| Miniproposals | ||||||||||||
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| 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 01:33:19:690PM | 1060525003 | Eric Edlund | 1 MW RF from D&E, density range looks good
try for 2MW |
| May 25 2006 01:47:57:343PM | 1060525004 | Eric Edlund | cascades detected near 0.175 seconds, initial frequency not measurable with PCI
try for higher power |
| May 25 2006 02:06:11:237PM | 1060525005 | Eric Edlund | P_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 02:19:30:953PM | 1060525006 | Eric Edlund | fizzle
|
| May 25 2006 02:27:14:080PM | 1060525007 | Eric Edlund | P_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 02:44:27:033PM | 1060525008 | Eric Edlund | P_RF(tot) ~ 3.6MW
no cascade activity, puzzling |
| May 25 2006 02:55:52:580PM | 1060525009 | Eric Edlund | P_RF(tot) ~ 3+ MW
again, no chirping modes, densities look similar to shot 7 with strong activity try for 4 MW |
| May 25 2006 03:25:25:343PM | 1060525010 | Eric Edlund | P_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 03:26:21:970PM | 1060525011 | Eric Edlund | change to 5.9 T
P_RF(tot) ~ 2.5MW no cascade activity, a few TAE's |
| May 25 2006 03:35:00:330PM | 1060525012 | Eric Edlund | P_RF(tot) ~ 3.0 MW
no cascades, some TAE's small sawteeth |
| May 25 2006 03:56:25:733PM | 1060525013 | Joseph Snipes | Snipes 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 04:07:42:047PM | 1060525014 | Joseph Snipes | Shot 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 04:24:51:093PM | 1060525015 | Joseph Snipes | Shot 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 04:35:06:860PM | 1060525016 | Joseph Snipes | Shot 16: Fizzle. |
| May 25 2006 04:53:08:580PM | 1060525017 | Joseph Snipes | Shot 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 05:13:33:877PM | 1060525018 | Joseph Snipes | Shot 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 08:42:27:847AM | 1060525002 | Ron Parker | There 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 09:07:17:753AM | 1060525002 | Ron Parker | Latest word is that the delay will be at least 2 hours. |
| May 25 2006 11:44:57:847AM | 1060525002 | Ron Parker | For 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 12:15:28:533PM | 1060525002 | Ron Parker | The 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 12:38:18:463PM | 1060525002 | Ron Parker | Good 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 01:28:50:690PM | 1060525003 | Ron Parker | First shot (3) went off well. RF ~ 1 MW.
Next: Increase RF to 2MW |
| May 25 2006 02:10:19:220PM | 1060525004 | Ron Parker | Shot 4 was OK, but disrupted at 0.6 s |
| May 25 2006 02:10:42:093PM | 1060525005 | Ron Parker | Shot 5 was OK, but disrupted at 0.4 s. |
| May 25 2006 02:11:01:767PM | 1060525006 | Ron Parker | Shot 6 fizzled. |
| May 25 2006 02:40:01:033PM | 1060525007 | Ron Parker | Shot started up OK, disrupted at 0.5 s. |
| May 25 2006 02:41:02:280PM | 1060525008 | Ron Parker | Shot disrupted at 0.27 s |
| May 25 2006 02:51:31:563PM | 1060525009 | Ron Parker | Shot 9 disrupted at 0.25 s |
| May 25 2006 03:09:58:610PM | 1060525010 | Ron Parker | Shot 10 disrupted at 0.42 s.
Next: Increase field to 5.9 T |
| May 25 2006 03:35:15:797PM | 1060525011 | Ron Parker | Shot 11 disrupted at ~ 0.41 s |
| May 25 2006 03:38:50:860PM | 1060525012 | Ron Parker | Shot 12 disrupted at ~ 0.39 s. |
| May 25 2006 03:57:50:610PM | 1060525013 | Ron Parker | A full length shot. |
| May 25 2006 03:58:33:470PM | 1060525014 | Ron Parker | Back to disruptions at 0.44 s |
| May 25 2006 04:22:11:813PM | 1060525015 | Ron Parker | Shot 15 disrupted at 0.38 s |
| May 25 2006 04:31:30:377PM | 1060525016 | Ron Parker | Fizzle |
| May 25 2006 04:46:25:797PM | 1060525017 | Ron Parker | Shot disrupted at 0.37 s. |
| May 25 2006 05:00:02:140PM | 1060525018 | Ron Parker | Shot 18 was the last shot. It disrupted at ~0.4 s. |
| Engineering Operator Comments | ||||
| Shot | Time | Type | Status | Comment |
| 1 | 08:18:16:470AM | Test | Ok | ok |
| 2 | 08:32:50:360AM | Test | Ok | |
| 3 | 01:18:52:610PM | Plasma | Ok | |
| 4 | 01:34:53:830PM | Plasma | Ok | |
| 5 | 01:51:14:360PM | Plasma | Ok | |
| 6 | 02:06:47:797PM | Plasma | Ok | |
| 7 | 02:19:21:297PM | Plasma | Ok | |
| 8 | 02:33:24:407PM | Plasma | Ok | |
| 9 | 02:46:00:110PM | Plasma | Ok | |
| 10 | 03:00:02:220PM | Plasma | Ok | PF breaker opened after disruption |
| 11 | 03:17:28:127PM | Plasma | Ok | PF breaker opened after disruption |
| 12 | 03:30:01:703PM | Plasma | Ok | PF breaker opened after diruption |
| 13 | 03:42:43:127PM | Plasma | Ok | |
| 14 | 03:55:21:533PM | Plasma | Ok | PF breaker opened after disruption |
| 15 | 04:17:03:017PM | Plasma | Ok | |
| 16 | 04:30:00:580PM | Plasma | Ok | |
| 17 | 04:42:25:313PM | Plasma | Ok | |
| 18 | 04:55:30:703PM | Plasma | Ok | |