Physical structure of the local interstellar medium
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 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
The Structure of the Local Interstellar Medium. V. Electron Densities
The three-dimensional physical structure of the local interstellar medium
Tomography/Power Spectrum Techniques for Removal of Fixed Pattern Noise from Hubble Space Telescope Spectra
Instrument
HRS, HRS/2
Temporal Coverage
1993-07-24T03:41:58Z/1993-07-24T15:11:28Z
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, Smith comma Andrew M., 1994, 'PHYSICAL PARAMETERS IN THE LOCAL INTERSTELLAR MEDIUM CYCLE 2', 1.0, European Space Agency, https://doi.org/10.5270/esa-iihqerv