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EFW%20operational%20on%20all%20four%20SC

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EFW internal burst mode statistics (NE) EFW SC 1 and 3 operations (AIE, YK) ... Burst Mode 1 Telemetry (hour) 2 E-field signals, 450 samples/s ... – PowerPoint PPT presentation

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Title: EFW%20operational%20on%20all%20four%20SC


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2
Welcome to Uppsala!
Mats André mats.andre_at_irfu.se
  • Thursday May 18
  • 1300, room Ã…4003
  • 1500 Coffee
  • (1730 Dinner)
  • Friday May 19
  • 0900, room Ã…4003
  • 1000 Coffee
  • splinters (other locations)
  • 1130 Lunch
  • 1300 Room Ã…4003
  • splinters (other locations)
  • 1530 end meeting

3
Draft Agenda May 18
  • Welcome, Cluster and EFW basics and status (MA)
  • EFW modes and operations (AIE)
  • EFW internal burst mode statistics (NE)
  • EFW SC 1 and 3 operations (AIE, YK)
  • Cluster data sets CDs, DDS, CSDS, CAA (PAL)
  • The CAA where we are and where we are going (HL)
  • Data exchange (beyond standard archives) (AV,
    SB)
  • Coffee
  • CAA data production (YK)
  • Revised look at plasma densities from Cluster SC
    potential (AP)
  • Polar wind measurements from wake studies (AIE)
  • ISADT analysis software (AIE, YK. RG)
  • Publications and future meetings (MA)
  • AOB

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5
Cluster Mission Overview
  • Launch summer 2000
  • Nominal mission 2001 and 2002 (50)
  • Extension 1 2002 to 2005 (100)
  • Extension 2 2005 to 2009 (100)
  • All spacecraft fully operational

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9
Separation distance strategy
C1,C2,C3
C3,C4
d
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Tail 2005
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14
Cluster Instrument Status
  • Most instruments are operational
  • Not operational
  • ASPOC C1 (presently no ASPOC running)
  • CIS C2
  • EDI C4

15
EFWElectric Field and Wave
www.cluster.irfu.se/efw gt operations gt EFW for
Dummies
16
Common EFW Modes
  • Normal Mode Telemetry (full orbit)
  • 2 E-field signals, 25 samples/s
  • 4 single probe signals, 5 samples/s
  • Burst Mode 1 Telemetry (hour)
  • 2 E-field signals, 450 samples/s
  • 4 single probe signals, 5 samples/s
  • Internal EFW burst (around 10 s)
  • 4 single probe signals, few 1000 samples/s

17
EFW operational on all four SC
  • SC 1 Problem probe 1, 2001-12-28,
  • somewhat reduced science data.
  • SC 2 Filter problem, 2001-07-25.
  • Solution use 180 Hz filter also
  • in NM (25 samples/s) on all probes.
  • SC 3 Problem probe 1, 2002-07-29,
  • somewhat reduced science data.
  • SC 4 OK

18
SC 1, probe 1 and SC 3, probe 1
  • First workaround use only probe pair 34
  • EFW prime parameters (4s) OK
  • Reprogrammed to use 3 probes to get
  • 2 orthogonal E (routine operations from
  • late September 2003)
  • From January 2006
  • In NM, use only probe pair 34 for E
  • use probe 2 to get SC potential at 25
    samples/s

19
SC spin axis tiltWHISPER proposal
20
SC spin axis tilt
  • Tilt is feasible
  • Thermal
  • main constraint
  • Decide later
  • Duration
  • a few weeks
  • 45 degrees?
  • Apil 2007?

21
http//sprg.ssl.berkeley.edu/themis/flash.html
22
EFW webpage
  • www.cluster.irfu.se
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