two parts of the spicule has a periodical treatment with the period of ∼90 s. Our results show that the strong pulses may lead to the quasi periodic rising of chromospheric plasma into the lower corona in the form of spicules. 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