Results 31 to 40 of about 150 (116)
A Drag-force Analysis of Solar Wind White-light Tracers in the Inner Heliosphere
We studied the propagation of blobs, which are a subset of density mesoscale structures observed in the solar corona. The detection of blobs in white-light data was performed during Solar Cycle 23.
Cynthia López-Portela +2 more
doaj +1 more source
We present an analysis of Wide-field Imager for Solar PRobe (WISPR) images of the near-Sun heliospheric current sheet (HCS) region from the Parker Solar Probe (PSP) in 2020 January and June.
Paulett C. Liewer +5 more
doaj +1 more source
We present a three-dimensional numerical model for the generation and evolution of the magnetic field in the solar convection zone, in which sunspots are produced and contribute to the cyclic reversal of the large-scale magnetic field. We then assess the
Rohit Kumar +3 more
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Radio Signature of the Strong Compression between a Streamer and a Coronal Hole Boundary
We present evidence of the first detection of the radio signature at metric wavelengths of the strong compression between a helmet streamer (HS) and the boundary of a coronal hole (CH) using radio observations from the Callisto MEXICO-LANCE and ALASKA ...
E. Aguilar-Rodriguez +10 more
doaj +1 more source
Imaging the Solar Corona from “Within”: A Cutting-edge Approach to Enhance PSP/WISPR Imagery
The unprecedented remote-sensing observations obtained by the Wide Field Imager for Solar Probe (WISPR) on board the Parker Solar Probe (PSP) from distances inside Mercury’s orbit are revolutionizing our perception of the fine-scale morphology and ...
Guillermo Stenborg +2 more
doaj +1 more source
The large-scale plasma density structure of the extended solar corona is a tracer of the underlying magnetic field configuration and dictates the structure of the solar wind in interplanetary space.
Liam T. Edwards +3 more
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The solar wind heavy ion composition in the ascending phases of the solar cycles 23 and 25
The approximately 11-year solar cycle has been shown to impact the heavy ion composition of the solar wind, even when accounting for streams of differing speeds; however, the heavy ion composition observed between the same specific phases of a past solar
D. T. Carpenter +8 more
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Coronal pseudostreamer flux systems have a specific magnetic configuration that influences the morphology and evolution of coronal mass ejections (CMEs) from these regions. Here we continue the analysis of the Wyper et al.
B. J. Lynch +13 more
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Can MHD Oscillations Modulate Quasi-periodic Plasma Release from Coronal Streamers?
Periodic density structures (PDS) in the slow solar wind are associated with quasi-periodic plasma release from coronal streamer and open–closed boundary regions, but the origin of their organization remains uncertain.
O. Podladchikova
doaj +1 more source

