Results 111 to 120 of about 36,388 (256)

Elemental Abundances at Coronal Hole Boundaries as a Means to Investigate Interchange Reconnection and the Solar Wind

open access: yesThe Astrophysical Journal
The origin of the slow solar wind is not well understood, unlike the fast solar wind that originates from coronal holes. In situ elemental abundances of the slow solar wind suggest that it originates from initially closed field lines that become open ...
Alexandros Koukras   +2 more
doaj   +1 more source

The non-negligible effect of magnetic holes on the magnitude-of-B magnetic power spectral density of the fast Alfvenic coronal-hole-origin solar wind at 1 AU

open access: yesFrontiers in Astronomy and Space Sciences
To estimate the effects of magnetic holes on the magnitude of B magnetic power spectral density, a 2-day interval of fast coronal-hole-origin plasma at 1 AU is examined. The magnetic holes are identified and removed from the magnetic time series, and the
Joseph E. Borovsky, Charles W. Smith
doaj   +1 more source

Parameters of the Magnetic Flux inside Coronal Holes

open access: yes, 2009
Parameters of magnetic flux distribution inside low-latitude coronal holes (CHs) were analyzed. A statistical study of 44 CHs based on Solar and Heliospheric Observatory (SOHO)/MDI full disk magnetograms and SOHO/EIT 284\AA images showed that the density
A.C. Balke   +51 more
core   +1 more source

Probing Upflowing Regions in the Quiet Sun and Coronal Holes. [PDF]

open access: yesSol Phys, 2021
Schwanitz C   +7 more
europepmc   +1 more source

Use of microsurfaced acellular dermal matrix for the generation of site‐appropriate keratinized tissue in soft tissue augmentation healing: Proof of concept

open access: yesClinical Advances in Periodontics, EarlyView.
Abstract Background Autogenous grafts remain the gold standard for soft tissue augmentation, but allogeneic dermal matrices (ADMs) offer a viable alternative. Limited cellular infiltration and neovascularization restrict ADM efficacy; this study investigates a novel microsurfaced ADM (MS‐ADM) designed to address these limitations. Methods This 180‐day,
Michael K. McGuire   +4 more
wiley   +1 more source

Microwave Bright Points with Multiple Periodic Oscillations in the Solar Polar Coronal Hole during Solar Cycle Minimum

open access: yesThe Astrophysical Journal
During solar cycle minimum, polar coronal holes show a prominent radio brightening cap. The analysis of polar microwave enhanced radiation in polar coronal holes is helpful for understanding the magnetic field characteristics and the origin of the solar ...
Jing Huang   +6 more
doaj   +1 more source

Velocity Structure of Jets in Coronal Hole

open access: yes, 2007
Velocity structures of jets in a coronal hole have been derived for the first time. Hinode observations revealed the existence of many bright points in coronal holes. They are loop-shaped and sometimes associated with coronal jets.
Culhane, Len   +6 more
core   +2 more sources

A guide to neuromodulation in drug‐resistant epilepsy

open access: yesEpileptic Disorders, EarlyView.
Abstract Neuromodulation is approved for the treatment of drug‐resistant epilepsy. It has been increasingly utilized over the past two decades with the approval of deep brain stimulation (DBS) and responsive neurostimulation (RNS) in addition to vagus nerve stimulation (VNS)—particularly in patients who are not deemed to be good resective surgical ...
Prachi Parikh   +10 more
wiley   +1 more source

Coronal and Chromospheric Dynamics of a Coronal Hole Bright Point

open access: yesThe Astrophysical Journal
Data from the Atmospheric Imaging Assembly (AIA) and the Helioseismic Magnetic Imager on board the Solar Dynamics Observatory and from the Interface Region Imaging Spectograph, are used to study the evolution at different atmospheric layers of a bright ...
Ana Cristina Cadavid, Mari Paz Miralles
doaj   +1 more source

Solar Origins of Short-Term Periodicities in Near-Earth Solar Wind and Interplanetary Magnetic Field

open access: yesApplied Sciences
This study investigates the solar origins of short-term periodicities in the near-Earth solar wind and interplanetary magnetic field (IMF) using long-term observations (1995–2024) and Potential Field Source Surface modeling.
Huichao Li   +5 more
doaj   +1 more source

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