-
1
-
-
0026664144
-
-
10.1121/1.402855
-
D. F. Gaitan, L. A. Crum, R. A. Roy, and C. C. Church, J. Acoust. Soc. Am. 91, 3166 (1992). 10.1121/1.402855
-
(1992)
J. Acoust. Soc. Am.
, vol.91
, pp. 3166
-
-
Gaitan, D.F.1
Crum, L.A.2
Roy, R.A.3
Church, C.C.4
-
2
-
-
78651312735
-
-
Ph.D. thesis, University of Mississippi
-
D. F. Gaitan, Ph.D. thesis, University of Mississippi, 1990.
-
(1990)
-
-
Gaitan, D.F.1
-
9
-
-
78651283334
-
-
By color temperature we understand the temperature derived from a best fit of a given spectrum to blackbody radiation, regardless of the origin of the spectrum.
-
By color temperature we understand the temperature derived from a best fit of a given spectrum to blackbody radiation, regardless of the origin of the spectrum.
-
-
-
-
11
-
-
0033095318
-
-
10.1103/PhysRevE.59.2986
-
W. C. Moss, D. A. Young, J. A. Harte, J. L. Levatin, B. F. Rozsnyai, G. B. Zimmerman, and I. H. Zimmerman, Phys. Rev. E 59, 2986 (1999). 10.1103/PhysRevE.59.2986
-
(1999)
Phys. Rev. e
, vol.59
, pp. 2986
-
-
Moss, W.C.1
Young, D.A.2
Harte, J.A.3
Levatin, J.L.4
Rozsnyai, B.F.5
Zimmerman, G.B.6
Zimmerman, I.H.7
-
12
-
-
0000283631
-
-
10.1103/PhysRevE.54.5004
-
A. K. Evans, Phys. Rev. E 54, 5004 (1996). 10.1103/PhysRevE.54.5004
-
(1996)
Phys. Rev. e
, vol.54
, pp. 5004
-
-
Evans, A.K.1
-
13
-
-
0000446916
-
-
10.1103/PhysRevLett.70.3424
-
C. C. Wu and P. H. Roberts, Phys. Rev. Lett. 70, 3424 (1993). 10.1103/PhysRevLett.70.3424
-
(1993)
Phys. Rev. Lett.
, vol.70
, pp. 3424
-
-
Wu, C.C.1
Roberts, P.H.2
-
14
-
-
33646348126
-
-
10.1103/PhysRevE.73.056302
-
W.-K. Tse and P. T. Leung, Phys. Rev. E 73, 056302 (2006). 10.1103/PhysRevE.73.056302
-
(2006)
Phys. Rev. e
, vol.73
, pp. 056302
-
-
Tse, W.-K.1
Leung, P.T.2
-
15
-
-
33747734117
-
-
10.1103/PhysRevE.74.026304
-
Yu. An, Phys. Rev. E 74, 026304 (2006). 10.1103/PhysRevE.74.026304
-
(2006)
Phys. Rev. e
, vol.74
, pp. 026304
-
-
An, Yu.1
-
16
-
-
0037071270
-
-
10.1103/PhysRevLett.88.197402
-
G. Vazquez, C. Camara, S. J. Putterman, and K. Weninger, Phys. Rev. Lett. 88, 197402 (2002). 10.1103/PhysRevLett.88.197402
-
(2002)
Phys. Rev. Lett.
, vol.88
, pp. 197402
-
-
Vazquez, G.1
Camara, C.2
Putterman, S.J.3
Weninger, K.4
-
19
-
-
0242663641
-
-
10.1103/PhysRevE.68.035303
-
M. T. Levinsen, N. Weppenaar, J. S. Dam, G. Simon, and M. Skogstad, Phys. Rev. E 68, 035303 (R) (2003). 10.1103/PhysRevE.68.035303
-
(2003)
Phys. Rev. e
, vol.68
, pp. 035303
-
-
Levinsen, M.T.1
Weppenaar, N.2
Dam, J.S.3
Simon, G.4
Skogstad, M.5
-
21
-
-
2542501962
-
-
10.1103/PhysRevLett.92.144301
-
J. S. Dam and M. T. Levinsen, Phys. Rev. Lett. 92, 144301 (2004). 10.1103/PhysRevLett.92.144301
-
(2004)
Phys. Rev. Lett.
, vol.92
, pp. 144301
-
-
Dam, J.S.1
Levinsen, M.T.2
-
22
-
-
57349197830
-
-
10.1103/PhysRevLett.101.234301
-
A. Bass, S. J. Ruuth, C. Camara, B. Merriman, and S. Putterman, Phys. Rev. Lett. 101, 234301 (2008). 10.1103/PhysRevLett.101.234301
-
(2008)
Phys. Rev. Lett.
, vol.101
, pp. 234301
-
-
Bass, A.1
Ruuth, S.J.2
Camara, C.3
Merriman, B.4
Putterman, S.5
-
23
-
-
78651301574
-
-
10.1209/0295-5075/80/27004
-
M. T. Levinsen and J. S. Dam, EPL 80, 27004 (2007). 10.1209/0295-5075/80/ 27004
-
(2007)
EPL
, vol.80
, pp. 27004
-
-
Levinsen, M.T.1
Dam, J.S.2
-
24
-
-
0040955040
-
-
10.1016/S0370-1573(96)00050-6
-
B. P. Barber, R. A. Hiller, R. Löfstedt, S. J. Putterman, and K. R. Weninger, Phys. Rep. 281, 65 (1997). 10.1016/S0370-1573(96)00050-6
-
(1997)
Phys. Rep.
, vol.281
, pp. 65
-
-
Barber, B.P.1
Hiller, R.A.2
Löfstedt, R.3
Putterman, S.J.4
Weninger, K.R.5
-
25
-
-
78651319023
-
-
In Ref. the authors note that the apparent temperatures found by fits to blackbody radiation scale roughly with the ionization potentials of the relevant noble gases. Interestingly, oxygen and nitrogen are found to follow approximately the same scaling if instead the dissociation potentials are used. Whether this observation has any deeper meaning or just represents a coincidence is not clear.
-
In Ref. the authors note that the apparent temperatures found by fits to blackbody radiation scale roughly with the ionization potentials of the relevant noble gases. Interestingly, oxygen and nitrogen are found to follow approximately the same scaling if instead the dissociation potentials are used. Whether this observation has any deeper meaning or just represents a coincidence is not clear.
-
-
-
-
31
-
-
0001609718
-
-
10.1103/PhysRevE.58.1899
-
L. Frommhold, Phys. Rev. E 58, 1899 (1998). 10.1103/PhysRevE.58.1899
-
(1998)
Phys. Rev. e
, vol.58
, pp. 1899
-
-
Frommhold, L.1
-
33
-
-
0006064075
-
-
10.1103/RevModPhys.5.257
-
R. B. Brode, Rev. Mod. Phys. 5, 257 (1933). 10.1103/RevModPhys.5.257
-
(1933)
Rev. Mod. Phys.
, vol.5
, pp. 257
-
-
Brode, R.B.1
-
35
-
-
42149165580
-
-
10.1103/PhysRevE.77.046304
-
J. Holzfuss and M. T. Levinsen, Phys. Rev. E 77, 046304 (2008). 10.1103/PhysRevE.77.046304
-
(2008)
Phys. Rev. e
, vol.77
, pp. 046304
-
-
Holzfuss, J.1
Levinsen, M.T.2
-
37
-
-
41349099641
-
-
10.1103/PhysRevE.66.066301
-
J. da Graça and H. Kojima, Phys. Rev. E 66, 066301 (2002). 10.1103/PhysRevE.66.066301
-
(2002)
Phys. Rev. e
, vol.66
, pp. 066301
-
-
Da Graça, J.1
Kojima, H.2
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