activity
20062009
most citedObserving the Roots of Solar Coronal Heating - in the Chromosphere

290 citations · 463 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.SR200934 cited

Estimating the Chromospheric Absorption of Transition Region Moss Emission

Bart De Pontieu, Viggo H. Hansteen, Scott W. McIntosh +1

Many models for coronal loops have difficulty explaining the observed EUV brightness of the transition region, which is often significantly less than theoretical models predict. Th…

astro-ph.SR2009290 cited

Observing the Roots of Solar Coronal Heating - in the Chromosphere

Bart De Pontieu, Scott W. McIntosh, Viggo H. Hansteen +1

The Sun's corona is millions of degrees hotter than its 5,000 K photosphere. This heating enigma is typically addressed by invoking the deposition at coronal heights of non-thermal…

astro-ph.SR2009

Interactions between reversed granulation, p-modes, and magnetism?

Alfred G. de Wijn, Scott W. McIntosh, Bart De Pontieu

We investigate features that are observed in Ca ii H sequences from Hinode in places where reversed granulation seems to interact with p-modes. These features appear ubiquitously i…

astro-ph.SR20091 cited

More of the Inconvenient Truth About Coronal Dimmings

Scott W. McIntosh, Joan Burkepile, Robert J. Leamon

We continue the investigation of a CME-driven coronal dimming from December 14 2006 using unique high resolution imaging of the chromosphere and corona from the Hinode spacecraft.…

astro-ph.SR20091 cited

What Goes Up Doesn't Necessarily Come Down! - Connecting the Dynamics of the Chromosphere and Transition Region with TRACE, Hinode and SUMER

S. W. McIntosh, Bart De Pontieu

We explore joint observations of the South-East limb made by Hinode, TRACE and SOHO/SUMER on April 12, 2008 as part of the Whole Heliosphere Interval (WHI) Quiet Sun Characterizati…

astro-ph200834 cited

A Coherence-Based Approach for Tracking Waves in the Solar Corona

Scott W. McIntosh, Bart De Pontieu, Steven Tomczyk

We consider the problem of automatically (and robustly) isolating and extracting information about waves and oscillations observed in EUV image sequences of the solar corona with a…