Limits on the Local Interstellar Atomic Hydrogen Density Determined from Copernicus Observations of Chromospheric Emission Profiles of a Cool Star

Details Limits on the Local Interstellar Atomic Hydrogen Density Determined from Copernicus Observations of Chromospheric Emission Profiles of a Cool Star Limits on the Local Interstellar Atomic Hydrogen Density Determined from Copernicus Observations of Chromospheric Emission Profiles of a Cool Star

Jun 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975baas....7..418m&link_type=gif

Bulletin of the American Astronomical Society, Vol. 7, p.418

Astronomy and Astrophysics

Astronomy

Scientific paper

Not Available

Affiliated with

Also associated with

No associations

Rating

Limits on the Local Interstellar Atomic Hydrogen Density Determined from Copernicus Observations of Chromospheric Emission Profiles of a Cool Star does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Limits on the Local Interstellar Atomic Hydrogen Density Determined from Copernicus Observations of Chromospheric Emission Profiles of a Cool Star, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Limits on the Local Interstellar Atomic Hydrogen Density Determined from Copernicus Observations of Chromospheric Emission Profiles of a Cool Star will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-748866