Constraints on the Structure of the Heliospheric Interface Based on Ly a Absorption Spectra
CoolCAT
Coronal Emission Measures and Abundances for Moderately Active K Dwarfs Observed by Chandra
Dependence of Heliospheric Lya Absorption on the Interstellar Magnetic Field
Heliospheric, Astrospheric, and Interstellar Lya Absorption toward 36 Ophiuchi
Hydrogen Lya Absorption Predictions by Boltzmann Models of the Heliosphere
In the Trenches of the Solar-Stellar Connection. VII. Wilson-Bappu 2022
Lya Absorption in a Croissant-like Heliosphere
Measured Mass-Loss Rates of Solar-like Stars as a Function of Age and Activity
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
Two New Low Galactic D/H Measurements from the Far Ultraviolet Spectroscopic Explorer
What Is the Total Deuterium Abundance in the Local Galactic Disk?
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA, STIS/NUV-MAMA
Temporal Coverage
1999-10-10T05:28:52Z/1999-10-10T11:05:18Z
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, Linsky comma Jeffrey L., 2006, 'Exploring the Outer Heliosphere with STIS', 1.0, European Space Agency, https://doi.org/10.5270/esa-2te2923
