activity
20152017
most citedSpatial deconvolution of spectropolarimetric data: an application to quiet Sun magnetic elements

36 citations · 88 across the 4 of their papers we have counts for

collaborators

7 papers

astro-ph.SR20177 cited

Detection of emission in the Si i 1082.7 nm line core in sunspot umbrae

D. Orozco Suarez, C. Quintero Noda, B. Ruiz Cobo +1

We analyze spectropolarimetric sunspot umbra observations taken in the near-infrared Si i 1082.7 nm line taking NLTE effects into account. The data were obtained with the GRIS inst…

astro-ph.SR201718 cited

Chromospheric polarimetry through multi-line observations of the 850 nm spectral region II: A magnetic flux tube scenario

C. Quintero Noda, Y. Kato, Y. Katsukawa +10

In this publication we continue the work started in Quintero Noda et al. (2017) examining this time a numerical simulation of a magnetic flux tube concentration. Our goal is to stu…

astro-ph.SR201727 cited

Solar polarimetry through the K I lines at 770 nm

C. Quintero Noda, H. Uitenbroek, Y. Katsukawa +9

We characterize the K I D1 & D2 lines in order to determine whether they could complement the 850 nm window, containing the Ca II infrared triplet lines and several Zeeman sensitiv…

astro-ph.SR2016

Analysis of a spatially deconvolved solar pore

C. Quintero Noda, T. Shimizu, B. Ruiz Cobo +3

Solar pores are active regions with large magnetic field strengths and apparent simple magnetic configurations. Their properties resemble the ones found for the sunspot umbra altho…

astro-ph.SR2016

Analysis of spatially deconvolved polar faculae

C. Quintero Noda, Y. Suematsu, B. Ruiz Cobo +2

Polar faculae are bright features that can be detected in solar limb observations and they are related to magnetic field concentrations. Although there is a large number of works s…

astro-ph.SR2016

Spectropolarimetric capabilities of Ca II 8542 A line

C. Quintero Noda, T. Shimizu, J. de la Cruz Rodríguez +4

The next generation of space and ground-based solar missions aim to study the magnetic properties of the solar chromosphere using the infrared Ca II lines and the He I 10830 Å line…