Evidence for Wave Dissipation through EUV Emission Line Narrowing

R. A. Harrison; A. W. Hood; C. D. Pike

Evidence for Wave Dissipation through EUV Emission Line Narrowing

R. A. Harrison
, A. W. Hood
, C. D. Pike

Applied Mathematics

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

Abstract

Using long-duration observations over closed-field, quiet Sun regions above the solar equator, evidence has been found for the narrowing of coronal emission lines with increasing altitude. This is interpreted as evidence for wave dissipation in the quiet Sun corona.

Original language	English
Pages (from-to)	229
Journal	Proceedings of 'SOHO 13 - Waves, Oscillations and Small-Scale Transient Events in the Solar Atmosphere: A Joint View from SOHO and TRACE'. 29 September - 3 October 2003, Palma de Mallorca, Balearic Islands, Spain (ESA SP-547, January 2004). Compiled by: H. Lacoste
Volume	547
Publication status	Published - 1 Jan 2004

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Harrison, R. A., Hood, A. W., & Pike, C. D. (2004). Evidence for Wave Dissipation through EUV Emission Line Narrowing. Proceedings of 'SOHO 13 - Waves, Oscillations and Small-Scale Transient Events in the Solar Atmosphere: A Joint View from SOHO and TRACE'. 29 September - 3 October 2003, Palma de Mallorca, Balearic Islands, Spain (ESA SP-547, January 2004). Compiled by: H. Lacoste, 547, 229. http://adsabs.harvard.edu/abs/2004ESASP.547..229H

Harrison, R. A. ; Hood, A. W. ; Pike, C. D. / Evidence for Wave Dissipation through EUV Emission Line Narrowing. In: Proceedings of 'SOHO 13 - Waves, Oscillations and Small-Scale Transient Events in the Solar Atmosphere: A Joint View from SOHO and TRACE'. 29 September - 3 October 2003, Palma de Mallorca, Balearic Islands, Spain (ESA SP-547, January 2004). Compiled by: H. Lacoste. 2004 ; Vol. 547. pp. 229.

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title = "Evidence for Wave Dissipation through EUV Emission Line Narrowing",

abstract = "Using long-duration observations over closed-field, quiet Sun regions above the solar equator, evidence has been found for the narrowing of coronal emission lines with increasing altitude. This is interpreted as evidence for wave dissipation in the quiet Sun corona.",

author = "Harrison, \{R. A.\} and Hood, \{A. W.\} and Pike, \{C. D.\}",

year = "2004",

month = jan,

day = "1",

language = "English",

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pages = "229",

journal = "Proceedings of 'SOHO 13 - Waves, Oscillations and Small-Scale Transient Events in the Solar Atmosphere: A Joint View from SOHO and TRACE'. 29 September - 3 October 2003, Palma de Mallorca, Balearic Islands, Spain (ESA SP-547, January 2004). Compiled by: H. Lacoste",

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Harrison, RA, Hood, AW & Pike, CD 2004, 'Evidence for Wave Dissipation through EUV Emission Line Narrowing', Proceedings of 'SOHO 13 - Waves, Oscillations and Small-Scale Transient Events in the Solar Atmosphere: A Joint View from SOHO and TRACE'. 29 September - 3 October 2003, Palma de Mallorca, Balearic Islands, Spain (ESA SP-547, January 2004). Compiled by: H. Lacoste, vol. 547, pp. 229. <http://adsabs.harvard.edu/abs/2004ESASP.547..229H>

Evidence for Wave Dissipation through EUV Emission Line Narrowing. / Harrison, R. A.; Hood, A. W.; Pike, C. D.
In: Proceedings of 'SOHO 13 - Waves, Oscillations and Small-Scale Transient Events in the Solar Atmosphere: A Joint View from SOHO and TRACE'. 29 September - 3 October 2003, Palma de Mallorca, Balearic Islands, Spain (ESA SP-547, January 2004). Compiled by: H. Lacoste, Vol. 547, 01.01.2004, p. 229.

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

TY - JOUR

T1 - Evidence for Wave Dissipation through EUV Emission Line Narrowing

AU - Harrison, R. A.

AU - Hood, A. W.

AU - Pike, C. D.

PY - 2004/1/1

Y1 - 2004/1/1

N2 - Using long-duration observations over closed-field, quiet Sun regions above the solar equator, evidence has been found for the narrowing of coronal emission lines with increasing altitude. This is interpreted as evidence for wave dissipation in the quiet Sun corona.

AB - Using long-duration observations over closed-field, quiet Sun regions above the solar equator, evidence has been found for the narrowing of coronal emission lines with increasing altitude. This is interpreted as evidence for wave dissipation in the quiet Sun corona.

M3 - Article

VL - 547

SP - 229

JO - Proceedings of 'SOHO 13 - Waves, Oscillations and Small-Scale Transient Events in the Solar Atmosphere: A Joint View from SOHO and TRACE'. 29 September - 3 October 2003, Palma de Mallorca, Balearic Islands, Spain (ESA SP-547, January 2004). Compiled by: H

JF - Proceedings of 'SOHO 13 - Waves, Oscillations and Small-Scale Transient Events in the Solar Atmosphere: A Joint View from SOHO and TRACE'. 29 September - 3 October 2003, Palma de Mallorca, Balearic Islands, Spain (ESA SP-547, January 2004). Compiled by: H

ER -

Harrison RA, Hood AW, Pike CD. Evidence for Wave Dissipation through EUV Emission Line Narrowing. Proceedings of 'SOHO 13 - Waves, Oscillations and Small-Scale Transient Events in the Solar Atmosphere: A Joint View from SOHO and TRACE'. 29 September - 3 October 2003, Palma de Mallorca, Balearic Islands, Spain (ESA SP-547, January 2004). Compiled by: H. Lacoste. 2004 Jan 1;547:229.

Evidence for Wave Dissipation through EUV Emission Line Narrowing

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