Distinguishing Solar Cycle Effects in Planetary Atmospheres

Details Distinguishing Solar Cycle Effects in Planetary Atmospheres Distinguishing Solar Cycle Effects in Planetary Atmospheres

Dec 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008agufmae13a0323a&link_type=abstract

American Geophysical Union, Fall Meeting 2008, abstract #AE13A-0323

Other

3304 Atmospheric Electricity, 3311 Clouds And Aerosols, 6207 Comparative Planetology, 6255 Neptune

Scientific paper

As solar radiation decreases with distance from the Sun, other sources of energy, such as ionization from galactic cosmic rays (GCR), assume a greater relative importance than at the terrestrial planets. Charged particle effects could therefore be more relevant to the formation of clouds and haze at the outer planets. The long-term solar modulation of Neptune's albedo is thought to be caused by either ion-induced nucleation of cloud-forming particles, or ultraviolet (UV) radiation effects on the colour of the clouds. On the basis of the 11 year solar cycle, the statistical evidence was slightly in favour of the UV mechanism, however distinguishing unambiguously between the two mechanisms will require more than the solar cycle variation alone. A 1.68 year quasi-periodicity, uniquely present at some times from heliospheric modulation of GCR, has previously been used to discriminate between solar UV and GCR effects in terrestrial data. The cosmic ray proton monitor data from both the Voyager spacecraft show this 1.68 year modulation during the 1980s when the spacecraft were close to the outer planets, indicating the possibility for applying a similar technique as far out as Neptune.

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