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| Author | : National Solar Observatory/Sacramento Peak. Summer Workshop |
| Publisher | : |
| Total Pages | : 598 |
| Release | : 1989 |
| Genre | : Solar telescopes |
| ISBN | : |
| Author | : National Solar Observatory/Sacramento Peak Summer Workshop |
| Publisher | : |
| Total Pages | : 366 |
| Release | : 2006 |
| Genre | : |
| ISBN | : 9781583812884 |
| Author | : C. Denker |
| Publisher | : |
| Total Pages | : |
| Release | : 1999 |
| Genre | : Interferometry |
| ISBN | : |
| Author | : Oddbjørn Engvold |
| Publisher | : Elsevier |
| Total Pages | : 522 |
| Release | : 2018-11-15 |
| Genre | : Science |
| ISBN | : 0128143355 |
The Sun as a Guide to Stellar Physics illustrates the significance of the Sun in understanding stars through an examination of the discoveries and insights gained from solar physics research. Ranging from theories to modeling and from numerical simulations to instrumentation and data processing, the book provides an overview of what we currently understand and how the Sun can be a model for gaining further knowledge about stellar physics. Providing both updates on recent developments in solar physics and applications to stellar physics, this book strengthens the solar–stellar connection and summarizes what we know about the Sun for the stellar, space, and geophysics communities. Applies observations, theoretical understanding, modeling capabilities and physical processes first revealed by the sun to the study of stellar physics Illustrates how studies of Proxima Solaris have led to progress in space science, stellar physics and related fields Uses characteristics of solar phenomena as a guide for understanding the physics of stars
| Author | : F. Sánchez |
| Publisher | : Cambridge University Press |
| Total Pages | : 274 |
| Release | : 1992 |
| Genre | : Science |
| ISBN | : 9780521402514 |
First Canary Islands Winter School Workshop in which four internationally respected scientists write on solar physics.
| Author | : |
| Publisher | : |
| Total Pages | : |
| Release | : 1999 |
| Genre | : |
| ISBN | : |
Until relatively recent advances in technology, astronomical observations from the ground were limited in image resolution by the blurring effects of earth's atmosphere. The blur extent, ranging typically from 0.5 to 2 seconds of arc at the best astronomical sights, precluded ground-based observations of the details of the solar system's moons, asteroids, and outermost planets. With the maturing of a high resolution image processing technique called speckle imaging the resolution limitation of the atmosphere can now be largely overcome. Over the past three years they have used speckle imaging to observe Titan, a moon of Saturn with an atmospheric density comparable to Earth's, Io, the volcanically active innermost moon of Jupiter, and Neptune, a gas giant outer planet which has continually changing planet-encircling storms. These observations were made at the world's largest telescope, the Keck telescope in Hawaii and represent the highest resolution infrared images of these objects ever taken.
| Author | : National Solar Observatory/Sacramento Peak. Summer Workshop |
| Publisher | : |
| Total Pages | : 608 |
| Release | : 1999 |
| Genre | : Science |
| ISBN | : |
| Author | : A. B. C. Walker |
| Publisher | : |
| Total Pages | : 48 |
| Release | : 1986 |
| Genre | : Government publications |
| ISBN | : |
| Author | : National Aeronautics and Space Administration (NASA) |
| Publisher | : Createspace Independent Publishing Platform |
| Total Pages | : 56 |
| Release | : 2018-06 |
| Genre | : |
| ISBN | : 9781720570929 |
This research contract investigating the radiative transfer and dynamic physics of the smallest observable magnetic structures in the solar photosphere. Due to the lack of a high-resolution visible light satellite instrument for solar studies, all data were acquired using ground-based instrumentation. The primary goal of the investigation was to understand the formation and evolution of "G-band bright points" in relation to the associated magnetic elements. G-band bright points are small (on the order of 100 kin or less in diameter) bright signatures associated with magnetic flux elements in the photosphere. They are seen in the A2A-X2 4308 A molecular bandhead of the CH radical ill the solar spectrum and offer the highest spatial resolution and highest contrast "tracers" of small magnetic structure on the Sun.Berger, Thomas E.Unspecified CenterMAGNETIC FIELD CONFIGURATIONS; RADIATIVE TRANSFER; SOLAR MAGNETIC FIELD; HIGH RESOLUTION; SUN; SPATIAL RESOLUTION; SOLAR SPECTRA; SIGNATURES; SATELLITE INSTRUMENTS; RADICALS; PHOTOSPHERE
| Author | : National Solar Observatory/Sacramento Peak. Summer Workshop |
| Publisher | : |
| Total Pages | : 504 |
| Release | : 2003 |
| Genre | : Science |
| ISBN | : |
