Astronomy and Astrophysics – Astronomy
Scientific paper
Jun 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982esasp.176..507p&link_type=abstract
In ESA 3rd European IUE Conf. p 507-512 (SEE N83-11889 02-88)
Astronomy and Astrophysics
Astronomy
Astronomical Observatories, Solar System, Spaceborne Astronomy, Ultraviolet Astronomy, Emission Spectra, Field Of View, Jupiter (Planet), Sensitivity, Spatial Resolution, Spectral Resolution
Scientific paper
The advantages of Earth orbiting observatories are outlined, taking investigation of the Jupiter-Io system as an example. The instrument requirements of such observatories are considered. Their wavelength range should be from 300 to 3000A with spectral resolution of a few hundredth A, and spatial resolution on the order of 1 arcsec. Their field of view and spatial resolution make simultaneous mapping of any extended system possible in a reasonable time for monochromatic emission lines and thus allow temporal survey. The spectral wavelength range and spectral resolution give access to the atomic (neutral and ionized) composition and thermodynamics.
No associations
LandOfFree
Observations in the solar system with the proposed Earth-orbiting observatory Magellan does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Observations in the solar system with the proposed Earth-orbiting observatory Magellan, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Observations in the solar system with the proposed Earth-orbiting observatory Magellan will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1353655