Results 121 to 130 of about 107,783 (198)

Observations of an increase in the flux from Tau A during occultation by the solar corona [PDF]

Flux increase from Tau A during solar corona ...
Erickson, W. C.
core   +1 more source

Connecting Solar Orbiter and L1 Measurements of Mesoscale Solar Wind Structures to Their Coronal Source Using the ADAPT-WSA Model

The Astrophysical Journal
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, Natalia Zambrana Prado, Irena Gershkovich, Nicholeen M. Viall, Peter Young, Therese A. Kucera, Susan T. Lepri, Stephanie L. Yardley, Jim M. Raines, Stefano A. Livi, Ryan M. Dewey   +10 more
doaj   +1 more source

Assessment of the pineapple drying with a forced convection solar-electrohydrodynamic dryer

Case Studies in Thermal Engineering
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, Ittichote Chuckpaiwong, Watcharapong Chookaew, Jetsadaporn Priyadumkol   +3 more
doaj   +1 more source

On the Origin of the Solar Wind [PDF]

Hydrodynamic mechanism of solar corona ...
Samokhin, M. V.
core   +1 more source

Solar Corona [PDF]

Science, 1883
openaire   +2 more sources

Coronal and chromospheric physics [PDF]

The Solar Maximum Mission support program is mentioned along with investigations of the solar corona, prominences, and chromosphere. The solar limb was studied using far infrared and submillimeter photometry.
Hall, D. N. B., Landman, D. A., Orrall, F. Q.   +2 more
core   +1 more source

Lyman alpha coronagraph research sounding rocket program [PDF]

The ultraviolet light coronagraph was developed and successfully flown on three rocket flights on 13 April 1979, 16 February 1980 and 20 July 1982. During each of these flights, the Ultraviolet Light Coronagraph was flown jointly with the White Light ...
Kohl, J. L., Parkinson, W. H.
core   +1 more source

A Parametric Study of Solar Wind Properties and Composition Using Fluid and Kinetic Solar Wind Models

The Astrophysical Journal
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, Alexis P. Rouillard, Michael A. Lavarra, Nicolas Poirier, Pierre-Louis Blelly, Jean-Baptiste Dakeyo, Viviane Pierrard, Victor Réville, Christian Vocks, Simon Thomas   +9 more
doaj   +1 more source

Kinetic Physics of the Solar Corona and Solar Wind

Living Reviews in Solar Physics, 2006
Kinetic plasma physics of the solar corona and solar wind are reviewed with emphasis on the theoretical understanding of the in situ measurements of solar wind particles and waves, as well as on the remote-sensing observations of the solar corona made by
Marsch Eckart
doaj  

Comprehensive Synthesis of Magnetic Tornado: Cospatial Incidence of Chromospheric Swirls and Extreme-ultraviolet Brightening

The Astrophysical Journal Letters
Magnetic tornadoes, characterized as impulsive Alfvén waves initiated by photospheric vortices in intergranular lanes, are considered efficient energy channels to the corona.
Hidetaka Kuniyoshi, Souvik Bose, Takaaki Yokoyama   +2 more
doaj   +1 more source