The 3D solar corona Cycle 24 rising phase from SDO/AIA tomography

Autor:	Ward B. Manchester, Federico A. Nuevo, Richard A. Frazin, Zhenguang Huang, A. M. Vásquez
Rok vydání:	2011
Předmět:	Physics Space and Planetary Science Astrophysics::High Energy Astrophysical Phenomena Physics::Space Physics Astrophysics::Instrumentation and Methods for Astrophysics Phase (waves) Astrophysics::Solar and Stellar Astrophysics Astronomy Astronomy and Astrophysics Tomography
Zdroj:	Proceedings of the International Astronomical Union. 7:238-241
ISSN:	1743-9221 1743-9213
Popis:	We recently extended the differential emission measure tomography (DEMT) technique to be applied to the six iron bands of the Atmospheric Imaging Assembly (AIA) instrument aboard the Solar Dynamics Observatory (SDO). DEMT products are the 3D reconstruction of the coronal emissivity in the instrument's bands, and the 3D distribution of the local differential emission measure, in the height range 1.0 to 1.25 R⊙. We show here derived maps of the electron density and temperature of the inner solar corona during the rising phase of solar Cycle 24. We discuss the distribution of our results in the context of open/closed magnetic regions, as derived from a global potential field source surface (PFSS) model of the same period. We also compare the results derived with SDO/AIA to those derived with the Extreme UltraViolet Imager (EUVI) instrument aboard the Solar TErrestrial RElations Observatory (STEREO).
Databáze:	OpenAIRE
Externí odkaz:	https://explore.openaire.eu/search/publication?articleId=doi_________::f169e132f18ebf96c04ab251943b99c9 https://doi.org/10.1017/s1743921312004905 Zobrazit plný text záznamu Plný text ve formátu PDF