The Stratification of Jupiter's Troposphere at the Galileo Probe Entry Site

Icarus ◽  
2002 ◽  
Vol 158 (2) ◽  
pp. 410-433 ◽  
Author(s):  
J Magalhães
Keyword(s):  
Entry Site ◽  
Galileo Probe

scholarly journals Galileo: Close-up Views of Jupiter’s Dynamic Atmosphere

2002 ◽  
Vol 12 ◽  
pp. 602-605 ◽  
Author(s):  
Ashwin R. Vasavada
Keyword(s):  
Near Infrared ◽  
Moist Convection ◽  
Entry Site ◽  
Zonal Jets ◽  
Night Side ◽  
New Ideas ◽  
Water Cloud ◽  
Galileo Probe ◽  
Auroral Phenomena

AbstractThe Galileo spacecraft’s Solid State Imager (SSI) has been returning mosaics of Jupiter since 1996. The combination of high spatial resolution, broad spectral range, and short mosaic time steps has revealed a dynamic, vertically extended cloud structure not detectable by Voyager. These data have stimulated new analyses of major features such as zonal jets, the Great Red Spot, White Ovals, and the Galileo Probe entry site. Near-infrared images have provided fundamental constraints on the vertical structure of clouds and hazes, including the first imaging of a water cloud. Results from night side imaging include an extensive search for lightning, the first matching of lightning events to day side storm clouds, and the first spectral and spatial measurements of visible-wavelength auroral phenomena (not discussed here, see Vasavada et al. 2000). The identification of several tall, energetic storm systems at specific latitudes has led to new ideas about the role of moist convection in Jupiter’s atmospheric energetics.

Characteristics of the Galileo probe entry site from Earth-based remote sensing observations

1998 ◽  
Vol 103 (E10) ◽  
pp. 22791-22814 ◽  
Author(s):  
Glenn S. Orton ◽  
Brendan M. Fisher ◽  
Kevin H. Baines ◽  
Sarah T. Stewart ◽  
A. James Friedson ◽  
...  
Keyword(s):  
Remote Sensing ◽  
Entry Site ◽  
Galileo Probe

Earth-Based Observations of the Galileo Probe Entry Site

Science ◽  
1996 ◽  
Vol 272 (5263) ◽  
pp. 839-840 ◽  
Author(s):  
G. Orton ◽  
J. L. Ortiz ◽  
K. Baines ◽  
G. Bjoraker ◽  
U. Carsenty ◽  
...  
Keyword(s):  
Entry Site ◽  
Galileo Probe

Histology of the vertebral artery–dural junction: relevance to posterolateral approaches to the skull base

2019 ◽  
pp. 1-6
Author(s):  
Robert C. Rennert ◽  
Martin P. Powers ◽  
Jeffrey A. Steinberg ◽  
Takanori Fukushima ◽  
John D. Day ◽  
...  
Keyword(s):  
Connective Tissue ◽  
Vertebral Artery ◽  
Skull Base ◽  
Histological Analysis ◽  
Foramen Magnum ◽  
Entry Site ◽  
Microsurgical Technique ◽  
Vessel Injury ◽  
Far Lateral ◽  
Clear Delineation

OBJECTIVEThe far-lateral and extreme-lateral infrajugular transcondylar–transtubercular exposure (ELITE) and extreme-lateral transcondylar transodontoid (ELTO) approaches provide access to lesions of the foramen magnum, inferolateral to mid-clivus, and ventral pons and medulla. A subset of pathologies in this region require manipulation of the vertebral artery (VA)–dural interface. Although a cuff of dura is commonly left on the VA to avoid vessel injury during these approaches, there are varying descriptions of the degree of VA-dural separation that is safely achievable. In this paper the authors provide a detailed histological analysis of the VA-dural junction to guide microsurgical technique for posterolateral skull base approaches.METHODSAn ELITE approach was performed on 6 preserved adult cadaveric specimens. The VA-dural entry site was resected, processed for histological analysis, and qualitatively assessed by a neuropathologist.RESULTSHistological analysis demonstrated a clear delineation between the intima and media of the VA in all specimens. No clear plane was identified between the connective tissue of the dura and the connective tissue of the VA adventitia.CONCLUSIONSThe VA forms a contiguous plane with the connective tissue of the dura at its dural entry site. When performing posterolateral skull base approaches requiring manipulation of the VA-dural interface, maintenance of a dural cuff on the VA is critical to minimize the risk of vascular injury.

scholarly journals In Situ exploration of the giant planets

2021 ◽  
Author(s):  
O. Mousis ◽  
D. H. Atkinson ◽  
R. Ambrosi ◽  
S. Atreya ◽  
D. Banfield ◽  
...  
Keyword(s):  
Solar System ◽  
Giant Planets ◽  
Atmospheric Composition ◽  
Formation History ◽  
History Of ◽  
Composition Structure ◽  
Galileo Probe ◽  
Probe Measurements

AbstractRemote sensing observations suffer significant limitations when used to study the bulk atmospheric composition of the giant planets of our Solar System. This impacts our knowledge of the formation of these planets and the physics of their atmospheres. A remarkable example of the superiority of in situ probe measurements was illustrated by the exploration of Jupiter, where key measurements such as the determination of the noble gases’ abundances and the precise measurement of the helium mixing ratio were only made available through in situ measurements by the Galileo probe. Here we describe the main scientific goals to be addressed by the future in situ exploration of Saturn, Uranus, and Neptune, placing the Galileo probe exploration of Jupiter in a broader context. An atmospheric entry probe targeting the 10-bar level would yield insight into two broad themes: i) the formation history of the giant planets and that of the Solar System, and ii) the processes at play in planetary atmospheres. The probe would descend under parachute to measure composition, structure, and dynamics, with data returned to Earth using a Carrier Relay Spacecraft as a relay station. An atmospheric probe could represent a significant ESA contribution to a future NASA New Frontiers or flagship mission to be launched toward Saturn, Uranus, and/or Neptune.

scholarly journals Treatment strategies for cerebrospinal shunt infections: a systematic review of observational studies

BMJ Open ◽  
2020 ◽  
Vol 10 (12) ◽  
pp. e038978
Author(s):  
Joan L Robinson ◽  
Dolores Freire ◽  
Liza Bialy
Keyword(s):  
Systematic Review ◽  
Small Sample Size ◽  
Treatment Strategies ◽  
Small Sample ◽  
Cochrane Library ◽  
Csf Shunt ◽  
Entry Site ◽  
Recurrence Rates ◽  
Ovid Medline ◽  
Shunt Infections

ObjectiveA systematic review was conducted of studies comparing time to cerebrospinal fluid (CSF) sterilisation or rate of recurrence with different treatment strategies for CSF shunt infections.MethodsA librarian-directed search was conducted of Epub Ahead of Print, In-Process & Other Non-Indexed Citations, Ovid Medline Daily and Ovid Medline, Ovid Embase, Wiley Cochrane Library, CINAHL Plus with Full Text via EBSCOhost, Scopus Advanced Search, and Web of Science Core Collection from 1990 to May 2019. Studies of any design that compared outcomes in groups of any age with different management strategies were included. Studies that compared complete versus incomplete shunt removal were excluded. Quality assessment was performed with the Newcastle-Ottawa Scale.ResultsThe search identified 2208 records, of which 8 met the inclusion criteria. All were cohort studies of moderate quality. Four studies compared the duration of antibiotics; none demonstrates that a longer course prevented recurrences. Two studies analysed addition of rifampin, with one showing a decrease in recurrences while the other had a small sample size. No studies analysed the addition of intraventricular antibiotics, but one showed equally good results with once versus twice daily administration. One study reported no difference in recurrences with placement of antibiotic-impregnated catheters. Recurrence rates did not differ with shunt replacement minimum of 7 days vs less than 7 days after CSF became sterile. There were no recurrences in either group when shunt replacement was performed after sterile CSF cultures were obtained at 24 vs 48 hours after antibiotics were discontinued. A new shunt entry site did not decrease recurrences.DiscussionThe main limitations are the lack of high-quality studies, the small sample sizes and the heterogeneity which precluded meta-analysis. Addition of rifampin for staphylococcal infections may decrease relapse but requires further study.

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