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pro vyhledávání: '"Woolsey, Lauren N."'
Autor:
Woolsey, Lauren N.
The steady, supersonic outflow from the Sun we call the solar wind was first posited in the 1950s and initial theories rightly linked the acceleration of the wind to the existence of the million-degree solar corona. Still today, the wind acceleration
Externí odkaz:
http://arxiv.org/abs/1605.04318
Autor:
Cranmer, Steven R., Woolsey, Lauren N.
The solar chromosphere contains thin, highly dynamic strands of plasma known as spicules. Recently, it has been suggested that the smallest and fastest (Type II) spicules are identical to intermittent jets observed by the Interface Region Imaging Spe
Externí odkaz:
http://arxiv.org/abs/1509.03263
Autor:
Woolsey, Lauren N., Cranmer, Steven R.
We investigate several key questions of plasma heating in open-field regions of the corona that connect to the solar wind. We present results for a model of Alfven-wave-driven turbulence for three typical open magnetic field structures: a polar coron
Externí odkaz:
http://arxiv.org/abs/1509.00377
Autor:
Woolsey, Lauren N.
Publikováno v:
JAESE, 2015, Vol. 2, Iss. 1
The paper presents an interactive module created through the Wolfram Demonstrations Project that visualizes the Zeeman effect for the small magnetic field strengths present in the interstellar medium. The paper provides an overview of spectral lines
Externí odkaz:
http://arxiv.org/abs/1506.00932
Autor:
Woolsey, Lauren N.
Publikováno v:
2015, JRAEO, Issue 3, Pages B49-55
This article presents a Python model and library that can be used for student investigation of the application of fundamental physics on a specific problem: the role of magnetic field in solar wind acceleration. The paper begins with a short overview
Externí odkaz:
http://arxiv.org/abs/1505.00727
Autor:
Woolsey, Lauren N., Cranmer, Steven R.
Forecasting models of the solar wind often rely on simple parameterizations of the magnetic field that ignore the effects of the full magnetic field geometry. In this paper, we present the results of two solar wind prediction models that consider the
Externí odkaz:
http://arxiv.org/abs/1404.5998
The solar wind is connected to the Sun's atmosphere by flux tubes that are rooted in an ever-changing pattern of positive and negative magnetic polarities on the surface. Observations indicate that the magnetic field is filamentary and intermittent a
Externí odkaz:
http://arxiv.org/abs/1303.0563
Autor:
Cranmer, Steven R., Asgari-Targhi, Mahboubeh, Miralles, Mari Paz, Raymond, John C., Strachan, Leonard, Tian, Hui, Woolsey, Lauren N.
Publikováno v:
Philosophical Transactions: Mathematical, Physical and Engineering Sciences, 2015 May . 373(2041), 1-16.
Externí odkaz:
http://www.jstor.org/stable/24506214
Akademický článek
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Autor:
Cranmer SR; Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138, USA Laboratory for Atmospheric and Space Physics, Department of Astrophysical and Planetary Sciences, University of Colorado, Boulder, CO 8030, USA scranmer@cfa.harvard.edu., Asgari-Targhi M; Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138, USA., Miralles MP; Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138, USA., Raymond JC; Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138, USA., Strachan L; Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138, USA., Tian H; Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138, USA., Woolsey LN; Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138, USA.
Publikováno v:
Philosophical transactions. Series A, Mathematical, physical, and engineering sciences [Philos Trans A Math Phys Eng Sci] 2015 May 13; Vol. 373 (2041).