Doppler Events in the Solar Photosphere: The Coincident Superposition of Fast Granular Flows and p-Mode Coherence Patches
Observations of the solar photosphere show spatially compact large-amplitude Doppler velocity events with short lifetimes. In data from the Imaging Magnetograph eXperiment (IMaX) on the first flight of the Sunrise balloon in 2009, events with velocities in excess of 4 σ from the mean can be identifi...
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Veröffentlicht in: | Solar physics 2019-02, Vol.294 (2), p.1-9, Article 18 |
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creator | McClure, R. Lee Rast, Mark P. Martínez Pillet, Valentin |
description | Observations of the solar photosphere show spatially compact large-amplitude Doppler velocity events with short lifetimes. In data from the
Imaging Magnetograph eXperiment
(IMaX) on the first flight of the
Sunrise
balloon in 2009, events with velocities in excess of 4
σ
from the mean can be identified in both intergranular downflow lanes and granular upflows. We show that the statistics of such events are consistent with the random superposition of strong convective flows and p-mode coherence patches. Such coincident superposition complicates the identification of acoustic wave sources in the solar photosphere, and may be important in the interpretation of spectral line profiles formed in solar photosphere. |
doi_str_mv | 10.1007/s11207-019-1395-9 |
format | Article |
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Imaging Magnetograph eXperiment
(IMaX) on the first flight of the
Sunrise
balloon in 2009, events with velocities in excess of 4
σ
from the mean can be identified in both intergranular downflow lanes and granular upflows. We show that the statistics of such events are consistent with the random superposition of strong convective flows and p-mode coherence patches. Such coincident superposition complicates the identification of acoustic wave sources in the solar photosphere, and may be important in the interpretation of spectral line profiles formed in solar photosphere.</description><identifier>ISSN: 0038-0938</identifier><identifier>EISSN: 1573-093X</identifier><identifier>DOI: 10.1007/s11207-019-1395-9</identifier><language>eng</language><publisher>Dordrecht: Springer Netherlands</publisher><subject>Acoustic waves ; Acoustics ; Astrophysics and Astroparticles ; Atmospheric Sciences ; Coherence ; Line spectra ; Magnetic fields ; Paths ; Photosphere ; Physics ; Physics and Astronomy ; Solar physics ; Space Exploration and Astronautics ; Space Sciences (including Extraterrestrial Physics ; Superposition (mathematics) ; Time series ; Velocity</subject><ispartof>Solar physics, 2019-02, Vol.294 (2), p.1-9, Article 18</ispartof><rights>The Author(s) 2019</rights><rights>Solar Physics is a copyright of Springer, (2019). All Rights Reserved. © 2019. This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c425t-f2289127e1cdd4574b9d0d62e2b20971e1cb0c8424f874d26c88bfd87d758cfa3</citedby><cites>FETCH-LOGICAL-c425t-f2289127e1cdd4574b9d0d62e2b20971e1cb0c8424f874d26c88bfd87d758cfa3</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://link.springer.com/content/pdf/10.1007/s11207-019-1395-9$$EPDF$$P50$$Gspringer$$Hfree_for_read</linktopdf><linktohtml>$$Uhttps://link.springer.com/10.1007/s11207-019-1395-9$$EHTML$$P50$$Gspringer$$Hfree_for_read</linktohtml><link.rule.ids>314,776,780,27901,27902,41464,42533,51294</link.rule.ids></links><search><creatorcontrib>McClure, R. Lee</creatorcontrib><creatorcontrib>Rast, Mark P.</creatorcontrib><creatorcontrib>Martínez Pillet, Valentin</creatorcontrib><title>Doppler Events in the Solar Photosphere: The Coincident Superposition of Fast Granular Flows and p-Mode Coherence Patches</title><title>Solar physics</title><addtitle>Sol Phys</addtitle><description>Observations of the solar photosphere show spatially compact large-amplitude Doppler velocity events with short lifetimes. In data from the
Imaging Magnetograph eXperiment
(IMaX) on the first flight of the
Sunrise
balloon in 2009, events with velocities in excess of 4
σ
from the mean can be identified in both intergranular downflow lanes and granular upflows. We show that the statistics of such events are consistent with the random superposition of strong convective flows and p-mode coherence patches. Such coincident superposition complicates the identification of acoustic wave sources in the solar photosphere, and may be important in the interpretation of spectral line profiles formed in solar photosphere.</description><subject>Acoustic waves</subject><subject>Acoustics</subject><subject>Astrophysics and Astroparticles</subject><subject>Atmospheric Sciences</subject><subject>Coherence</subject><subject>Line spectra</subject><subject>Magnetic fields</subject><subject>Paths</subject><subject>Photosphere</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Solar physics</subject><subject>Space Exploration and Astronautics</subject><subject>Space Sciences (including Extraterrestrial Physics</subject><subject>Superposition (mathematics)</subject><subject>Time series</subject><subject>Velocity</subject><issn>0038-0938</issn><issn>1573-093X</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2019</creationdate><recordtype>article</recordtype><sourceid>C6C</sourceid><sourceid>BENPR</sourceid><recordid>eNp1kF1LwzAUhoMoOKc_wLuA19Ek_UjinUw3hYmDTfAutElqO2pSk1bZvzelgldencPhed4DLwCXBF8TjNlNIIRihjARiCQiQ-IIzEjGEoRF8nYMZhgnfNz5KTgLYY_xaGUzcLh3XdcaDx--jO0DbCzsawO3ri083NSud6GrjTe3cBfPC9dY1ehIwu3QGd-50PSNs9BVcFmEHq58YYdRXbbuO8DCatihZ6dHdYyxysBN0avahHNwUhVtMBe_cw5elw-7xSNav6yeFndrpFKa9aiilAtCmSFK6zRjaSk01jk1tKRYMBLvJVY8pWnFWapprjgvK82ZZhlXVZHMwdWU23n3OZjQy70bvI0vJSUsJzmPoZEiE6W8C8GbSna--Sj8QRIsx67k1LCMDcuxYSmiQycnRNa-G_-X_L_0A74Tfuc</recordid><startdate>20190201</startdate><enddate>20190201</enddate><creator>McClure, R. 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Imaging Magnetograph eXperiment
(IMaX) on the first flight of the
Sunrise
balloon in 2009, events with velocities in excess of 4
σ
from the mean can be identified in both intergranular downflow lanes and granular upflows. We show that the statistics of such events are consistent with the random superposition of strong convective flows and p-mode coherence patches. Such coincident superposition complicates the identification of acoustic wave sources in the solar photosphere, and may be important in the interpretation of spectral line profiles formed in solar photosphere.</abstract><cop>Dordrecht</cop><pub>Springer Netherlands</pub><doi>10.1007/s11207-019-1395-9</doi><tpages>9</tpages><oa>free_for_read</oa></addata></record> |
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subjects | Acoustic waves Acoustics Astrophysics and Astroparticles Atmospheric Sciences Coherence Line spectra Magnetic fields Paths Photosphere Physics Physics and Astronomy Solar physics Space Exploration and Astronautics Space Sciences (including Extraterrestrial Physics Superposition (mathematics) Time series Velocity |
title | Doppler Events in the Solar Photosphere: The Coincident Superposition of Fast Granular Flows and p-Mode Coherence Patches |
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