The 2008 SPS electron cloud transmission experiment: first results F. Caspers, E. Mahner, T. Kroyer...

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The 2008 SPS electron cloud transmission experiment: The 2008 SPS electron cloud transmission experiment: first results first results F. Caspers, E. Mahner, T. Kroyer B. Henrist, J.M. Jimenez Thanks to the SPSU study team members For helpful discussions Outline Layout Basics and history First results during scrubbing run Conclusion and outlook ILCDR 08 July 2008 Cornell

Transcript of The 2008 SPS electron cloud transmission experiment: first results F. Caspers, E. Mahner, T. Kroyer...

Page 1: The 2008 SPS electron cloud transmission experiment: first results F. Caspers, E. Mahner, T. Kroyer B. Henrist, J.M. Jimenez Thanks to the SPSU study team.

The 2008 SPS electron cloud transmission experiment: first The 2008 SPS electron cloud transmission experiment: first resultsresults

F. Caspers, E. Mahner, T. KroyerB. Henrist, J.M. Jimenez

Thanks to the SPSU study team membersFor helpful discussions

Outline

Layout Basics and history First results during scrubbing run

Conclusion and outlook

ILCDR 08 July 2008 Cornell

Page 2: The 2008 SPS electron cloud transmission experiment: first results F. Caspers, E. Mahner, T. Kroyer B. Henrist, J.M. Jimenez Thanks to the SPSU study team.

F. Caspers, E. Mahner, T. Kroyer ILCDR 08 Cornell July 2008 2

Basic layout for microwave transmission setup (SPS 2008)

Principle idea:“When electromagnetic waves are

transmittedthrough a not too dense plasma, theyexperience a phase shift and possibly a

smallattenuation”

Antenna1 Antenna3

14.4 m 33.1 m

Antenna2 (excitation)

dipolequad

F. Caspers, T. Kroyer

2008 is similar to the 2004 setup

Page 3: The 2008 SPS electron cloud transmission experiment: first results F. Caspers, E. Mahner, T. Kroyer B. Henrist, J.M. Jimenez Thanks to the SPSU study team.

F. Caspers, E. Mahner, T. Kroyer ILCDR 08 Cornell July 2008 3

Some basics and history (1)

Page 4: The 2008 SPS electron cloud transmission experiment: first results F. Caspers, E. Mahner, T. Kroyer B. Henrist, J.M. Jimenez Thanks to the SPSU study team.

F. Caspers, E. Mahner, T. Kroyer ILCDR 08 Cornell July 2008 4

Some basics and history (2)

Page 5: The 2008 SPS electron cloud transmission experiment: first results F. Caspers, E. Mahner, T. Kroyer B. Henrist, J.M. Jimenez Thanks to the SPSU study team.

F. Caspers, E. Mahner, T. Kroyer ILCDR 08 Cornell July 2008 5

Some basics and history (3)

Page 6: The 2008 SPS electron cloud transmission experiment: first results F. Caspers, E. Mahner, T. Kroyer B. Henrist, J.M. Jimenez Thanks to the SPSU study team.

F. Caspers, E. Mahner, T. Kroyer ILCDR 08 Cornell July 2008 6

Some basics and history (4)

Page 7: The 2008 SPS electron cloud transmission experiment: first results F. Caspers, E. Mahner, T. Kroyer B. Henrist, J.M. Jimenez Thanks to the SPSU study team.

F. Caspers, E. Mahner, T. Kroyer ILCDR 08 Cornell July 2008 7

Some basics and history (5)

Page 8: The 2008 SPS electron cloud transmission experiment: first results F. Caspers, E. Mahner, T. Kroyer B. Henrist, J.M. Jimenez Thanks to the SPSU study team.

F. Caspers, E. Mahner, T. Kroyer ILCDR 08 Cornell July 2008 8

Some basics and history (6)

The presently used setup in BA5 is rather similar, except that we have dedicated button like PU‘s and kickers with a circulator after the hybrid and rather narrow-band filters (40 MHz) with steep slopes.

The filters are centered at 2.5 GHz. We used this time as receiver a conventional spectrum analyzer and a vector spectrum analyzer.

Page 9: The 2008 SPS electron cloud transmission experiment: first results F. Caspers, E. Mahner, T. Kroyer B. Henrist, J.M. Jimenez Thanks to the SPSU study team.

F. Caspers, E. Mahner, T. Kroyer ILCDR 08 Cornell July 2008 9

Preliminary measurement results in 2008 - scrubbing run (1)

SPS super-cycle 17656

Display from a conventional spectrum analzyer.

The phase modulation is in the small peaks, which are +/- 44 kHz away from the center.

The beam induced signal are the two bigger peaks next to the center line.

Page 10: The 2008 SPS electron cloud transmission experiment: first results F. Caspers, E. Mahner, T. Kroyer B. Henrist, J.M. Jimenez Thanks to the SPSU study team.

F. Caspers, E. Mahner, T. Kroyer ILCDR 08 Cornell July 2008 10

Preliminary measurement results in 2008 - scrubbing run (2)

Display from a conventional spectrum analzyer.

The phase modulation is in the small peaks, which are +/- 44 kHz away from the center.

The beam induced signal are the two bigger peaks next to the center line.

In this display one can see the true width of the carrier, the modulation sideband and the beam signals.

SPS super-cycle 17651

Page 11: The 2008 SPS electron cloud transmission experiment: first results F. Caspers, E. Mahner, T. Kroyer B. Henrist, J.M. Jimenez Thanks to the SPSU study team.

F. Caspers, E. Mahner, T. Kroyer ILCDR 08 Cornell July 2008 11

Preliminary measurement results in 2008 - scrubbing run (3)

SPS super-cycle 17568-69

Time axis is from top to bottom, intensity is color coded. CW signal on

Page 12: The 2008 SPS electron cloud transmission experiment: first results F. Caspers, E. Mahner, T. Kroyer B. Henrist, J.M. Jimenez Thanks to the SPSU study team.

F. Caspers, E. Mahner, T. Kroyer ILCDR 08 Cornell July 2008 12

Preliminary measurement results in 2008 - scrubbing run (4)

SPS super-cycle 17585-87

CW signal off-on-off-on

Page 13: The 2008 SPS electron cloud transmission experiment: first results F. Caspers, E. Mahner, T. Kroyer B. Henrist, J.M. Jimenez Thanks to the SPSU study team.

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Preliminary measurement results in 2008 - scrubbing run (5)

SPS super-cycle 17606-08

Shift of CW frequency

Page 14: The 2008 SPS electron cloud transmission experiment: first results F. Caspers, E. Mahner, T. Kroyer B. Henrist, J.M. Jimenez Thanks to the SPSU study team.

F. Caspers, E. Mahner, T. Kroyer ILCDR 08 Cornell July 2008 14

Preliminary measurement results in 2008 - scrubbing run (6)

SPS super-cycle 17601-03

Higher harmonics of the modulation sidebands since the modulation is rather rectangular than sinewave

Page 15: The 2008 SPS electron cloud transmission experiment: first results F. Caspers, E. Mahner, T. Kroyer B. Henrist, J.M. Jimenez Thanks to the SPSU study team.

F. Caspers, E. Mahner, T. Kroyer ILCDR 08 Cornell July 2008 15

Preliminary measurement results in 2008 - scrubbing run (7)

SPS super-cycle 17552Expanded view of one modulation sideband vs time.

Page 16: The 2008 SPS electron cloud transmission experiment: first results F. Caspers, E. Mahner, T. Kroyer B. Henrist, J.M. Jimenez Thanks to the SPSU study team.

F. Caspers, E. Mahner, T. Kroyer ILCDR 08 Cornell July 2008 16

Preliminary measurement results in 2008 - scrubbing run (8)

SPS super-cycle 17641Intensity of the modulation sideband vs time in logarithmic scale

Page 17: The 2008 SPS electron cloud transmission experiment: first results F. Caspers, E. Mahner, T. Kroyer B. Henrist, J.M. Jimenez Thanks to the SPSU study team.

F. Caspers, E. Mahner, T. Kroyer ILCDR 08 Cornell July 2008 17

Preliminary measurement results in 2008 - scrubbing run (9)

SPS super-cycle 17650Intensity of the modulation sideband vs time in linear scale

Page 18: The 2008 SPS electron cloud transmission experiment: first results F. Caspers, E. Mahner, T. Kroyer B. Henrist, J.M. Jimenez Thanks to the SPSU study team.

F. Caspers, E. Mahner, T. Kroyer ILCDR 08 Cornell July 2008 18

Preliminary measurement results in 2008 –AM contamination (1)

SPS super-cycle 21196, July 9th 2008

How about AM contamination?

Are we really sure that what we see on the green trace (upper half) is pure FM or PM

At least in this case its pure AM since the demodulation function of the VSA tells us that there is NO FM or PM signal where we would expect it.(lower trace)

Page 19: The 2008 SPS electron cloud transmission experiment: first results F. Caspers, E. Mahner, T. Kroyer B. Henrist, J.M. Jimenez Thanks to the SPSU study team.

F. Caspers, E. Mahner, T. Kroyer ILCDR 08 Cornell July 2008 19

Preliminary measurement results in 2008 –AM contamination (2)

SPS super-cycle 21200, July 9th 2008

Here one can see a small assymetry in height of the modulation lines in the conventional SPA display which is ALWAYS a hint for superposition of AM and FM or PMAND we also see a very small FM –PM Linie in the lower half of the display where we expect it.

Page 20: The 2008 SPS electron cloud transmission experiment: first results F. Caspers, E. Mahner, T. Kroyer B. Henrist, J.M. Jimenez Thanks to the SPSU study team.

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Preliminary measurement results in 2008 –AM contamination (3)

SPS super-cycle 17024, July 7th 2008

Another exampleUpper half:Conventional spectrumLower halfPM demodulation

This shot was taken after acceleration at flattop where usually we observed the strongest PM signals

2 batches

Page 21: The 2008 SPS electron cloud transmission experiment: first results F. Caspers, E. Mahner, T. Kroyer B. Henrist, J.M. Jimenez Thanks to the SPSU study team.

F. Caspers, E. Mahner, T. Kroyer ILCDR 08 Cornell July 2008 21

Preliminary measurement results in 2008 –AM contamination (4)

SPS super-cycle 16972, July 7th 2008

Here we have in the upper half the conventional spectrum and in the lower half the PM demodulated partObviously we cannot see anything during accerlation and a quantitative evaluation from this colour coded plot is not really possible.

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F. Caspers, E. Mahner, T. Kroyer ILCDR 08 Cornell July 2008 22

LHC beam in SPS, 25 ns bunch spacing, 72 bunches, 1 batch

Preliminary measurement results in 2008 - scrubbing run (10)

PS-type shielded button pickup signals

Yellow traceYellow trace stripline in stainless steel chamber #1Blue traceBlue trace pickup in chamber #1 containing enamel clearing electrodeMagenta traceMagenta trace pickup in stainless steel chamber #2 w/o enamel, for referenceNote, that there is some (unexpected) low frequency ringing (EMI) in the blue and magenta traceWe will try to understand its origin and get it removed in the future

Note that depite EMI contamination one can clearly see (light blue trace) the buildup of the e-cloud related current over the duration of the batch

Page 23: The 2008 SPS electron cloud transmission experiment: first results F. Caspers, E. Mahner, T. Kroyer B. Henrist, J.M. Jimenez Thanks to the SPSU study team.

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Conclusion and Outlook

The intermodulation problem observed in 2003 (experiments in BA2) has been considerably reduced using a proper RF setup with highly selective filters at the frontend, both, for excitation and on the pickup side. However the application of the phase demodulation function (using a vector spectrum analyzer) is strongly recommended for the elimination of residual AM contamination due to faint saturation effects [gain compression] (more than 50 dB below the carrier) caused by beam induced signals.

First electron cloud transmission experiments performed during the 2008 SPS scrubbing run in June have shown very promising results in BA5. The presence of electron clouds was identified simultaneously with button pickups.

Microwave transmission over a full LHC arc at cryogenic temperature has been already successfully demonstrated around 7 GHz. The technique discussed here can be directly applied for integral electron cloud diagnostics over a full arc in the LHC. For this purpose the installed in situ reflectometer couplers at the end of each arc could be used.

Many thanks to Christian Carli for lending us the real-time spectrum analyzer and contributing during data taking.