Density Structure in Active Regions from Hinode/EIS

Details Density Structure in Active Regions from Hinode/EIS Density Structure in Active Regions from Hinode/EIS

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aspc..397...45t&link_type=abstract

First Results From Hinode ASP Conference Series, Vol. 397, Proceedings of the conference held 20-24 August, 2007, at Trinity Col

Astronomy and Astrophysics

Astronomy

2

Scientific paper

The Extreme-ultraviolet Imaging Spectrometer (EIS) on board Hinode provides an excellent opportunity to study the physical plasma parameters in spatially resolved coronal features. In this paper we present the density structure in an active region at many different temperatures. The active region was rastered on May 01, 2007 with the 2^{''} slit. We find that the electron density is highest in the core of the active region where it exceeds log_{10} N_e = 10.5.

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