Zodiacal light observed by HELIOS throughout solar cycle no. 21 - Stable dust and varying plasma

Details Zodiacal light observed by HELIOS throughout solar cycle no. 21 - Stable dust and varying plasma Zodiacal light observed by HELIOS throughout solar cycle no. 21 - Stable dust and varying plasma

Feb 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...210..399l&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 210, no. 1-2, Feb. 1989, p. 399-402.

Astronomy and Astrophysics

Astrophysics

11

Interplanetary Dust, Solar Cycles, Solar Wind, Space Probes, Zodiacal Light, Helios 1, Secular Variations

Scientific paper

The zodiacal light observations performed by the Helios space probes covered a period of more than 11 years, from December 1974 through February 1986. During this time no variation in zodiacal light brightness was detected, with limits of + or - 2 percent for secular variations. However, the density of solar wind at high heliographic latitudes showed a strong enhancement during the maximum of solar cycle.

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