Results 101 to 110 of about 280,119 (256)
While the amount of solar coronal energy flux leaving the “quiet” Sun, coronal holes, and active regions has been estimated by many, similar calculations for transients like coronal mass ejections (CMEs) based on observations are few. Using spectroscopic
R. Ramesh +5 more
doaj +1 more source
Improvements on coronal hole detection in SDO/AIA images using supervised classification
We demonstrate the use of machine learning algorithms in combination with segmentation techniques in order to distinguish coronal holes and filaments in SDO/AIA EUV images of the Sun.
Reiss Martin A. +7 more
doaj +1 more source
Abstract High tibial osteotomy is a key option for patients with unicompartmental overload or instability. Although coronal correction for varus deformity is well established, excessive posterior tibial slope (PTS) is increasingly recognized as a contributor to anterior cruciate ligament graft failure.
Julien Druel +5 more
wiley +1 more source
Interchange reconnection as the source of the fast solar wind within coronal holes. [PDF]
Bale SD +16 more
europepmc +1 more source
Abstract The anterior cruciate ligament (ACL) and anterolateral ligament (ALL) play key roles in maintaining rotational stability of the knee joint. Injuries that cause ACL tears have been shown to also frequently compromise the integrity of the ALL.
Taidhgin J. Keel +6 more
wiley +1 more source
The variation of coronal holes with solar cycle
Coronal holes are commonly known to be the source of the open magnetic flux and the high-speed solar wind. In EUV and X-ray emission lines, coronal holes are seen as the regions with reduced emission due to lower temperatures and electron density than ...
Chapman, Steven Anthony
core +6 more sources
Field-aligned currents are strongly modulated by corotating solar wind high-speed streams
Birkeland field-aligned currents (FACs) are associated with solar wind-magnetosphere energy coupling leading to substorms/convection events. FAC intensity enhancements have been studied during geomagnetic storms driven by interplanetary coronal mass ...
Hajra Rajkumar +8 more
doaj +1 more source
Automated coronal hole identification via multi-thermal intensity segmentation
Coronal holes (CH) are regions of open magnetic fields that appear as dark areas in the solar corona due to their low density and temperature compared to the surrounding quiet corona.
Garton Tadhg M. +2 more
doaj +1 more source
Quantifying the Consistency and Characterizing the Confidence of Coronal Holes Detected by Active Contours Without Edges (ACWE). [PDF]
Grajeda JA +4 more
europepmc +1 more source
Abstract Developmental hip dysplasia due to insufficient acetabular coverage and excessive pressure on the femoral head can easily lead to labral tears, damage to the labrum–cartilage junction, cam and pincer deformities, and joint capsule laxity. This may ultimately result in osteoarthritis.
Dongdong Zhou +7 more
wiley +1 more source

