Results 141 to 150 of about 13,652 (241)
Magnetic Rope Is an Electron Selector: Discovery in Space and Conceptual Application to Medicine
Abstract Magnetic rope is a helical structure existing ubiquitously in astrophysical and space plasmas. Such structure has been conventionally known to accelerate electrons, convert energy, and play key roles in driving solar eruptions. Here, in contrast to the conventional concept, we report that the magnetic rope can divert electrons efficiently in ...
H. S. Fu +8 more
wiley +1 more source
Energized Oxygen in the Magnetotail: Onset and Evolution of Magnetic Reconnection. [PDF]
George DE, Jahn JM.
europepmc +1 more source
Abstract Magnetosheath high‐speed jets with enhanced dynamic pressure are common in Earth's magnetosheath and can impinge on the magnetopause, driving pronounced boundary deformation. Recent observations indicate that shock–discontinuity interactions (SDIs) can generate magnetosheath jets, but the formation mechanism is still unclear.
Jin Guo +13 more
wiley +1 more source
Evolution of Magnetic Reconnection in an Electron-scale Current Sheet
Recently, a new type of magnetic reconnection, electron-only reconnection—where there is no obvious ion flow and heating—has been observed in various plasma environments.
Yundan Guan +3 more
doaj +1 more source
Direct observations of pure electron outflow in magnetic reconnection. [PDF]
Sakai K +23 more
europepmc +1 more source
Laboratory evidence of magnetic reconnection hampered in obliquely interacting flux tubes. [PDF]
Bolaños S +13 more
europepmc +1 more source
Magnetic skeletons and 3D magnetic reconnection
Electronic version does not contain additional mpeg filesThe upper atmosphere of the sun, the solar corona, is approximately 1,000,000K hotter than the surface of the Sun, a property which cannot be explained by the normal processes of heat conduction ...
Haynes, Andrew L.
core
The Location of Magnetic Reconnection at Earth's Magnetopause. [PDF]
Trattner KJ, Petrinec SM, Fuselier SA.
europepmc +1 more source
Alfvén waves play a significant role in solar coronal heating, solar wind acceleration, and Alfvénic turbulence formation. As a fundamental process, magnetic reconnection has long been credited as a crucial source of Alfvén waves.
Liping Yang +12 more
doaj +1 more source
Author Correction: Direct observations of pure electron outflow in magnetic reconnection. [PDF]
Sakai K +23 more
europepmc +1 more source

