Detection of a significant change in the solar diameter

Details Detection of a significant change in the solar diameter Detection of a significant change in the solar diameter

May 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993soph..145..205w&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 145, no. 1, p. 205, 206.

Physics

17

Size Determination, Solar Diameter, Optimization, Solar Activity

Scientific paper

It is found that drift-time measurements of the solar diameter made at Izana, Tenerife, and Locarno, Switzerland, during 1990-1992 show a significant increase of the observed angular semidiameter when compared to results obtained at the same sites in 1981. The observed increase of about 0.4 arsec is not due to a systematic or long-term variation, but reflects a more complicated behavior over time. It is argued that a variation in phase with solar activity can be ruled out.

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