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The temporal cadence of the time series is of 60 seconds and the starting date on April 11, 1996. (2015) and were updated as longer time series were available.

They were extracted from one-year (365 days) GOLF time series, with a four-time overlap (91.25 days).

This age has been confirmed by analysis of zircons in minerals, radiometric dating using a variety of elements and methods both with Earth rocks, lunar rocks and asteroid material.

It has further been verified by conclusions from the field of stellar evolution (helioseismic dating), which all confirm an age of approx.

Whenever helioseismology opens a new window into the solar interior, surprises are possible. (2) is perhaps the most notable helioseismology result since the launch of the Helioseismic and Magnetic Imager (HMI) (5) on board the National Aeronautics and Space Administration’s Solar Dynamics Observatory (SDO).

HMI measures the motions on the solar surface caused by the random superposition of seismic waves excited by near-surface convection.

He concurrently served as interim UCAR President for thirteen months form 2015 to 2016.

For a short overview of helioseismology, click here.

Michael's scientific research activity is principally in helioseismology, asteroseismology, solar physics, and inverse problems.

He has worked extensively over more than 25 years in developing and applying inverse techniques in helioseismology, and in particular measuring the stratification, rotation, and large-scale flows in the solar interior.

Solar turbulent convection is notoriously difficult to model across the entire convection zone, where the density spans many orders of magnitude. (2) use recent helioseismic observations to derive stringent empirical constraints on the amplitude of large-scale convective velocities in the solar interior.

They report an upper limit that is far smaller than predicted by a popular hydrodynamic numerical simulation.