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most citedPlanck 2015 results. XIII. Cosmological parameters

10.6k citations

Showing 2009 · astro-ph.SRShow all

6 papers · 2 filters

astro-ph.SR2009★ 63 cited

Turbulence, Complexity, and Solar Flares

R. T. James McAteer, Peter T. Gallagher, Paul A. Conlon

The issue of predicting solar flares is one of the most fundamental in physics, addressing issues of plasma physics, high-energy physics, and modelling of complex systems. It also…

astro-ph.SR2009★ 31 cited

TEXES Observations of M Supergiants: Dynamics and Thermodynamics of Wind Acceleration

G. M. Harper, M. J. Richter, N. Ryde +4

We have detected [Fe II] 17.94 um and 24.52 um emission from a sample of M supergiants using TEXES on the IRTF. These low opacity emission lines are resolved at R = 50, 000 and pro…

astro-ph.SR2009★ 24 cited

Reconstructing the 3-D Trajectories of CMEs in the Inner Heliosphere

Shane A. Maloney, Peter T. Gallagher, R. T. James McAteer

A method for the full three-dimensional (3-D) reconstruction of the trajectories of coronal mass ejections (CMEs) using Solar TErrestrial RElations Observatory (STEREO) data is pre…

astro-ph.SR2009★ 120 cited

Automated Coronal Hole Detection using Local Intensity Thresholding Techniques

Larisza D. Krista, Peter T. Gallagher

We identify coronal holes using a histogram-based intensity thresholding technique and compare their properties to fast solar wind streams at three different points in the heliosph…

astro-ph.SR2009★ 388 cited

A Critical Assessment of Nonlinear Force-Free Field Modeling of the Solar Corona for Active Region 10953

Marc L. DeRosa, Carolus J. Schrijver, Graham Barnes +16

Nonlinear force-free field (NLFFF) models are thought to be viable tools for investigating the structure, dynamics and evolution of the coronae of solar active regions. In a series…

astro-ph.SR2009★ 49 cited

The kinematics of coronal mass ejections using multiscale methods

Jason P. Byrne, Peter T. Gallagher, R. T. James McAteer +1

The diffuse morphology and transient nature of coronal mass ejections (CMEs) make them difficult to identify and track using traditional image processing techniques. We apply multi…