activity
20102022
most citedMeasuring the magnetic field of a trans-equatorial loop system using coronal seismology

57 citations · 201 across the 8 of their papers we have counts for

collaborators

9 papers

astro-ph.SR2022

Scaling Laws of Quiet-Sun Coronal Loops

C. Mac Cormack, M. López Fuentes, C. H. Mandrini +3

We study a series of relations between physical parameters in coronal loops of the quiet Sun reconstructed by combining tomographic techniques and modeling of the coronal magnetic…

astro-ph.SR2022★ 5 cited

Enthalpy-based modeling of tomographically reconstructed quiet-Sun coronal loops

C. Mac Cormack, M. López Fuentes, C. H. Mandrini +2

The structure of the solar corona is made of magnetic flux tubes or loops. Due to the lack of contrast with their environment, observing and studying coronal loops in the quiet Sun…

astro-ph.SR2017★ 57 cited

Measuring the magnetic field of a trans-equatorial loop system using coronal seismology

David M. Long, Gherardo Valori, David Pérez-Suárez +2

"EIT waves" are freely-propagating global pulses in the low corona which are strongly associated with the initial evolution of coronal mass ejections (CMEs). They are thought to be…

astro-ph.SR2015★ 28 cited

Parallel Evolution of Quasi-separatrix Layers and Active Region Upflows

C. H. Mandrini, D. Baker, P. Démoulin +6

Persistent plasma upflows were observed with Hinode's EUV Imaging Spectrometer (EIS) at the edges of active region (AR) 10978 as it crossed the solar disk. We analyze the evolution…

astro-ph.SR2015★ 20 cited

Multimodal Differential Emission Measure in the Solar Corona

Federico A. Nuevo, Alberto M. Vásquez, Enrico Landi +1

The Atmospheric Imaging Assembly (AIA) telescope on board the Solar Dynamics Observatory (SDO) provides coronal EUV imaging over a broader temperature sensitivity range than the pr…

astro-ph.SR2015

Seeing The Solar Corona in Three Dimensions

Alberto Marcos Vásquez

The large availability and rich spectral coverage of today's observational data of the solar corona, and the high spatial and temporal resolution of many instruments, has enabled t…

astro-ph.SR2014★ 28 cited

How Can Active Region Plasma Escape into the Solar Wind from below a Closed Helmet Streamer?

C. H. Mandrini, F. A. Nuevo, A. M. Vásquez +6

Recent studies show that active-region (AR) upflowing plasma, observed by the EUV-Imaging Spectrometer (EIS), onboard Hinode, can gain access to open field-lines and be released in…

astro-ph.SR2012★ 25 cited

Newly Discovered Global Temperature Structures in the Quiet Sun at Solar Minimum

Zhenguang Huang, Richard A. Frazin, Enrico Landi +3

Magnetic loops are building blocks of the closed-field corona. While active region loops are readily seen in images taken at EUV and X-ray wavelengths, quiet Sun loops are seldom i…

astro-ph.SR2010★ 38 cited

The WHI Corona from Differential Emission Measure Tomography

Alberto M. Vásquez, Zhenguang Huang, Ward B. Manchester +1

A three dimensional (3D) tomographic reconstruction of the local differential emission measure (LDEM) of the global solar corona during the whole heliosphere interval (WHI, Carring…