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Ingersoll, A. P.

Publications and source records attributed to Ingersoll, A. P..

66 records · Page 4
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NASA NTRS1974

Lateral inhomogeneities in the Venus atmosphere - Analysis of thermal infrared maps

The thermal infrared maps of Venus published by Murray, Wildey, and Westphal (1963) and Westphal, Wildey, and Murray (1965) have been analyzed systematically in order to separate the observed intensity into a limb-darkening component and a solar-associated component representing fixed patterns of intensity corotating with the earth and sun, respectively. Interesting new results are obtained for the solar-associated component. Regions near the subsolar point and the poles are not covered in the original maps or in the analysis. The solar-associated pattern of intensity is very nearly symmetric about the equator. In both northern and southern hemispheres, an intensity minimum seems to occur near the morning terminator at middle to high latitudes, slightly beyond the limit of the maps. An intensity maximum occurs on the equator slightly to the east of the antisolar point.

Ingersoll, A. P.↗
NASA NTRS1973

Jupiter's Great Red Spot - A free atmospheric vortex

A simple hydrodynamic model yields steady-state solutions with many of the properties of the Great Red Spot and the neighboring belts and zones of Jupiter. No special forcing mechanism is necessary to maintain the circulation of the Spot. This is consistent with observations which indicate that the Great Red Spot and the zones have similar dynamic properties.

Ingersoll, A. P.↗
NASA NTRS1973

Faculae and the solar oblateness - A summary

Dicke and Goldenberg (1967) inferred a value of the solar oblateness by projecting an image of the sun on a circular occulting disk and measuring the light flux from the portion of the sun exposed beyond the disk. These measurements have the implication that if the optical oblateness measured is mirrored in a true gravitational oblateness, then the non-Newtonian part of Mercury's perihelion advance cannot agree with Einstein's prediction based on general relativity. The present analysis shows that faculae may have contributed all of Dicke and Goldenberg's excess signal. There is overwhelming evidence that this signal is contaminated by faculae at some level, and very little evidence to exclude faculae as a cause of the signal.

Chapman, G. A.↗
NASA NTRS1973

Faculae and the '25-day' solar fluctuation

The evidence presented suggests that the 25-d period of the fluctuation is caused, inadvertently, by the irregular nature of the observing pattern. The effects of irregular sampling as against regular sampling of the facular signal are compared in order to show that the characteristics of Dicke's (1972) fluctuations can be caused by the observing pattern provided that faculae are an important source of the excess solar oblateness.

Chapman, G. A.↗
NASA NTRS1973

Photospheric faculae and the solar oblateness - A reply to 'Faculae and the solar oblateness' by R. H. Dicke.

Dicke has recently contested our statement in an earlier paper that faculae could account for a large part, if not all, of the solar oblateness signal measured by Dicke and Goldenberg in 1966. Using the facular oblateness signal published in our earlier paper and some hitherto unpublished data from his 1966 observations, he concludes that faculae account for only a small part (11%) of the observed excess oblateness. His analysis considers data only from a restricted 48-day sample and is based on the assumption that only the observed oblateness signal is subject to error. Our analysis considers data from all 64 days on which observations were made, and is based on the assumption that both the observed oblateness signal and the facular signal are subject to error. We find that faculae account for at least one-third to one-half of the observed excess oblateness, depending on whether 48 days or 64 days are used in the analysis.

Chapman, G. A.↗
NASA NTRS1973

Radiative instability of a cloudy planetary atmosphere.

A cloudy planetary atmosphere at rest is shown to be unstable to disturbances of large horizontal scale. The energy source for the instability is the change in radiative heat flux associated with vertical displacement near the emitting level. A simple model is described in which the net heating rate in the cloud is proportional to the vertical displacement of the cloud. The constant of proportionality may be either positive or negative. Disturbances may take the form of either quasi-steady geostrophic motions or amplified inertia-gravity waves. The model is applied to Jupiter's zonal winds and to motions near the Venus cloud tops, and provides a possible explanation for many important features of these two flows.

Gierasch, P. J.↗
NASA NTRS1972

Photospheric faculae and the solar oblateness.

Dicke and Goldenberg (1967) on the basis of the value of the solar oblateness obtained had concluded that the excess perihelion motion of mercury is not in accord with Einstein's prediction according to general relativity. However, the observations from which the oblateness value was derived might be simply the result of an excess brightness at the equatorial solar limb. Such brightness might be due to the presence of faculae. Dicke (1970) had concluded that the effect of faculae on the oblateness determination is insignificant. In a reexamination of Dicke's argument it was found that his reasons for rejecting faculae as a source of oblateness are unjustified.

Chapman, G. A.↗
NASA NTRS1971

The atmospheres of Mars and Venus

Mars, Venus and earth atmospheres, considering abundance of volatiles such as carbon dioxide, water, oxygen, nitrogen, argon, carbon monoxide, chlorine and fluorine

Ingersoll, A. P.↗
NASA NTRS1969

Dynamics of Jupiter's cloud bands

Jupiter upper atmosphere cloud bands zonal motion velocities, examining barotropic stability criterion and geostrophic balance hypothesis

Cuzzi, J. N.↗