Results 151 to 160 of about 962 (184)

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

Characteristics of Ionospheric Responses over China During the November 2023 Geomagnetic Storm and Evaluation of Positioning Performance of CORS in Low-Latitude Regions. [PDF]

Sensors (Basel)
Li L, Wang Y, Zhang J, Tang J, Yu F, Wang J, Zhang Z.   +6 more
europepmc   +1 more source

Direct imaging of magnetohydrodynamic wave mode conversion near a 3D null point on the sun. [PDF]

Nat Commun
Kumar P, Nakariakov VM, Karpen JT, Cho KS.   +3 more
europepmc   +1 more source

Algorithms and Resources for the Monitoring of Very-Low-Frequency Signal Deviations Due to Solar Activity Using a Web-Based Software-Defined Radio-Distributed Network. [PDF]

Sensors (Basel)
Iliev I, Tudjarov K, Nachev I, Petkov PZ, Velchev Y, Ilieva A.   +5 more
europepmc   +1 more source

Super-Intense Geomagnetic Storm on 10-11 May 2024: Possible Mechanisms and Impacts. [PDF]

Space Weather
Tulasi Ram S, Veenadhari B, Dimri AP, Bulusu J, Bagiya M, Gurubaran S, Parihar N, Remya B, Seemala G, Singh R, Sripathi S, Singh SV, Vichare G.   +12 more
europepmc   +1 more source

Observations and seismology of waves in solar filaments and coronal loops

, 2018
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Coronal heating and solar activity: The role of waves

Advances in Space Research, 1993
Abstract Coronal heating and solar activity are manifestations of the complex interaction between the magnetic field and the photospheric plasma motions. As a result of such an interaction magnetohydrodynamic waves are generated: their dissipation may provide the basic physical mechanism to heat the corona.
EINAUDI G, CHIUDERI C, CALIFANO, FRANCESCO   +2 more
openaire   +2 more sources

Alfvén waves in the solar polar coronal holes

AIP Conference Proceedings, 1999
We study the variation of the line width and electron density as a function of height above two coronal holes from forbidden spectral lines of Si VIII. The spectra were obtained with the Solar Ultraviolet Measurements of Emitted Radiation spectrometer flown on the Solar and Heliospheric Observatory spacecraft.
Banerjee, D., Teriaca, L., Doyle, J., Wilhelm, K.   +3 more
openaire   +2 more sources

Solar coronal heating by plasma waves

Journal of Plasma Physics, 2009
AbstractThe solar coronal plasma is maintained at temperatures of millions of degrees, much hotter than the photosphere, which is at a temperature of just 6000 K. In this paper, the plasma particle heating based on the kinetic theory of wave–particle interactions involving kinetic Alfvén waves and lower-hybrid drift modes is presented.
Bingham, R., Shukla, P.K., Eliasson, Bengt, Stenflo, L.   +3 more
openaire   +3 more sources