The performance of a position sensitive wire chamber in the presence of a magnetic field
We have built a position sensitive wire chamber and tested it with X-rays and cosmic ray muons. Using a fill gas of 62% CF"4 and 38% CO"2, we have achieved resolutions of 38 μm for 1 keV X-rays, 42 μm for normally incident cosmic ray muons in the absence of a magnetic field, and 46 μm for...
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| Autor*in: |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
1994 |
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| Reproduktion: |
Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 |
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| Übergeordnetes Werk: |
in: Nuclear Instruments and Methods in Physics Research Section A: - Amsterdam : Elsevier, 349(1994), 1, Seite 37-46 |
| Übergeordnetes Werk: |
volume:349 ; year:1994 ; number:1 ; pages:37-46 |
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| 520 | |a We have built a position sensitive wire chamber and tested it with X-rays and cosmic ray muons. Using a fill gas of 62% CF"4 and 38% CO"2, we have achieved resolutions of 38 μm for 1 keV X-rays, 42 μm for normally incident cosmic ray muons in the absence of a magnetic field, and 46 μm for cosmic rays incident at the gas's Lorentz angle for a 0.8 T magnetic field. For throughgoing charged particles, the degradation in position resolution with angle away from the optimum incident angle has been found to be 11 μm/^o (added in quadrature). | ||
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| 700 | 1 | |a Gebhard, M.W. |4 oth | |
| 700 | 1 | |a Heinz, R.M. |4 oth | |
| 700 | 1 | |a Musser, J.A. |4 oth | |
| 700 | 1 | |a Pitts, J.J. |4 oth | |
| 700 | 1 | |a Miller, J.L. |4 oth | |
| 700 | 1 | |a Mufson, S.L. |4 oth | |
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(DE-627)NLEJ181686635 (DE-599)GBVNLZ181686635 DE-627 ger DE-627 rakwb eng The performance of a position sensitive wire chamber in the presence of a magnetic field 1994 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier We have built a position sensitive wire chamber and tested it with X-rays and cosmic ray muons. Using a fill gas of 62% CF"4 and 38% CO"2, we have achieved resolutions of 38 μm for 1 keV X-rays, 42 μm for normally incident cosmic ray muons in the absence of a magnetic field, and 46 μm for cosmic rays incident at the gas's Lorentz angle for a 0.8 T magnetic field. For throughgoing charged particles, the degradation in position resolution with angle away from the optimum incident angle has been found to be 11 μm/^o (added in quadrature). Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 Bower, C.R. oth Gebhard, M.W. oth Heinz, R.M. oth Musser, J.A. oth Pitts, J.J. oth Miller, J.L. oth Mufson, S.L. oth in Nuclear Instruments and Methods in Physics Research Section A: Amsterdam : Elsevier 349(1994), 1, Seite 37-46 (DE-627)NLEJ180854372 (DE-600)1466532-3 0168-9002 nnns volume:349 year:1994 number:1 pages:37-46 http://dx.doi.org/10.1016/0168-9002(94)90606-8 GBV_USEFLAG_H ZDB-1-SDJ GBV_NL_ARTICLE AR 349 1994 1 37-46 |
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(DE-627)NLEJ181686635 (DE-599)GBVNLZ181686635 DE-627 ger DE-627 rakwb eng The performance of a position sensitive wire chamber in the presence of a magnetic field 1994 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier We have built a position sensitive wire chamber and tested it with X-rays and cosmic ray muons. Using a fill gas of 62% CF"4 and 38% CO"2, we have achieved resolutions of 38 μm for 1 keV X-rays, 42 μm for normally incident cosmic ray muons in the absence of a magnetic field, and 46 μm for cosmic rays incident at the gas's Lorentz angle for a 0.8 T magnetic field. For throughgoing charged particles, the degradation in position resolution with angle away from the optimum incident angle has been found to be 11 μm/^o (added in quadrature). Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 Bower, C.R. oth Gebhard, M.W. oth Heinz, R.M. oth Musser, J.A. oth Pitts, J.J. oth Miller, J.L. oth Mufson, S.L. oth in Nuclear Instruments and Methods in Physics Research Section A: Amsterdam : Elsevier 349(1994), 1, Seite 37-46 (DE-627)NLEJ180854372 (DE-600)1466532-3 0168-9002 nnns volume:349 year:1994 number:1 pages:37-46 http://dx.doi.org/10.1016/0168-9002(94)90606-8 GBV_USEFLAG_H ZDB-1-SDJ GBV_NL_ARTICLE AR 349 1994 1 37-46 |
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(DE-627)NLEJ181686635 (DE-599)GBVNLZ181686635 DE-627 ger DE-627 rakwb eng The performance of a position sensitive wire chamber in the presence of a magnetic field 1994 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier We have built a position sensitive wire chamber and tested it with X-rays and cosmic ray muons. Using a fill gas of 62% CF"4 and 38% CO"2, we have achieved resolutions of 38 μm for 1 keV X-rays, 42 μm for normally incident cosmic ray muons in the absence of a magnetic field, and 46 μm for cosmic rays incident at the gas's Lorentz angle for a 0.8 T magnetic field. For throughgoing charged particles, the degradation in position resolution with angle away from the optimum incident angle has been found to be 11 μm/^o (added in quadrature). Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 Bower, C.R. oth Gebhard, M.W. oth Heinz, R.M. oth Musser, J.A. oth Pitts, J.J. oth Miller, J.L. oth Mufson, S.L. oth in Nuclear Instruments and Methods in Physics Research Section A: Amsterdam : Elsevier 349(1994), 1, Seite 37-46 (DE-627)NLEJ180854372 (DE-600)1466532-3 0168-9002 nnns volume:349 year:1994 number:1 pages:37-46 http://dx.doi.org/10.1016/0168-9002(94)90606-8 GBV_USEFLAG_H ZDB-1-SDJ GBV_NL_ARTICLE AR 349 1994 1 37-46 |
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(DE-627)NLEJ181686635 (DE-599)GBVNLZ181686635 DE-627 ger DE-627 rakwb eng The performance of a position sensitive wire chamber in the presence of a magnetic field 1994 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier We have built a position sensitive wire chamber and tested it with X-rays and cosmic ray muons. Using a fill gas of 62% CF"4 and 38% CO"2, we have achieved resolutions of 38 μm for 1 keV X-rays, 42 μm for normally incident cosmic ray muons in the absence of a magnetic field, and 46 μm for cosmic rays incident at the gas's Lorentz angle for a 0.8 T magnetic field. For throughgoing charged particles, the degradation in position resolution with angle away from the optimum incident angle has been found to be 11 μm/^o (added in quadrature). Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 Bower, C.R. oth Gebhard, M.W. oth Heinz, R.M. oth Musser, J.A. oth Pitts, J.J. oth Miller, J.L. oth Mufson, S.L. oth in Nuclear Instruments and Methods in Physics Research Section A: Amsterdam : Elsevier 349(1994), 1, Seite 37-46 (DE-627)NLEJ180854372 (DE-600)1466532-3 0168-9002 nnns volume:349 year:1994 number:1 pages:37-46 http://dx.doi.org/10.1016/0168-9002(94)90606-8 GBV_USEFLAG_H ZDB-1-SDJ GBV_NL_ARTICLE AR 349 1994 1 37-46 |
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(DE-627)NLEJ181686635 (DE-599)GBVNLZ181686635 DE-627 ger DE-627 rakwb eng The performance of a position sensitive wire chamber in the presence of a magnetic field 1994 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier We have built a position sensitive wire chamber and tested it with X-rays and cosmic ray muons. Using a fill gas of 62% CF"4 and 38% CO"2, we have achieved resolutions of 38 μm for 1 keV X-rays, 42 μm for normally incident cosmic ray muons in the absence of a magnetic field, and 46 μm for cosmic rays incident at the gas's Lorentz angle for a 0.8 T magnetic field. For throughgoing charged particles, the degradation in position resolution with angle away from the optimum incident angle has been found to be 11 μm/^o (added in quadrature). Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 Bower, C.R. oth Gebhard, M.W. oth Heinz, R.M. oth Musser, J.A. oth Pitts, J.J. oth Miller, J.L. oth Mufson, S.L. oth in Nuclear Instruments and Methods in Physics Research Section A: Amsterdam : Elsevier 349(1994), 1, Seite 37-46 (DE-627)NLEJ180854372 (DE-600)1466532-3 0168-9002 nnns volume:349 year:1994 number:1 pages:37-46 http://dx.doi.org/10.1016/0168-9002(94)90606-8 GBV_USEFLAG_H ZDB-1-SDJ GBV_NL_ARTICLE AR 349 1994 1 37-46 |
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performance of a position sensitive wire chamber in the presence of a magnetic field |
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The performance of a position sensitive wire chamber in the presence of a magnetic field |
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We have built a position sensitive wire chamber and tested it with X-rays and cosmic ray muons. Using a fill gas of 62% CF"4 and 38% CO"2, we have achieved resolutions of 38 μm for 1 keV X-rays, 42 μm for normally incident cosmic ray muons in the absence of a magnetic field, and 46 μm for cosmic rays incident at the gas's Lorentz angle for a 0.8 T magnetic field. For throughgoing charged particles, the degradation in position resolution with angle away from the optimum incident angle has been found to be 11 μm/^o (added in quadrature). |
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We have built a position sensitive wire chamber and tested it with X-rays and cosmic ray muons. Using a fill gas of 62% CF"4 and 38% CO"2, we have achieved resolutions of 38 μm for 1 keV X-rays, 42 μm for normally incident cosmic ray muons in the absence of a magnetic field, and 46 μm for cosmic rays incident at the gas's Lorentz angle for a 0.8 T magnetic field. For throughgoing charged particles, the degradation in position resolution with angle away from the optimum incident angle has been found to be 11 μm/^o (added in quadrature). |
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We have built a position sensitive wire chamber and tested it with X-rays and cosmic ray muons. Using a fill gas of 62% CF"4 and 38% CO"2, we have achieved resolutions of 38 μm for 1 keV X-rays, 42 μm for normally incident cosmic ray muons in the absence of a magnetic field, and 46 μm for cosmic rays incident at the gas's Lorentz angle for a 0.8 T magnetic field. For throughgoing charged particles, the degradation in position resolution with angle away from the optimum incident angle has been found to be 11 μm/^o (added in quadrature). |
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<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a22002652 4500</leader><controlfield tag="001">NLEJ181686635</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20210706160804.0</controlfield><controlfield tag="007">cr uuu---uuuuu</controlfield><controlfield tag="008">070505s1994 xx |||||o 00| ||eng c</controlfield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)NLEJ181686635</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-599)GBVNLZ181686635</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rakwb</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="245" ind1="1" ind2="4"><subfield code="a">The performance of a position sensitive wire chamber in the presence of a magnetic field</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">1994</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">nicht spezifiziert</subfield><subfield code="b">zzz</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">nicht spezifiziert</subfield><subfield code="b">z</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">nicht spezifiziert</subfield><subfield code="b">zu</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">We have built a position sensitive wire chamber and tested it with X-rays and cosmic ray muons. Using a fill gas of 62% CF"4 and 38% CO"2, we have achieved resolutions of 38 μm for 1 keV X-rays, 42 μm for normally incident cosmic ray muons in the absence of a magnetic field, and 46 μm for cosmic rays incident at the gas's Lorentz angle for a 0.8 T magnetic field. For throughgoing charged particles, the degradation in position resolution with angle away from the optimum incident angle has been found to be 11 μm/^o (added in quadrature).</subfield></datafield><datafield tag="533" ind1=" " ind2=" "><subfield code="f">Elsevier Journal Backfiles on ScienceDirect 1907 - 2002</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Bower, C.R.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Gebhard, M.W.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Heinz, R.M.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Musser, J.A.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Pitts, J.J.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Miller, J.L.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Mufson, S.L.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">in</subfield><subfield code="t">Nuclear Instruments and Methods in Physics Research Section A:</subfield><subfield code="d">Amsterdam : Elsevier</subfield><subfield code="g">349(1994), 1, Seite 37-46</subfield><subfield code="w">(DE-627)NLEJ180854372</subfield><subfield code="w">(DE-600)1466532-3</subfield><subfield code="x">0168-9002</subfield><subfield code="7">nnns</subfield></datafield><datafield tag="773" ind1="1" ind2="8"><subfield code="g">volume:349</subfield><subfield code="g">year:1994</subfield><subfield code="g">number:1</subfield><subfield code="g">pages:37-46</subfield></datafield><datafield tag="856" ind1="4" ind2="0"><subfield code="u">http://dx.doi.org/10.1016/0168-9002(94)90606-8</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_USEFLAG_H</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">ZDB-1-SDJ</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_NL_ARTICLE</subfield></datafield><datafield tag="951" ind1=" " ind2=" "><subfield code="a">AR</subfield></datafield><datafield tag="952" ind1=" " ind2=" "><subfield code="d">349</subfield><subfield code="j">1994</subfield><subfield code="e">1</subfield><subfield code="h">37-46</subfield></datafield></record></collection>
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