Discussion on the classification of fine structures in continua

Details Discussion on the classification of fine structures in continua Discussion on the classification of fine structures in continua

Mar 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986soph..104...41e&link_type=abstract

(CNR, Workshop on Radio Continua during Solar Flares, Duino, Italy, May 27-31, 1985) Solar Physics (ISSN 0038-0938), vol. 104, M

Physics

Continuous Spectra, Fine Structure, Solar Radio Emission, Solar Spectra, Classifications, Radio Spectra, Terminology

Scientific paper

In response to the need for greater clarity in the classification and terminology connected with fine structures in solar continuum emission at radio frequencies, the following recommendations were made: (1) the first name given to a particular type of fine structure should be the one used; (2) if different names originated from papers published simultaneously, the name which best meets the criteria of scientific style should be selected; (3) introduction of new names should occur only when previously unknown phenomena are detected; (4) when coining new names, only those terms which are relevant to solar radio physics and which give some information on the character of the phenomenon in question should be used; and (5) those who still strongly insist on using their own denotations should give reference to the origional designation.

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