A 2.84 GHz ms-resolution receiver and the question about the reliability of the 205 solar UFFS data taken with it

Details A 2.84 GHz ms-resolution receiver and the question about the reliability of the 205 solar UFFS data taken with it A 2.84 GHz ms-resolution receiver and the question about the reliability of the 205 solar UFFS data taken with it

Jul 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993soph..146..191l&link_type=abstract

Solar Physics, Volume 146, Issue 1, pp.191-197

Physics

1

Scientific paper

A query on the behaviour of a 2.84 GHz ms-resolution receiver developed by Jinet al. at the Beijing Astronomical Observatory (BAO) in the early 1980s is raised in this paper. As an inappropriate use of an electrically controlled attenuator (ECA) and a A/D converter in the receiver, taking an attenuation by 12 db (i.e., a factor of 16) in the intermediate frequency (IF) flux for the equivalent of a data shift to the right by 4 bits, along with other design defects, could have made artificial errors creep into the observations, we throw doubt upon the 205 published solar ultrafast fine structure (UFFS) data taken with such a receiver.

Affiliated with

Also associated with

No associations

Rating

A 2.84 GHz ms-resolution receiver and the question about the reliability of the 205 solar UFFS data taken with it 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 A 2.84 GHz ms-resolution receiver and the question about the reliability of the 205 solar UFFS data taken with it, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A 2.84 GHz ms-resolution receiver and the question about the reliability of the 205 solar UFFS data taken with it will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1232362