NASA216 pages

Crew Post-Mission Debriefing

NASA UAP D015 Astronaut Scientific Debriefings 1962 1963

Date range15 NOVEMBER 1963

Originating officeNASA

Crew Post-Mission Debriefing from the NASA archive. 216 pages. Document references the date(s) 15 NOVEMBER 1963, 21 FEBRUARY 1962, 24 MAY 1962. Excerpt and key details below are extracted directly from the text layer. Drawing directly from the text layer of the document: · C 11.gbt. tll&t ,, C COIie t I bo • • at boti. ,tbeil l ltlQ'ecl 1n 1 j( tbe ~ ont.bento • Dee' · ~--...........--......................,..__. t

Significance

A NASA-released voice or debriefing record from a crewed lunar / orbital mission.

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Key entities (auto-extracted)

Date-time groups, coordinates, aircraft types, weapons, classification markings — pulled by regex straight from the PDF text layer.

Classification Markings

FOR OFFICIAL USE ONLY

Per-page highlights

The most signal-bearing sentences on each page (mentioning UAP / radar / observation / altitude / coordinates). Kept in the original language to avoid translation drift.

p.5
EN
· C 11.gbt. tll&t ,, C COIie t I bo • • at boti. ,tbeil l ltlQ'ecl 1n 1 j( tbe ~ ont.bento • Dee'
中文
· C 11.gbt. tll&t ,, C COIie t I bo • • at boti. ,tbeil l ltlQ'ecl 1n 1 j( tbe ~ ont.bento • Dee'
p.15
EN
· 4
中文
· 4
p.32
EN
· ~--...........--......................,..__. t
中文
· ~--...........--......................,..__. t
p.34
EN
· From t.l¼e~-eie Vconsiderations alone, it may be stated that the luminous Jparticles observed by Col
中文
· From t.l¼e~-eie Vconsiderations alone, it may be stated that the luminous Jparticles observed by Col
p.35
EN
· The fact that the coloring a,~aPen~ ~~~,~ was a yellow-green and the eiiee~ive observational pi,e became fluorescent in sunlight.~e particles observed in shadow were observed in the scattered light from the spacecraft and were probably illuminated only by visible ~ ~~f the spectrum. - ;l- The change of angles of t…· Glenn to observe the particles under improper dark adaptation ~ indicate'that an astronaut would be in a position to carry through a series of experi'1nents to investigate C.o~.L" the physics of Q.QmROMS in the solar environment
中文
· The fact that the coloring a,~aPen~ ~~~,~ was a yellow-green and the eiiee~ive observational pi,e became fluorescent in sunlight.~e particles observed in shadow were observed in the scattered light from the spacecraft and were probably illuminated only by visible ~ ~~f the spectrum. - ;l- The change of angles of t…· Glenn to observe the particles under improper dark adaptation ~ indicate'that an astronaut would be in a position to carry through a series of experi'1nents to investigate C.o~.L" the physics of Q.QmROMS in the solar environment
p.36
EN
· Glenn's observation -.'t o{ '- band six to eight degrees 9'f t~e twill a-eix-~e-eiga~-aegPee-e&Ba above the horizon, with a haze layer about two degrees Although it has been speculated that wide at the top. ~5'~~1!:irl~-.eilli-il~e observation = ~\: the multipa~wl:l:,ers of the1'window cause the high 0~ angle~ the …· Au-6her investigations of the air glow and haze layerKiG£ should be carried out . ~~ Meteorology
中文
· Glenn's observation -.'t o{ '- band six to eight degrees 9'f t~e twill a-eix-~e-eiga~-aegPee-e&Ba above the horizon, with a haze layer about two degrees Although it has been speculated that wide at the top. ~5'~~1!:irl~-.eilli-il~e observation = ~\: the multipa~wl:l:,ers of the1'window cause the high 0~ angle~ the …· Au-6her investigations of the air glow and haze layerKiG£ should be carried out . ~~ Meteorology
p.37
EN
· It is of se.e:~ a:t-importanli" that proper dark adaptation methods be incorporated into the spacecraft system so that the astronaut may optimize his visual observations. c o"'tl'le\.s Investigations of the physics of OQB!!fteft~s and the feasibility of the ~l " th-tificial ~omet "experiment may be carried out direc…
中文
· It is of se.e:~ a:t-importanli" that proper dark adaptation methods be incorporated into the spacecraft system so that the astronaut may optimize his visual observations. c o"'tl'le\.s Investigations of the physics of OQB!!fteft~s and the feasibility of the ~l " th-tificial ~omet "experiment may be carried out direc…
p.38
EN
· A..~,:...... >MC,--. p .,..c,,h ...~ o... multi lier :Be! "b systeml ~ series of filters r: 4,-~J ►"'-> --~c.~... ~-- .t..~--~ ~ u.v. ~\_,..,, - ...~ (including~a J;,Oii~e flaorceeent ~lain fi]:l;er to stuely ½ ~t-..Av,.u.,,,-.o:..c.. ) tac ultra viole:!T) should be incorporated into the spacecraft. ~iUJ£e -a :au.m…
中文
· A..~,:...... >MC,--. p .,..c,,h ...~ o... multi lier :Be! "b systeml ~ series of filters r: 4,-~J ►"'-> --~c.~... ~-- .t..~--~ ~ u.v. ~\_,..,, - ...~ (including~a J;,Oii~e flaorceeent ~lain fi]:l;er to stuely ½ ~t-..Av,.u.,,,-.o:..c.. ) tac ultra viole:!T) should be incorporated into the spacecraft. ~iUJ£e -a :au.m…
p.39
EN
· B 2 3 196? 0 U.\h <!.°""""U)4.. '2'"3ol!I- '3oco 0 ~ -~ Vje0/2 w~Jo...:, caJ v-nf c~-4
中文
· B 2 3 196? 0 U.\h <!.°""""U)4.. '2'"3ol!I- '3oco 0 ~ -~ Vje0/2 w~Jo...:, caJ v-nf c~-4
p.40
EN
· It seemed possible that the layer he described could be . accounted for as a region of relatively large nitrogen peroxide (N02 ) concentration, and the past two weeks have been spent in checking this hypothesis • Unfortunately I am not familiar with either photochemistry or upper atmosphere physics so the following …
中文
· It seemed possible that the layer he described could be . accounted for as a region of relatively large nitrogen peroxide (N02 ) concentration, and the past two weeks have been spent in checking this hypothesis • Unfortunately I am not familiar with either photochemistry or upper atmosphere physics so the following …
p.41
EN
· Figure 1 I Vertical path (No. 1) No. 3 No. 2 Figure 2
中文
· Figure 1 I Vertical path (No. 1) No. 3 No. 2 Figure 2
p.42
EN
· Ju}¥ 13, 1962 Fox- th, followins I will assume that the concentr.ation ot absorbins mo1ecu1es in the region of interest can be described adequate}¥ by an exponential decrease w1th altitude above the bottom, of the layer, hence, can be represented by where Y is the scale height in the layer and H must lie in the .ia.yer
中文
· Ju}¥ 13, 1962 Fox- th, followins I will assume that the concentr.ation ot absorbins mo1ecu1es in the region of interest can be described adequate}¥ by an exponential decrease w1th altitude above the bottom, of the layer, hence, can be represented by where Y is the scale height in the layer and H must lie in the .ia.yer

Open original

Open in new tab ↗Source transcript ↗

Per-page highlights

The most signal-bearing sentences on each page (mentioning UAP / radar / observation / altitude / coordinates). Kept in the original language to avoid translation drift.

p.5

· C 11.gbt. tll&t ,, C COIie t I bo • • at boti. ,tbeil l ltlQ'ecl 1n 1 j( tbe ~ ont.bento • Dee'

中文

· C 11.gbt. tll&t ,, C COIie t I bo • • at boti. ,tbeil l ltlQ'ecl 1n 1 j( tbe ~ ont.bento • Dee'

p.15

· 4

中文

· 4

p.32

· ~--...........--......................,..__. t

中文

· ~--...........--......................,..__. t

p.34

· From t.l¼e~-eie Vconsiderations alone, it may be stated that the luminous Jparticles observed by Col

中文

· From t.l¼e~-eie Vconsiderations alone, it may be stated that the luminous Jparticles observed by Col

p.35

· The fact that the coloring a,~aPen~ ~~~,~ was a yellow-green and the eiiee~ive observational pi,e became fluorescent in sunlight.~e particles observed in shadow were observed in the scattered light from the spacecraft and were probably illuminated only by visible ~ ~~f the spectrum. - ;l- The change of angles of t…· Glenn to observe the particles under improper dark adaptation ~ indicate'that an astronaut would be in a position to carry through a series of experi'1nents to investigate C.o~.L" the physics of Q.QmROMS in the solar environment

中文

p.36

· Glenn's observation -.'t o{ '- band six to eight degrees 9'f t~e twill a-eix-~e-eiga~-aegPee-e&Ba above the horizon, with a haze layer about two degrees Although it has been speculated that wide at the top. ~5'~~1!:irl~-.eilli-il~e observation = ~\: the multipa~wl:l:,ers of the1'window cause the high 0~ angle~ the …· Au-6her investigations of the air glow and haze layerKiG£ should be carried out . ~~ Meteorology

中文

p.37

· It is of se.e:~ a:t-importanli" that proper dark adaptation methods be incorporated into the spacecraft system so that the astronaut may optimize his visual observations. c o"'tl'le\.s Investigations of the physics of OQB!!fteft~s and the feasibility of the ~l " th-tificial ~omet "experiment may be carried out direc…

中文

p.38

· A..~,:...... >MC,--. p .,..c,,h ...~ o... multi lier :Be! "b systeml ~ series of filters r: 4,-~J ►"'-> --~c.~... ~-- .t..~--~ ~ u.v. ~\_,..,, - ...~ (including~a J;,Oii~e flaorceeent ~lain fi]:l;er to stuely ½ ~t-..Av,.u.,,,-.o:..c.. ) tac ultra viole:!T) should be incorporated into the spacecraft. ~iUJ£e -a :au.m…

中文

p.39

· B 2 3 196? 0 U.\h <!.°""""U)4.. '2'"3ol!I- '3oco 0 ~ -~ Vje0/2 w~Jo...:, caJ v-nf c~-4

中文

· B 2 3 196? 0 U.\h <!.°""""U)4.. '2'"3ol!I- '3oco 0 ~ -~ Vje0/2 w~Jo...:, caJ v-nf c~-4

p.40

· It seemed possible that the layer he described could be . accounted for as a region of relatively large nitrogen peroxide (N02 ) concentration, and the past two weeks have been spent in checking this hypothesis • Unfortunately I am not familiar with either photochemistry or upper atmosphere physics so the following …

中文

p.41

· Figure 1 I Vertical path (No. 1) No. 3 No. 2 Figure 2

中文

· Figure 1 I Vertical path (No. 1) No. 3 No. 2 Figure 2

p.42

· Ju}¥ 13, 1962 Fox- th, followins I will assume that the concentr.ation ot absorbins mo1ecu1es in the region of interest can be described adequate}¥ by an exponential decrease w1th altitude above the bottom, of the layer, hence, can be represented by where Y is the scale height in the layer and H must lie in the .ia.yer

中文