HRTS observations of the fine structure and dynamics of the solar chromosphere and transition zone

Details HRTS observations of the fine structure and dynamics of the solar chromosphere and transition zone HRTS observations of the fine structure and dynamics of the solar chromosphere and transition zone

Nov 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983nascp.2280..33d&link_type=abstract

In JPL Solar Wind Five p 33-44 (SEE N84-13067 03-92)

Physics

Optics

Cassegrain Optics, Chromosphere, Magnetohydrodynamic Turbulence, Solar Wind, High Resolution, Limb Brightening, Plasma Jets, Solar Limb, Spatial Resolution

Scientific paper

Arc-second UV observations of the Sun by the NRL High Resolution Telescope and Spectrograph (HRTS) have led to the discovery of dynamic fine structures such as 400 km s-1 coronal jets and chromospheric jets (spicules) and have provided new information about the structure and dynamics of the transition zone. These observations are reviewed and their relevance to the origin of the solar wind is discussed.

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