ID |
Date |
Author |
Type |
Category |
Subject |
Text |
 |
55
|
Wed Jul 8 18:12:25 2009 |
Damien Gallop | Routine | General | 18O2+ emittance scan | A/q = 9 FC6 = 50.0nA MB = 1470.8G @ 90.8A |
 |
56
|
Wed Jul 8 18:20:43 2009 |
Damien Gallop | Routine | General | 18O3+ emittance scan | A/q = 6 FC6 = 49.5nA MB = 1201.4G @ 73.1A |
 |
57
|
Wed Jul 8 18:38:21 2009 |
Damien Gallop | Routine | General | 18O4+ emittance scan | A/q = 4.5 FC6 = 29.5nA MB = 1041.8G @ 62.4A |
 |
58
|
Wed Jul 8 18:47:43 2009 |
Damien Gallop | Routine | General | 18O5+ emittance scan | A/q = 3.6 FC6 = 12.5nA MB = 931.8G @ 55.3A |
 |
59
|
Wed Jul 8 18:57:09 2009 |
Damien Gallop | Routine | General | 18O6+ emittance scan | A/q = 3 FC6 = 5.5nA MB = 851.5G @ 50.1A |
 |
60
|
Wed Jul 8 19:07:15 2009 |
Damien Gallop | Routine | General | 18O7+ emittance scan | A/q = 2.57 FC6 = 0.25nA MB = 790.0G @ 46.2A
Not enough intensity for an emittance
scan. |
|
61
|
Wed Jul 8 19:13:15 2009 |
Damien Gallop | Routine | General | 18O8+ emittance scan | A/q = 2.25 FC6 at reverse bias MB = 736.9G
@ 42.9A
Not enough intensity for an emittance |
  |
62
|
Wed Jul 8 19:51:33 2009 |
Damien Gallop | Routine | General | 18On+ summary for the day | The 18O source gas bottle is online. The
ion source was optimized for 18O4+ and kept
the same throughout. Emittance scans of each |
  |
63
|
Thu Jul 9 16:07:56 2009 |
Damien Gallop | Routine | General | 18O8+ frequency scans | Keerthi did some 18On+ frequency scans
this morning. He observed 18O8+! I am attempting
to repeat it myself now. Reverse bias on |
6x |
64
|
Fri Jul 10 09:55:25 2009 |
Damien Gallop | Routine | General | 18O8+ beam overnight | Here is a striptool of 18O8+ beam (magenta
trace) last evening from about 18:00 to 22:30
when there was a large power bump coincident |
|
65
|
Fri Jul 10 11:46:55 2009 |
Damien Gallop | Routine | General | 18On+ frequency scans & resonances | The Supernanogan was restarted this morning,
after last night's power bump. 18O4+ on FC6,
cooking for about an hour. Looks very good. |
|
66
|
Fri Jul 10 11:47:07 2009 |
Damien Gallop | Routine | General | 18On+ frequency scans & resonances | The Supernanogan was restarted this morning,
after last night's power bump. 18O4+ on FC6,
cooking for about an hour. Looks very good. |
|
133
|
Fri Sep 11 23:42:45 2009 |
Keerthi | Other | General | MCIS turbo pump | MCIS TP1 is not running well. Needs investigation
as soon as S1219 is completed.
Later... TP1 failed completely, and |
|
138
|
Tue Sep 15 19:46:21 2009 |
Keerthi | Routine | General | Supernanogan emittance scans | 090915_1915ILTEMIT.txt = 17O +3, 4.4uA
new tune, scanner offset +10V, scanner
scale 100nA , 100x50 matrix |
9x |
140
|
Wed Sep 16 12:12:04 2009 |
Keerthi | Routine | General | 17O+3 emittance sacns | 090916_1156ILTEMIT.txt
17O+3 good settings 50x100 ,
333nA Scale, ~4uA |
|
142
|
Wed Sep 16 12:26:51 2009 |
Keerthi | Routine | General | 17O+3 emittance with changed steering | 090916_1222ILTEMIT.txt Changed the
MCIS steering to center the beam in the EL.
17O+3 ~5uA, 50x100 |
|
148
|
Fri Oct 2 09:38:26 2009 |
Keerthi | Routine | General | 33Sulfur development completed successfully. |
Sulfur-33
development completed successfully.
|
|
264
|
Fri May 7 19:10:05 2010 |
Keerthi Jayamanna | Routine | General | OLIS status | MW source is back and running.
A new vacuum
chamber is added to the Supernanogan RF block.
SO2
is not filled in yet. |
|
417
|
Wed Aug 3 00:15:39 2011 |
Keerthi Jayamanna | Other | General | 22Ne+2 | Source started at 800W of microwave power
and 2cc/min neon gas easily. New magnetron
produces more power than the old one. |
|
469
|
Sun Dec 2 22:32:19 2012 |
Keerthi Jayamanna | Routine | General | Still cannot write anything other than Subject | |
|