collaborators

8 papers

astro-ph2007211 cited

Emergence of Small-Scale Magnetic Loops in the Quiet Sun Internetwork

R. Centeno, H. Socas-Navarro, B. Lites +11

We study the emergence of magnetic flux at very small spatial scales (less than 2 arcsec) in the quiet Sun internetwork. To this aim, a time series of spectropolarimetric maps was…

astro-ph2006129 cited

Spectral Line Selection for HMI: A Comparison of Fe I 6173 and Ni I 6768

A. A. Norton, J. Pietarila Graham, R. K. Ulrich +8

We present a study of two spectral lines, Fe I 6173 Angstroms and Ni I 6768 Angstroms, that were candidates to be used in the Helioseismic and Magnetic Imager (HMI) for observing D…

astro-ph2005

Evidence for Fine Structure in the Chromospheric Umbral Oscillation

R. Centeno, H. Socas-Navarro, M. Collados +1

Novel spectro-polarimetric observations of the \ion{He}{1} multiplet are used to explore the dynamics of the chromospheric oscillation above sunspot umbrae. The results presented h…

astro-ph2004

Motivation and Initial Results from SPINOR in the Near Infrared

H. Socas-Navarro, D. Elmore, W. Lites

SPINOR is a new spectro-polarimeter that will serve as a facility instrument for the Dunn Solar Telescope at the National Solar Observatory. This instrument is capable of achromati…

astro-ph2004

Shocks in the Quiet Solar Photosphere: A Rather Common Occurrence

H. Socas-Navarro, R. Manso

We present observations of the quiet solar photosphere in the \ion{Fe}{1} lines at 6302 Åwhere at least four different spatial locations exhibit upwards-directed supersonic flows.…

astro-ph2004

Strategies for Spectral Profile Inversion using Artificial Neural Networks

H. Socas-Navarro

This paper explores three different strategies for the inversion of spectral lines (and their Stokes profiles) using artificial neural networks. It is shown that a straightforward…