Wave Properties in the Upper Chromosphere and at the Base of the Corona
K. Bocchialini, J. C. Vial, S. Koutchmy
Abstract
K. Bocchialini, J. C. Vial, S. Koutchmy
Abstract
Abstract From a 83 min long sequence of observations of Ca II K and He I (1083 nm) line profiles, some dynamical properties of the main components of the quiet upper chromosphere are derived: for both the magnetic network and the internetwork, amplitude and phase spectra of the Doppler velocities are presented.
A significance statement is not available in the OpenAlex record.
A contribution statement is not available in the OpenAlex record.
Method details are not available in the OpenAlex metadata.
Findings are not separately available in the OpenAlex metadata.
Limitations are not available in the OpenAlex metadata.
Application details are not available in the OpenAlex metadata.
Abstract From a 83 min long sequence of observations of Ca II K and He I (1083 nm) line profiles, some dynamical properties of the main components of the quiet upper chromosphere are derived: for both the magnetic network and the internetwork, amplitude and phase spectra of the Doppler velocities are presented.
Key concepts: Chromosphere, QUIET, Corona (planetary geology), Amplitude, Physics, Spectral line, Astrophysics, Line (geometry)