Results 11 to 20 of about 6,518 (160)
Solar Physics—the Chemistry of the Sun 1 [PDF]
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Joseph Norman Lockyer
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Solar Flares, the Solar Corona, and Solar Physics [PDF]
The Sun serves as the local physics laboratory for studying the suprathermal activity phenomena of stars. Scrutiny of the Sun has led to the discovery of a host of previously unknown physical effects, largely within the classical physics of Newton and Maxwell, but including quantum mechanics and lepton physics as well.
E. N. Parker
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Galactic cosmic rays and solar energetic particles (SEPs) with energies larger than 100 MeV/n are able to penetrate and charge the test masses of the LISA experiment. As this process constitutes one of the major sources of noise for the experiment, a small telescope of silicon detectors will be located on board the LISA PathFinder and, possibly, the ...
C. Grimani, H. Vocca
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The solar flare myth in solar-terrestrial physics [PDF]
Early observations of associations between solar flares and large non- recurrent geomagnetic storms, large {open_quote}solar{close_quote} energetic particle events, and transient shock wave disturbances in the solar wind led to a paradigm of cause and effect that gave flares a central position in the chain of events leading from solar activity to major
J. T. Gosling
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This year's annual UK Solar Physics meeting took place in Dublin from 7–11 April 2003, overlapping with the National Astronomy Meeting. R Erdelyi, L Fletcher and G J Doyle summarize.
R. Erdélyi, L. Fletcher, Ginny Doyle
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Review and comparison of MHD wave characteristics at the Sun and in Earth’s magnetosphere
Magnetohydrodynamic (MHD) waves play a crucial role in the plasma processes of stellar atmospheres and planetary magnetospheres. Wave phenomena in both media are known to have similarities and unique traits typical of each system.
Chelpanov M. A.+6 more
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Multiwave Siberian Radioheliograph
The article discusses characteristics, fundamental and applied tasks of the Siberian Radioheliograph that is developed at the ISTP SB RAS Radio Astrophysical Observatory and spectropolarimetric complex that measures the total flux of solar radio emission.
Altyntsev A.T.+13 more
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HF radio channel modeling by a waveguide approach
We present a modified method of HF radio channel modeling based on a waveguide approach. The waveguide approach represents the electromagnetic field of radiation inside the Earth—ionosphere waveguide as an eigenfunction series of a radial boundary ...
Kurkin V. I.+4 more
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Solar neutrinos: Solar physics and neutrino physics [PDF]
Abstract It is shown that the current solar neutrino situation, with results from the Homestake experiment, the Kamiokande experiment, GALLEX and SAGE is unfortunately still ambiguous. The differences between observations and the standard solar theory may still be due to either astrophysical inputs or new neutrino physics.
D.N. Schramm, D.N. Schramm, X. Shi
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