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High resolution telescope and spectrograph (hrts)
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Moore, R. |
| Copyright Year | 1986 |
| Description | The major objectives of the high resolution telescope and spectrograph (HRTS) are: (1) the investigation of the energy balance and mass balance of the temperature minimum, chromosphere, transition zone, and corona in quiet regions on the Sun as well as in plages, flares, and sunspots; (2) the investigation of the velocity field of the lower corona to study the origin of the solar wind; and (3) the investigation of preflare and flare phenomena. The HRTS instruments consists of a telescope, an ultraviolet spectrograph, an ultraviolet spectroheliograph, and an H alpha slit display system, all housed in a thermal control cannister mounted on an instrument pointing system. |
| File Size | 42138 |
| Page Count | 1 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19860009882 |
| Archival Resource Key | ark:/13960/t2s51jh4v |
| Language | English |
| Publisher Date | 1986-01-01 |
| Access Restriction | Open |
| Subject Keyword | Spacecraft Instrumentation Solar Flares Display Devices Energy Distribution Mass Distribution Sun Spectroheliographs Space Stations Pointing Control Systems Ultraviolet Spectrometers Telescopes Spacelab Payloads Sunspots Solar Observatories Ntrs Nasa Technical Reports Server (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Article |
