50 citations · 122 across the 6 of their papers we have counts for
6 papers · 1 filter
The S-Web Origin of Composition Enhancement in the Slow-to-Moderate Speed Solar Wind
B. J. Lynch, N. M. Viall, A. K. Higginson +3
Connecting the solar wind observed throughout the heliosphere to its origins in the solar corona is one of the central aims of heliophysics. The variability in the magnetic field,…
The Origin of Solar Filament Plasma Inferred from in situ Observations of Elemental Abundances
Hongqiang Song, Yao Chen, Bo Li +6
Solar filaments/prominences are one of the most common features in the corona, which may lead to energetic coronal mass ejections (CMEs) and flares when they erupt. Filaments are a…
Eruptions of Two Coupled Filaments Observed by SDO, GONG and STEREO
Z. K. Xue, X. L. Yan, Z. Q. Qu +2
On 2012 July 11, two solar filaments were observed in the northeast of the solar disk and their eruptions due to the interaction between them are studied by using the data from the…
Tracking Solar Active Region Outflow Plasma from its Source to the near-Earth Environment
J. L. Culhane, D. H. Brooks, L. van Driel-Gesztelyi +6
Seeking to establish whether active region upflow material contributes to the slow solar wind, we examine in detail the plasma upflows from Active Region (AR)10978, which crossed t…
Observation of Energetic particles between a pair of Corotating Interaction Regions
Z. Wu, Y. Chen, G. Li +11
We report observations of the acceleration and trapping of energetic ions and electrons between a pair of corotating interaction regions (CIRs). The event occurred in Carrington Ro…
Comparison of Two Solar Minima: Narrower Streamer Stalk Region and Conserved Open Magnetic Flux in the Region Outside of Streamer Stalk
Liang Zhao, Len Fisk
To explore the difference between the most two recent solar minima, we analyze the in-situ ACE and ULYSSES observations and examine the distributions of the three types of solar wi…