A Comparison of the Outer Atmosphere of the Flat Activity Star t Ceti (G8 V) with the Sun (G2 V) and a Centauri A (G2 V)
Constraints on the Structure of the Heliospheric Interface Based on Ly a Absorption Spectra
CoolCAT
Dependence of Heliospheric Lya Absorption on the Interstellar Magnetic Field
In the Trenches of the Solar-Stellar Connection. VI. Total EclipSS
Lya Absorption from Heliosheath Neutrals
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 emission line near 1319 A in solar and stellar spectra
The Magnetic Future of the Sun
The Outer Solar Atmosphere during the Maunder Minimum: A Stellar Perspective
UV and EUV observations of stellar coronal structure and activity
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA
Temporal Coverage
2000-08-01T02:44:14Z/2000-08-01T09:54:59Z
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, Saar et al., 2006, 'A Search for Acoustic Heating in the Chromospheres of Low Activity Dwarfs', 1.0, European Space Agency, https://doi.org/10.5270/esa-n592vei
