Realization of ITS-90 Radiance Temperature Scale from 961.78 °C to 3000 °C at CSIR-NPL

MAPAN ◽  
2021 ◽  
Author(s):  
Umesh Pant ◽  
Gaurav Gupta ◽  
Hansraj Meena ◽  
Ashish Bhatt ◽  
Komal Bapna ◽  
...  
Keyword(s):  
Temperature Scale ◽  
Radiance Temperature ◽  
Radiance Temperature Scale

Design and characterization of Si and InGaAs pyrometers for radiance temperature scale realization between 232 °C and 962 °C

2006 ◽  
Author(s):  
M. Noorma ◽  
S. Mekhontsev ◽  
V. Khromchenko ◽  
A. Gura ◽  
M. Litorja ◽  
...  
Keyword(s):  
Temperature Scale ◽  
Radiance Temperature ◽  
Radiance Temperature Scale

Pilot Comparison of Radiance Temperature Scale Realization Between NIMT and NMIJ

2014 ◽  
Vol 36 (2-3) ◽  
pp. 315-326 ◽  
Author(s):  
T. Keawprasert ◽  
Y. Yamada ◽  
J. Ishii
Keyword(s):  
Temperature Scale ◽  
Radiance Temperature ◽  
Radiance Temperature Scale

scholarly journals A Superfluid Perspective on Neutron Star Dynamics

Universe ◽  
2021 ◽  
Vol 7 (1) ◽  
pp. 17
Author(s):  
Nils Andersson
Keyword(s):  
Neutron Star ◽  
Degrees Of Freedom ◽  
Temperature Scale ◽  
Fluid System ◽  
Fluid Core ◽  
State Of Matter ◽  
Entrainment Effect ◽  
Neutron Component ◽  
The Impact

As mature neutron stars are cold (on the relevant temperature scale), one has to carefully consider the state of matter in their interior. The outer kilometre or so is expected to freeze to form an elastic crust of increasingly neutron-rich nuclei, coexisting with a superfluid neutron component, while the star’s fluid core contains a mixed superfluid/superconductor. The dynamics of the star depend heavily on the parameters associated with the different phases. The presence of superfluidity brings new degrees of freedom—in essence we are dealing with a complex multi-fluid system—and additional features: bulk rotation is supported by a dense array of quantised vortices, which introduce dissipation via mutual friction, and the motion of the superfluid is affected by the so-called entrainment effect. This brief survey provides an introduction to—along with a commentary on our current understanding of—these dynamical aspects, paying particular attention to the role of entrainment, and outlines the impact of superfluidity on neutron-star seismology.

The Temperature Scale, a Proposed Change in Definition

1940 ◽  
Vol 11 (6) ◽  
pp. 371-372
Author(s):  
F. G. Brickwedde
Keyword(s):  
Temperature Scale
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