Design and Integration meeting: 27 October 2025 11:00 BST
Zoom: https://ukri.zoom.us/j/99571436156
Agenda
- CDR.
- Simulations.
- AOB.
Notes
Present: WS MMC CW TJK KL JP JM
Absent: RR HO MP
- CDR
- A few minor issues required discussion on the CDR:
- Eqn 2.17 has a factor t in it which cannot be correct. Author unknown, JP to read references & correct.
- Emittance not consistent in table 2.12, WS pointed out that MAD-X assumes constant emittance whereas BDSIM & GPT do not. JM to remove MAD-X emittance value from that table.
- Font is small on a number of figures. WS can easily replot with larger fonts. JM & KL to send list of figures that need modifying.
- WS to send JM the updated LhARA schematic diagram with updated caption.
- WS to add dimensions to the diagram.
- KL highlighted preferred use of mm & m, and to avoid cm. Text can be changed but modifying figures might be troublesome. Is context specific.
- A few minor issues required discussion on the CDR:
- Simulations
- WS: no update due to time toward Imperial Lates last week.
- TJK: plots shown on field leakage (see attached).
- End leakage small & away from the cavity, not thought to be significant.
- Field in the aperture/GFR does is larger. JP pointed out that the cores are at the edge of the aperture, not in it.
- 250mm long cavity included but planned device is 200mm long
- JP: Presented on chromatic effects in the Stage 1 arc. Slides will be attached.
- Dispersion calculated to be small. Higher order dispersion is finite & thought may be contributing to the effects MP sees.
- The impact on the beam size is small but this is noted to be recorded at the arc exit, not the end station (2m downstream).
- AOB
- WS raised that the IPAC abstracts have opened. We agreed to submit a general LhARA update abstract.
- JP recalculated RF cavity frequencies for protons & ions.
- LhARA range should be 1.46 MHz to 6.51 MHz. Lower number comes from carbon ions at 4 MeV/u, upper from protons.
- Stage 2 carbon ion energies will be limited to no lower than ~ 25 MeV/u. Radiobiological needs are unclear. A degrader may be needed for intermediate energies but fragmentation will be an issue.
Last modified
6 days ago
Last modified on Oct 27, 2025, 4:04:44 PM
Attachments (3)
- TJK Field Leakage 1.png (903.0 KB ) - added by 6 days ago.
- TJK Field Leakage 2.png (1.1 MB ) - added by 6 days ago.
- ArcStudy27102025.pdf (121.0 KB ) - added by 6 days ago.
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