# $Log: OIOR_PI6RSO_D_0010_MR_03____.ITL,v $
#
# Revision 1.5  2007/10/04  L.Kamp
# Changed VMRG2501 from 2007.317.20.52.44 to 2007.317.20.50.07, per latest estimate
# of CA by Flight Dynamics.  Changed filename for final final ORFA delivery.  Removed
# some tab characters.
#
# Revision 1.4  2007/08/16 18:38:01  kwirth
# Almost final ESB2 OIOR for MR03 submitted via ROFTS/ORFA on 15 Aug 2007.
# Pending update of value of formal parameter VMRG2501 "Astrd Mode#1 (StartTime)" of
# sequence AMRF500A "MIRO Asteroid Obs" according to new Earth closest approach time.
# Original filename: OIOR_PI6RSO_D_0010_MR_03____00020.ROS
#
#
# Changed filename for final ORFA delivery - 2007/08/15 - L.Kamp
#
# Revision 1.3  2007/07/06 21:53:57  kwirth
# Increased End_time to include duration of last sequence.
#
# Revision 1.2  2007/06/24 16:48:41  kwirth
# Updates for EPS run of complete MR ESB2.
#
# Revision 1.1  2007/06/23 20:15:18  kwirth
# Preliminary ESB2 MR03 OIOR submitted via ROFTS/ORFA on 18 Jun 2007.
# Original filename: OIOR_PI6RSO_D_0010_MR_03____00015.ROS
#
# Renamed OIOR_PI6RSO_D_0010_MR_E2O03_00015.ROS to OIOR_PI6RSO_D_0010_MR_03____00015.ROS
# at request of RSOC, added Ref_data, Start/End_time - 2007/06/15 - L.Kamp
#
# Initial ESB2 OIOR for MR03 - 2007/06/11 - L.Kamp
#
#=======================================================================================#
# Filename:     OIOR_PI6RSO_D_0010_MR_03____00024.ROS
# Type:         Orbiter Instrument Operation Request file
#
# Description:  Asteroid Flyby Exercise for the Earth-2 Swing-by
#
# Author:       Lucas Kamp
#
#               JPL
#
# Date:         11 Jun 2007 
#
# (c) ESA/Estec
#
#=======================================================================================#

Version: 00001

Ref_date: 01-Jan-2000  # Irrelevant because will be overridden by top-level ITL, but needed for ORFA.
# RSOC change: Replaced our standard Ref_date.

# NOTE: Actual Start_time of this sequence must be 12 minutes prior to the Astrd_Mode_1_StartTime
# in the AMRF500A command issued in Step 2, below.  This time in turn was determined as being
# 00:07:16 prior to the current estimate of the Earth Closest Approach.
# Therefore:  Start_time = CA - 00:19:16.

Start_time: 000_00:00:00
End_time:   000_03:10:00
# RSOC change: Increased End_time to include duration of last sequence.
# Init_Mode:        MIRO       CTS_DualCntm

#---------------------------------------------------------------------------------------#
Description: "1. | Assume MIRO is fully warmed up, because it was not turned off in"
Description: "   | preceding observation (MR05), which ended with Disable Science."
Description: "   | Therefore, this starts with Enable Science."
Description: "   | We also want to do a LNA off (background determination) before"
Description: "   | the Ast.Mode sequence."
#---------------------------------------------------------------------------------------#

+00:00:00    MIRO       CTS_DualCntm  AMRS631A # Enable Science

+00:01:00    MIRO       CTS_DualCntm  AMRF032A # "SMM LNA Power Off v04"

#---------------------------------------------------------------------------------------#
Description: "2. | Issue Asteroid Mode command."
Description: "   | This requires that MIRO be in Dual Continuum mode."
Description: "   | Since this shuts off the CTS, we also need a CTS warmup command"
Description: "   | at least 5' before the start time."
#---------------------------------------------------------------------------------------#

+00:04:00    MIRO       CTS_DualCntm  AMRF500A( \ # "MIRO Asteroid Obs v05" 
                                          VMRG2501 = 2007.317.20.50.07 \ # Astrd_Mode_1_StartTime_
                                          VMRD2502 = 56 \ # Execution_Time
                                          VMRD2503 = 1 [RAW]) # Starting_LO_Frequency

+00:05:00    MIRO       CTS_DualCntm  AMRF013A # "Mode Dual Continuum v05"

+00:07:00    MIRO       DualContinuum AMRF009A # "CTS Warm-up v06"

#---------------------------------------------------------------------------------------#
Description: "3. | Perform first Asteroid mode observation, which is done automatically."
Description: "   | This starts at the time specified by parameter VMRG2501 of AMRF500A"
Description: "   | and lasts for 9.9 minutes, preceded and followed by calibrations of"
Description: "   | 2.3 minutes each."
Description: "   | At the end, MIRO is automatically switched to DualContinuum mode."
#---------------------------------------------------------------------------------------#

#---------------------------------------------------------------------------------------#
Description: "4. | Switch back to CTS/DualCont mode for high-rate data playback."
Description: "   | Playback will take about 2.4 hours, then switch MIRO off."
#---------------------------------------------------------------------------------------#

+00:28:00     MIRO       DualContinuum AMRF011A # CTS/Dual Continuum

+02:56:00     MIRO       CTS_DualCntm  AMRF016A # Engineering

+03:00:00     MIRO       Engineering   AMRF003A # Power Off MIRO via OBCP

# ----------------- End of MIRO Pointing Scenario  -------------------- #