G. D. Gilmore, Spacecraft thermal control handbook 2nd edition (The Aerospace Corporation, 2002)
2002
Cited alongside, same era.
L. K. Scheffer, Phys. Rev. D 67
2003
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J. R. Brownstein and J. W. Moffat, Classical and Quantum Gravity 23
2006
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L. Iess, J. Armstrong, S. Asmar, M. Di Benedetto, A. Graziani, R. Mackenzie, P. Racioppa, N. Rappaport, and P. Tortora, in Proceedings of the XX International Symposium on Space Flight Dynamics (ISSFD), Annapolis, MD, USA (September 24-28, 2007)
2007
Cited alongside, same era.
S. Reynaud and M. Jaekel, Arxiv preprint arXiv:0801.3407, 1(2008), arXiv:0801.3407v1 , http://arxiv.org/abs/0801.3407
Original
2008
Cited alongside, same era.
V. T. TOTH, International Journal of Modern Physics D 18
2009
Cited alongside, same era.
B. Levy, A. Christophe, P. C. J. M. Metris, G. Bério, and S. Reynaud, Space Science Reviews 151
2009
Cited alongside, same era.
V. T. Toth and S. G. Turyshev, Phys. Rev. D 79
2009
Cited alongside, same era.
TRW Systems Group, Pioneer F/G Spacecraft Operational Characteristics PC-202.pdf , Tech. Rep
Cited in the paper.
Averaged over all directions and wavelengths of radiation
Cited in the paper.
M. F. Modest, Radiative Heat Transfer , 2nd ed. (Academic Press)
Cited in the paper.
A lambertian emitter is a surface for which the directional radiative flux (energy flow per unit angle per unit surface area), is proportional to the cosine of the polar angle [ 19 ] . In an analogous manner can be defined a lambertian reflector. Gray assumption further implies that reflectance ρ \rho equals 1 − ε 1-\varepsilon
Cited in the paper.