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--- tripleg_group [2018/09/14 01:30]
gastis
+++ tripleg_group [2018/09/14 09:32] (current)
gao
@@ Line 6: / Line 6: @@
 **Q3.**
 We use the example from the wiki [[https://wikihost.nscl.msu.edu/JIOSS/lib/exe/fetch.php?media=dispersion.zip|Dispersion]] as a starting point and do the following:
 , Find the lines as shown in the picture below:
 {{:dispersion_ele.png?direct&400|}}
 In the picture above, each of the commands (DL, DP, MQ ...) represents an ion optics element. (For a complete reference of the commands used in the cosy script, one has to refer to the manual). Here in the step 3 of [[https://wikihost.nscl.msu.edu/JIOSS/lib/exe/fetch.php?media=project_for_the_jina_ion_optics_for_recoil_separator_school_v4.pdf|this project]], what we want is very simple:a drift, 45-degree dipole magnet with a 1 meter bending
 radius and a drift. So we modify this part of the script as shown in the picture below:
@@ Line 47: / Line 49: @@
 For reaching the maximum angular acceptance we need energies above 20MeV/u.
-It is interested to mention that the lower energy that we use for measuring this reaction (using the most intense charge state) is 0.5MeV/u since at this point we reach the lower limit of SECAR on Brho (Tmin = 0.14 Tm)
-* all energies that were mentioned are in the lab system.
+* all energies are in the lab system.

JINA-CEE ION OPTICS SUMMER SCHOOL: JIOSS 2018