ntrs.nasa.gov · infrared-active species (h20, c02, 03, n20, co, ch 4 , 02), even,though some of...

76
NASA-TM-8328919820014948 NASA Technical Memorandum 83289 ,tJI¥£ . £a >J2:& * -# '. " .•-,"! ,..I COMPILATION OF ATMOSPHERIC GAS CONCENTRATION PROFILES FROM 0 TO 50 KM M. A. H. Smith MARCH 1982 I " ", " jA" \ I . Llt-: i ) . '..' ." .. 'r, H,\",::ll'N, VIRGINIA NAS/\ National Aeronautics and Space Administration Langley Research Center Hampton, Virginia 23665 https://ntrs.nasa.gov/search.jsp?R=19820014948 2020-01-11T10:30:46+00:00Z

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Page 1: ntrs.nasa.gov · infrared-active species (H20, C02, 03, N20, CO, CH 4 , 02), even,though some of these profiles may not be of great interest for photochemical studies. The fundamental

NASA-TM-8328919820014948

NASA Technical Memorandum 83289

,tJI¥£ . £a >J2:&* -#

77t1-"~z,,

'.

" .•-,"! -;'~;J

,..I

COMPILATION OF ATMOSPHERIC GAS CONCENTRATION

PROFILES FROM 0 TO 50 KM

M. A. H. Smith

MARCH 1982

I

"", " jA",~~ • \ I . Llt-: i

). '..' .".. 'r,

~j,!'~'?l)~\, r\::<-~r'!\R,~~·i ~; i'Jn-]~

Lif-:':':'~,~;'i', :\!).,r~,A

H,\",::ll'N, VIRGINIA

NAS/\National Aeronautics andSpace Administration

Langley Research CenterHampton, Virginia 23665

https://ntrs.nasa.gov/search.jsp?R=19820014948 2020-01-11T10:30:46+00:00Z

Page 2: ntrs.nasa.gov · infrared-active species (H20, C02, 03, N20, CO, CH 4 , 02), even,though some of these profiles may not be of great interest for photochemical studies. The fundamental
Page 3: ntrs.nasa.gov · infrared-active species (H20, C02, 03, N20, CO, CH 4 , 02), even,though some of these profiles may not be of great interest for photochemical studies. The fundamental

INTRODUCTION

The compilation of atmospheric gas concentration profiles described in

this report was created at NASA Langley Research Center as a convenient

on-line reference data set for line-by-line simulations of atmospheric

infrared absorption and emission signals. Profiles from this compilation

are also useful as "initial guesses" in iterative procedures for retrieval

of gas concentrations from measured atmospheric infrared data. Since a

number of researchers in the field of atmospheric remote sensing have

informally requested copies of this compilation, the author has decided to

release these data in the form of a Technical Memorandum.

In this report, a brief description of the data will be followed by a

listing of the data set as it appears on the NASA Langley computer system,

and a list of references. The final section of this report contains plots

.. of each of the 52 gas concentration profiles included in the ·compilation.

The author ackriowledges the assistance of Ms. Pamela L. Rarig, of the

Systems and Applied Sciences Corporation, who developed the plotting

program used to produce the figures in this report.

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2

DESCRIPTION OF THE DATA

The first 28 gases on the compilation are those for which spectro­

scopic data are given on the AFGL (Rothman, 1981; Rothman et al., 1981) and

GEISA (Chedin et al., 1980, 1981) atmospheric absorption line parameter

compilations. Concentration profiles for these gases are listed in order

according to their AFGL integer gas codes. Since this gas profile

compilation has been developed primarily as a data base for simulation of

atmospheric absorption or emission, profiles are included for all the major

infrared-active species (H20, C02, 03, N20, CO, CH 4 , 02), even,though some

of these profiles may not be of great interest for photochemical studies.

The fundamental collision-induced bands of both N2 and 02 appear quite

strong in tropospheric and lower-stratospheric spectra (Rinsland et al.,

1981, 1982), and the atmospheric N2 profile has also been included in this

compilation. PH3 is not known to exist'in the unpolluted terrestrial

atmosphere, but its line parameters are included in the GEISA tape and are

used in analysis of atmospheric spectra of the outer planets. In this

compilation, the terrestrial PH3 volume mixing ratio has been set to a

negligible value (1.0 X10-20 ).

The last 24 gases in this compilation are species which have either

been measured in the stratosphere or are considered to be important

sources, sinks or intermediate reservoirs for photochemically active

species in the stratosphere (Hudson and Reed, 1979; Hudson et al., 1981).

All of these gases have molecular spectra in the infrared, but detailed

listings of their absorption line parameters are not yet available.

However, the concentration profiles listed here may be used in conjunction

with laboratory spectra such as those compiled by Murcray and Goldman

Page 5: ntrs.nasa.gov · infrared-active species (H20, C02, 03, N20, CO, CH 4 , 02), even,though some of these profiles may not be of great interest for photochemical studies. The fundamental

3

(1981) to estimate the m.agnitude of atmospheric absorption by these species

at various altitudes. These concentration profiles are loosely grouped

according to category, ie., hydrocarbons, halocarbons, odd-hydrogen

species, odd-nitrogen species, and sulfur-containing molecules.

The data file is written in the form of 80-character card images~ For

each species there is a header card containing the gas name left-justified

in the first 15 columns, and columns 16 through 80 contain a description of

the major references for the gas concentration profile. This header card

is followed by one to six cards containing the atmospheric volume mixing

ratios at 2-km intervals, beginning at 50 km and ending at the ground

(0 km).

The gas concentration profiles in this data set have been based on

both atmospheric measurements and the results of photochemical models,

compiled from an extensive literature search by the author. The majority

of references for these profiles are included in the Hudson et al. (1981)

report, and a few more recent results are added here. Although for a

number of species many measurements and model studies have been reported in

the literature, the references on the header cards are limited to the more

recent results and to review articles. Unless otherwise stated on the

header card, the set of volume mixing ratios for each species represents

the "typical" diurnally averaged, seasonally averaged Northern Hemisphere

midlatitude gas concentration profile. When both model results and

atmospheri c measurements were avail abl e, the measurements have been

weighted more heavily in the determination of the average concentration

profil e. In some cases where neither measurements nor model results were

available over the entire 0-50 km altitude range (e.g. NH3, HI, HCN, C2H4,

Page 6: ntrs.nasa.gov · infrared-active species (H20, C02, 03, N20, CO, CH 4 , 02), even,though some of these profiles may not be of great interest for photochemical studies. The fundamental

4

CHCt2F, HN02, H02N02 and H2S), the author has extrapolated the

concentration' profiles based on available information such as spectroscopic

upper limits, expected ground-level concentrations or estimated

tropospheric lifetimes.

The average gas concentration profil es presented here, whil e useful

for "ball-park" estimates of atmospheric absorption or emission or for

initialization of retrieval algorithms, may be quite different from

concentration profiles actually measured at specific times and locations on

the Earth, particularly in the case of diurnally varying species. The

reader interested in simulation of atmospheric absorption or emission for a

specific case, for example, a sunset spectrum taken in mid-winter at high

latitude, should consult the individual references given here and in the

Hudson et al. (1981) report to obtain more detailed gas cqncentration

profiles.

Page 7: ntrs.nasa.gov · infrared-active species (H20, C02, 03, N20, CO, CH 4 , 02), even,though some of these profiles may not be of great interest for photochemical studies. The fundamental

--------- ---------- ------

EllSAESSER ET4.8£-06,4.4E~06,

-- 3-~-9E;';'C6,

3 ~'4E-06,

6. 5E-04,-

-1916 O".-·s. STAN DA-'rfo-"'A'f-M~--_. __.~----- ------

H20---S-.O E- 06,---4;-5E;;:;06,

-- --- 4:1 i:--o6;-_._---. -3;-5 E;'06, -

- -2-~ OE--<JSj-1 ~oE"'62

-C02-----2-6* 3-~f4E ';"0403----- --- 1976 u.s. STANDARD A-OC- - ------ --------------------

----·--3.1E;;':06·j- '-- ---3. -8E~(f6, ~ '~-4--;7 E-06, 5.8 E-Ob, 6.4 E-06,-----·----·--7-~·3-E-:.b6, -7~8E~o6, 8.1-E~-06,--· 7.7E-06, 7.2E-06, -----------------------b~6E:...o6, 6.ZE-ob, 5~7E-:':'-06, 4.7E-06, 3.6E-06,----.-- Z-;-6E--06-,- T.6E:",ob,"-e. 5E-07l- 5. OE-07, 3.1 E-07,-------r;TE~o1i------6~ OE~O8-,--- it -;1 E-08l---3~-4 E-08, 2* 3.3 E-0aNZ1J-- --- ---- - -Go[5.~fN--E r AU 19-ffO;-8IT~-FA-lrrAN ET AU 1981 A" COFFEY ET At ( 1 9a1 A)

1. OE-,:-09-;----- Z;OE-:..:O-9;---- 4.0 E-Oq, 7. OE-09, 1.0 E-08,---------1~6E.:-08, 2~2E=6a, -----3--;-2t'-Oa,...------ S.OE-oa, 7.0E-08,

-- ~·-·--,·----·--9--~'·OE·:.(ftr;--- ··-1··.· i-E-~C'7 ~ _·--f-;~3 E-:;07, 1.6 E-O 7, 2.0 E-07, --------.--------.-- -----2. 4E ...-07;---2--~-fE---tF7,-----2~--9E-O-7; 3. OE-07, 3.1 E-Or;----------------

- --6*3-;ZE-;;:cf1 ----------- - --------..----- ---- ---------- c--O-------- ----F-ABI AN E1 AL • -( l'9-aYA'T;--EHI-j"ALrANOTONNl'SSE N--:(:-=1:-=q:-=8C--=0"7)-------------------- 5*3·;OE-O-8-~----·---.. ----- ..~ ------ _..---,,-~------------3-~-O-E ~(ja,- - -3.0 E-O 8, --2-;7 e":offi - 2 • 4 E-O 8, 2.2 E-O 8,

-----Z--;-OE..: 08 -, 1.9e..:o 8, i .8E:;:-08,--------- 1. 7 E-08, 1 • bE-08,1.5E-oa, 2. OE-O 8, 3.or;,;.ol:f,------- 5.0 £-0 8, 8.0 E-O 8;--------------- -----1 • (fE -0 7 , 1. Z"E -01, '1 ~·3-·E-~-07~;_------T_:_3H-7-;-·_· 1.4 E-0 7, ---~-- .,----- -1.5E-07 ------------- ---..---

'CH4-" FABIAt,f ET AL. ffi:faLfj--;- -EHHAl T AND TONNCSSEN-(T980) -.-----.....--.--.-..---i--'-OE-07, 1. 5E-07, 2-.-0E-.:..07-~-------~-5E-=-07;"-------3.·-2E-07;-------------- ---

---------'t~-OE-07, 4.8E-07,5~-;fE::07;------ 6.6E-07, .-~-R7-;--- ....----------- - ---_. ----------·8-~0E:.-07. .-.- 8 ~ 6 E-~(f7, 9 .·3-E=6·7·~---·--- ----1. OE-06, ----1-~1E-06, ..-.--. -.----.-.- -.--.----------·---1-·~·3E~O-b~--·· -i-~-'4E:"06, ·"-1.5E--cfb··;- 1.5E"06, 1.bE-06, .- .._-_._--

-- -----1.6E.:..06, -f~6-E-Obi-;-iE':"06, 1. 7E-06,-----2'*-1.7E-06--------02 --_._-.- .-,--.-.----.-- '-"'-"-I'976--Li ."~ •. ~ 1" Jf~rbA-R-D··-ATr-1.-·- - -_.....~-_._----, ._.._-----

-···'·-·26*2 .-O·9·E~'()1 --.--.-,-.---..,-,.-.~--------.-.. ----. -.-.. -----...

Page 8: ntrs.nasa.gov · infrared-active species (H20, C02, 03, N20, CO, CH 4 , 02), even,though some of these profiles may not be of great interest for photochemical studies. The fundamental

1.OE-1l,2.0E-IO,3.0E--U9,1.1E-Oq-;B.OE-li,

YLIN (; ETA L. (1980) , - TURt-oEt If[-;Tf98rBr~-ANOEffs-o~rfI97I-:'T976 r----7.0E-"lO, 6.0E-IO,·- ·~--5--;Ot·:':·lO~-------------4.0E-IO, ------------2.2 E-10, 1. 3"E-l 0, -"-- ~-8·E-~1·I,---- 2. 8E-ll, -_ - --_ _, __ ..6.1 E-12 ,----2. cH:":iz, ---------r:OE-12, 5. 2 E-13,-------------~-----1 • 3 E-13, 8.1 E-14; ------ -5~3I':- 14 ;--------4-~-9E-::r4;---

5*4. 4E.:-14-----------------------------------CRUTzE NET AL.( 1978 ), SzEC197aj-Mo-DE LS---+--AL L-MEAS-~---tHRU-- l"9sT

It. 4E-Io, 4 ~ 3 E-l 0 ~ ·4-.2l~-~·I·(f,~----· -----4 ;·1-e-::10;······" ---..... _.- .._..----_._-_.__.3 • 8 E-1 0 , 3 • 6 E-1 0, --3~. -4E~"l'b, .-'3";-Z'E-;.:fer, _._-_. -_ ....-.---.- -.- -z·'."S-E-IC·, 2~~-O·E::-i·(f~·_· 1.5E-10, 1.OE-IO, ._-~._-~-_.----

2. 5E-ll, i-~O-E-ll, ---·~--·4·~-·-5·E·:.-12~---2.0E.:.-i2,--- -.-------..--- ..2.3E-13, 9. OE-f4, ·-3--;OE":i4~---2-*1.oT.;;.T4--------------------

OH8.0E-IO,3.IE-IO,

--1;-OE--ll, -1.91:-13,

- 4.11::-14,

4.5E-IO,4.0E-lO,

------ ----3-~-(,.E- Io,6.0£:-11,

--6~br-i3,

HN035.0E-12,

- _....~-- -- -I.OE-IO,2.0E-09,2.0E-C9,9.0E-llJ3-.0E-ll

3.5E-ll,-l:3"E-=1I;-i~3E-ii,

- .-3 .1E- iI,6.0E-ll,------------:r:oE-lo

-NO-------- -----C(WFEy-Ef--Ar-~(1981A)AND OTHERSI.OE-oa, -1.OE":08,-- --r~OE~(fa;--------I~OE-08, I.IE-oa,1.2E-oa, I.OE-06, 9.0E-09, 7.0E:..09,·-------4~-6E-09;--_~-:~~:_-__- _2.5E-09, 1.5E-'='09, - S.OE.:;lO,---- 4.0E-IO, 3.0E-IO,

----,-2-.-5E-fo~-------2~jE:..fc;-----_~..!.?_~=l0, 3. Of-IO, 3. OE-IO,---6*Y~ OE-I0S02 -- -

------------------------- - --- ------

Page 9: ntrs.nasa.gov · infrared-active species (H20, C02, 03, N20, CO, CH 4 , 02), even,though some of these profiles may not be of great interest for photochemical studies. The fundamental

He L1.3E-09,1.5'E-09,1.OE-09,5. cyr:'·To;2.4e-1111.0E--YO

CR'.lTZEN ET AL.(1978), i1ILLER-·Ef-A'L".<l980) + ALL MEAS. THRL!..981 ..1 • 3 E- 09, 1 • 3E:"'09, --1:'31=09, --- 1 .4 E-0 9,1. 7 E-09, 1 • 8 E-0 9, 1 ~ 6['::'09 , ·-----T~::-69,- .-- -----,-. --.- - -,-7.0E-10, 6.5 E-10, - ~6~_·o-E-':1-O;--'---- - 5. 5 E-IO, .- -------_.-...._-----_ ..-

._. -··4-.0E~·io, ·--·--2-.5E~-i·o~--' 1.0E-ll, ·---3:0E-ll, -------.--.-2.2E-II, 2. 6E"'lt; - -j~3E"'Tr,--' 6.5E-Il,

---------._,------..

---- ._--------~-

7.4E-IZ,3.9E-12,1.7E"';;12,

BOUGHt-iER AND. ·-4.4E-l1,

3.2E-IO,. 2.1 E-lO,i.6E-ll,4.5E-12,

.-.----- -.-.- 3'·'~ -2-·e--ll ,--2: 8E-lO,

" ---2;-6e"'i 0 ,3~-OE"'11 ,4 .IE-12,

-~1~ 7e--i 2 .-

H2CO.. ·_----4.-0E-11 ,-r~TE-I0,

'-9~oE-lf,

3 ~'3E-Il,.-- 3~-4E"'ll,

2.4-E-OQ-·"HO(C .. -

7. 4E~12,5.1E"';12,

.. '~-1'~' 8 E~':':12, .'-"11*r~'rE"';1"2

·~Hl--··-------- .__...~--- .. 'ClCER'O-NE"( i-98l) ------. -...--_.-._,-26*j.OE";12CLO .---,- -., PAQ ~ I Si.fE-t At.( 1981)-,- AN iYE-R-sm" (1980) , wATERS ET AL. (1981)-==

.-,--,-.- T;OE::l0, --1: 3E-IO, - t. 7 E-IO, 3.0 E-I0, 6.0 E-IO,7.2 E-lO,'----·r;OE-10,--- 6 ~ aE-IO, 5.0 E-I0, 4 .OE -10,

-'----2-:OE-.;.lo~---'---1 -;oE-::I();-- ----5;Or~11, 2. OE-11, 1.0E-ll,~'--'.- '---6-. 'OE":':-lZ', - 2. -S"E-"lZ ;--_._- . ---i"-~-'3-E~~'1-2-;----'-' 7. OE --13, 4.0 E--13, --~--------

.2-.-·(fE·-~ 13 , -----'-1 • 5E -:-13, -1: ~ 2" e-::-i-3' I - --3*-'i-~ 0 E--13 --.-------------------

ats- .,.- lURC OETAl·.( 19'8 fin, 'TNNET AL. (1979,1981) AND OTHERS-----y. 0 E'';';'14, f.-o E-14 ,._2_~_~.E_=I4;---.~ ~. 0 E-14, 2 .0 E-'13,

-' -------5 ~·(fE~ i 3, 1. 0 E-12 , 2 • 5 E-12, 6 • 0 E-12, 1 • 7 E-11,_..._- --3~-OE-ll, i .0 E~':'-i"i, -i-~'TI-=-fo~;-·---- -----·--1-. 4 E"l0, 1.9E-l 0, --~-----.---------¥---._----

'--·-Z.-4-E·';;:To, 3'.lE':10; 3.9E-Io;--'~"7E-IO,---SM-IO, -----------... -.. -.. .. _~5 '-ZE -10, 5.3 E-1 0, .. ~. 5 ~ ...~Q-;~_~=--~.!- 6 E-!~ ~_.• !tE-10~-.~~=_==~~=~~-

b.OE-I0

Page 10: ntrs.nasa.gov · infrared-active species (H20, C02, 03, N20, CO, CH 4 , 02), even,though some of these profiles may not be of great interest for photochemical studies. The fundamental

l.5E-10, 1.OE-lO, 3.0E-ll, 1.OE-ll, 3.0E-l2,..__.---r;OE- i 2----·-------------

··CH3Cl---- -' - . RA·SMUS·SE}·r ET-A[.TI9~fo f;-L ElF ER ET ·-Al.-( 1981)----r;-ot-;,;:-F.,- .... 3~Ot-14,----T. OE~T3, 2.0E-13, 5.0E-13,---····1·~-OE-12, -2. OE':"12, ... -5-~oT:.:r2l---- 1.0E-ll, Z. OE-11,--'-'--'5'~'OE~11,"-r;OE';';To, -'Z~-oE-':"lo, 2.6 E-IO, 3.2 E-10,-·--·-----"""'3:7"E:..-io-,··· 4 .-2 E-':::YO ,---" 4 • 8 E-1 0 , 5 • 3E-10, 5 • 7 E-10,----·--S-;-qE-iO,- 6;OE-ioj 6~OE-fo,--- b.OE-IO, 6.4E-IO,---' ·-------7;(fE-~-1-(f-· - ---------_._--.-.- ...-----

C2H6-5*1.·6E-13,

1.OE-13,-'2.CJE-12,6.0E-ll,

-T.7E-OQ'"-2..0E-09

1.OE-13,5-;OE-12,'I.OE-le,1.-SE"':09,

-PH3- .----.------.. NO REFS

-26*1.01:-20

00

Page 11: ntrs.nasa.gov · infrared-active species (H20, C02, 03, N20, CO, CH 4 , 02), even,though some of these profiles may not be of great interest for photochemical studies. The fundamental

_.... - -

RUDOLPH El AL.(1~81)t3~f8- ,IO·:1.0E-14,

I.OE-14, 3.0E-14,4-.0E-iz, 1.IE-II".--- -----r. BE -10, ----,Z=-"'. 0 'E-::-i 0,

-"4. 0E'-l 0 --t 2H4 _~-A~ MUS S~ N-E l' ~L ~ (' rQ8~~)~ {;R 9-Ij'N~~~I\[tL:,r~~~ .:=bNTY-~~-'-''-- ,,--- ...-,

"to*Y;b-e'-i4, ," ,- ----f~r":i4;

f-.OE':"12,~~-, ."1." 1.• 6E~1(>";-

-2'~OE-I0-' ­'t F"cL3 ,-- -,,- G-Ot'OAN--nET Af. Ci. 9-80)",- FAiHAN ET AL. (1981 A',S')----~-~ -~~------~- .. ,'

, - ''''5'' l-~ O'E ";14, ,- - - -- , .. ,,-"--.-- - ---~ .. -- -~-~------~ --- -- --- -- ----- - ----- , 1 ~ 0 E-:.. r4, 1. 0 E:':'14 , 1-;-!5t-'1t;-,- -"- -- - T~-O-E-':14~,~--------=r;i:fE~14 , ..-~--- --- -....,---- -- --2 '-o-f:':13, - t ~ 0E":'1 :3, ----- - 'i~ {J-e~I 2~-- .. -- -- '6-. 0E-12, ---1: fE~11, _.--_ .._-_=~~ ~

------4-. OE-:-fi', _.. -"_·"5"~-6E-fr,---"--·--- 7. 8E-.1~~__ ,__~l.!..!..~-lO, J !_~_t::_!O_-!._., __ , __ ._ .. -,6*1;-5-E":'lO

CF'itT2--- .. - --~ ,,-- ~

1.0E-13,------ 'i-.-ie -1 z,__________.0.' "2. BE-Il,-------1 ;3 E-:';1 0,- -----2-~ 8E":'lO,tF3cr --- -, 1'.3E-12,

1.'8E~12,

-Z.2E-12,.3 ~3E";1t,

6*5-.0e-12'tHe CF-~ -

5*1.0E-15,- - -1-.0[-15, -- r.Oe-15" 3~OE-15, - -- - 'i'~-(ff-:"14;'---'--3;-OE~4~-------- - .~. ,---

1.0e-13"- 3-. OE-13, 1 ~oE~12,- -----3-.OE'.:-y2:t .-~,~ i--:-t)'e':fi," -------- .---- --3-;-o-r';"Tl, - 4.5 t -1'1'- "' -5-;-O-E~1r;----~· _·--~wE-11, 5. It E-II, "-- -"~-'-- ._- _.--

--6*5-~5t-11--- ---- ---- ----,,-"".-,- .. -.,,---- ,-.. .--,,------,,-,"--,CHC(-ZF -- ··-PENKETT ET Al. (].'980) ·GROU~f)-:"LE·'VEi---·MEAS·'~'·ONL y -._~~-------_._.__._-, - "- ~ --- -- ---- , 1OtT. 0 E-16; - -- --,.-- - ----.. ,,-------,,-----,--- ---.----- --- , ..- -~- - ... , -- .

-- - ----- 3. 0r~1 b, 1. OE -15, 3 • oE -1'i" --,., -" i ~-OE': 1'4 ,- .. -----~ z-;0 E";14-;--- ---- -- -. -,- --- ,- --5~ OE~14, i ;O-E-13, 2. CfE:-13,--- 4-;O'E~-13;- _··---··1-;-QE~·i3-,--- --- _.. ,~-,-, -~., ._-~,

--~--_r_~~~:i,~' -(.IE-li ~ .... --- l._?f-~};-'--· 1. 3 ~:'"_l2..!_ " ~__ ,~.,4 ~-=!,2!_ -' ,-__ , _

Page 12: ntrs.nasa.gov · infrared-active species (H20, C02, 03, N20, CO, CH 4 , 02), even,though some of these profiles may not be of great interest for photochemical studies. The fundamental

.. -_.__._-------_._. -~-- .....o

--_._-----

-----------

6.2E-II,6.4E-ll,6.9E-11,

..- _.... "_._-.__._~---------------_. __.._-

'6;TE-TI;--- 6. lE-11,6~-3E=11;- 6. 4E-11,6 ~ 7 E- rr,----~ 6. 8 E-11 ,

----'-_._-~~--.;.....------

6-.Te"'11,6.31:-11i6.6E-Ir,

--r;-oE';';;14,--5·~ aE"'}3,

CRUTZEN- ET -AL.(i9f8,-,--~TU.IAMS ET Al.(1916), LEIFER1~OE-t4, l'.0·e-1.4,·---- 2.0E-14, 5.0E-14,

. 2. Oe-13, . . 5 .or~i j-;--·-·-T-~-OE-12, 2.3 E-l Z,8.oE"'12, T ~'2-E":Il, --2.0 E-l b 4.0 e"'111

... --- 9';0e-':i li"- ,- -"-~Te-';'Y6, 1 • 3 E-10, 1 .4 E-10,.- ... _. .._-

. FABIAN E1" AL.<l981Sf, pff·fKETl·-'El AL.(1981}, GOLDMAN ET AC~'(1919}

CCl4

._--.. ---- "'-- -. __._-_._-------------------

------1~-bE~i4,­'..--T~-oE-13-,----4~-5E...T2,

.---.-a;oE"'TI,·-.-- 6*r~4-E"'10 .-tF'4---- .-- - .,------- '6 ~-OE~·ll,

-----·-6-~2t·~ 11,- ----6~ ,f';;;ll, --,.. - -'-IT*1·;-oI~11--CF3TfR .------'-'1'0*1. oE~f6,

.. ---- ----·3~Ot ...'r5,·... -----. --it-;-oE"'13,

6*9.0E-13CH3C CL3 '-'--- CriFERE-f-A1~'TfgeTT; CRUT ZENET AL. ( 191 e). ---s*r~oE:':1-4, . ----.------.- ---------------- -'-----'=-:--'-'-~-'--=-~~---------

~-._---~----.._.._--_.. - .. _.-- -----_._-~_ .._..- " •.. _--_._ .._-.-- - ...-----_ ... _-_.-,._--_.._-------4.0E-14, 1.0E-13, 2.5E-13, 6.0E-13, 1.OE-12,

·------2~3E:':1'2 ~ ---~_4~ 6I::'J2;-_:--:-:~=?:;:9 (:l2;~_=~-1. 2E-11, --2~.O='-E~--1:::-1:::-,~-------'--.·--·----·--3·-~3E---l--l,· 6. OE-ll, 1. OE-10, -:-1-'.-2-:E----:l:-0-:c,---I~.-'--3';:O'E----"-1-=0,;.,--- --.------ ,._-'·---f.-*f~-4E=fo .- --.- - - .--..-.--.-, ---,-------.-.---CZ'F 3C L-3--- -'~---"""" ---"'F'Aij I"A~N' ETAl. ( 19 8~1~B)-, SIN GH ET AL • ( 1q 79 )--- -- -f~-o E"'15, I .0E-IS; -- -..--r~oE.:f5~'·----·-2-. 0 E-15, ·,--'--''--:-S-.-0-E---'OI-'05-,

--------r;<yE ~I4 ;_-- -- '2 ~ Of~14;--------5.:0e:.14-;----· 1. 0 E-13, 2 .0 E-13,.-- ---·--5~O'E ... 13 ; - 7. 5I~1 3 -~ - -- ~-OE=-f2-;' ---- --2 • 0 E-12 , 3 • 2 E-12,~"_~-:--_~5'~9I-l?;-- .i~o E:"12, .-- ..--~~~ QE.::-li! ='--.=--=--1. i E-ll, 1. 3E-l1, ,__~-=-~~=~~==--~ __ • 00 .J_'_,?E-l!,_. .__~ 1 .• ~I::-.ll~ .. _.~_l,!.J_E-11.L_,__,_ . 1.8 E-l1.1 2*1.9E-l1

C2F4CL2 FABIAN ET AL.(1~81a), SINGH ET Al.(1919}_~~==_--.-7~~<iJ~·~4~_·. i. it~13~ .... -i~4E~J3.!---__-- ?~_?_E_:].f~.__--_=·=__=_4._!_Q..~,_-_1~3_,--

1.0E-13, I.OE-12, 1.5E-12, 2.3E-12, 3.2E-12,--4-~-OE-12, 4. 2E-l2, 4.5 E-i 2,------4~9E-I2~-----'----5.4 e::lz:;------------ -----.-----6~·-fE.:-12, 7 .·"oe-i 2, 1. 5·-E-~-1.2-;···-··----.- 8. OE-12~ 8. 5E-12, ------- _v__ • -- --._._.

9~OE-i2, 9.5E-12, l.CE-ll, ----·1.-OE-11,------i*T~TE-::1T---------·,---(:-'2 f·s-e'l" ..... ,- < • F-A BI AN '-E~t AL • (1-981BJ, .P·E N'K E'if~'TT AL:(1981 ) ~~----- ~.~._.¥ ~-~~ ~.'--'

---------- 4. 2E---13,4~5E:"13, -,- 4-. 9E-13,----------5. 4E~13~' 6.1 E-13;--------------- --'7 .·oE~f-3, 8". O"E :"'13 ~_. 9.0 E-13, ·---,·-----i-~-6-E-12; 1.1 E.-12, -.-...--.-.-------,--.-- ..J.__?E-12, 1.3E-12,· 1.4E:::fz;- '--i~E.:'i-2,-·-·-- 1.9E-12,

.2. ?E_-12, 2. 6f~12, 3.0 E-1i, .. ~:~~~_-:__3.• 5 e-=1L--- 4. OE-IZ,_._,__~ 6 *,4_~Q.t-1:2

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Al~19th)--=----=------

------------_.._-_.... -------.~--

ll.~.7_~ f~:-=-riQ~_C'R AYETAL. (_~ 117 9--.! ~~~_~~-- .. --- ....----4.0E-12, 7.0E-Il, 1.IE-11,

... i-.-~E--l 0;-~ 4 • 0 E-10, 6 • 0 E-1 O~

B-. 5E=fo,-· .. --7~-5e=1-o;------4 •3E-TO;.8_. <Lf::t!?~_-~~~~ 0 E-11, --3;2E-11,~ --- .._.__~~~~-~_~_1_._?J=111___ 1. 0 E-111 8 .0 E-1 Z, __ ~ ....._~_. _

BOUGHN EIt AND NEAL. y (19iq)~ -H-UDSONETAl. (1981), KING If- ~J~.]}97-9j·1.0e--13,· 3-;-6E-':ii~---- 9.6E-ll, _. 3.6E-IO,1.0£-09, 9-'-4E::fo,-~- a.8E-IO, 8.0E-IO,:3. 8E::lo,- ·I:-4E-':TO~··-- 6.0E-II, 3.0E-lb5.0E-IZ, 2.-5E~T2;·-- 1.2r-12, 7.0E-13,;2 .:~_~-i ~_-, i ~9~-::-13-!_~ ~. 3E-13, . I.OE-I3,

1.5E-12,------- -_._---

2.0E-IZ,3-~-bE"~1:z,

--'Yf*"4-~-OE-':':T2 -,-H'tfZ------ -YUNG Et" AL.<l9~(H;~10GAN E:T Al.(1979), ANDERSON ET

----"-----1-;BE~Io, 7 .2E"':lti.,--- -6-.-bE--IO-,- b.OE-10, 5.'fE-lO,-- --- --4-~"8E'"-n> ,--- 4 -.3 e -1 c,---:r;sf:':-l 0 , --:-3~.-:-3~E--7-1-=-O-=--,-------->-3--=-.--i-l~E--7l--;;-O":-,---

'-r~ '6 E:;10-,---EJ ~-('-E'--l l', -5 .-0 E';'iI;- 2. 5E-ll, 1.2 E-11,--- ------1~6E':" i 2 ~.-5~TE --12 ~ t;-;3E:;"-::.,:12::.;-,~--_---=---=---=---=-~3~.----=-O=----;;:=-E~-:'1:Z=,= __=-1..::...• ..::...8=-E---:;.1.=.2.::...., _-----T~ ..·2"E· - f2", .... -,'*T;'o-e":Ti--· ,.- .,.-- -HNOZ' -- ----- --~.ljR-C-RAY (19i9) ;-P-lAT(~-_AN{L~ER~ER (1960) uPPtR LIMITS---. ··10.-i ~oE-=fo-,--

-----··---i-.oT.:.:.-10, 1. OE-lO,'---7~cfE =-i1, 6 '-5 -E"~ i 1;- -------- 4-. '~fE':':il, 4.0 E-11,---·----i:OE~':~- ----- -----..-. ---H-OZ'NOZ--- --..,.- - "_~~~C-RA.'( - ( 1_979) . '(j~~}~_~1~ I I" Ar 2 b K11- _. --2-6.-4 ~ "J E-::} 0 ---'------'--'-----------------~,~~.-~-.--. -----" -

-N03--- --.-.------ -- -NOXON ETA L• (iQ-ia, fQ8tff;--N'.,fUD ET ET AL. (1981) NIGHT I I1E~ ~----- -5 *-4-~ ci"e ~lcf, -- -- - --- - --. -- - .. ~. -- -__0-_'

----- ·4;oE~IO, 3.5 E-IO, 2. 7T;':"[o~- -----01,-----.8 E-IO, 1.0E-IO,-_._~ .. "7~-O E=1 f~ -~ T ;-2 E:';rf, .-- ,--8". 0 E':-f2~,-----=5;..:-:.~O:-:E;--....::1:..::Z:-O::,-----.:;3:-::.~O:-=E;---=1:.:2:-::,--

.. ----2~-ol~y2, LO-,E-';'lZ, - 1.0'[-12-;----- 1.5E-12, 2.0E-12, ----------- ~ "-6". j ; (fE:'"i'2 ~ ---"- ~--- -----~----

--_._ .... _...NZ05

elFb

-' .i-~-2 t:~14 ,6.8E-IO,

-. '~~'~-"7-'~ 61 ;'-10,_.~~- ----

1.2E-11,--------- -'+ .-z-:r;. i j ,--... --.. -. --·-7. O-E ~-f 4tlON02------ H-t,;O'SON-A-NO ~EED

1.6~~i2, Z.OE-IZ,--'~2~'lE-if~---'---" t~5-E~11,

--Y .. _._-- 8. OE-10, B. 3E-10,--------- [,.-bE-TO, -1.5 E-10',- ...----o-i~~OE-l-i~--~ - ·'-··-i-~-iE-~-ff, - -==---?~pE-=f?_ ---- - -- -

-------_._---------------------------------- ------ - --,.. - -- ----- _. ----- ..........

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SZE-AND-K01l9801, TURCO Ef AL.1l98!81 MODELS + ALL MEAS.

1.OE-f5,1.0E-13,1.DE-li;- -

CS~2~--

1o'*f-;{)!: -1 5,3.0E-15, l.OE-14, 3.0E-14, ·i.oE·...:13', ... ---T:D'E--r3';--'-'l.OE-12, 3.OE-12, 1.OE-fr;-------3:or::-rr;--- 3.5E-ll,

---It. OE-:.-rr;--~----4--~-5·E:.:TI,--'-~·-5. DE-II, 5. bE-II, b.2 E-ll,-- --- -- --1~-OE;:'Il --.- - ----.~~,

His--ro'•.c-OE -15' ,-------·~-:OE~-15 ,

-'"3.CE-14,-- ~-:r:-(fE-1 '2,-- --LOE-'CdH2504----- ARNOLD ET AL.H9S1f'-luRCO ET AL,(198lAl--" ---·--1.-oE"':12,' ---1. lE-i 1, 1.. 4-E-Il~--- --1-.9f-ll, -~~E-ll--;'------

--- 3-.6E-..;rr, 4,OE-il, b.ot-1Tt--------~:f;9E::Tf,-- 2.5E-ll,'.ZE-li, i~7E-i3, l.ltE-I), 8.2£--14, 5.2E-14~--·--------

---,,1510'-14.-----2; 8E-..cHi --2.-0E'-14, 1. 5 E- 14, 1.lE-14,'$-;-1E-15, 6.4r-15,~5.-1E--15, ----4-~rE:.-T5~- --- -3~-3E-Y5,-2.7<-15

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, 13

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Page 16: ntrs.nasa.gov · infrared-active species (H20, C02, 03, N20, CO, CH 4 , 02), even,though some of these profiles may not be of great interest for photochemical studies. The fundamental

Cronn, 0.; and Robinson, E. 1979: Tropospheric and LowerStratospheric Vertical Profiles of Ethane and Acetylene.Geophys. Res. Lett~, vol. 6, no. 8, pp~ 641-644.

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14

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Goldan, P. D.; Kuster, W. C.; Schmeltekopf, A. L.; Fehsenfeld, F. C.;and Albritton, D. L. 1981: Correction of Atmospheric N20 Mixing­Ratio Data. J. Geophys. Res., vol. 86, no. C6, pp. 5385-5386.

Goldman, A.; Murcray, D. G.; Murcray, F. J.; Cook, G. R.; VanAllen,J. W.; Bonomo, F. S.; and Blatherwick, R. D. 1979: Identifica­tion of the Vg Vibration-Rotation Band of CF~ in Balloon-BorneInfrared Solar Spectra. Geophys. Res. Lett., vol. 6, no. 7, pp.609-612.

Goldman, A; Murcray, F. J.; Blatherwick, R. D.; Bonomo, F. S.;Murcray, F. H.; and Murcray, D. G. 1981a: Spectroscopic Identi­fication of CHC1F2 (F-22) in the Lower Stratosphere. Geophys.Res. Lett., vol. 8, no. 9, pp. 1012-1014.

Goldman, A.; Murcray, F. J.; Blatherwick, R. D.; Gillis, J. R.;Bonomo, F. S.; Murcray, F. H.; Murcray, D. G.; and Cicerone, R.J. 1981b: Identification of Acetylene (C2H2) in InfraredAtmospheric Absorption Spectra. J. Geophys. Res., vol. 86, no.C12, pp. 12143-12146.

Page 17: ntrs.nasa.gov · infrared-active species (H20, C02, 03, N20, CO, CH 4 , 02), even,though some of these profiles may not be of great interest for photochemical studies. The fundamental

15

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16

Noxon, J. F.; Norton, R. B.; and Henderson, W. R. 1978: Observation ofAtmospheric N03. Geophy. Res. Lett., vol. 5, no. 8, pp. 675-678.

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17

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Williams, W. J.; Kosters, J. J.; Goldman, A.; and Murcray, D. G. 1976:Measurements of Stratospheric Halocarbon Distributions Using InfraredTechniques. Geophys. Res. Lett., vol. 3, no. 7, pp. 379-382.

Yung, Y. L.; Pinto, J. P.; Watson, R. T.; and Sander, S. P. 1980:Atmospheric Bromine and Ozone Perturbations in the LowerStratosphere. J. Atmos. Sci., vol. 37, no. 2, pp. 339-353.

Page 20: ntrs.nasa.gov · infrared-active species (H20, C02, 03, N20, CO, CH 4 , 02), even,though some of these profiles may not be of great interest for photochemical studies. The fundamental

50

45

40

35

30..........~~'-'

w 250:::>I-i=-1«

20

15

10

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18

H20 VOLUME MIXING RATIO

Page 21: ntrs.nasa.gov · infrared-active species (H20, C02, 03, N20, CO, CH 4 , 02), even,though some of these profiles may not be of great interest for photochemical studies. The fundamental

19

50 0I

0I

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0I

0I

40 0I

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0I

30 0- I~ 0~ I.......,

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0I

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10-6 10-5 10-4 10-3 10-2 10- 1

CO 2 VOLUME MIXING RATIO

Page 22: ntrs.nasa.gov · infrared-active species (H20, C02, 03, N20, CO, CH 4 , 02), even,though some of these profiles may not be of great interest for photochemical studies. The fundamental

20

pO 0\ .0. \0

45 \0\0\

40 0\0\0

35 /0/

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30 0,,-... ./::i!: 0~ I'-'

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10-9 10-4

°3 VOLUME MIXING RATIO

Page 23: ntrs.nasa.gov · infrared-active species (H20, C02, 03, N20, CO, CH 4 , 02), even,though some of these profiles may not be of great interest for photochemical studies. The fundamental

50 Db .45 .. ~

\0\

40 0\0

\0

35 \0

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N 0 MIXING RATIO2

21

Page 24: ntrs.nasa.gov · infrared-active species (H20, C02, 03, N20, CO, CH 4 , 02), even,though some of these profiles may not be of great interest for photochemical studies. The fundamental

22

50 0I

0I

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0I

0I

40 0I

0I

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0I

0I

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10 0\0\0

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CO VOLUME MIXING RATIO

Page 25: ntrs.nasa.gov · infrared-active species (H20, C02, 03, N20, CO, CH 4 , 02), even,though some of these profiles may not be of great interest for photochemical studies. The fundamental

50 0\0

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40 0\0\0

35 \0\0\

30 0~ \

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\0

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CH 4 VOLUME MIXING RATIO

23

Page 26: ntrs.nasa.gov · infrared-active species (H20, C02, 03, N20, CO, CH 4 , 02), even,though some of these profiles may not be of great interest for photochemical studies. The fundamental

50 0I

0I

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0010-3

°2 VOLUME MIXING RATIO

24

Page 27: ntrs.nasa.gov · infrared-active species (H20, C02, 03, N20, CO, CH 4 , 02), even,though some of these profiles may not be of great interest for photochemical studies. The fundamental

50 0I

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5°2 VOLUME MIXING RATIO

25

Page 28: ntrs.nasa.gov · infrared-active species (H20, C02, 03, N20, CO, CH 4 , 02), even,though some of these profiles may not be of great interest for photochemical studies. The fundamental

-..:.:

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01

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10-7

NO VOLUME MIXING RATIO

26

Page 29: ntrs.nasa.gov · infrared-active species (H20, C02, 03, N20, CO, CH 4 , 02), even,though some of these profiles may not be of great interest for photochemical studies. The fundamental

50 0\0\0

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N0 2 VOLUME MIXING RATIO

27

Page 30: ntrs.nasa.gov · infrared-active species (H20, C02, 03, N20, CO, CH 4 , 02), even,though some of these profiles may not be of great interest for photochemical studies. The fundamental

28

! Wlll.----7----l.-~ 10-1 0UllL-...........~

MIXING RATIO

-------0 .. -----0_____

·------D~

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10

5

Page 31: ntrs.nasa.gov · infrared-active species (H20, C02, 03, N20, CO, CH 4 , 02), even,though some of these profiles may not be of great interest for photochemical studies. The fundamental

29

500""

0""

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HN03 VOLUME MIXING RATIO

Page 32: ntrs.nasa.gov · infrared-active species (H20, C02, 03, N20, CO, CH 4 , 02), even,though some of these profiles may not be of great interest for photochemical studies. The fundamental

30

50 0I

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10-9

OH VOLUME MIXING RATIO

Page 33: ntrs.nasa.gov · infrared-active species (H20, C02, 03, N20, CO, CH 4 , 02), even,though some of these profiles may not be of great interest for photochemical studies. The fundamental

50

45

40

35

30

~ 25:::>I::~«

20

15

10

HF VOLUME MIXING RATIO

31

Page 34: ntrs.nasa.gov · infrared-active species (H20, C02, 03, N20, CO, CH 4 , 02), even,though some of these profiles may not be of great interest for photochemical studies. The fundamental

32

50 0I

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Hel VOLUME MIXING RATIO

Page 35: ntrs.nasa.gov · infrared-active species (H20, C02, 03, N20, CO, CH 4 , 02), even,though some of these profiles may not be of great interest for photochemical studies. The fundamental

50 0I

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HBr VOLUME MIXING RATIO

33

Page 36: ntrs.nasa.gov · infrared-active species (H20, C02, 03, N20, CO, CH 4 , 02), even,though some of these profiles may not be of great interest for photochemical studies. The fundamental

34

50 0I

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HI VOLUME MIXING RATIO

Page 37: ntrs.nasa.gov · infrared-active species (H20, C02, 03, N20, CO, CH 4 , 02), even,though some of these profiles may not be of great interest for photochemical studies. The fundamental

30.,......~~'-J

LLJ 250:::>!=~..(

20

CIO MIXING RATIO

35

Page 38: ntrs.nasa.gov · infrared-active species (H20, C02, 03, N20, CO, CH 4 , 02), even,though some of these profiles may not be of great interest for photochemical studies. The fundamental

36

5

5

15

10

40

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35

45

30.........~~.........

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20

oes VOLUME MIXING RATIO

Page 39: ntrs.nasa.gov · infrared-active species (H20, C02, 03, N20, CO, CH 4 , 02), even,though some of these profiles may not be of great interest for photochemical studies. The fundamental

37

50 0\0\0

45 \0\0\

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H2CO VOLUME MIXING RATIO

Page 40: ntrs.nasa.gov · infrared-active species (H20, C02, 03, N20, CO, CH 4 , 02), even,though some of these profiles may not be of great interest for photochemical studies. The fundamental

50 0\

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HOCI VOLUME MIXING RATIO

38

Page 41: ntrs.nasa.gov · infrared-active species (H20, C02, 03, N20, CO, CH 4 , 02), even,though some of these profiles may not be of great interest for photochemical studies. The fundamental

39

50 0I

0I

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N2 VOLUME MIXING RATIO

Page 42: ntrs.nasa.gov · infrared-active species (H20, C02, 03, N20, CO, CH 4 , 02), even,though some of these profiles may not be of great interest for photochemical studies. The fundamental

40

50 DI

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HeN VOLUME MIXING RATIO

Page 43: ntrs.nasa.gov · infrared-active species (H20, C02, 03, N20, CO, CH 4 , 02), even,though some of these profiles may not be of great interest for photochemical studies. The fundamental

• 5

45

40

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10

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CH 3 CI VOLUME MIXING RATIO

41

Page 44: ntrs.nasa.gov · infrared-active species (H20, C02, 03, N20, CO, CH 4 , 02), even,though some of these profiles may not be of great interest for photochemical studies. The fundamental

50 0\0\0

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42

H2

0 2 VOLUME MIXING RATIO

Page 45: ntrs.nasa.gov · infrared-active species (H20, C02, 03, N20, CO, CH 4 , 02), even,though some of these profiles may not be of great interest for photochemical studies. The fundamental

43

15

10

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3

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MIXING RATIO

Page 46: ntrs.nasa.gov · infrared-active species (H20, C02, 03, N20, CO, CH 4 , 02), even,though some of these profiles may not be of great interest for photochemical studies. The fundamental

44

C2

HS

VOLUME MIXING RATIO

Page 47: ntrs.nasa.gov · infrared-active species (H20, C02, 03, N20, CO, CH 4 , 02), even,though some of these profiles may not be of great interest for photochemical studies. The fundamental

5

4

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1

10-19

PH 3 VOLUME MIXING RATIO

10-15

45

Page 48: ntrs.nasa.gov · infrared-active species (H20, C02, 03, N20, CO, CH 4 , 02), even,though some of these profiles may not be of great interest for photochemical studies. The fundamental

46

5O ]---

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Page 49: ntrs.nasa.gov · infrared-active species (H20, C02, 03, N20, CO, CH 4 , 02), even,though some of these profiles may not be of great interest for photochemical studies. The fundamental

5

4

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15

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C2 H4 VOLUME MIXING RATIO

47

Page 50: ntrs.nasa.gov · infrared-active species (H20, C02, 03, N20, CO, CH 4 , 02), even,though some of these profiles may not be of great interest for photochemical studies. The fundamental

-::i~.

'-'

w 250::::>.-I-...J«

20

15

10

5

~D~D~D~

D~

D~0"",

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CFCI3 VOLUME MIXING RATIO

48

Page 51: ntrs.nasa.gov · infrared-active species (H20, C02, 03, N20, CO, CH 4 , 02), even,though some of these profiles may not be of great interest for photochemical studies. The fundamental

50 0\.

0\0

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10-9

CF2CI2 VOLUME MIXING RATIO

49

Page 52: ntrs.nasa.gov · infrared-active species (H20, C02, 03, N20, CO, CH 4 , 02), even,though some of these profiles may not be of great interest for photochemical studies. The fundamental

50

50 0I0I0

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CF3CI VOLUME MIXINO RATIO

Page 53: ntrs.nasa.gov · infrared-active species (H20, C02, 03, N20, CO, CH 4 , 02), even,though some of these profiles may not be of great interest for photochemical studies. The fundamental

5

4

35

30........::E~......,w 250;:)

t::~«

20

15

10

5

~o~o

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CHCIF2 VOLUME MIXING RATIO

51

10-10

Page 54: ntrs.nasa.gov · infrared-active species (H20, C02, 03, N20, CO, CH 4 , 02), even,though some of these profiles may not be of great interest for photochemical studies. The fundamental

52

10-15 10-14 10-13

CHCI2 F VOLUME MIXING RATIO

5

20

10

15

30 ~O~O"" .O~

0"0 .""'0"0 .

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Page 55: ntrs.nasa.gov · infrared-active species (H20, C02, 03, N20, CO, CH 4 , 02), even,though some of these profiles may not be of great interest for photochemical studies. The fundamental

5

40

35

30,......:'IE::lC:'-"

w 25Cl::>!:::r--l-e(

20

15

10

5

"'-~.0"'0

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b\o'0,

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CCI4 VOLUME MIXING RATIO

53

Page 56: ntrs.nasa.gov · infrared-active species (H20, C02, 03, N20, CO, CH 4 , 02), even,though some of these profiles may not be of great interest for photochemical studies. The fundamental

54

50 0I

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010-13 10-12 10-11 10-10 10-9 10-8 •

CF4 VOLUME MIXING RATIO

Page 57: ntrs.nasa.gov · infrared-active species (H20, C02, 03, N20, CO, CH 4 , 02), even,though some of these profiles may not be of great interest for photochemical studies. The fundamental

55

15

20

10

5

4

30 --------0~o~ .0"n

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5

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CF3Br VOLUME MIXING RATIO

Page 58: ntrs.nasa.gov · infrared-active species (H20, C02, 03, N20, CO, CH 4 , 02), even,though some of these profiles may not be of great interest for photochemical studies. The fundamental

56

10- 0 .

5

40 ~O"'0

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CH3

CCI3

VOLUME MIXING RATIO

Page 59: ntrs.nasa.gov · infrared-active species (H20, C02, 03, N20, CO, CH 4 , 02), even,though some of these profiles may not be of great interest for photochemical studies. The fundamental

5

35

30.........:::i~"'-J

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20

15

10

5

"'0~

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57

Page 60: ntrs.nasa.gov · infrared-active species (H20, C02, 03, N20, CO, CH 4 , 02), even,though some of these profiles may not be of great interest for photochemical studies. The fundamental

58

50 D

b •\D

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\0

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35 \0

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15 .I0\0\

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5 I0\0I

10-11 10-10

C2F4CI2 VOLUME MIXING RATIO

Page 61: ntrs.nasa.gov · infrared-active species (H20, C02, 03, N20, CO, CH 4 , 02), even,though some of these profiles may not be of great interest for photochemical studies. The fundamental

59

50 0\0\0

45 \0\0

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\0\0

35 \0\0\

30 0"""" \~ 0y

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15 \0\0I

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10- 11 10- 10

C2 F5 CI VOLUME MIXING RATIO

Page 62: ntrs.nasa.gov · infrared-active species (H20, C02, 03, N20, CO, CH 4 , 02), even,though some of these profiles may not be of great interest for photochemical studies. The fundamental

60

50 0\0\0

45 I0\0I

40 0I0\0

35 \0\0\

30 0..-,. . I:::E 0y I.......,

w 0C1 25 I::) 0r- Ir--J 0,« \

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10 0I

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05 I

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010-15 10-13 10- 12 10- 11 10- 10

C2FS VOLUME MIXING RATIO

Page 63: ntrs.nasa.gov · infrared-active species (H20, C02, 03, N20, CO, CH 4 , 02), even,though some of these profiles may not be of great interest for photochemical studies. The fundamental

61

50 0f

0f

045 f

0f

0f

40 0f

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30 D~......... if:::E:x:: /'-'

w 25 ~0:::::> ?I-i=...J 0« /

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0I

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10-9 10-8

H0 2 VOLUME MIXING RATIO

Page 64: ntrs.nasa.gov · infrared-active species (H20, C02, 03, N20, CO, CH 4 , 02), even,though some of these profiles may not be of great interest for photochemical studies. The fundamental

62

50 0I

0I

045 I

0I

tJI

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0I

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0I

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HN0 2 VOLUME MIXING RATIO

Page 65: ntrs.nasa.gov · infrared-active species (H20, C02, 03, N20, CO, CH 4 , 02), even,though some of these profiles may not be of great interest for photochemical studies. The fundamental

50 0I

0• I

045 I

0I

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63

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69

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Page 73: ntrs.nasa.gov · infrared-active species (H20, C02, 03, N20, CO, CH 4 , 02), even,though some of these profiles may not be of great interest for photochemical studies. The fundamental
Page 74: ntrs.nasa.gov · infrared-active species (H20, C02, 03, N20, CO, CH 4 , 02), even,though some of these profiles may not be of great interest for photochemical studies. The fundamental

1. Report No.

NASA TM- 83289I2. Government Accession No. 3. Recipient's ~talog No.

4. Title and Subtitle

COMPILATION OF ATMOSPHERIC GAS CONCENTRATIONPROFILES FROM 0 TO 50 KM

5. Report Date

Mtlrr-h 1QA?6. Performing Organization Code

147-30-01-037. Author(s) 8. Performing Organization Report No.

Mary Ann H. Smith

9. Performing Organization Name and Addressr-----------------------------......J 10. Work Unit No.

NASA Langley Research CenterHampton, VA 23665

11. Contract or Grant No. •

12. Sponsoring Agency Name and Address

National Aeronautics and Space AdministrationWashington, DC 20546

14. Sponsoring Agency Code

15. Supplementary Notes

16. Abstract

A set of 52 atmospheric gas concentration profiles between o and 50 km has beencompiled as a convenient reference data set for calculation of atmospheric infraredabsorption or emission signals and for initialization of iterative procedures forretrieval of gas concentrations from measured data. The distributions of volumemixing ratio as a function of altitude generally correspond' to typical diurnallyaveraged, seasonally averaged Northern Hemisphere midlatitude gas concentrationprofiles. Profiles are given for all gases included in current infraredatmospheric absorption line parameter compilations; and for a number of additionalimportant trace gases.

17. Key Words (Suggested by Author(s))

Atmospheric GasesRemote SensingAtmospheric Transmission Models

18. Distribution Statement

Unclassified - UnlimitedSubject Category 46

19. Security Oassif. (of this report)

Unclassified20. Security Classif. (of this page)

Unclassified21. No. of Pages

7022. Price

A04

S-J05 For sale by the National Technical Information Service. Springfield, Virginia 22161

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