Results 291 to 300 of about 509,189 (338)
The delayed arrival of faster solar energetic particles as a probe into the shock acceleration process. [PDF]
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Solar PhysicsSolar monitors on space platforms are discussed. Several experiments, utilizing different techniques for solar constants, spectral irradiance, and cross calibration carried out either on a space platform or a nearby satellite are included.
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2005
We present the fundamental equations which govern the physics of quiescent solar prominences. The mechanical equilibrium of prominences is described by the equations of magneto-hydrostatics. The radiative properties of the structures have to be modelled by non-LTE equations.
Heinzel, P., Anzer, U.
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We present the fundamental equations which govern the physics of quiescent solar prominences. The mechanical equilibrium of prominences is described by the equations of magneto-hydrostatics. The radiative properties of the structures have to be modelled by non-LTE equations.
Heinzel, P., Anzer, U.
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2020
Solar physics is one of the liveliest branches of astrophysics at the current time, with many major advances that have been stimulated by observations from a series of space satellites and ground-based telescopes as well as theoretical models and sophisticated computational experiments.
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Solar physics is one of the liveliest branches of astrophysics at the current time, with many major advances that have been stimulated by observations from a series of space satellites and ground-based telescopes as well as theoretical models and sophisticated computational experiments.
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Physics Bulletin, 1973
S-I Akasofu and S Chapman London: Oxford University Press 1972 pp xxiii + 901 price £25 During the last few years of his life Sydney Chapman was, among many other activities, collaborating with S-I Akasofu in writing a book on solar–terrestrial physics. A first draft was sent to the Clarendon Press in April, 1970; the final version was not completed by
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S-I Akasofu and S Chapman London: Oxford University Press 1972 pp xxiii + 901 price £25 During the last few years of his life Sydney Chapman was, among many other activities, collaborating with S-I Akasofu in writing a book on solar–terrestrial physics. A first draft was sent to the Clarendon Press in April, 1970; the final version was not completed by
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1977
Magnetic observatories monitor continuously the geomagnetic field at various latitudes and longitudes of the Earth. With the advent of rockets and satellites, it has been studied also in space.
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Magnetic observatories monitor continuously the geomagnetic field at various latitudes and longitudes of the Earth. With the advent of rockets and satellites, it has been studied also in space.
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Proceedings of the International Astronomical Union, 2004
Specific features of magnetic reconnection in solar flares are briefly reviewed and illustrated. In particular, the large-scale structure and dynamics of large flares are interpreted in terms of the rainbow reconnection model. The role of the betatron effect in collapsing magnetic traps is considered. To search for other articles by the author(s) go to:
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Specific features of magnetic reconnection in solar flares are briefly reviewed and illustrated. In particular, the large-scale structure and dynamics of large flares are interpreted in terms of the rainbow reconnection model. The role of the betatron effect in collapsing magnetic traps is considered. To search for other articles by the author(s) go to:
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Physics Bulletin, 1988
The European Space Agency has decided as a 'first cornerstone' of its programme for the next 20 years to finance new space satellites for studying solar and magnetospheric plasma physics, and UK scientists hope to play key roles in this project.
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The European Space Agency has decided as a 'first cornerstone' of its programme for the next 20 years to finance new space satellites for studying solar and magnetospheric plasma physics, and UK scientists hope to play key roles in this project.
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