Changes between Version 2 and Version 3 of MSP342


Ignore:
Timestamp:
Nov 9, 2015 9:45:11 AM (9 years ago)
Author:
hwalker
Comment:

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  • MSP342

    v2 v3  
    44
    5531 October: The data fill is now 115% to compensate for the eclipse PL OFF period. Several MP, BS and WBD BM2 periods are added, the location on the Bryant plots appears shifted because C1 (the satellite used for the plotting) is separated in time from C2, C3, C4 at the boundaries. For the WBD BM2, C2, C3 and C4 are used to determine the optimum timing.
     6
     79 November: The final version is available. The GI Blanco-Cano proposal for long (15-hour) NM1 periods around the outbound and inbound Bow Shock has been added, to take place in late March and early April. Several 3-hour BM1 MP periods have been added, at the end of the Blanco-Cano periods. The final Bryant plots are attached, together with the 'by-orbit' analysis (which includes the timings for the NM1 periods), the list of D0 periods, and the list of BM2 periods.