28 citations · 126 across the 7 of their papers we have counts for
8 papers
Measured energy exchange in coronal hole solar wind from its solar origins to the heliosphere
Yeimy J. Rivera, Alin R. Paraschiv, Samuel T. Badman +33
Coordinated ground- and space-based remote observations are used to provide a comprehensive, multi-perspective view of the solar atmosphere that we connect with in situ measurement…
Three-Dimensional Reconstruction and Thermal Modelling of Observed Loops
F. A. Nuevo, C. Mac Cormack, M. López Fuentes +2
Due to their characteristic temperature and density, loop structures in active regions (ARs) can be seen bright in extreme ultraviolet (EUV) and soft X-ray images. The semiempirica…
Thermodynamic Structure of the Solar Corona: Tomographic Reconstructions and MHD Modeling
D. G. Lloveras, A. M. Vásquez, F. A. Nuevo +5
We carry out a study of the global three-dimensional (3D) structure of the electron density and temperature of the quiescent inner solar corona () by means of tomog…
Energy Input Flux in the Global Quiet-Sun Corona
C. Mac Cormack, A. M. Vásquez, M. López Fuentes +3
We present first results of a novel technique that provides, for the first time, constraints on the energy input flux at the coronal base () of the qui…
Mass Loss Evolution in the EUV Low Corona from SDO/AIA Data
Fernando M. López, Hebe Cremades, Federico A. Nuevo +2
We carry out an analysis of the evacuated mass from three coronal dimming regions observed by the {\it Atmospheric Imaging Assembly} (AIA) on board the {\it Solar Dynamics Observat…
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…
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…
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…