Results 151 to 160 of about 6,474 (200)

BepiColombo cruise science: overview of the mission contribution to heliophysics. [PDF]

Earth Planets Space
Sánchez-Cano B, Hadid LZ, Aizawa S, Murakami G, Bamba Y, Chiba S, Hara T, Heyner D, Ho G, Iwai K, Kilpua E, Kinoshita G, Lavraud B, Miyoshi Y, Pinto M, Schmid D, Shiota D, Vainio R, Andre N, Aronica A, Asmar S, Auster HU, Barabash S, Barthe A, Baumjohann W, Benkhoff J, Bentley M, Bunce E, Cappuccio P, Delcourt D, di Stefano I, Doria I, Dresing N, Fedorov A, Fischer D, Fiethe B, Fränz M, Gieseler J, Giner F, Giono G, Harada Y, Hussmann H, Iess L, Imamura T, Jeszenszky H, Jones G, Katra B, Kazakov A, Kozyrev A, Laky G, Lefevre C, Lichtenegger H, Lindsay S, Lucente M, Magnafico C, Magnes W, Martindale A, Matsuoka A, Milillo A, Mitrofanov I, Nishiyama G, Oleynik P, Orsini S, Paik M, Palmroos C, Plainaki C, Penou E, Persson M, Quarati F, Quémerais E, Richter I, Robidel R, Rojo M, Saito Y, Santoli F, Stark A, Stumpo M, Tian R, Varsani A, Verdeil C, Williamson H, Witasse O, Yokota S.   +82 more
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Experimental and Theoretical Study of Defect Evolution in InSb Epilayers under Gamma Irradiation: A Comparative Analysis of MOCVD vs MBE Growth Methods. [PDF]

ACS Omega
Marroquin JFR, Derc AC, Nascimento Lima E, de Oliveira ISS, Gunes M, Akyol M, Archanjo BS, de Azevedo WM, Henini M, Felix JF.   +9 more
europepmc   +1 more source

From Foreshock 30-Second Waves to Magnetospheric Pc3 Waves. [PDF]

Space Sci Rev
Turc L, Takahashi K, Kajdič P, Kilpua EKJ, Sarris T, Palmroth M, Soucek J, Pfau-Kempf Y, Dimmock A, Takahashi N.   +9 more
europepmc   +1 more source

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Multicolor photometry of outer Jovian satellites

Icarus, 1984
Multicolor photometry was obtained of satellites J6 Himalia, J7 Elara, and J10 Lysithea in the prograde cloud of outer Jovian satellites, and of J8 Pasiphae, J9 Sinope, and J11 Carme in the retrograde cloud. The data for J9 are fragmentary; otherwise, the satellites all look like C-class asteroids, except J11, which shows a remarkable brightness in the
David J. Tholen, B. Zellner
openaire   +3 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.
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Galilean Satellites and Jovian Energetic Particles

Science, 1975
The observed infrared temperatures of the four Galilean satellites, Io, Europa, Ganymede, and Callisto, are inconsistent with their equilibrium temperatures. Since these satellites appear to have little or no atmosphere, the discrepancies may be explained as due to the heating of their surfaces by energetic particles from Jupiter's radiation belts. The
openaire   +3 more sources

Erosion of Galilean Satellite Surfaces by Jovian Magnetosphere Particles

Science, 1981
The Galilean satellites of Jupiter—Io (J1), Europa (J2), Ganymede (J3), and Callisto (J4)—are embedded in the intense ion and electron fluxes of the Jovian magnetosphere. The effect of these particles on the icy surfaces of the outer three satellites depends on the fluxes and the efficiency of the sputtering of water ice by such particles.
R E, Johnson, L J, Lanzerotti, W L, Brown, T P, Armstrong   +3 more
openaire   +4 more sources

Angular momentum transfer to the inner Jovian satellites

Nature, 1975
Transfer of angular momentum from Jupiter to the four inner satellites in the presence of the Jovian magnetic field is considered. Electron-flux measurements near Io's flux tube and theoretical estimates of the electric currents flowing through the same flux tube are used to estimate the angular-momentum transfer during the evolutionary history of the ...
openaire   +3 more sources

Near-Infrared Observations of the Outer Jovian Satellites

Icarus, 2000
Abstract On September 21, 1998, the outer jovian satellites Himalia (J6), Elara (J7), Carme (J11), Pasiphae (J8), and Sinope (J9) were detected in the J , H , and K s bandpasses in the course of the Two-Micron All Sky Survey. Similarities in near-infrared colors are consistent with the hypothesis that the outer satellites in prograde orbits are ...
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Thermal history of the Jovian satellite Io

Icarus, 1987
Abstract The discovery of large volcanic eruptions on Io suggests that Io is one of the most geologically active planetary bodies. The energy source of this geologic activity is believed to be tidal heating induced by Jupiter. A number of thermal history calculations were done to investigate the effect of tidal heating on the thermal history of Io ...
Shin-Ichi Kawakami, Hitoshi Mizutani
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