Results 161 to 170 of about 1,198,926 (208)

Global heliospheric termination shock strength in the solar-interstellar interaction. [PDF]

Nat Astron
Zirnstein EJ, Kumar R, Shrestha BL, Swaczyna P, Dayeh MA, Heerikhuisen J, Szalay JR.   +6 more
europepmc   +1 more source

Geomagnetic disturbances and grid vulnerability: Correlating storm intensity with power system failures. [PDF]

PLoS One
Figueroa MG, Acevedo DDH, Porta DS.
europepmc   +1 more source

Science development study for the Atacama Large Aperture Submillimeter Telescope (AtLAST): Solar and stellar observations. [PDF]

Open Res Eur
Wedemeyer S, Barta M, Brajša R, Chai Y, Costa J, Gary D, Gimenez de Castro G, Gunar S, Fleishman G, Hales A, Hudson H, Kirkaune M, Mohan A, Motorina G, Pellizzoni A, Saberi M, Selhorst CL, Simoes PJA, Shimojo M, Skokić I, Sudar D, Menezes F, White SM, Booth M, Klaassen P, Cicone C, Mroczkowski T, Cordiner MA, Di Mascolo L, Johnstone D, van Kampen E, Lee M, Liu D, Maccarone T, Orlowski-Scherer J, Saintonge A, Smith M, Thelen AE.   +37 more
europepmc   +1 more source

Space-climatic feedback of the magnetic solar cycle through the interplanetary space. [PDF]

Sci Rep
Carbone V, Alberti T, Reda R, Giovannelli L.   +3 more
europepmc   +1 more source

A solar cycle clock for extreme space weather. [PDF]

Sci Rep
Chapman SC, Dudok de Wit T.
europepmc   +1 more source

Differential effects of rice irrigation modes on hydrothermal environment and yield from the perspective of TOPSIS model. [PDF]

Sci Rep
Xuemei S, Siyu W, Yan H, Yanling S, Mo C.   +4 more
europepmc   +1 more source

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Coronal holes as sources of solar wind

Solar Physics, 1976
We investigate the association of high-speed solar wind with coronal holes during the Skylab mission by: (1) direct comparison of solar wind and coronal X-ray data; (2) comparison of near-equatorial coronal hole area with maximum solar wind velocity in the associated streams; and (3) examination of the correlation between solar and interplanetary ...
A F Timothy, A S Krieger, A J Lazarus
exaly   +2 more sources

Observations of the solar wind from coronal holes

Space Science Reviews, 1994
The solar wind emanating from coronal holes (CH) constitutes a quasi-stationary flow whose properties change only slowly with the evolution of the hole itself. Some of the properties of the wind from coronal holes depend on whether the source is a large polar coronal hole or a small near-equatorial hole.
exaly   +2 more sources

Coronal Holes in Solar Cycles 21 to 23

Solar Physics, 2013
We present identifications of coronal holes (CHs) from observations in the He i 10 830 A line made at Kitt Peak Observatory (from 1975 to 2003) and in the EUV 195 A wavelength with SOHO/EIT (from 1996 to 2012). To determine whether a feature is a CH we have developed semi-automatic techniques for delineating CH borders on synoptic charts and for ...
Valeriya Vasil'Eva
exaly   +2 more sources