Results 201 to 210 of about 6,029 (233)
Some of the next articles are maybe not open access.

The Jovian period in the Sun?

Advances in Space Research, 2015
The 41-year measurements of the Doppler effect of the photosphere performed at the Crimean Astrophysical Observatory, discovered two periods of global oscillations of the Sun: 9600.606(12) s and 9597.929(15) s. Their beat period, 398.4(2.9) d, well agrees with a synodic orbital period of Jupiter, PJPJ = 398.9 d, raising a new problem for solar physics,
openaire   +2 more sources

Jovian sulfur nebula

Journal of Geophysical Research, 1977
We present further results of our observations of the nebula of singly ionized sulfur in the magnetosphere of Jupiter. We have calculated the occupation numbers of the five lowest energy levels of ionized sulfur and have used their results together with our observed intensities to evaluate the number density of ionized sulfur.
Irena Kupo, Yuri Mekler, Aharon Eviatar
openaire   +2 more sources

Jovian proton Aurora

Icarus, 1975
Auroral and polar cap emissions in a model Jovian atmosphere are determined for proton precipitation. The incident protons, which are characterized by representative spectra, are degraded in energy by applying the continuous slowing down approximation.
M.G. Heaps, B.C. Edgar, A. E. S. Green
openaire   +2 more sources

The Jovian Upper Atmosphere

1973
The upper atmosphere of Jupiter represents a refreshing change from the aeronomy of the terrestrial planets. The solar fluxes incident on it are smaller by a factor of 27 and the temperature and temperature gradients are correspondingly less than on the terrestrial planets.
openaire   +2 more sources

Jovian magnetospheric processes

AIP Conference Proceedings, 1986
Jupiter's rotational energy (6 x 10 to the 34th J) powers a large number of processes such as auroral UV emission, radio waves, and charged particle energization. How the rotational energy may be dissipated by injection of plasma, magnetic pumping and field aligned electric fields is described.
openaire   +2 more sources

Jovian and Saturnian satellites

Reviews of Geophysics, 1987
The years 1983‐1987 follow mankind's epochal first spacecraft encounters with the giant planets Jupiter and Saturn. Possibly the most spectacular “discoveries” there were the diversity and level of geological activity on the satellites that circle each.
openaire   +2 more sources

The Jovian Magnetosphere And Magnetopause

1976
It is convenient to divide the magnetosphere into three regions. The inner magnetosphere extends from the surface to about 25 7R J and is dominated by the basically dipolar field. The outer magnetosphere, on the sunward side, occupies a layer roughly 15R J thick just inside the magnetopause.
Davis, Leverett, Jr., Smith, E. J.
openaire   +3 more sources

Images of embedded Jovian planet formation at a wide separation around AB Aurigae

Nature Astronomy, 2022
Thayne Currie   +2 more
exaly  

Grand tours of the Jovian planets.

Journal of Spacecraft and Rockets, 1967
This preliminary analysis deals with the "Grand Tour" mission, comprising successive unpowered swingbys of each of the Jovian planets: Jupiter, Saturn, Uranus, and Neptune. The swingby technique allows the trip time to Neptune (as low as 8 years) to be greatly reduced from that of a comparable Hohmann transfer (30 years).
openaire   +3 more sources

Moist convection drives an upscale energy transfer at Jovian high latitudes

Nature Physics, 2022
Lia Siegelman   +2 more
exaly  

Home - About - Disclaimer - Privacy