Abstract

The response of thin sputtered thermocouples to interrupted radiation of low frequency has been studied and corroboration with the theory obtained. The anomalous behavior of bismuth-tellurium couples has been observed. These couples when used in conjunction with a low frequency amplifier are more sensitive than wire thermocouples used with the most sensitive galvanometers, but without "multipliers."

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  1. L. Harris, Phys. Rev. 45, 635 (1934).
  2. L. Harris and E. A. Johnson, Rev. Sci. Inst. 4, 454 (1933).
  3. L. Harris and E. A. Johnson, Rev. Sci. Inst. 5, 153 (1934).
  4. L. Harris and A. C. Scholp, Rev. Sci. Inst. 11, 23 (1940).
  5. E. A. Johnson and C. Neitzert, Rev. Sci. Inst. 5, 196 (1934).
  6. E. A. Johnson and L. Harris, Phys. Rev. 44, 944 (1933).
  7. W. Haken, Ann. d. Physik 32, 291 (1910).
  8. C. H. Cartwright, Ann. d. Physik [5] 18, 656 (1933).
  9. C. H. Cartwright and M. Haberfeld-Schwartz, Proc. Roy. Soc. London A148, 648 (1935).
  10. For comparison of radiation recording instruments, see P. Moon and L. R. Steinhardt, J. Opt. Soc. Am. 28, 148 (1938).

Cartwright, C. H.

C. H. Cartwright, Ann. d. Physik [5] 18, 656 (1933).

C. H. Cartwright and M. Haberfeld-Schwartz, Proc. Roy. Soc. London A148, 648 (1935).

Haberfeld-Schwartz, M.

C. H. Cartwright and M. Haberfeld-Schwartz, Proc. Roy. Soc. London A148, 648 (1935).

Haken, W.

W. Haken, Ann. d. Physik 32, 291 (1910).

Harris, L.

E. A. Johnson and L. Harris, Phys. Rev. 44, 944 (1933).

L. Harris, Phys. Rev. 45, 635 (1934).

L. Harris and E. A. Johnson, Rev. Sci. Inst. 4, 454 (1933).

L. Harris and E. A. Johnson, Rev. Sci. Inst. 5, 153 (1934).

L. Harris and A. C. Scholp, Rev. Sci. Inst. 11, 23 (1940).

Johnson, E. A.

E. A. Johnson and C. Neitzert, Rev. Sci. Inst. 5, 196 (1934).

L. Harris and E. A. Johnson, Rev. Sci. Inst. 5, 153 (1934).

L. Harris and E. A. Johnson, Rev. Sci. Inst. 4, 454 (1933).

E. A. Johnson and L. Harris, Phys. Rev. 44, 944 (1933).

Moon, P.

For comparison of radiation recording instruments, see P. Moon and L. R. Steinhardt, J. Opt. Soc. Am. 28, 148 (1938).

Neitzert, C.

E. A. Johnson and C. Neitzert, Rev. Sci. Inst. 5, 196 (1934).

Scholp, A. C.

L. Harris and A. C. Scholp, Rev. Sci. Inst. 11, 23 (1940).

Steinhardt, L. R.

For comparison of radiation recording instruments, see P. Moon and L. R. Steinhardt, J. Opt. Soc. Am. 28, 148 (1938).

Other (10)

L. Harris, Phys. Rev. 45, 635 (1934).

L. Harris and E. A. Johnson, Rev. Sci. Inst. 4, 454 (1933).

L. Harris and E. A. Johnson, Rev. Sci. Inst. 5, 153 (1934).

L. Harris and A. C. Scholp, Rev. Sci. Inst. 11, 23 (1940).

E. A. Johnson and C. Neitzert, Rev. Sci. Inst. 5, 196 (1934).

E. A. Johnson and L. Harris, Phys. Rev. 44, 944 (1933).

W. Haken, Ann. d. Physik 32, 291 (1910).

C. H. Cartwright, Ann. d. Physik [5] 18, 656 (1933).

C. H. Cartwright and M. Haberfeld-Schwartz, Proc. Roy. Soc. London A148, 648 (1935).

For comparison of radiation recording instruments, see P. Moon and L. R. Steinhardt, J. Opt. Soc. Am. 28, 148 (1938).

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