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Outer atmospheres of cool stars observed with iue
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Baliunas, S. L. |
| Organization | The National Aeronautics and Space Administration (NASA) |
| Copyright Year | 1984 |
| Abstract | Ultrviolet observations of cool stars in conjuction with coronal X-ray or ground based chromospheric measurements, or both have served both to refine and define understanding of stellar activity. The sensitivity of IUE down to a reasonable limiting magnitude made accessible many different stars' ultraviolet spectra. Understanding of stellar activity throughout stellar atmospheres has progressed because observation in the ultraviolet range of particular stars can be done in great detail. |
| File Size | 793161 |
| File Format | |
| Alternate Webpage(s) | http://www.archive.org/details/nasa_techdoc_19850012658 |
| Archival Resource Key | ark:/13960/t39z9w97n |
| Language | English |
| Publisher Date | 1984-12-01 |
| Access Restriction | Open |
| Subject Keyword | Axisymmetric Flow Finite Element Method Interpolation Nozzle Flow Nozzle Geometry Three Dimensional Flow Weighting Functions Computational Fluid Dynamics Navier-stokes Equation Space Shuttle Main Engine Thrust Chambers Viscous Flow Cobalt Acetates Differential Equations Finite Difference Theory Ntrs Nasa Technical Reports Server (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
