Bibcode
Pérez-Hernández, F.; Hill, F.; Braun, D. C.; Jain, K.; Tobiska, W. K.; González Hernández, I.; Díaz Alfaro, M.
Bibliographical reference
Solar Physics, Volume 289, Issue 2, pp.503-514
Advertised on:
2
2014
Journal
Citations
6
Refereed citations
4
Description
Solar magnetic indices are used to model the solar irradiance and
ultimately to forecast it. However, the observation of such indices is
generally limited to the Earth-facing hemisphere of the Sun. Seismic
maps of the far side of the Sun have proven their capability to locate
and track medium-large active regions at the non-visible hemisphere. We
present here the possibility of using the average signal from these
seismic far-side maps, combined with similarly calculated near-side
maps, as a proxy to the full-Sun magnetic activity.
Related projects
Helio and Astero-Seismology and Exoplanets Search
The principal objectives of this project are: 1) to study the structure and dynamics of the solar interior, 2) to extend this study to other stars, 3) to search for extrasolar planets using photometric methods (primarily by transits of their host stars) and their characterization (using radial velocity information) and 4) the study of the planetary
Savita
Mathur