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    No. 111 - Routine Operations

    02 Jan 2008 12:00

    Report for Period 23 December to 29 December 2007

    It took several days to download the VIRTIS data stored onboard the spacecraft after the problems at Cebreros reported in the previous week.

    The Radio Science Dual band ranging in NNO has failed during this week. The reason is the drop in the S-band signal present in the HGA1 antenna. A fine tuning of the configuration is being attempted in order to optimise the setting.

    The table below shows a chronology of the main activities in the reporting period:

    MET (Day) Date DOY Main Activity
    775 23/12/07 357 Routine Operations
    776 24/12/07 358 Routine Operations
    777 25/12/07 359 Routine Operations
    VIRTIS data download
    778 26/12/07 360 Routine Operations
    779 27/12/07 361 Routine Operations
    Dual band ranging failed
    780 28/12/07 362 Routine Operations
    781 29/12/07 363 Routine operations
    Dual band ranging failed

    At the end of the last Cebreros pass in the reporting period (DOY 363, 12:00z) Venus Express was orbiting Venus at 169.6 million km from the Earth. The one-way signal travel time was 565 seconds.

    Payload Activities

    ASPERA
    The instrument was regularly operated as part of the routine plan.

    MAG
    The instrument was regularly operated as part of the routine plan.

    PFS
    The instrument was not operated during the reporting period.

    SPICAV
    The instrument was regularly operated as part of the routine plan.

    VeRA
    No RSI activities took place this week.

    VIRTIS
    The instrument was regularly operated as part of the routine plan.

    VMC
    The instrument was regularly operated as part of the routine plan.

    Ground Facilities

    New Norcia support of radio science
    NNO was used in two occasions for Radio Science dual ranging. The activity failed on both occasions on 27 & 29 December 2007. The reason is understood to be due to the signal drop observed in the S-band link.

    The current ranging standard does not permit different integration times for different bands. The problem is the relatively high signal-to-noise ratio in X-band with respect to S-band making it challenging to optimise integration time. This needs to be short enough to avoid saturation in X-band and long enough to allow tone lock in S-band. New configurations setting will be tried in the next reporting period.

    Future Milestones

    • NNO and Cebreros scheduling for 2008


    Last Update: 27 Feb 2008

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