Alcator C-Mod Run 1060525 Information

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Miniproposals
Miniproposal:444
Date Filed:11/23/2005
Title:Alfvén cascade studies during current ramp-up with ICRF Heating
First Author:Eric Edlund
Session Leader:Eric Edlund (shots 1-12)
Session Leader:Joseph Snipes (shots 13-18)

Operators
Session leader(s):Eric Edlund,Joseph Snipes
Physics operator(s):Jim Irby,Ron Parker
Engineering operator(s):Bill Cochran,Sam Pierson,Bill Parkin

Engineering Operator Run Comment
MP444: Alfven cascade studies during current ramp with ICRF heating.

Session Leader Plans
Entered: May 24 2006 05:35:15:383PM
Author: Eric Edlund
SL: Eric Edlund
PO: Ron Parker

MP #444a
Alfvén cascade studies during the current ramp-up with ICRF Heating

The purpose of these experiments is to expand the database of Alfven cascades, specifically looking at the dependence of the initial frequency on temperature. Excitation of the cascade modes is induced by resonant interaction with the RF generated ion tail. Previous thresholds for activity were about 2.5 MW. It is expected that stong activity will be seen at 3 and 4 MW. A scan of RF power at 1 MW steps will be used to vary the bulk temperature. Furthermore, a change to off-axis heating at 5.9 T will be used to look for variations in cascade characteristics due to modification of the pressure profile. Concluding the plan is a change to lower density, 0.5 10^19 in nl_04 to look for density dependence.

Setup:

RF, all 4 transmitters run-on by 8:30 am

diagnostics, PCI and magnetics are the principal diagnostics. ECE and Thomson are required for temperature and density profile measurements. The CNPA, Hirex, and neutrons are requested to help monitor ion temperatures.


Run Plan:

Use a target plasma similar to 1050429015.

Begin at 5.4 T, Ip = 800 kA, nl_04 = 0.7 10^19 in flattop.

RF on at 3MW total power beginning at 0.09 sec, full power by 0.10 sec.
Establish Alfven cascade activity and then proceed with power scan from 2MW to 5MW (if possible) in 1MW steps. Shots will be repeated to improve the RF matching, if necessary.

Change to off-axis heating at 5.9 T. Repeat the power scan.

Perform a power scan in lower density, nl_04 = 0.5 10^19, at 5.4T.


Physics Operators Plans
Entered: May 24 2006 06:36:03:723PM
Author: Ron Parker
Physop plan and engineering setup for Thursday, May 25, 2006

MP444: Alfven cascade studies during current ramp with ICRF heating.
SL: Eric Edlund
PO: Ron Parker

Overnight ECDC


Engineering setup:
-------------------
Power system setup as on 1060524014

Gas Setup:
fill B-Top with 6 psi D2 Hybrid enabled (PG4)
fill B-side lower with 1 psi Ar + 2 psi Ne Hybrid disabled (PG1)
leave B-side upper with 15psi He3 as is. Hybrid disabled (PG2)
fill B-main with 40 psi D2 Hybrid enabled (PG3)
leave NINJA as is. Hybrid disabled.

Enable the following gate valves and shutters, assuming no vacuum problems:
ECE, VUV, Z-bolo shutters

FMIT#1,2,3,4 in Run-on by 8:30AM; turn on earlier if requested by RF
(ICRF (D,E and J ports) ready for first shot at 9:00 AM)


Run Plan:
---------------------
Start with 1060524014 with RF beginning at 0.09 sec. Full power by 0.10 sec.

Tune discharge for rapid current rise and density ne_l(04) ~ 0.7e20 cm-2

Establish Alfven cascade and do power scan from 2 MW up in 1 MW steps.

Change to off-axis heating at 5.9 T. Repeat power scan.

Reduce density to ne_l(04) ~ 0.5e20 cm-2 at 5.4T, repeat power scan.


Session Leader Summaries
Entered: May 25 2006 05:16:33:360PM
Author: Joseph Snipes
The run got off to a slow start because of alternator problems. The RF behaved reasonably well, but as
always, it is difficult to maintain good coupling during the current rise. So, there were a number of
trips of the RF that made it difficult to get good cascades before the current profile evolved into
positive shear. Still, we managed to get 14 plasmas, most of which had AE activity in the current rise.
There were a number of shots with Alfven cascades including shots 4, 5, 7, 14, and 15. There may have been
very weak cascades on the PCI for a couple of other shots. Still, with the goal of the MP to try to
determine a scaling for the starting frequency of the Alfven cascades, it will be quite difficult because
the cascades were not all that clear at the low frequency end. So, while there are a number of shots with
cascade data, it is unlikely that the data will provide a clear scaling for the minimum frequency as
desired by the MP. An interesting set of what look like tornado modes were seen on the magnetics and PCI
from 0.175 to 0.188 s and from 520 to 600 kHz on shot 1060525015. It is possible that they appear just
before the first very small sawtooth, but the ECE data is not clear that it is indeed a sawtooth at that
time.

Physics Operator Summaries
Entered: May 25 2006 04:57:45:173PM
Author: Ron Parker
The run was delayed by 4 hours due to alternator problem in the drive motor circuitry.

When underway at 1:00, the run was devoted to producing Alfven cascades by ramping the current rapidly and simultaneously coupling strong ICRF heating during the early current ramp phase. This combination resulted in disruptions at ~ 0.4 s for most of the shots. However, since the cascades terminated when sawteeth appeared, typically at 0.22 s, the early disruption did not interfere with the cascade studies. Up to 4 MW of ICRF was applied, both on and off axis, and cascade modes were produced on most shots.

Scorecard: 16 plasma attempts, 2 fizzles, 2 full length plasmas and the rest early disruptions.

Session Leader Comments
May 25 2006 01:33:19:690PM1060525003Eric Edlund1 MW RF from D&E, density range looks good
try for 2MW
May 25 2006 01:47:57:343PM1060525004Eric Edlundcascades detected near 0.175 seconds, initial frequency not measurable with PCI
try for higher power
May 25 2006 02:06:11:237PM1060525005Eric EdlundP_RF (tot) ~ 2-3 MW
stronger cascade activity, still no initial frequencies visible
try again with J ramp from 0.10 to 0.15 seconds


May 25 2006 02:19:30:953PM1060525006Eric Edlundfizzle



May 25 2006 02:27:14:080PM1060525007Eric EdlundP_RF(tot) ~ 3MW
using J port power ramp from 0.10 to 0.15 seconds
good cascade data, interesting mode (possibly n=2 or 3) mode coming in much later
than usual, possibly q=1 mode???

May 25 2006 02:44:27:033PM1060525008Eric EdlundP_RF(tot) ~ 3.6MW
no cascade activity, puzzling
May 25 2006 02:55:52:580PM1060525009Eric EdlundP_RF(tot) ~ 3+ MW
again, no chirping modes, densities look similar to shot 7 with strong activity
try for 4 MW

May 25 2006 03:25:25:343PM1060525010Eric EdlundP_RF(tot) ~ 3MW
one early up-chirping mode followed by a down-chirping mode
no other significant cascade activity

Sawtooth modes seen near 0.35 seconds
May 25 2006 03:26:21:970PM1060525011Eric Edlundchange to 5.9 T
P_RF(tot) ~ 2.5MW

no cascade activity, a few TAE's
May 25 2006 03:35:00:330PM1060525012Eric EdlundP_RF(tot) ~ 3.0 MW
no cascades, some TAE's
small sawteeth
May 25 2006 03:56:25:733PM1060525013Joseph SnipesSnipes taking over for Edlund as Session Leader. Shot 13 is OK, but no Alfven Cascades were observed.
There were some TAEs between 0.11 and 0.16 s in the range from 350 to 500 kHz.
May 25 2006 04:07:42:047PM1060525014Joseph SnipesShot 14: Finally got the Alfven cascades back. It appears that slightly higher density is important to get
the cascades. We also got 4 MW of RF.
May 25 2006 04:24:51:093PM1060525015Joseph SnipesShot 15: Got 4 MW again and Alfven cascades, though the RF trips at 0.15 s and so do the AEs. No AEs after
about 0.2 s.
May 25 2006 04:35:06:860PM1060525016Joseph SnipesShot 16: Fizzle.
May 25 2006 04:53:08:580PM1060525017Joseph SnipesShot 17: RF tripped. Got about 2.5 MW early which eventually reached 4 MW after
0.22 s, but by then the AEs are gone. No cascades. Try raising the density
early between 0.05 and 0.1 s as well as after 0.1 s in segment 2
for the next and last shot.
May 25 2006 05:13:33:877PM1060525018Joseph SnipesShot 18: Very similar modes to shot 17. No cascades. RF trips keep the power around 2.5 MW until after
0.22 s when it reaches 4 MW.

Physics Operator Comments
May 25 2006 08:42:27:847AM1060525002Ron ParkerThere will be a delay this morning due to an alternator problem.
Stay tuned for more details. Delay looks like at least an hour.
May 25 2006 09:07:17:753AM1060525002Ron ParkerLatest word is that the delay will be at least 2 hours.
May 25 2006 11:44:57:847AM1060525002Ron ParkerFor those of you waiting, here is my uunderstanding: The alternator problem has to do with the switching out of an autotransformer in the drive motor excitation. This should happen at around 1200 RPM, but it chattered when this speed was passed earlier, causing a drop out. At the moment the alternator crew is awaitng some instrumentation to monitor the problem. They will then try to pass the transfer speed again. If successful, there will be a run; if not, it will likely be scrubbed. In any event, the earliest that we could have plasma shots would be 12:00.
May 25 2006 12:15:28:533PM1060525002Ron ParkerThe alternator is coming up to speed, about 1030 RPM as this is written. It should be passing the critical speed soon and we'll know then if there will be a run. The earliest start time now looks to be about 1:00 or shortly thereafter.
May 25 2006 12:38:18:463PM1060525002Ron ParkerGood news. The alternator went through the critical speed with no problem (although we may see this problem again on another day!) and we'll have a run, although abbrieviated (we need a spell check for the logbook!). First shot should be at ~1:15.
May 25 2006 01:28:50:690PM1060525003Ron ParkerFirst shot (3) went off well. RF ~ 1 MW.

Next: Increase RF to 2MW
May 25 2006 02:10:19:220PM1060525004Ron ParkerShot 4 was OK, but disrupted at 0.6 s
May 25 2006 02:10:42:093PM1060525005Ron ParkerShot 5 was OK, but disrupted at 0.4 s.
May 25 2006 02:11:01:767PM1060525006Ron ParkerShot 6 fizzled.
May 25 2006 02:40:01:033PM1060525007Ron ParkerShot started up OK, disrupted at 0.5 s.
May 25 2006 02:41:02:280PM1060525008Ron ParkerShot disrupted at 0.27 s
May 25 2006 02:51:31:563PM1060525009Ron ParkerShot 9 disrupted at 0.25 s
May 25 2006 03:09:58:610PM1060525010Ron ParkerShot 10 disrupted at 0.42 s.

Next: Increase field to 5.9 T
May 25 2006 03:35:15:797PM1060525011Ron ParkerShot 11 disrupted at ~ 0.41 s
May 25 2006 03:38:50:860PM1060525012Ron ParkerShot 12 disrupted at ~ 0.39 s.
May 25 2006 03:57:50:610PM1060525013Ron ParkerA full length shot.
May 25 2006 03:58:33:470PM1060525014Ron ParkerBack to disruptions at 0.44 s
May 25 2006 04:22:11:813PM1060525015Ron ParkerShot 15 disrupted at 0.38 s
May 25 2006 04:31:30:377PM1060525016Ron ParkerFizzle
May 25 2006 04:46:25:797PM1060525017Ron ParkerShot disrupted at 0.37 s.
May 25 2006 05:00:02:140PM1060525018Ron ParkerShot 18 was the last shot. It disrupted at ~0.4 s.

Engineering Operator Comments
ShotTimeTypeStatusComment
108:18:16:470AMTestOkok
208:32:50:360AMTestOk
301:18:52:610PMPlasmaOk
401:34:53:830PMPlasmaOk
501:51:14:360PMPlasmaOk
602:06:47:797PMPlasmaOk
702:19:21:297PMPlasmaOk
802:33:24:407PMPlasmaOk
902:46:00:110PMPlasmaOk
1003:00:02:220PMPlasmaOkPF breaker opened after disruption
1103:17:28:127PMPlasmaOkPF breaker opened after disruption
1203:30:01:703PMPlasmaOkPF breaker opened after diruption
1303:42:43:127PMPlasmaOk
1403:55:21:533PMPlasmaOkPF breaker opened after disruption
1504:17:03:017PMPlasmaOk
1604:30:00:580PMPlasmaOk
1704:42:25:313PMPlasmaOk
1804:55:30:703PMPlasmaOk