Charge and mass resolved time of flight observations of 140 fs laser produced ions : Proceedings of the tenth topical conference on high temperature plasma diagnostics
Guethlein, G. ; Bonlie, J. ; Price, D. ; Shepherd, R. ; Young, B. ; Stewart, R.
[S.l.] : American Institute of Physics (AIP)
Published 1995
[S.l.] : American Institute of Physics (AIP)
Published 1995
| ISSN: |
1089-7623
|
|---|---|
| Source: |
AIP Digital Archive
|
| Topics: |
Physics
Electrical Engineering, Measurement and Control Technology
|
| Notes: |
Ions from this plasma are self-extracting with energies of 0.1 to 100 keV, the extraction potential being one of the desired observables. The charge/mass (z/μ, μ is mass in AMU) separation is provided by a static magnetic field (B⋅L=1280 G cm, FWHM=14 mm) located 5 cm from the linear (1−d) detector. Displacement along the detector axis is thus proportional to z/μ(1/v). The detector is a gold cathode MCP with a fast (sub-ns) phosphor. The phosphor output is coupled into a streak camera (typical sweep 8.5 or 24 μs total) through a coherent fiber bundle. Streak images are grabbed with a 14-bit CCD. The signature of any specific ion is a straight line of slope proportional to z/μ. Since there are usually more than one charge state of a given ion, integer multiple slopes appear. Thus z and m can be found. Absolute calibration is taken from the slope of the proton streak, which is always present with our plasmas. While providing the same information as a Thomson parabola, the straight line images are easier to extract information from and offer resolution with less energy dependence. By providing mass and time of flight information, the product of z⋅Te can be determined unambiguously during the hydrodynamic acceleration of the plasma. © 1995 American Institute of Physics.
|
| Type of Medium: |
Electronic Resource
|
| URL: |
| _version_ | 1798289701791072258 |
|---|---|
| autor | Guethlein, G. Bonlie, J. Price, D. Shepherd, R. Young, B. Stewart, R. |
| autorsonst | Guethlein, G. Bonlie, J. Price, D. Shepherd, R. Young, B. Stewart, R. |
| book_url | http://dx.doi.org/10.1063/1.1146404 |
| datenlieferant | nat_lic_papers |
| hauptsatz | hsatz_simple |
| identnr | NLZ219461740 |
| issn | 1089-7623 |
| journal_name | Review of Scientific Instruments |
| materialart | 1 |
| notes | Ions from this plasma are self-extracting with energies of 0.1 to 100 keV, the extraction potential being one of the desired observables. The charge/mass (z/μ, μ is mass in AMU) separation is provided by a static magnetic field (B⋅L=1280 G cm, FWHM=14 mm) located 5 cm from the linear (1−d) detector. Displacement along the detector axis is thus proportional to z/μ(1/v). The detector is a gold cathode MCP with a fast (sub-ns) phosphor. The phosphor output is coupled into a streak camera (typical sweep 8.5 or 24 μs total) through a coherent fiber bundle. Streak images are grabbed with a 14-bit CCD. The signature of any specific ion is a straight line of slope proportional to z/μ. Since there are usually more than one charge state of a given ion, integer multiple slopes appear. Thus z and m can be found. Absolute calibration is taken from the slope of the proton streak, which is always present with our plasmas. While providing the same information as a Thomson parabola, the straight line images are easier to extract information from and offer resolution with less energy dependence. By providing mass and time of flight information, the product of z⋅Te can be determined unambiguously during the hydrodynamic acceleration of the plasma. © 1995 American Institute of Physics. |
| package_name | American Institute of Physics (AIP) |
| publikationsjahr_anzeige | 1995 |
| publikationsjahr_facette | 1995 |
| publikationsjahr_intervall | 8004:1995-1999 |
| publikationsjahr_sort | 1995 |
| publikationsort | [S.l.] |
| publisher | American Institute of Physics (AIP) |
| reference | 66 (1995), S. 333-335 |
| search_space | articles |
| shingle_author_1 | Guethlein, G. Bonlie, J. Price, D. Shepherd, R. Young, B. Stewart, R. |
| shingle_author_2 | Guethlein, G. Bonlie, J. Price, D. Shepherd, R. Young, B. Stewart, R. |
| shingle_author_3 | Guethlein, G. Bonlie, J. Price, D. Shepherd, R. Young, B. Stewart, R. |
| shingle_author_4 | Guethlein, G. Bonlie, J. Price, D. Shepherd, R. Young, B. Stewart, R. |
| shingle_catch_all_1 | Guethlein, G. Bonlie, J. Price, D. Shepherd, R. Young, B. Stewart, R. Charge and mass resolved time of flight observations of 140 fs laser produced ions : Proceedings of the tenth topical conference on high temperature plasma diagnostics Ions from this plasma are self-extracting with energies of 0.1 to 100 keV, the extraction potential being one of the desired observables. The charge/mass (z/μ, μ is mass in AMU) separation is provided by a static magnetic field (B⋅L=1280 G cm, FWHM=14 mm) located 5 cm from the linear (1−d) detector. Displacement along the detector axis is thus proportional to z/μ(1/v). The detector is a gold cathode MCP with a fast (sub-ns) phosphor. The phosphor output is coupled into a streak camera (typical sweep 8.5 or 24 μs total) through a coherent fiber bundle. Streak images are grabbed with a 14-bit CCD. The signature of any specific ion is a straight line of slope proportional to z/μ. Since there are usually more than one charge state of a given ion, integer multiple slopes appear. Thus z and m can be found. Absolute calibration is taken from the slope of the proton streak, which is always present with our plasmas. While providing the same information as a Thomson parabola, the straight line images are easier to extract information from and offer resolution with less energy dependence. By providing mass and time of flight information, the product of z⋅Te can be determined unambiguously during the hydrodynamic acceleration of the plasma. © 1995 American Institute of Physics. 1089-7623 10897623 American Institute of Physics (AIP) |
| shingle_catch_all_2 | Guethlein, G. Bonlie, J. Price, D. Shepherd, R. Young, B. Stewart, R. Charge and mass resolved time of flight observations of 140 fs laser produced ions : Proceedings of the tenth topical conference on high temperature plasma diagnostics Ions from this plasma are self-extracting with energies of 0.1 to 100 keV, the extraction potential being one of the desired observables. The charge/mass (z/μ, μ is mass in AMU) separation is provided by a static magnetic field (B⋅L=1280 G cm, FWHM=14 mm) located 5 cm from the linear (1−d) detector. Displacement along the detector axis is thus proportional to z/μ(1/v). The detector is a gold cathode MCP with a fast (sub-ns) phosphor. The phosphor output is coupled into a streak camera (typical sweep 8.5 or 24 μs total) through a coherent fiber bundle. Streak images are grabbed with a 14-bit CCD. The signature of any specific ion is a straight line of slope proportional to z/μ. Since there are usually more than one charge state of a given ion, integer multiple slopes appear. Thus z and m can be found. Absolute calibration is taken from the slope of the proton streak, which is always present with our plasmas. While providing the same information as a Thomson parabola, the straight line images are easier to extract information from and offer resolution with less energy dependence. By providing mass and time of flight information, the product of z⋅Te can be determined unambiguously during the hydrodynamic acceleration of the plasma. © 1995 American Institute of Physics. 1089-7623 10897623 American Institute of Physics (AIP) |
| shingle_catch_all_3 | Guethlein, G. Bonlie, J. Price, D. Shepherd, R. Young, B. Stewart, R. Charge and mass resolved time of flight observations of 140 fs laser produced ions : Proceedings of the tenth topical conference on high temperature plasma diagnostics Ions from this plasma are self-extracting with energies of 0.1 to 100 keV, the extraction potential being one of the desired observables. The charge/mass (z/μ, μ is mass in AMU) separation is provided by a static magnetic field (B⋅L=1280 G cm, FWHM=14 mm) located 5 cm from the linear (1−d) detector. Displacement along the detector axis is thus proportional to z/μ(1/v). The detector is a gold cathode MCP with a fast (sub-ns) phosphor. The phosphor output is coupled into a streak camera (typical sweep 8.5 or 24 μs total) through a coherent fiber bundle. Streak images are grabbed with a 14-bit CCD. The signature of any specific ion is a straight line of slope proportional to z/μ. Since there are usually more than one charge state of a given ion, integer multiple slopes appear. Thus z and m can be found. Absolute calibration is taken from the slope of the proton streak, which is always present with our plasmas. While providing the same information as a Thomson parabola, the straight line images are easier to extract information from and offer resolution with less energy dependence. By providing mass and time of flight information, the product of z⋅Te can be determined unambiguously during the hydrodynamic acceleration of the plasma. © 1995 American Institute of Physics. 1089-7623 10897623 American Institute of Physics (AIP) |
| shingle_catch_all_4 | Guethlein, G. Bonlie, J. Price, D. Shepherd, R. Young, B. Stewart, R. Charge and mass resolved time of flight observations of 140 fs laser produced ions : Proceedings of the tenth topical conference on high temperature plasma diagnostics Ions from this plasma are self-extracting with energies of 0.1 to 100 keV, the extraction potential being one of the desired observables. The charge/mass (z/μ, μ is mass in AMU) separation is provided by a static magnetic field (B⋅L=1280 G cm, FWHM=14 mm) located 5 cm from the linear (1−d) detector. Displacement along the detector axis is thus proportional to z/μ(1/v). The detector is a gold cathode MCP with a fast (sub-ns) phosphor. The phosphor output is coupled into a streak camera (typical sweep 8.5 or 24 μs total) through a coherent fiber bundle. Streak images are grabbed with a 14-bit CCD. The signature of any specific ion is a straight line of slope proportional to z/μ. Since there are usually more than one charge state of a given ion, integer multiple slopes appear. Thus z and m can be found. Absolute calibration is taken from the slope of the proton streak, which is always present with our plasmas. While providing the same information as a Thomson parabola, the straight line images are easier to extract information from and offer resolution with less energy dependence. By providing mass and time of flight information, the product of z⋅Te can be determined unambiguously during the hydrodynamic acceleration of the plasma. © 1995 American Institute of Physics. 1089-7623 10897623 American Institute of Physics (AIP) |
| shingle_title_1 | Charge and mass resolved time of flight observations of 140 fs laser produced ions : Proceedings of the tenth topical conference on high temperature plasma diagnostics |
| shingle_title_2 | Charge and mass resolved time of flight observations of 140 fs laser produced ions : Proceedings of the tenth topical conference on high temperature plasma diagnostics |
| shingle_title_3 | Charge and mass resolved time of flight observations of 140 fs laser produced ions : Proceedings of the tenth topical conference on high temperature plasma diagnostics |
| shingle_title_4 | Charge and mass resolved time of flight observations of 140 fs laser produced ions : Proceedings of the tenth topical conference on high temperature plasma diagnostics |
| sigel_instance_filter | dkfz geomar wilbert ipn albert |
| source_archive | AIP Digital Archive |
| timestamp | 2024-05-06T08:05:01.781Z |
| titel | Charge and mass resolved time of flight observations of 140 fs laser produced ions : Proceedings of the tenth topical conference on high temperature plasma diagnostics |
| titel_suche | Charge and mass resolved time of flight observations of 140 fs laser produced ions Proceedings of the tenth topical conference on high temperature plasma diagnostics |
| topic | U ZN |
| uid | nat_lic_papers_NLZ219461740 |