AMS02 Thermal Vacuum and Thermal Balance Tests in the Large Space Simulator at ESTEC J' Burger AMS02 - PowerPoint PPT Presentation

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AMS02 Thermal Vacuum and Thermal Balance Tests in the Large Space Simulator at ESTEC J' Burger AMS02

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Possibility to send some information using RS232 link to EGSE ... Procedure reviews. Data handling configuration. WP2: AMS specific preparation prior to pre-test ... – PowerPoint PPT presentation

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Title: AMS02 Thermal Vacuum and Thermal Balance Tests in the Large Space Simulator at ESTEC J' Burger AMS02


1
AMS-02 Thermal Vacuum and Thermal Balance Tests
in the Large Space Simulator at ESTECJ.
BurgerAMS-02 TIMCERN, July 23, 2004
2
AMS data sheet
  • Size 3.2 m x 5.1 m x 4.1 m in test stand
  • Mass 6700 Kg8944 Kg test article
  • 10817 Kg crane wt.
  • Power 2kW

3
Two Meetings at ESA/ESTECNoordwijk,
Netherlandsto request overall AMS-02 TVTin
Large Space Simulator (LSS)
  • June 11 2003 - Presentation of AMS request to
    ESA
  • S.C.C. Ting Martin Zell Head of Human
    Spaceflight ESA
  • Martin Pohl Wolfgang Supper Head of
    Thermal ESTEC
  • Joseph Burger Jean Jamar Head of
    Testing ESTEC
  • Robert Becker
  • July 3, 2003 Follow-up Meeting
  • Joseph Burger Jean Jamar Head of
    Testing ESTEC
  • Marco Molina Wolfgang Supper Head of
    Thermal ESTEC
  • Alexander Grechko Gaetan Piret Test
    Manager ESTEC
  • Peter Berges R. Effenberger Managing
    Director ETS
  • Y. Hoyet ESTEC
  • Matin Zell Head of Human Spaceflight ESA

4
LMSO Visit to LSS
  • Trent Martin, Phil Mott, Ross Harold, and Craig
    Clark were at ESTEC last year for planning
    acoustic test.
  • Also visited the Large Space Simulator

5
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6
Large Space Simulator DimensionsUseable Volume
diameter 9.5m, height 10m
7

8
Our Original Request from ESA/ESTEC
  • Test equipment
  • 300 temperature sensors with DAS and cables
    (provided in advance)
  • Test heaters or IR lamps (TBC)
  • Cabling Power (120VDC) and data, including
    fiber optics (provided by ESTEC cables inside
    the chamber, feedthrough, cables outside chamber
    to control room)
  • Corrugated stainless steel tubes from AMS02
    venting ports to external vacuum pumps for He and
    TRD gas venting
  • Space
  • Clean room area 150 m2, with 8m crane
    height
  • 40 m2 control room for 13 people with
    pc/control terminals
  • 30 m2 storage room for shipping equipment
  • Personnel - people to operate facility, plus 2
    people full time during integration/deintegration
    (plus crane drivers, )
  • Office space for 10-15 people including phones,
    fax, xerox, network plugs
  • Other list of elecrical and vent feedthroughs
    needed
  • Time original request 42 days in chamber plus 3
    weeks installation and checkout, 2 weeks
    deinstallation and shipping
  • Mechanical and electrical interface data
  • Thermal model of LSS in SINDA/TRASYS and support
    in using it

9
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10
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11
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12
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13
90 ton seismic block can support 60 tonsexternal
dimensions 3.2m x 3.2 mmechanically decoupled
from LSS and building
14
Example of mounting HST Solar Wing on block
15
Vacuum system typical pumping times
16
Vent lines needed for He and TRD gas
  • The turbomolecular pumps cannot handle the
    nominal He venting rate of 2 mg/s, nor a TRD gas
    venting, and a cryopump wont work on He
  • Vent lines are needed for normal He and TRD gas
    venting and venting from the cryosystem burst
    disk outputs

17
Shrouds and Nitrogen Supply
  • C1 covering the main chamber
  • LN2 mode (lt100K)(max. heat load 170kW)
  • or GN2 mode (150-350K) (max. heat load 10kW)
  • C2 covering the auxiliary chamber LN2 mode only

18
Solar Simulator
  • Horizontal beam 6m diameter, 5m deep
  • Maximum intensity at nominal lamp power
    2000W/square meter
  • Intensity distribution in reference plane within
    /-4

19
Thermal Data Handling
  • Thermocouple recording
  • - 864 t/c internal
  • - 216 t/c direct
  • Platinum sensors
  • - 98 Pt100
  • - 8 Pt500
  • Power supplies (P-U-I)
  • 40 PSU 24 W - 40V 0.6A
  • 94 PSU 240 W 80V 6A
  • Possibility to record other signals using
    external scanners
  • Possibility to send some information using RS232
    link to EGSE
  • A total of 2000 channels with a minimum scan time
    of 30 seconds
  • User interface using Dynaworks real time display

20
WP1 Standard Facility preparation (seismic
block configuration)
  • Chamber configuration
  • Meetings
  • Procedure reviews
  • Data handling configuration

21
WP2 AMS specific preparation prior to pre-test
  • Provision of t/c harness (300 t/c) (no special
    calibration)
  • Provision of internal harness including loan of
    vacuum connectors
  • Provision of Helium venting line
  • Provision of test heater/IR lamp setup (to be
    clarified)
  • Support during installation of the compact
    superfluid cooling system around the chamber
  • Support during installation of the specimen
    support stand
  • Installation of test heater/IR lamp

22
WP3 4 days of pre-test
  • 4 days of pre-test in VTC modes
  • Standard post test activity for facility and data
    handling
  • Pre-test facility data report
  • Note Pre-test is to check the facility
    configuration including new flanges for line
    feedthrough,
  • submit to vacuum all the test aids (test
    support stands, piping, test harness,)

23
WP4 Satellite preparation support
  • Support to customer during installation of the
    specimen (2 persons/3weeks)
  • Verification of specimen instrumentation
  • Chamber close-out
  • Normally, we have to do our own handling (crane
    operations) of the AMS-02 payload

24
WP5 42 days of TB/TV test
  • 42 days of TB/TV test including 28 days of TV
    test and 14 days of sun illumination

25
WP6 Post-Test Activities
  • Support for satellite removal (2 persons/1 week)
  • Standard data handling post test activities
    (including 1 set of all data in electronic
    format)
  • Standard facility post test activities
  • Preparation of facility data report
  • Support during specimen support stand

26
WP7 General Support
  • Preparation of office, check-out area and clean
    room
  • 150 sq.m. clean room class 100,000 during 12
    weeks
  • (assembly area)
  • 30 sq.m. clean room class 100,000 during 12 weeks
  • (shipping equipment storage)
  • 40 sq.m. clean room class 100,000 during 12 weeks
  • (this is requested control room)
  • Provision of offices for 15 persons incl. Phones,
    FAX, access to copying machines during 12 weeks
  • Cleaning of equipment entering the clean room

27
ESTEC meeting outcome
  • A new stand for the TV/TB tests will be designed
    and manufactured by AMS Collaboration
  • (Shandong University will send a mechanical
    engineer to stay at CERN, who will work on
    designing the stand with Robert Becker)

28
ESTEC feedbackAction Items
  • 1. AMS Collaboration should try reducing time
    spent inside LSS to 30 days.
  • 2. ESTEC will investigate the sensitivity of the
    facility vacuum gauges to the magnetic field
  • 3. Thermal model of LSS delivery in the requested
    format (SINDA/TRASYS) will be confirmed end of
    August, 2003
  • 4. AMS Collaboration to check how long AMS can be
    disconnected from the vacuum pump

29
Status of Action Items fromJuly 3, 2003 Meeting
(1)
  • We confirm 30 day thermal vacuum/balance test
    schedule, while recommending reserving 12 days
    contingency, because of the complexity of the
    cryogenic system

30
  • Simulations have been run in order to estimate
    the time needed for the
  • Thermal Cycles
  • Thermal Balance
  • in HOT and COLD phases

31
Preliminary TV-Test schedule 30 days
32
Response for Action Item 1
  • Geneva, September 18, 2003
  • Dear Dr. Zell,
  • After discussion of the studies of the times
    needed to obtain stable conditions during thermal
    vacuum
  • cycling and thermal balance, we can confirm that
    we request thirty days in the Large Space
    Simulator
  • for the thermal vacuum test of the AMS-02
    experiment. This time includes allowance for pump
    down of
  • the chamber, cycling to the highest and lowest
    permissible non-operating temperatures, four
    thermal
  • cycles to the hottest and coldest operating
    temperatures, hot and cold thermal balance tests,
    followed
  • By return to ambient conditions, as shown in the
    accompanying preliminary schedule.
  • Following the suggestion of Dr. Eric Ettlinger we
    wish to report to you that you may want to set a
  • contingency of the order of twelve days in the
    test time to allow for the possibility of
    unexpected
  • difficulties during the test, especially because
    of the complexity of the superconducting magnet
  • cryogenic system with 2500 liters of superfluid
    helium.
  • With best regards,
  • Joseph Burger
  • cc Jean Jamar

33
Status of Action Items fromJuly 3, 2003 Meeting
(2)
  • G. Piret says he has not yet gotten a response
    from manufacturer on ability of LSS vacuum gauges
    to withstand 5 gauss field at walls.
  • We offer to make a test in a weak field if ESTEC
    supplies a probe and its electronics.

34
Action Item 3
  • LSS Geometrical Mathemetical Model and Thermal
    Mathematical Model available only in
    ESATAN/ESARAD (developed by ESA)
  • We asked model be translated into SINDA/TRASYS
    (used by NASA and most others)
  • We were told this would probably be possible, but
    no answer came
  • Now told they will help support the translation.
    Two thermal engineers from SDU are now at CERN
    and will work on this with ESTEC and CGS

35
Status of Action Items fromJuly 3, 2003 Meeting
(4)
  • S. Harrison confirms cryosystem can remain
    disconnected from vacuum pump at least one day,
    so there is no danger of losing superfluidity in
    case of a crane failure while installing AMS-02
    in the LSS

36
Conclusion
  • Martin Zell and Wolfgang Supper have stated they
    do not expect any problem for ESA/ESTEC
    supporting the AMS-02 thermal vacuum test
  • M. Zell has funds to start support for test
    studies and preparation this year
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