activity
20102019
most citedCoronal magnetic reconnection driven by CME expansion -- the 2011 June 7 event

69 citations · 191 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.SR20195 cited

Comprehensive Determination of the Hinode/EIS Roll Angle

Gabriel Pelouze, Frédéric Auchère, Karine Bocchialini +5

We present a new coalignment method for the EUV Imaging Spectrometer (EIS) on board the Hinode spacecraft. In addition to the pointing offset and spacecraft jitter, this method det…

astro-ph.SR201612 cited

Evolution of the Magnetic Field Distribution of Active Regions

Sally Dacie, Pascal Démoulin, Lidia van Driel-Gesztelyi +5

Aims. Although the temporal evolution of active regions (ARs) is relatively well understood, the processes involved continue to be the subject of investigation. We study how the ma…

astro-ph.SR201559 cited

FIP Bias Evolution in a Decaying Active Region

D. Baker, D. H. Brooks, P. Démoulin +4

Solar coronal plasma composition is typically characterized by first ionization potential (FIP) bias. Using spectra obtained by Hinode's EUV Imaging Spectrometer (EIS) instrument,…

astro-ph.SR201418 cited

The energetics of a global shock wave in the low solar corona

David M. Long, Deborah Baker, David R. Williams +3

As the most energetic eruptions in the solar system, coronal mass ejections (CMEs) can produce shock waves at both their front and flanks as they erupt from the Sun into the helios…

astro-ph.SR201428 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.SR201469 cited

Coronal magnetic reconnection driven by CME expansion -- the 2011 June 7 event

L. van Driel-Gesztelyi, D. Baker, T. Torok +10

Coronal mass ejections (CMEs) erupt and expand in a magnetically structured solar corona. Various indirect observational pieces of evidence have shown that the magnetic field of CM…