Solar astrometry: the status of art in 2011

TL;DR

This paper reviews the progress and current state of solar astrometry techniques used to measure the Sun's diameter and shape, emphasizing their importance for understanding solar properties and climate impact.

Contribution

It provides a comprehensive overview of the advancements in solar astrometry methods up to 2011 and discusses their relevance to solar physics and climate studies.

Findings

Multiple techniques have been developed for solar diameter measurement.

Space-based measurements are crucial for accurate solar irradiance data.

Solar astrometry significantly contributes to climate research understanding.

Abstract

Solar astrometry deals with the accurate measumerent of the solar diameter, and in general with the measurement of the shape of the Sun. During the last decades several techniques have been developed to monitor the radius and the irradiance of the Sun: meridian transits, telescopes in drift-scan mode, solar astrolabes, balloons, and satellites dedicated to the measurements of the solar diameter, and space measurements of the total solar irradiance are now performed to know the relationship radius-luminosity for the Sun in this evolutionary stage of its life. The feedback of solar astrometry in climate studies is of paramount importance. The status of art in the various fields of research here adressed is outlined.