activity
20062011
most citedObserving the Roots of Solar Coronal Heating - in the Chromosphere

290 citations · 790 across the 13 of their papers we have counts for

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Showing 2009Show all

5 papers · 1 filter

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…