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
Inhomogeneity within Local Interstellar Clouds
Lya Absorption from Heliosheath Neutrals
New Mass-Loss Measurements from Astrospheric Lya Absorption
Stellar Lya Emission Lines in the Hubble Space Telescope Archive: Intrinsic Line Fluxes and Absorption from the Heliosphere and Astrospheres
Suppressed Far-UV Stellar Activity and Low Planetary Mass Loss in the WASP-18 System
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA
Temporal Coverage
2003-03-23T08:27:03Z/2003-07-26T22:32:56Z
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, Saar comma Steven H., 2007, 'Exploring the Role of Acoustic Heating in Cool Dwarfs and Subgiants', 1.0, European Space Agency, https://doi.org/10.5270/esa-zizi0wt