Physics of Partial Ionization in the Solar Chromosphere Revealed by the Solar Optical Telescope Onboard Hinode

Chapter
Part of the Astrophysics and Space Science Library book series (ASSL, volume 449)

Abstract

The Solar Optical Telescope (SOT) onboard Hinode revealed that small-scale explosions and jet phenomena are common occurrences in the chromosphere and the photosphere of the Sun. Their morphology, dynamics, and associated time scales normalized by the local Alfvén speed are similar to those in the coronal microflares and jets driven by magnetic reconnection. However, the lower atmosphere has very different plasma parameters from the corona: the former is partially ionized and fully collisional, while the latter is fully ionized and almost collisionless. Thus the findings of the SOT pose an important question in plasma physics about how such fast magnetic reconnection similar to that in the corona is accommodated in the photosphere and the chromosphere? In this paper we will review the chromospheric observations by the SOT and their implications for the physics of partially ionized plasmas.

Keywords

Sun: photosphere Sun: chromosphere Partial ionization 

Notes

Acknowledgements

This work was partially supported by JSPS KAKENHI Grant Number 16H03955.

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Copyright information

© Springer Nature Singapore Pte Ltd. 2018

Authors and Affiliations

  1. 1.Graduate School of Advanced Integrated Studies in Human SurvivabilityKyoto UniversitySakyo-kuJapan

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