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1

Tripathi, Ratikanta. Universal parameterization of absorption cross sections. National Aeronautics and Space Administration, Langley Research Center, 1997.

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2

Tripathi, Ram K. Universal parameterization of absorption cross sections. National Aeronautics and Space Administration, Langley Research Center, 1997.

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3

Townsend, Lawrence W. Tables of nuclear cross sections for galactic cosmic rays: Absorption cross sections. National Aeronautics and Space Administration, Scientific and Technica[l] Information Branch, 1985.

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4

Tripathi, Ram K. New parameterization of neutron absorption cross sections. National Aeronautics and Space Administration, Langley Research Center, 1997.

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5

Tripathi, Ram K. New parameterization of neutron absorption cross sections. National Aeronautics and Space Administration, 1997.

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6

Tripathi, Ram K. Universal parameterization of absorption cross sections: Light systems. National Aeronautics and Space Administration, Langley Research Center, 1999.

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7

Tripathi, Ratikanta. Universal parameterization of absorption cross sections: Light systems. National Aeronautics and Space Administration, Langley Research Center, 1999.

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8

Wilson, John W. Nucleon-nucleus interaction data base: Total nuclear and absorption cross sections. Langley Research Center, 1988.

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9

Chen, K. S. (Kun-Shan), 1959-, ed. Microwave scattering and emission models for users. Artech House, 2010.

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10

Microwave scattering and emission models and their applications. Artech House, 1994.

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11

Norbury, John W. Photonuclear absorption cross sections: Final report (October 1, 1987 - August 15, 1989). National Aeronautics and Space Administration, 1989.

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12

Nicolet, M. Rotational structure and absorption cross sections from 300K to 190K of the Schumann-Runge bands. Institut d'Ae ronomie Spatiale de Belgique, 1987.

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13

Collision processes and excitation of UV emission from planetary atmospheric gases: A handbook of cross sections. Gordon and Breach Science Publishers, 1998.

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14

Maung, Khin Maung. Radiation transport and shielding for space exploration and high speed flight transportation: Final report on NAG1-1789. National Aeronautics and Space Administration, 1997.

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15

Chance, Kelly, and Randall V. Martin. Radiative Transfer. Oxford University Press, 2017. http://dx.doi.org/10.1093/oso/9780199662104.003.0004.

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Radiative transfer is the process of energy transfer during the propagation of electromagnetic radiation through a medium. The processes of extinction, due to absorption and scattering, and thermal emission are described. It is shown how they can be represented by wavelength-dependent optical thickness, due to absorption or emission cross sections and the number of absorbers, emitters, or scatterers. Cloud optical thickness and conservative scattering are described. The scattering phase function is introduced. Next, the general form of radiative transfer is given, and its applicability to the
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16

Berkowitz, Joseph. Atomic and Molecular Photoabsorption: Partial Cross Sections. Elsevier Science & Technology Books, 2015.

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17

W, Townsend Lawrence, Wilson J. W, and United States. National Aeronautics and Space Administration. Scientific and Technical Information Program., eds. Target correlation effects on neutron-nucleus total, absorption, and abrasion cross sections. National Aeronautics and Space Administration, Office of Management, Scientific and Technical Information Program, 1991.

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18

A, Cucinotta Francis, Wilson John W. 1940-, and Langley Research Center, eds. A simple method for nucleon-nucleon cross sections in a nucleus. National Aeronautics and Space Administration, Langley Research Center, 1999.

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19

Ping, Wang, and United States. National Aeronautics and Space Administration., eds. An x-ray analysis database of photoionization cross sections including variable ionization. National Aeronautics and Space Administration, 1997.

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20

String fragmentation model in space radiation problems. National Aeronautics and Space Administration, Langley Research Center, 2002.

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21

Avakyan, SV, R. N. II'in, G. N. Ogurtsov, and V. M. Lavrov. Collision Processes and Excitation of UV Emission from Planetary Atmospheric Gases: A Handbook of Cross Sections. CRC, 1999.

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22

International Commission on Radiation Units and Measurements., ed. Secondary electron spectra from charged particle interactions. International Commission on Radiation Units and Measurements, 1996.

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23

Shielding materials for highly penetrating space radiations: Final technical report, NASA cooperative agreement NCC-1-151. National Aeronautics and Space Administration, 1995.

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24

A, Orwoll Robert, and United States. National Aeronautics and Space Administration., eds. Shielding materials for highly penetrating space radiations: Final technical report, NASA cooperative agreement NCC-1-151. National Aeronautics and Space Administration, 1995.

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25

Kachelriess, Michael. Scattering processes. Oxford University Press, 2018. http://dx.doi.org/10.1093/oso/9780198802877.003.0009.

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The unitarity of the S-matrix is used to derive the optical theorem. The connection between Green functions and scattering amplitudes given by the LSZ reduction formula is derived. The trace and the helicity method are developed and applied to the calculation of QED processes. The emission of soft photons and gravitons is discussed. In an appendix, the connection between S-matrix elements, Feynman amplitudes and decay rates or cross-sections is derived.
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26

Chance, Kelly, and Randall V. Martin. Spectroscopy Fundamentals. Oxford University Press, 2017. http://dx.doi.org/10.1093/oso/9780199662104.003.0005.

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This chapter provides a broad overview of the spectroscopic principles required in order to perform quantitative spectroscopy of atmospheres. It couples the details of atmospheric spectroscopy with the radiative transfer processes and also with the assessment of rotational, vibrational, and electronic spectroscopic measurements of atmospheres. The principles apply from line-resolved measurements (chiefly microwave through infrared) through ultraviolet and visible measurements employing absorption cross sections developed from individual transitions. The chapter introduces Einstein coefficients
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27

Launay, Jean-Pierre, and Michel Verdaguer. The excited electron: photophysical properties. Oxford University Press, 2018. http://dx.doi.org/10.1093/oso/9780198814597.003.0004.

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After a review of fundamental notions such as absorption, emission and the properties of excited states, the chapter introduces excited-state electron transfer. Several examples are given, using molecules to realize photodiodes, light emitting diodes, photovoltaic cells, and even harnessing photochemical energy for water photolysis. The specificities of ultrafast electron transfer are outlined. Energy transfer is then defined, starting from its theoretical description, and showing its involvement in photonic wires or molecular assemblies realizing an antenna effect for light harvesting. Photom
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