Eamon Scullion

Prof. Eamon Scullion

orcid

Research Focus & Metrics

Academic Career Length

18Years (2009-Present)

(Calculated once Scilit publication data is synced: current year − year of first publication + 1)

Representative Publications

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27 June 2012 in Nature
Verified
Journal Article
Closed access
SWSven Wedemeyer-Böhm
Sven Wedemeyer-Böhm
ESEamon Scullion
Eamon Scullion
OSOskar Steiner
Oskar Steiner
LVLuc Rouppe van der Voort
Luc Rouppe van der Voort
JRJaime de la Cruz Rodriguez
Jaime de la Cruz Rodriguez
Robertus ErdelyiRobertus Erdelyi
Robertus Erdelyi

22 December 2015 in Space Science Reviews
Verified
Journal Article
Closed access
PDF file
SWS. Wedemeyer
S. Wedemeyer
TBT. Bastian
T. Bastian
RBR. Brajša
R. Brajša
HHH. Hudson
H. Hudson
Gregory FleishmanGregory Fleishman
Gregory Fleishman
MBM. Barta
M. Barta

3 March 2017 in Scientific Reports
Verified
Journal Article
Open access
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ASAbhishek Kumar Srivastava
Abhishek Kumar Srivastava
JSJuie Shetye
Juie Shetye
KMKrzysztof Murawski
Krzysztof Murawski
JDJohn Gerard Doyle
John Gerard Doyle
MSMarco Stangalini
Marco Stangalini
BDBhola N. Dwivedi
Bhola N. Dwivedi
The existence of the Sun’s hot atmosphere and the solar wind acceleration continues to be an outstanding problem in solar-astrophysics. Although magnetohydrodynamic (MHD) modes and dissipation of magnetic energy contribute to heating and the mass cycle of the solar atmosphere, yet direct evidence of such processes often generates debate. Ground-based 1-m Swedish Solar Telescope (SST)/CRISP, Hα 6562.8 Å observations reveal, for the first time, the ubiquitous presence of high frequency (~12–42 mHz) torsional motions in thin spicular-type structures in the chromosphere. We detect numerous oscillating flux tubes on 10 June 2014 between 07:17 UT to 08:08 UT in a quiet-Sun field-of-view of 60” × 60” (1” = 725 km). Stringent numerical model shows that these observations resemble torsional Alfvén waves associated with high frequency drivers which contain a huge amount of energy (~105 W m−2) in the chromosphere. Even after partial reflection from the transition region, a significant amount of energy (~103 W m−2) is transferred onto the overlying corona. We find that oscillating tubes serve as substantial sources of Alfvén wave generation that provide sufficient Poynting flux not only to heat the corona but also to originate the supersonic solar wind.

9 June 2015 in The Astrophysical Journal
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Journal Article
Closed access
PAP. Antolin
P. Antolin
GVG. Vissers
G. Vissers
TPT. M. D. Pereira
T. M. D. Pereira
LVL. Rouppe van der Voort
L. Rouppe van der Voort
ESEamon Scullion
Eamon Scullion

19 April 2021 in Solar Physics
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Journal Article
Open access
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DNDkist Project Nso
Dkist Project Nso
MRMark Rast
Mark Rast
TGthe DKIST Science Working Group
the DKIST Science Working Group
TCthe DKIST Critical Science Plan Community
the DKIST Critical Science Plan Community
NGNazaret Bello González
Nazaret Bello González
YWYi-Ming Wang
Yi-Ming Wang
The National Science Foundation’sDaniel K. Inouye Solar Telescope(DKIST) will revolutionize our ability to measure, understand, and model the basic physical processes that control the structure and dynamics of the Sun and its atmosphere. The first-light DKIST images, released publicly on 29 January 2020, only hint at the extraordinary capabilities that will accompany full commissioning of the five facility instruments. With this Critical Science Plan (CSP) we attempt to anticipate some of what those capabilities will enable, providing a snapshot of some of the scientific pursuits that the DKIST hopes to engage as start-of-operations nears. The work builds on the combined contributions of the DKIST Science Working Group (SWG) and CSP Community members, who generously shared their experiences, plans, knowledge, and dreams. Discussion is primarily focused on those issues to which DKIST will uniquely contribute.

3 May 2013 in The Astrophysical Journal
Verified
Journal Article
Closed access
DSD. H. Sekse
D. H. Sekse
LVL. Rouppe van der Voort
L. Rouppe van der Voort
BPB. De Pontieu
B. De Pontieu
ESEamon Scullion
Eamon Scullion