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The Evolving Magnetic Scales of the Outer Solar Atmosphere and Their Potential Impact on Heliospheric Turbulence
Scott W. McIntosh, Christian Bethge, James Threlfall +3
The presence of turbulent phenomena in the outer solar atmosphere is a given. However, because we are reduced to remotely sensing the atmosphere of a star with instruments of limit…
First comparison of wave observations from CoMP and AIA/SDO
J. Threlfall, I. De Moortel, S. W. McIntosh +1
Waves have long been thought to contribute to the heating of the solar corona and the generation of the solar wind. Recent observations have demonstrated evidence of quasi-periodic…
A Detailed Comparison Between The Observed and Synthesized Properties of a Simulated Type ii Spicule
Juan Martinez-Sykora, Bart De Pontieu, Jorrit Leenaarts +7
We performed a 3D radiative MHD simulation of the solar atmosphere. This simulation shows a jet-like feature that shows similarities to the type II spicules observed for the first…
Hemispheric Asymmetries of Solar Photospheric Magnetism: Radiative, Particulate, and Heliospheric Impacts
Scott W. McIntosh, Robert J. Leamon, Joseph B. Gurman +7
Among many other measurable quantities the summer of 2009 saw a considerable low in the radiative output of the Sun that was temporally coincident with the largest cosmic ray flux…