Precise Timings of Galilean Satellite Eclipses and Assessment of the E5 Ephemeris

Icarus ◽  
2000 ◽  
Vol 147 (2) ◽  
pp. 348-352 ◽  
Author(s):  
A Mallama
Keyword(s):  
Galilean Satellite

Precise Timings of Galilean Satellite Eclipses and Assessment of the E-3 Ephemeris

Icarus ◽  
1994 ◽  
Vol 107 (1) ◽  
pp. 212-214 ◽  
Author(s):  
Anthony Mallama ◽  
Douglas S. Caprette ◽  
Peter Nelson ◽  
James Park ◽  
Donald F. Collins ◽  
...  
Keyword(s):  
Galilean Satellite

Observation and analysis of some recent Galilean satellite phenomena

1992 ◽  
Vol 58 (2) ◽  
pp. 105-114
Author(s):  
W. H. Allen ◽  
M. Loudon ◽  
E. Budding
Keyword(s):  
Galilean Satellite

Galilean satellite mission concepts

1982 ◽  
Author(s):  
J. SOLDNER ◽  
M. STANCATI ◽  
H. FEINGOLD
Keyword(s):  
Galilean Satellite ◽  
Satellite Mission

Galilean satellite tour orbit determination assessment

1987 ◽  
Author(s):  
B. MOULTRIE ◽  
P. KENYON ◽  
J. KECHICHIAN ◽  
R. DAVIS ◽  
F. NICHOLSON
Keyword(s):  
Orbit Determination ◽  
Galilean Satellite

Assessment of the resonant perturbation errors in Galilean satellite ephemerides using precisely measured eclipse times

Icarus ◽  
2010 ◽  
Vol 210 (1) ◽  
pp. 346-357 ◽  
Author(s):  
Anthony Mallama ◽  
Chris Stockdale ◽  
Bruce A. Krobusek ◽  
Peter Nelson
Keyword(s):  
Galilean Satellite

Erosion of Galilean Satellite Surfaces by Jovian Magnetosphere Particles

Science ◽  
1981 ◽  
Vol 212 (4498) ◽  
pp. 1027-1030 ◽  
Author(s):  
R. E. JOHNSON ◽  
L. J. LANZEROTTI ◽  
W. L. BROWN ◽  
T. P. ARMSTRONG
Keyword(s):  
Galilean Satellite ◽  
Jovian Magnetosphere

scholarly journals Atmospheric Properties of Jupiter Determined from Galilean Satellite Eclipse Light Curves

1974 ◽  
Vol 65 ◽  
pp. 401-405
Author(s):  
R. W. Shorthill ◽  
T. F. Greene ◽  
D. W. Smith
Keyword(s):  
Rayleigh Scattering ◽  
Normal Incidence ◽  
Scale Height ◽  
Light Curves ◽  
The Other ◽  
Galilean Satellite ◽  
Molecular Absorption ◽  
Galilean Satellites ◽  
Aerosol Distribution ◽  
Path Lengths

Twelve eclipse light curves for the Galilean satellites have been observed at 30 colors. The shape of the curves depend upon Jovian atmospheric properties such as Rayleigh scattering, aerosol distribution, molecular absorption, scale height and cloud top altitude, as well as the satellite diameter. Different zenographic latitudes and longitudes along the sunrise and sunset terminator have been observed. Very long absorption path lengths are obtained compared to normal incidence because of the tangential passage of the Sun's rays. Refractive tails are observed in most cases which allow aerosol distributions to be determined. The other atmospheric properties may also be derived.

The Effect of lo on Jupiter’s Decametric Emissions

1968 ◽  
Vol 1 (3) ◽  
pp. 81-82 ◽  
Author(s):  
P.M. McCulloch
Keyword(s):  
Galilean Satellite

The innermost Galilean satellite of Jupiter, Io, has been observed to strongly modulate the probability and intensity of Jupiter’s decametric emissions. The effect is most pronounced at frequencies greater than 30 MHz. Radiation occurs from two configurations of Jupiter and Io, the first when Io is 90° from superior geocentric conjunction (s.g.c.) and Jupiter’s longitude is near 120°, and the second when Io is 240° from s.g.c. and Jupiter’s longitude is near 230°.

Sign in / Sign up

Export Citation Format

Share Document