Oscillatory signatures above quiet sun magnetic elements

D. Shaun Bloomfield; R. T. James McAteer; Bruce W. Lites; Philip G. Judge; Mihalis Mathioudakis; Francis P. Keenan

Oscillatory signatures above quiet sun magnetic elements

D. Shaun Bloomfield, R. T. James McAteer, Bruce W. Lites, Philip G. Judge, Mihalis Mathioudakis, Francis P. Keenan

Solar Frontiers

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

Abstract

A new application of wavelet analysis is presented. The data used are part of Joint Observing Proposal 72 between SoHO and TRACE, obtained on 1998 May 16 with accompanying groundbased data taken with the Dunn Solar Telescope at Sacramento Peak, New Mexico. A weak magnetic network region is studied and the temporal variation of phase difference between TRACE 1700Å and SoHO/SUMER C II intensities is shown. The example clearly highlights the advantages of wavelet analysis over more classical techniques such as Fourier analysis, where the effectiveness of the technique to identify wavepackets with differing phase difference relations is emphasised.

Original language	English
Pages (from-to)	51-55
Number of pages	5
Journal	European Space Agency, (Special Publication) ESA SP
Issue number	547
State	Published - 2004
Event	Proceedings of the Conference SOHO 13 - Waves, Oscillations and Small-Scale Transient Events in the Solar Atmosphere: A Joint View from SOHO and TRACE - Balearic Islands, Spain Duration: Sep 29 2003 → Oct 3 2003

Keywords

Chromosphere
Oscillations
Phase difference
Wavelet analysis

Cite this

@article{30de43c2c37648a6bd70f7c7828cc694,

title = "Oscillatory signatures above quiet sun magnetic elements",

abstract = "A new application of wavelet analysis is presented. The data used are part of Joint Observing Proposal 72 between SoHO and TRACE, obtained on 1998 May 16 with accompanying groundbased data taken with the Dunn Solar Telescope at Sacramento Peak, New Mexico. A weak magnetic network region is studied and the temporal variation of phase difference between TRACE 1700{\AA} and SoHO/SUMER C II intensities is shown. The example clearly highlights the advantages of wavelet analysis over more classical techniques such as Fourier analysis, where the effectiveness of the technique to identify wavepackets with differing phase difference relations is emphasised.",

keywords = "Chromosphere, Oscillations, Phase difference, Wavelet analysis",

author = "\{Shaun Bloomfield\}, D. and \{James McAteer\}, \{R. T.\} and Lites, \{Bruce W.\} and Judge, \{Philip G.\} and Mihalis Mathioudakis and Keenan, \{Francis P.\}",

year = "2004",

language = "English",

pages = "51--55",

journal = "European Space Agency, (Special Publication) ESA SP",

issn = "0379-6566",

publisher = "European Space Agency",

number = "547",

note = "Proceedings of the Conference SOHO 13 - Waves, Oscillations and Small-Scale Transient Events in the Solar Atmosphere: A Joint View from SOHO and TRACE ; Conference date: 29-09-2003 Through 03-10-2003",

}

TY - JOUR

T1 - Oscillatory signatures above quiet sun magnetic elements

AU - Shaun Bloomfield, D.

AU - James McAteer, R. T.

AU - Lites, Bruce W.

AU - Judge, Philip G.

AU - Mathioudakis, Mihalis

AU - Keenan, Francis P.

PY - 2004

Y1 - 2004

N2 - A new application of wavelet analysis is presented. The data used are part of Joint Observing Proposal 72 between SoHO and TRACE, obtained on 1998 May 16 with accompanying groundbased data taken with the Dunn Solar Telescope at Sacramento Peak, New Mexico. A weak magnetic network region is studied and the temporal variation of phase difference between TRACE 1700Å and SoHO/SUMER C II intensities is shown. The example clearly highlights the advantages of wavelet analysis over more classical techniques such as Fourier analysis, where the effectiveness of the technique to identify wavepackets with differing phase difference relations is emphasised.

AB - A new application of wavelet analysis is presented. The data used are part of Joint Observing Proposal 72 between SoHO and TRACE, obtained on 1998 May 16 with accompanying groundbased data taken with the Dunn Solar Telescope at Sacramento Peak, New Mexico. A weak magnetic network region is studied and the temporal variation of phase difference between TRACE 1700Å and SoHO/SUMER C II intensities is shown. The example clearly highlights the advantages of wavelet analysis over more classical techniques such as Fourier analysis, where the effectiveness of the technique to identify wavepackets with differing phase difference relations is emphasised.

KW - Chromosphere

KW - Oscillations

KW - Phase difference

KW - Wavelet analysis

UR - https://www.scopus.com/pages/publications/18644371479

M3 - Conference article

AN - SCOPUS:18644371479

SN - 0379-6566

SP - 51

EP - 55

JO - European Space Agency, (Special Publication) ESA SP

JF - European Space Agency, (Special Publication) ESA SP

IS - 547

T2 - Proceedings of the Conference SOHO 13 - Waves, Oscillations and Small-Scale Transient Events in the Solar Atmosphere: A Joint View from SOHO and TRACE

Y2 - 29 September 2003 through 3 October 2003

ER -

Oscillatory signatures above quiet sun magnetic elements

Abstract

Keywords

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