Results 101 to 110 of about 12,081 (211)

Magnetic Connectivity in the Time-dependent Corona and Heliosphere

The Astrophysical Journal Letters
Magnetic flux fills the heliosphere, expands outward from the solar corona, and is fundamentally related to the structure and dynamics of the solar corona and solar wind.
Roberto Lionello, Cooper Downs, Emily I. Mason, Jon A. Linker, Pete Riley, Mathew J. Owens   +5 more
doaj   +1 more source

On an Electrical Corona resembling the Solar Corona.

, 1876
(Uploaded by Plazi from the Biodiversity Heritage Library) No abstract provided.
openaire   +2 more sources

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

MHD mode conversion of fast and slow magnetoacoustic waves in the solar corona

, 2010
There are three main wave types present in the Sun’s atmosphere: Alfvén waves and fast and slow magnetoacoustic waves. Alfvén waves are purely magnetic and would not exist if it was not for the Sun’s magnetic field.
McDougall-Bagnall, A. M. Dee
core  

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

Effect of structuring on coronal loop oscillations

, 2007
In this Thesis the theoretical understanding of oscillations in coronal structures is developed. In particular, coronal loops are modelled as magnetic slabs of plasma.
McEwan, Michael P.
core  

Diagnostics of energetic electrons with anisotropic distributions in solar flares

, 2010
Aims. The paper aims are to simulate steady-state distributions of electrons beams precipitating in collisional and Ohmic losses with pitch angle anisotropy into a flaring atmosphere with converging magnetic field and to apply these to the interpretation
A. A. Kuznetsov, Siversky, Taras V., V. V. Zharkova, Zharkova, Valentina, T. V. Siversky, Kuznetsov, Alexey A.   +5 more
core   +1 more source

Solar wind Acceleration from the Upper Chromosphere to the Corona in Coronal Hole Regions

, 1998
The dynamic behavior of the plasma in the chromosphere/transition region /inner corona is vital for the acceleration of the solar wind. With new theoretical descriptions of the solar atmosphere and corona, and the increased observational possibilities ...
Esser, Ruth
core  

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

On the solar corona

, 1941
QC 20200430"Communicated February 26th 1941 by M. SIEGBAHN and B. LINDBLAD."
openaire   +2 more sources