Results 91 to 100 of about 9,774 (241)
Downstream structure and evolution of a simulated CME-driven sheath in the solar corona [PDF]
Y. C.-M. Liu +3 more
openalex +1 more source
Embracing the politics of transformation: Policy action as “battle‐settlement events”
Abstract Societal transformations for addressing climate change are intensely contested and at risk of resistance and backlash to ambitious policy action. But they are frequently modeled through heuristics such as S‐curves which abstract from such conflicts, assuming increasing returns to scale as a driver of transformations.
James Patterson, Matthew Paterson
wiley +1 more source
The suggestion is advanced that heating of the solar corona results from Landau damping of ion-acoustic waves generated in the motion of photospheric granules. Laboratory experiments relevant to the question of corona heating are discussed, together with the available observational information on the extent of energy deposition in the corona.
openaire +1 more source
Much of the dynamics of the ambient solar wind (SW) manifests at mesoscales—scales larger than kinetic but smaller than global structures. Mesoscale structures often form at the Sun, survive to 1 au, and are geoeffective.
Samantha Wallace +10 more
doaj +1 more source
Reconnection-generated Plasma Flows in the Quasi-separatrix Layer in Localized Solar Corona [PDF]
Sripan Mondal +10 more
openalex +1 more source
Assessment of the pineapple drying with a forced convection solar-electrohydrodynamic dryer
Drying assumes a pivotal role in the preservation of high-moisture products over extended durations. Despite the widespread utilization of solar dryers owing to their energy-efficient nature, they are often plagued by prolonged drying durations ...
Chakrit Suvanjumrat +3 more
doaj +1 more source
This paper provides a brief review of basic solar wind theory and makes use of the Laval nozzle analogy to elucidate the characteristic features of a solar wind driven by thermal and Alfven wave pressure. It is argued that there is a considerable body of evidence in favour of wave acceleration of high speed solar wind.
openaire +2 more sources
The Solar Helium Abundance in the Outer Corona Determined from Observations with SUMER/SOHO [PDF]
J. M. Laming, U. Feldman
openalex +1 more source
STITCH: A Subgrid-scale Model for Energy Buildup in the Solar Corona [PDF]
Joel Dahlin +2 more
openalex +1 more source
The physical processes in the solar corona that shape the solar wind remain an active research topic. Modeling efforts have shown that energy and plasma exchanges near the transition region play a crucial role in modulating solar wind properties ...
Paul Lomazzi +9 more
doaj +1 more source

