Influence of unresolved optically-thin irregularities on quiet Sun magnetic field determinations.
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Almeida, J.
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1999
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Influence of Unresolved Optically-Thin Irregularities on Quiet Sun Magnetic Field DeterminationsObservations and theory both point out that the magnetic photosphere is not smooth but irregular at optically-thin scales. The relevance of these irregularities for a proper magnetic field diagnostics depends upon the not yet known structure of the magnetic field fluctuations (and, of course, on the purpose of our determination). Sánchez Almeida &Sánchez Almeida, J.
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Implementation of a Filter for the Restoration of Solar Granulation ImagesNot AvailableSánchez Cuberes, M. et al.
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How Binary Stars affect Galactic Chemical EvolutionAt least 60% of stars appear to be binary and about half of these are close enough to interact. Because of the enormous expansion on the AGB, many of these interactions will involve an AGB star and a relatively compact companion, anything from a low-mass main-sequence star to a degenerate remnant. Mass loss plays the dominant role in determiningTout, C. A. et al.
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High Spatial Resolution Imaging in Solar PhysicsPhysical processes in the Sun give rise to an ample variety of structures on different spatial scales that in many cases are very small, with sizes probably below the resolution limit of existing solar telescopes (see Sánchez Almeida, 1997; Sánchez Almeida and Bonet, 1997). Thus, the interpretation of solar phenomena requires the study of theseBonet, J. A.
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HI Observations of Early-Type GalaxiesNot Availabledel Río, M. S. et al.
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