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Chapter 4 4 44 Show that for overhead parallel beam radiation incident on an isothermal atmosphere in which the mixing ratio of the absorbing gas r and the volume absorption coeffi cient k are both independent of height the absorption per unit volume i e dI dz is strongest at the level of unit optical depth Solution From Eq 4 17 if r and k are both independent of height dI dz I T k r 1 where I is the intensity of the radiation incident on the top of the atmosphere T I I is the transmissivity of the overlying layer and is the density of the ambient air From 4 28 for an overhead beam T e 2 For an isothermal atmosphere p therefore from 3 26 0e z H 3 where H is the scale height Substituting 2 and 3 into 1 we obtain dI dz I k r 0e z He 4 From 4 32 k 0r Z z e z Hdz H k r 0 e z H 5 Using 5 to express e z Hin 4 in terms of optical depth we obtain dI dz I H e At the level where the absorption is strongest d dz dI dz I H d dz e 0 6 Performing the diff erentiation on the right hand side of 6 we obtain e d dz 1 0 14 from which it follows that 1 Although this result is strictly ap plicable only to an isothermal atmosphere in whichk and r are inde pendent of height it is qualitatively representative of conditions in plan etary atmospheres in which the mixing ratios of the principal absorbing constituents do not change rapidly with height It was originally devel oped by Sidney Chapman for understanding radiative and photochemical processes related to the stratospheric ozone layer see Section 5 7 4 48 Prove that the expression for the heating rate as approximated by cooling to space namely eqn 4 54 in text dT dt 2 cp Z 1 0 k rB z e d 1 can be integrated over solid angle to obtain eqn 4 56 in the text that is dT dt cp k rB z e 2 where is as defi ned in Eq 4 47 in the text Solution Equation 1 can be rewritten in the form dT dt cp k rB z 2 Z 1 0 e d 3 The integral in 3 can be rewritten 2 Z 1 0 e d 2 Z 1 0 de d d 2 Z 1 0 d e d d Exchanging the order of the diff erentiation and the intergration yields 2 Z 1 0 e d d d 2 Z 1 0 e d e Substituting for the integral in 3 yields 2 4 51 Show that Schwarszchild s equation 4 41 in the text which is dI I B T k rds 1 can be integrated along a path extending from 0 to s1in Fig 4 26 in the text to obtain I s1 I 0e s1 0 Z s1 0 k rB T s e s1 s ds which appears as Eq 4 42 in the text 15 Solution The diff erential form of the slant path optical depth is d s k s rds 2 where ds which is directed along the path of the radiation may be either upward or downward as depicted in Fig 4 26 The minus sign appears in this expression because ds and d sare in opposite directions Incorpo rating this relationship into eqn 4 36 in the text yields dI s I d s B T s d s 3 Multiplying 3 by the factor e s where sis the optical thickness along the path length from s to s1 we have e sdI s I e sd s B T s e sd s Moving the fi rst term on the right hand side to the left hand side and combining it with the other term yields d I s e s B T s e sd s Integrating along the path from s 0 to s s1we have I s e s s 0 Z

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