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At least 91 records · Page 5Linked to original sources
PubMed1997

The response of Jupiter's magnetosphere to an outburst on Io.

A 6-month-long monitoring campaign of the Io plasma torus and neutral cloud was conducted to determine the characteristics of their interaction. During the observations, a large outburst of material from Io-inferred to be caused by the eruption of a volcanic plume on Io-caused a transient increase in the neutral cloud and plasma torus masses. The response of the plasma torus to this outburst shows that the interaction between Io and Jupiter's magnetosphere is stabilized by a feedback mechanism in which increases in the plasma torus mass cause a nonlinear increase in loss from the plasma torus, limiting plasma buildup.

Atmosphere↗
PubMed1998

The formation of HCS and HCSH molecules and their role in the collision of comet Shoemaker-Levy 9 with Jupiter.

The reaction of hydrogen sulfide with ground-state atomic carbon was examined with crossed molecular beams experiments and ab initio calculations. The thiohydroxycarbene molecule, HCSH, was the reactive intermediate, which fragmented into atomic hydrogen and the thioformyl radical HCS. This finding may account for the unassigned HCS source and an unidentified HCSH radical needed to match observed CS abundances from the collision of comet Shoemaker-Levy 9 into Jupiter. In the shocked jovian atmosphere, HCS could further decompose to H and CS, and CS could react with SH and OH to yield the observed CS2 and COS.

Atmosphere↗
PubMed1995

Ab initio calculation of the sound velocity of dense hydrogen: implications for models of Jupiter.

First-principles molecular dynamics simulations were used to calculate the sound velocity of dense hydrogen, and the results were compared with extrapolations of experimental data that currently conflict with either astrophysical models or data obtained from recent global oscillation measurements of Jupiter. Excellent agreement with the extrapolated experimental data was obtained. These results strongly support the notion that the existing models for the jovian interior need to be revised.

Chemical Phenomena↗
PubMed1995

Collision of comet Shoemaker-Levy 9 with Jupiter observed by the NASA infrared telescope facility.

The National Aeronautics and Space Administration (NASA) Infrared Telescope Facility was used to investigate the collision of comet Shoemaker-Levy 9 with Jupiter from 12 July to 7 August 1994. Strong thermal infrared emission lasting several minutes was observed after the impacts of fragments C, G, and R. All impacts warmed the stratosphere and some the troposphere up to several degrees. The abundance of stratospheric ammonia increased by more than 50 times. Impact-related particles extended up to a level where the atmospheric pressure measured several millibars. The north polar near-infrared aurora brightened by nearly a factor of 5 a week after the impacts.

Ammonia↗
PubMed1995

Impact debris particles in Jupiter's stratosphere.

The aftermath of the impacts of periodic comet Shoemaker-Levy 9 on Jupiter was studied with the Wide Field Planetary Camera 2 on the Hubble Space Telescope. The impact debris particles may owe their dark brown color to organic material rich in sulfur and nitrogen. The total volume of aerosol 1 day after the last impact is equal to the volume of a sphere of radius 0.5 kilometer. In the optically thick core regions, the particle mean radius is between 0.15 and 0.3 micrometer, and the aerosol is spread over many scale heights, from approximately 1 millibar to 200 millibars of pressure or more. Particle coagulation can account for the evolution of particle radius and total optical depth during the month following the impacts.

Atmosphere↗
PubMed1995

HST far-ultraviolet imaging of Jupiter during the impacts of comet Shoemaker-Levy 9.

Hubble Space Telescope far-ultraviolet images of Jupiter during the Shoemaker-Levy 9 impacts show the impact regions darkening over the 2 to 3 hours after the impact, becoming darker and more extended than at longer wavelengths, which indicates that ultraviolet-absorbing gases or aerosols are more extended, more absorbing, and at higher altitudes than the absorbers of visible light. Transient auroral emissions were observed near the magnetic conjugate point of the K impact site just after that impact. The global auroral activity was fainter than average during the impacts, and a variable auroral emission feature was observed inside the southern auroral oval preceding the impacts of fragments Q1 and Q2.

Atmosphere↗
PubMed2000

Nonlinear simulations of Jupiter's 5-micron hot spots.

Large-scale nonlinear simulations of Jupiter's 5-micron hot spots produce long-lived coherent structures that cause subsidence in local regions, explaining the low cloudiness and the dryness measured by the Galileo probe inside a hot spot. Like observed hot spots, the simulated coherent structures are equatorially confined, have periodic spacing, propagate west relative to the flow, are generally confined to one hemisphere, and have an anticyclonic gyre on their equatorward side. The southern edge of the simulated hot spots develops vertical shear of up to 70 meters per second in the eastward wind, which can explain the results of the Galileo probe Doppler wind experiment.

Ammonia↗
PubMed1995

Emotional processing in survivors of the Jupiter cruise ship disaster.

Twenty-three survivors of the Jupiter cruise ship disaster completed the Impact of Events Scale, a measure of intrusion and avoidance, as well as measures of arousal and affect at two points in time: between 3 and 7 months (Time 1) and between 12 and 14 months (Time 2) following the event. The aim of the present study was to explore the relationship between intrusion and avoidance and symptoms of depression and anxiety. The results suggest that although higher scores on intrusion and avoidance are strongly associated with poorer psychological outcome at each point in time, it is only intrusion which may be predictive of later symptoms. Avoidance would seem to be a response to early distress. These data are discussed with reference to a cognitive--emotional processing model of post-traumatic stress disorder.

Adaptation, Psychological↗
PubMed1979

Detection of Jupiter's ring at 2.2 microm.

FOLLOWING the announcement of the discovery of a ring around Jupiter by the Voyager spacecraft(1) a successful attempt was made to detect the reflected sunlight from this ring at 2.2microm. We describe here the results of this experiment and the precautions taken to separate the radiation from the ring and the scattered radiation from the planet.

Journal Article↗
PubMed1999

A low-temperature origin for the planetesimals that formed Jupiter.

The four giant planets in the Solar System have abundances of 'metals' (elements heavier than helium), relative to hydrogen, that are much higher than observed in the Sun. In order to explain this, all models for the formation of these planets rely on an influx of solid planetesimals. It is generally assumed that these planetesimals were similar, if not identical, to the comets from the Oort cloud that we see today. Comets that formed in the region of the giant planets should not have contained much neon, argon and nitrogen, because the temperatures were too high for these volatile gases to be trapped effectively in ice. This means that the abundances of those elements on the giant planets should be approximately solar. Here we show that argon, krypton and xenon in Jupiter's atmosphere are enriched to the same extent as the other heavy elements, which suggests that the planetesimals carrying these elements must have formed at temperatures lower than predicted by present models of giant-planet formation.

Cold Temperature↗
PubMed2001

Statistical equilibrium predictions of jets and spots on Jupiter.

An equilibrium statistical theory of coherent structures is applied to midlatitude bands in the northern and southern hemispheres of Jupiter. The theory imposes energy and circulation constraints on the large-scale motion and uses a prior distribution on potential vorticity fluctuations to parameterize the small-scale turbulent eddies. Nonlinearly stable coherent structures are computed by solving the constrained maximum entropy principle governing the equilibrium states of the statistical theory. The theoretical predictions are consistent with the observed large-scale features of the weather layer if and only if the prior distribution has anticyclonic skewness, meaning that intense anticyclones predominate at small scales. Then the computations show that anticyclonic vortices emerge at the latitudes of the Great Red Spot and the White Ovals in the southern band, whereas in the northern band no vortices form within the zonal jets. Recent observational data from the Galileo mission support the occurrence of intense small-scale anticyclonic forcing. The results suggest the possibility of using equilibrium statistical theory for inverse modeling of the small-scale characteristics of the Jovian atmosphere from observed features.

Journal Article↗
PubMed2000

Jupiter: Aerosol Chemistry in the Polar Atmosphere.

Aromatic compounds have been considered a likely candidate for enhanced aerosol formation in the polar region of Jupiter. We develop a new chemical model for aromatic compounds in the Jovian auroral thermosphere/ionosphere. The model is based on a previous model for hydrocarbon chemistry in the Jovian atmosphere and is constrained by observations from Voyager, Galileo, and the Infrared Space Observatory. Precipitation of energetic electrons provides the major energy source for the production of benzene and other heavier aromatic hydrocarbons. The maximum mixing ratio of benzene in the polar model is 2x10-9, a value that can be compared with the observed value of 2+2-1x10-9 in the north polar auroral region. Sufficient quantities of the higher ring species are produced so that their saturated vapor pressures are exceeded. Condensation of these molecules is expected to lead to aerosol formation.

Journal Article↗
PubMed1990

The 'Jupiter' sinking: effects on children's fears, depression and anxiety.

Twenty-five girls who survived the sinking of the cruise ship 'Jupiter' were compared with three other groups of girls--71 controls from a separate school; 46 girls in the same school who had not wanted to go on the cruise; and 13 girls who were in a 'near miss' group in that they wanted to go but did not get places. All completed the Fear Survey Schedule for Children (revised form), the Children's Manifest Anxiety Scale and the Birleson Depression Inventory. Survivors did not become generally more fearful. Rather, they developed significantly greater fears to stimuli related to the traumatic event. The results are discussed in relation to the conditioning theory of the acquisition of phobias.

Adaptation, Psychological↗
PubMed1991

Screening child survivors for post-traumatic stress disorders: experiences from the 'Jupiter' sinking.

Twenty-four girls who survived the sinking of the 'Jupiter' in October 1988 were screened 10 days after the accident on the Impact of Events Scale, the Birleson Depression Scale and the Revised Children's Manifest Anxiety Scale. Scores at 10 days were associated strongly with help seeking over the following few months and were highly predictive of scores five months after the accident. Survivors were clearly differentiated from controls on all three measures. The battery seems useful in screening post-traumatic stress disorders in teenage children.

Adolescent↗
PubMed1992

Crisis support and psychiatric symptomatology in adult survivors of the Jupiter cruise ship disaster.

The aim of the present study was to explore the relationship between crisis support and psychiatric symptomatology among adult survivors in the year following the Jupiter cruise ship disaster. Evidence is presented that support decreases over the following year, and that higher levels of crisis support are strongly related to better psychological outcome. Crisis support is shown to retain its association with symptomatology even when satisfaction with support is partialled out. These data are discussed with reference to the debate over the relative importance of received vs. perceived support.

Adaptation, Psychological↗
PubMed2001

Organic composition of C/1999 S4 (LINEAR): a comet formed near Jupiter?

In the current paradigm, Oort cloud comets formed in the giant planets' region of the solar nebula, where temperatures and other conditions varied greatly. The measured compositions of four such comets (Halley, Hyakutake, Hale-Bopp, and Lee) are consistent with formation from interstellar ices in the cold nebular region beyond Uranus. The composition of comet C/1999 S4 (LINEAR) differs greatly, which suggests that its ices condensed from processed nebular gas, probably in the Jupiter-Saturn region. Its unusual organic composition may require reevaluation of the prebiotic organic material delivered to the young Earth by comets.

Journal Article↗
PubMed1996

Galileo Doppler Measurements of the Deep Zonal Winds at Jupiter

Changes in the speed of the Galileo probe caused by zonal winds created a small but measurable Doppler effect in the probe relay carrier frequency. Analysis of the probe relay link frequency allows direct measurements of the speed of Jupiter's zonal winds beneath the cloud tops. The deep winds were prograde and strong, reaching a sustained 190 to 200 meters per second at an altitude marked by a pressure of 24 bars. The depth and strength of the zonal winds severely constrain dynamic modeling of the deeper layers and begin to rule out many shallow weather theories.

Journal Article↗
PubMed1996

Structure of the Atmosphere of Jupiter: Galileo Probe Measurements

Temperatures and pressures measured by the Galileo probe during parachute descent into Jupiter's atmosphere essentially followed the dry adiabat between 0.41 and 24 bars, consistent with the absence of a deep water cloud and with the low water content found by the mass spectrometer. From 5 to 15 bars, lapse rates were slightly stable relative to the adiabat calculated for the observed H2/He ratio, which suggests that upward heat transport in that range is not attributable to simple radial convection. In the upper atmosphere, temperatures of >1000 kelvin at the 0.01-microbar level confirmed the hot exosphere that had been inferred from Voyager occultations. The thermal gradient increased sharply to 5 kelvin per kilometer at a reconstructed altitude of 350 kilometers, as was recently predicted. Densities at 1000 kilometers were 100 times those in the pre-encounter engineering model.

Journal Article↗