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tokens: This work is dedicated to the memory of our friend and colleague, Mike Bradford. SDO data are provided courtesy of NASA/ SDO and AIA and HMI science teams. EUVI data are provided courtesy of the STEREO Sun Earth Connection Coronal and Heliospheric Investigation (SECCHI) team. FIRS has been developed by the Institute for Astronomy at the University of Hawai‘i, jointly with the National Solar Observatory (NSO). The FIRS project was funded by the National Science Foundation Major Research Instrument program, grant number ATM-0421582. T.A.S. gratefully acknowledges colleagues at the High Altitude Obseratory for interesting discussions regarding this work during a scientific visit. This work also benefited from discussions at the International Space Science Institute (ISSI) meetings on “Sub-arcsec Observations and Interpretation of the Chromosphere” and “Implications for Coronal Heating and Magnetic Fields from Coronal Rain Observations and Modelling.” This research has made use of NASA’s Astrophysics Data System. The authors thank the referee for a careful review and fruitful comments. Facilities: Dunn(FIRS) , SDO (AIA) , SDO (HMI) , STEREO (EUVI-A). Software: SSWIDL, SolarSoft, Crispex (Vissers Rouppe van der Voort 2012 ), HeLIx + (Lagg et al. 2004 ; Lagg 2007 ), PIKAIA (Charbonneau 1995 ).