High spatial resolution solar observations
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High spatial resolution solar observations proceedings of the Tenth Sacramento Peak Summer Workshop, Sunspot, New Mexico, 22-26 August 1988

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Published by National Solar Observatory in Sunspot, N.M .
Written in English


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Edition Notes

Statementedited by Oskar von der Luhe.
ID Numbers
Open LibraryOL18082816M

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  High spatial resolution observations of solar flares at mm wavelength. Author links open overlay panel M.R. Kundu ∗ S.M. White ∗ W.J. Welch ∗∗ J.H. Bieging ∗∗Cited by: Part of the Astrophysics and Space Science Library book series (ASSL, volume and consequently high spatial resolution observations are necessary to understand the physics of the Sun. These observations must be complemented by an equally important high-resolution spectroscopic analysis, including polarimetric measurements to determine the Cited by: 2. adshelp[at] The ADS is operated by the Smithsonian Astrophysical Observatory under NASA Cooperative Agreement NNX16AC86AAuthor: M. R. Kundu. The Case for High Resolution in Solar Physics: 1: Thomas, J. Small Scale Magnetic Flux Tubes in the Photosphere: A Simulation Perspective: Steiner, O. Dynamics of Magnetic Elements in the Photosphere and the Formation of Spicules: van Ballegooijen, A. A.; Nisenson, P. High Resolution Observations of the Dynamics of Magnetic Elements:

To achieve high spatial resolution capability for IR solar observations, we suggest the use of a special mask placed before the entrance aperture of large conventional optical telescopes. Such a mask would match well the resolution of a non-redundant array and would provide safe operation of a large telescope used for solar observations. The proposed solution has the additional advantage of. High Resolution in Solar Physics High resolution solar observations. Alan Title. Pages Adaptive image stabilization of solar observations: A review The interest of simultaneous spectral and spatial high resolution spectroscopy in the infrared. L. Delbouille, N. Grevesse, A. J. Sauval.   The recent expansion of the SuperDARN coverage to polar latitudes provides a new opportunity to perform high spatial resolution observations of ULF waves occurring within the polar caps. 2 Instrumentation. This work utilizes data from the McMurdo (MCM), Dome C East (DCE), South Pole Station (SPS), and Zhongshan (ZHO) SuperDARN radars.   This site uses cookies. By continuing to use this site you agree to our use of cookies. To find out more, see our Privacy and Cookies policy.

High Spatial Resolution Solar Microwave Observations High Spatial Resolution Solar Microwave Observations Marsh, K. A.; Hurford, G. J. Optical, UV, EUV and soft X-ray observations have revealed that the solar atmosphere is spatially inhomogeneous, with many of the morphological features (e.g. supergranulation, X-ray bright points, spicules, sunspots, flares) having spatial.   L. Rouppe van der Voort, M. van Noort, M. Carlsson, et spatial resolution observations of solar magnetic structures Solar MHD Theory and Observations: A High Spatial Resolution Perspective ASP Conference Series, vol. (), pp. HIGH SPATIAL RESOLUTION OBSERVATIONS OF LOOPS IN THE SOLAR CORONA David H. Brooks 1,4, Harry P. Warren2, Ignacio Ugarte-Urra, and Amy R. Winebarger3 1 College of Science, George Mason University, University Drive, Fairfax, VA , USA 2 Space Science Division, Naval Research Laboratory, Washington, DC , USA. The effects of atmospheric turbulence on solar observations are reviewed, and methods that achieve high angular resolution on the Sun, such as adaptive optics and interferometry, are discussed. Some experiments that provide solar observations of high spatial resolution are presented.