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Exploring EUV Spicules Using 304 Angstrom He II Data from SDO AIAWe present results from a statistical study of He II 304 Angstrom Extreme Ultraviolet (EUV) spicules at the limb of the Sun. We also measured properties of one macrospicule; macrospicules are longer than most spicules, and much broader in width than spicules. We use high-cadence (12 second) and high-resolution (0.6 arcseconds pixels) resolution data from the Atmospheric Imaging Array (AIA) instrument on the Solar Dynamic Observatory (SDO). All of the observed events occurred near the solar north pole, where quiet Sun or coronal hole environments ensued. We examined the maximum lengths, maximum rise velocities, and lifetimes of 33 Extreme Ultraviolet (EUV) spicules and the macrospicule. For the bulk of the Extreme Ultraviolet (EUV) spicules these quantities are, respectively, approximately 10,000-40,000 kilometers, 20-100 kilometers per second, and approximately 100- approximately 1000 seconds. For the macrospicule the corresponding quantities were respectively approximately 60,000 kilometers, approximately 130 kilometers per second, approximately 1800 seconds, which is typical of macrospicules measured by other workers. Therefore macrospicules are taller, longer-lived, and faster than most Extreme Ultraviolet (EUV) spicules. The rise profiles of both the spicules and the macrospicules match well a second-order ("parabolic" ) trajectory, although the acceleration was often weaker than that of solar gravity in the profiles fitted to the trajectories. Our macrospicule also had an obvious brightening at its base at birth, while such brightening was not apparent for the Extreme Ultraviolet (EUV) spicules. Most of the Extreme Ultraviolet (EUV) spicules remained visible during their descent back to the solar surface, although a small percentage of the spicules and the macrospicule faded out before falling back to the surface. Our sample of macrospicules is not yet large enough to determine whether their initiation mechanism is identical to that of Extreme Ultraviolet (EUV) spicules.
Document ID
20150001400
Acquisition Source
Marshall Space Flight Center
Document Type
Presentation
Authors
Snyder, Ian R.
(Vassar Coll. Poughkeepsie, NY, United States)
Sterling, Alphonse C.
(NASA Marshall Space Flight Center Huntsville, AL United States)
Falconer, David A.
(Alabama Univ. Huntsville, AL, United States)
Moore, Ron L.
(Alabama Univ. Huntsville, AL, United States)
Date Acquired
February 5, 2015
Publication Date
December 15, 2014
Subject Category
Solar Physics
Report/Patent Number
MSFC-E-DAA-TN19908
Report Number: MSFC-E-DAA-TN19908
Meeting Information
Meeting: AGU Fall Meeting
Location: San Francisco, CA
Country: United States
Start Date: December 15, 2014
End Date: December 19, 2014
Sponsors: American Geophysical Union
Funding Number(s)
CONTRACT_GRANT: NSF-AGS1157027
WBS: WBS 13314
CONTRACT_GRANT: NNM11AA01A
Distribution Limits
Public
Copyright
Public Use Permitted.
Keywords
spicules
EUV
angstrom
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