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Investigating prominence turbulence with Hinode SOT Dopplergrams
Andrew Hillier, Takeshi Matsumoto, Kiyoshi Ichimoto
Quiescent prominences host a diverse range of flows, including Rayleigh-Taylor instability driven upflows and impulsive downflows, and so it is no surprise that turbulent motions a…
Chromospheric polarimetry through multi-line observations of the 850 nm spectral region
C. Quintero Noda, T. Shimizu, Y. Katsukawa +6
Future solar missions and ground-based telescopes aim to understand the magnetism of the solar chromosphere. We performed a supporting study in Quintero Noda et al. (2016) focused…
Analysis of a spatially deconvolved solar pore
C. Quintero Noda, T. Shimizu, B. Ruiz Cobo +3
Solar pores are active regions with large magnetic field strengths and apparent simple magnetic configurations. Their properties resemble the ones found for the sunspot umbra altho…
Spectropolarimetric capabilities of Ca II 8542 A line
C. Quintero Noda, T. Shimizu, J. de la Cruz Rodríguez +4
The next generation of space and ground-based solar missions aim to study the magnetic properties of the solar chromosphere using the infrared Ca II lines and the He I 10830 Å line…