Earth-based observations of the Galileo probe entry site

G. Orton; J. L. Ortiz; K. Baines; G. Bjoraker; U. Carsenty; F. Colas; A. Dayal; D. Deming; P. Drossart; E. Frappa; J. Friedson; J. Goguen; W. Golisch; D. Griep; C. Hernandez; W. Hoffmann; D. Jennings; C. Kaminski; J. Kuhn; P. Laques; S. Limaye; H. Lin; J. Lecacheux; T. Martin; G. McCabe; T. Momary; D. Parker; R. Puetter; M. Ressler; G. Reyes; P. Sada; J. Spencer; J. Spitale; S. Stewart; John Varsik; J. Warell; W. Wild; P. Yanamandra-Fisher; G. Fazio; J. Hora; L. Deutsch

doi:10.1126/science.272.5263.839

Earth-based observations of the Galileo probe entry site

G. Orton, J. L. Ortiz, K. Baines, G. Bjoraker, U. Carsenty, F. Colas, A. Dayal, D. Deming, P. Drossart, E. Frappa, J. Friedson, J. Goguen, W. Golisch, D. Griep, C. Hernandez, W. Hoffmann, D. Jennings, C. Kaminski, J. Kuhn, P. LaquesS. Limaye, H. Lin, J. Lecacheux, T. Martin, G. McCabe, T. Momary, D. Parker, R. Puetter, M. Ressler, G. Reyes, P. Sada, J. Spencer, J. Spitale, S. Stewart, John Varsik, J. Warell, W. Wild, P. Yanamandra-Fisher, G. Fazio, J. Hora, L. Deutsch

Center For Solar Terrestrial Research - Big Bear Solar Observatory

Research output: Contribution to journal › Article › peer-review

55 Scopus citations

Abstract

Earth-based observations of Jupiter indicate that the Galileo probe probably entered Jupiter's atmosphere just inside a region that has less cloud cover and drier conditions than more than 99 percent of the rest of the planet. The visual appearance of the clouds at the site was generally dark at longer wavelengths. The tropospheric and stratospheric temperature fields have a strong longitudinal wave structure that is expected to manifest itself in the vertical temperature profile.

Original language	English (US)
Pages (from-to)	839-840
Number of pages	2
Journal	Science
Volume	272
Issue number	5263
DOIs	https://doi.org/10.1126/science.272.5263.839
State	Published - 1996

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Orton, G., Ortiz, J. L., Baines, K., Bjoraker, G., Carsenty, U., Colas, F., Dayal, A., Deming, D., Drossart, P., Frappa, E., Friedson, J., Goguen, J., Golisch, W., Griep, D., Hernandez, C., Hoffmann, W., Jennings, D., Kaminski, C., Kuhn, J., ... Deutsch, L. (1996). Earth-based observations of the Galileo probe entry site. Science, 272(5263), 839-840. https://doi.org/10.1126/science.272.5263.839

@article{a2fb44cbeefd4ed6b3365238ea816498,

title = "Earth-based observations of the Galileo probe entry site",

abstract = "Earth-based observations of Jupiter indicate that the Galileo probe probably entered Jupiter's atmosphere just inside a region that has less cloud cover and drier conditions than more than 99 percent of the rest of the planet. The visual appearance of the clouds at the site was generally dark at longer wavelengths. The tropospheric and stratospheric temperature fields have a strong longitudinal wave structure that is expected to manifest itself in the vertical temperature profile.",

author = "G. Orton and Ortiz, {J. L.} and K. Baines and G. Bjoraker and U. Carsenty and F. Colas and A. Dayal and D. Deming and P. Drossart and E. Frappa and J. Friedson and J. Goguen and W. Golisch and D. Griep and C. Hernandez and W. Hoffmann and D. Jennings and C. Kaminski and J. Kuhn and P. Laques and S. Limaye and H. Lin and J. Lecacheux and T. Martin and G. McCabe and T. Momary and D. Parker and R. Puetter and M. Ressler and G. Reyes and P. Sada and J. Spencer and J. Spitale and S. Stewart and John Varsik and J. Warell and W. Wild and P. Yanamandra-Fisher and G. Fazio and J. Hora and L. Deutsch",

year = "1996",

doi = "10.1126/science.272.5263.839",

language = "English (US)",

volume = "272",

pages = "839--840",

journal = "Science",

issn = "0036-8075",

publisher = "American Association for the Advancement of Science",

number = "5263",

}

Orton, G, Ortiz, JL, Baines, K, Bjoraker, G, Carsenty, U, Colas, F, Dayal, A, Deming, D, Drossart, P, Frappa, E, Friedson, J, Goguen, J, Golisch, W, Griep, D, Hernandez, C, Hoffmann, W, Jennings, D, Kaminski, C, Kuhn, J, Laques, P, Limaye, S, Lin, H, Lecacheux, J, Martin, T, McCabe, G, Momary, T, Parker, D, Puetter, R, Ressler, M, Reyes, G, Sada, P, Spencer, J, Spitale, J, Stewart, S, Varsik, J, Warell, J, Wild, W, Yanamandra-Fisher, P, Fazio, G, Hora, J & Deutsch, L 1996, 'Earth-based observations of the Galileo probe entry site', Science, vol. 272, no. 5263, pp. 839-840. https://doi.org/10.1126/science.272.5263.839

TY - JOUR

T1 - Earth-based observations of the Galileo probe entry site

AU - Orton, G.

AU - Ortiz, J. L.

AU - Baines, K.

AU - Bjoraker, G.

AU - Carsenty, U.

AU - Colas, F.

AU - Dayal, A.

AU - Deming, D.

AU - Drossart, P.

AU - Frappa, E.

AU - Friedson, J.

AU - Goguen, J.

AU - Golisch, W.

AU - Griep, D.

AU - Hernandez, C.

AU - Hoffmann, W.

AU - Jennings, D.

AU - Kaminski, C.

AU - Kuhn, J.

AU - Laques, P.

AU - Limaye, S.

AU - Lin, H.

AU - Lecacheux, J.

AU - Martin, T.

AU - McCabe, G.

AU - Momary, T.

AU - Parker, D.

AU - Puetter, R.

AU - Ressler, M.

AU - Reyes, G.

AU - Sada, P.

AU - Spencer, J.

AU - Spitale, J.

AU - Stewart, S.

AU - Varsik, John

AU - Warell, J.

AU - Wild, W.

AU - Yanamandra-Fisher, P.

AU - Fazio, G.

AU - Hora, J.

AU - Deutsch, L.

PY - 1996

Y1 - 1996

N2 - Earth-based observations of Jupiter indicate that the Galileo probe probably entered Jupiter's atmosphere just inside a region that has less cloud cover and drier conditions than more than 99 percent of the rest of the planet. The visual appearance of the clouds at the site was generally dark at longer wavelengths. The tropospheric and stratospheric temperature fields have a strong longitudinal wave structure that is expected to manifest itself in the vertical temperature profile.

AB - Earth-based observations of Jupiter indicate that the Galileo probe probably entered Jupiter's atmosphere just inside a region that has less cloud cover and drier conditions than more than 99 percent of the rest of the planet. The visual appearance of the clouds at the site was generally dark at longer wavelengths. The tropospheric and stratospheric temperature fields have a strong longitudinal wave structure that is expected to manifest itself in the vertical temperature profile.

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U2 - 10.1126/science.272.5263.839

DO - 10.1126/science.272.5263.839

M3 - Article

AN - SCOPUS:0001149547

SN - 0036-8075

VL - 272

SP - 839

EP - 840

JO - Science

JF - Science

IS - 5263

ER -

Earth-based observations of the Galileo probe entry site

Abstract

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