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    • [ В начало ] Пред. | 8 | 9 | 10 | 11 | 12 | 13 | 14 | 15 | 16 | 17 | След.

    111. http://www.stsci.edu/ftp/observing/status_reports/old_reports_96/hst_status_08_09_96
    ... 1.1 Completed WF/PC-2 6774 (Temporal Variability in Io's Surface and = Plumes) The WF/PC-2 was used to make observations of Jupiter's moon Io at = longitude 215 degrees in order to study temporal variability in its plums = and surface markings ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_96/hst_status_08_09_96 -- 4.4 Кб -- 09.08.1996
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    112. http://www.stsci.edu/ftp/observing/status_reports/old_reports_93/hst_status_07_08_93
    ... 1.7 Completed FOC/96 4113 (Auroral Imaging of Jupiter With the FOC Cycle 2, February- March 1993) The Faint Object Camera was used to make two images of the auroral emissions on the planet Jupiter at 1600 A0. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_93/hst_status_07_08_93 -- 7.2 Кб -- 09.07.1993
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    113. http://www.stsci.edu/ftp/observing/status_reports/old_reports_93/hst_status_06_08_93
    ... Telescope: Imaging of Io: Cycle 3 High) The Faint Object Camera was used to make one ultraviolet observation of Jupiter's moon Io in order to determine the abundance and distribution of surface and atmospheric constituents, particularly sulfur dioxide ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_93/hst_status_06_08_93 -- 7.0 Кб -- 10.06.1993
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    114. http://www.stsci.edu/ftp/observing/status_reports/old_reports_93/hst_status_07_03_93
    ... 1.8 Completed GHRS/2 4966 (Spatially Resolved Spectroscopy of Jupiter - Cycle 3 High) The High Resolution Spectrograph was used to make ultraviolet spectral observations at given latitudes of the planet Jupiter. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_93/hst_status_07_03_93 -- 5.9 Кб -- 07.07.1993
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    115. http://www.stsci.edu/ftp/observing/status_reports/old_reports_96/hst_status_06_20_96
    ... as of 172/0000Z 1.0 ACTIVITIES SCHEDULED AND ACCOMPLISHED: 1.1 Completed GHRS/1 6027 (HST-Galileo Torus Observations) The High Resolution Spectrograph (Side One) was used to make = observations of the plasma torus which is formed by Jupiter's moon Io ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_96/hst_status_06_20_96 -- 3.4 Кб -- 20.06.1996
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    116. http://www.stsci.edu/ftp/observing/status_reports/old_reports_96/hst_status_08_13_96
    ... SCHEDULED AND ACCOMPLISHED: 1.1 Competed Two sets of FOS/RD 6552 (Spectrophotometry of Inner = Jovian Satellites) The Faint Object Spectrograph was used to make spectrographic = observations of Jupiter's inner moon Thebe during its eastern elongation ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_96/hst_status_08_13_96 -- 5.5 Кб -- 13.08.1996
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    117. http://www.stsci.edu/ftp/observing/status_reports/old_reports_94/hst_status_07_19_94
    ... Five Sets of GHRS/1, and WF/PC-2 5642 (Observations of the Impact of Comet Shoemaker-Levy (1993E) and Jupiter) The High Resolution Spectrograph (Side One) and the WF/PC-2 were used to make observations to support the Jupiter/ Shoemaker-Levy impact events ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_94/hst_status_07_19_94 -- 5.5 Кб -- 20.07.1994
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    118. http://www.stsci.edu/ftp/observing/status_reports/old_reports_96/hst_status_08_15_96
    ... High Resolution Spectrograph (Side Two) was used to make = ultraviolet observations of Jupiter's moon Io as it made a transit across = the face of Jupiter's surface, to determine the abundance and = distribution of SO2 (Sulfur Dioxide) in its atmosphere ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_96/hst_status_08_15_96 -- 5.0 Кб -- 15.08.1996
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    119. http://www.stsci.edu/ftp/observing/status_reports/old_reports_93/hst_status_06_03_93
    ... 1.4 Completed FOS/BL 4203 (Spatially Resolved Spectroscopy of Jupiter - Cycle 2) The Faint Object Spectrograph was used to make spectroscopic observations of the Great Red Spot and North Pole regions on the planet Jupiter. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_93/hst_status_06_03_93 -- 6.7 Кб -- 05.06.1993
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    120. http://www.stsci.edu/ftp/observing/status_reports/old_reports_96/hst_status_08_02_96
    ... RD 6725 (Io's SO2 Atmosphere: Patchy or Not) The Faint Object Spectrograph (Red Side) was used to make = spatially resolved, both visually and ultravioletly, spectrographic = observations of Jupiter's moon Io in order to study the SO2 in its = atmosphere ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_96/hst_status_08_02_96 -- 4.0 Кб -- 02.08.1996
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