Enhancement of the helium resonance lines in the solar atmosphere by suprathermal electron excitation - I. Non-thermal transport of helium ions
Far-Ultraviolet Continuum of G-Type Stars: A Signature of the Temperature Minimum Region
In the Trenches of the Solar-Stellar Connection. VII. Wilson-Bappu 2022
Mg II h + k Flux--Rotational Period Correlation for G-type Stars
Physical structure of the local interstellar medium
The Abundance of Interstellar Tin and Cadmium
The interstellar cloud surrounding the Sun: a new perspective
The Structure of the Local Interstellar Medium. I. High-Resolution Observations of Fe II, Mg II, and Ca II toward Stars within 100 Parsecs
The Structure of the Local Interstellar Medium. III. Temperature and Turbulence
The three-dimensional physical structure of the local interstellar medium
Instrument
HRS, HRS/1, HRS/2
Temporal Coverage
1996-08-18T04:04:10Z/1996-08-22T06:34:51Z
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, Jordan comma Carole, 1997, 'XI BOO A: STRUCTURE AND NON-THERMAL HEATING', 1.0, European Space Agency, https://doi.org/10.5270/esa-ktc8c48