1.4k citations · 5.7k across the 81 of their papers we have counts for
9 papers · 1 filter
Estimating the "Dark" Energy Content of the Solar Corona
Scott W. McIntosh, Bart De Pontieu
The discovery of ubiquitous low-frequency (3-5mHz) Alfvenic waves in the solar chromosphere (with Hinode/SOT), and corona (with CoMP and the Solar Dynamics Observatory, SDO) has pr…
Persistent Doppler shift oscillations observed with HINODE/EIS in the solar corona: spectroscopic signatures of Alfvenic waves and recurring upflows
Hui Tian, Scott W. McIntosh, Tongjiang Wang +4
Using data obtained by the EUV Imaging Spectrometer (EIS) onboard Hinode, we have per- formed a survey of obvious and persistent (without significant damping) Doppler shift oscilla…
The chromosphere and prominence magnetometer
Alfred G. de Wijn, Christian Bethge, Steven Tomczyk +1
The Chromosphere and Prominence Magnetometer (ChroMag) is conceived with the goal of quantifying the intertwined dynamics and magnetism of the solar chromosphere and in prominences…
Recent Observations of Plasma and Alfvenic Wave Energy Injection at the Base of the Fast Solar Wind
Scott W. McIntosh
We take stock of recent observations that identify the episodic plasma heating and injection of Alfvenic energy at the base of fast solar wind (in coronal holes). The plasma heatin…
Propagating Disturbances in Coronal Loops: A Detailed Analysis of Propagation Speeds
G. Kiddie, I. De Moortel, G. Del Zanna +2
Quasi-periodic disturbances have been observed in the outer solar atmosphere for many years now. Although first interpreted as upflows (Schrijver et al. (1999)), they have been wid…
On The Doppler Velocity of Emission Line Profiles Formed in the "Coronal Contraflow" that is the Chromosphere-Corona Mass Cycle
Scott W. McIntosh, Hui Tian, Marybeth Sechler +1
This analysis begins to explore the complex chromosphere-corona mass cycle using a blend of imaging and spectroscopic diagnostics. Single Gaussian fits to hot emission line profile…