Physical Parameters in the Local Interstellar Medium Cycle 2

Details Physical Parameters in the Local Interstellar Medium Cycle 2 Physical Parameters in the Local Interstellar Medium Cycle 2

Jul 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992hst..prop.3941s&link_type=abstract

HST Proposal ID #3941

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Hst Proposal Id #3941

Scientific paper

Using the 10 (super 5) resolving power mode of the HRS it is proposed to observe neutral as well as multiply ionized species in the local interstellar medium at distances less than 50 pc from the Sun. The primary goal is to determine local hydrogen atom densities using fine structure populations in carbon and silicon atoms. Other goals are to determine electron densities from the populations of fine structure levels in C (super +) and S (super +) ions and to set limits on local gas temperatures by combining observations of line profiles, doppler parameters and ionization equilibria in atoms and first ions of carbon, silicon and magnesium.

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