A Far-Ultraviolet Spectroscopic Survey of Luminous Cool Stars
Constraints on the Structure of the Heliospheric Interface Based on Ly a Absorption Spectra
Dependence of Heliospheric Lya Absorption on the Interstellar Magnetic Field
Inhomogeneity within Local Interstellar Clouds
Space Telescope Imaging Spectrograph Survey of Far-Ultraviolet Coronal Forbidden Lines in Late-Type Stars
Stellar Lya Emission Lines in the Hubble Space Telescope Archive: Intrinsic Line Fluxes and Absorption from the Heliosphere and Astrospheres
The Remarkable Far-Ultraviolet Spectrum of FK Comae Berenices: King of Spin
The Structure of the Local Interstellar Medium. III. Temperature and Turbulence
The Structure of the Local Interstellar Medium. II. Observations of D I, C II, N I, O I, Al II, and Si II toward Stars within 100 Parsecs
UV and EUV observations of stellar coronal structure and activity
What Is the Total Deuterium Abundance in the Local Galactic Disk?
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA
Temporal Coverage
2001-03-13T13:33:04Z/2001-09-25T15:01:56Z
Version
1.0
Mission Description
Launched in 1990, the NASA/ESA Hubble Space Telescope remains the premier UV and visible light telescope in orbit. With well over 1.6 million observations from 10 different scientific instruments, the ESA Hubble Science Archive is a treasure trove of astronomical data to be exploited.
European Space Agency, Ayres comma Thomas R., 2006, 'Tortured Coronae in the Rapid Breaking Zone', 1.0, European Space Agency, https://doi.org/10.5270/esa-zjxy0ss