https://github.com/virtualagc/virtualagc
Revision 078c79d8734a9ed2860303a7c1662004284fe853 authored by Ron Burkey on 07 August 2022, 15:04:04 UTC, committed by Ron Burkey on 07 August 2022, 15:04:04 UTC
assembly listings from yaASM and yaLEMAP. Added some debugging messages
to 'make install'.  Tweaked debugging messages that VirtualAGC embeds in
'simulate'.  Verified buildability in Mint 21, 20, 19, 17, and verified
buildability using clang in Mint 17.
1 parent 6bb1acc
Raw File
Tip revision: 078c79d8734a9ed2860303a7c1662004284fe853 authored by Ron Burkey on 07 August 2022, 15:04:04 UTC
Fixed a potential string-overflow bug in yaASM. Removed timestamps from
Tip revision: 078c79d
POWERED_FLIGHT_SUBROUTINES.agc
### FILE="Main.annotation"
## Copyright:	Public domain.
## Filename:	POWERED_FLIGHT_SUBROUTINES.agc
## Purpose:	Part of the source code for Colossus 2A, AKA Comanche 055.
##		It is part of the source code for the Command Module's (CM)
##		Apollo Guidance Computer (AGC), for Apollo 11.
## Assembler:	yaYUL
## Contact:	Ron Burkey <info@sandroid.org>.
## Website:	www.ibiblio.org/apollo.
## Pages:	1365-1372 
## Mod history: 2009-05-10 SN   (Sergio Navarro).  Started adapting
##                              from the Colossus249/ file of the same
##                              name, using Comanche055 page images.
##		2010-08-29 JL	Fixed indentation.
##		2016-12-22 RSB	Proofed comment text using octopus/ProoferComments
##				and corrected the errors found.
##		2017-01-18 RSB	Fixed comment-text errors noted while diff'ing
##				vs Colossus 249.
##
## This source code has been transcribed or otherwise adapted from digitized
## images of a hardcopy from the MIT Museum.  The digitization was performed
## by Paul Fjeld, and arranged for by Deborah Douglas of the Museum.  Many
## thanks to both.  The images (with suitable reduction in storage size and
## consequent reduction in image quality as well) are available online at
## www.ibiblio.org/apollo.  If for some reason you find that the images are
## illegible, contact me at info@sandroid.org about getting access to the
## (much) higher-quality images which Paul actually created.
##
## Notations on the hardcopy document read, in part:
##
##    Assemble revision 055 of AGC program Comanche by NASA
##    2021113-051.  10:28 APR. 1, 1969 
##
##    This AGC program shall also be referred to as
##            Colossus 2A


## Page 1365
		BANK	14		# SAME FBANK AS THE FINDCDUD SUB-PROGRAM
		SETLOC	POWFLITE
		BANK

		EBANK=	DEXDEX
		COUNT*	$$/POWFL

# CDUTRIG, CDUTRIG1, CDUTRIG2, AND CD*TR*GS ALL COMPUTE THE SINES AND
# COSINES OF THREE 2'S COMPLEMENT ANGLES AND PLACE THE RESULT, DOUBLE
# PRECISION, IN THE SAME ORDER AS THE INPUTS, AT SINCDU AND COSCDU.  AN
# ADDITIONAL OUTPUT IS THE 1'S COMPLEMENT ANGLES AT CDUSPOT.  THESE
# ROUTINES GO OUT OF THEIR WAY TO LEAVE THE MPAC AREA AS THEY FIND IT,
# EXCEPT FOR THE GENERALLY UNIMPORTANT MPAC +2.  THEY DIFFER ONLY IN
# WHERE THEY GET THE ANGLES, AND IN METHOD OF CALLING.
#
# CDUTRIG (AND CDUTRIG1, WHICH CAN BE CALLED IN BASIC) COMPUTE THE
# SINES AND COSINES FROM THE CURRENT CONTENTS OF THE CDU REGISTERS.
# THE CONTENTS OF CDUTEMP, ETC., ARE NOT TOUCHED SO THAT THEY MAY
# CONTINUE TO FORM A CONSISTENT SET WITH THE LATEST PIPA READINGS.
#
# CDUTRIG1 IS LIKE CDUTRIG EXCEPT THAT IT CAN BE CALLED IN BASIC.
#
# CD*TR*GS FINDS CDU VALUES IN CDUSPOT RATHER THAN IN CDUTEMP.  THIS
# ALLOWS USERS TO MAKE TRANSFORMATIONS USING ARBITRARY ANGLES, OR REAL
# ANGLES IN AN ORDER OTHER THAN X Y Z.  A CALL TO THIS ROUTINE IS
# NECESSARY IN PREPARATION FOR A CALL TO AX*SR*T IN EITHER OF ITS TWO
# MODES (SMNB OR NBSM).  SINCE AX*SR*T EXPECTS TO FIND THE SINES AND
# COSINES IN THE ORDER Y Z X THE ANGLES MUST HAVE BEEN PLACED IN CDUSPOT
# IN THIS ORDER.  CD*TR*GS NEED NOT BE REPEATED WHEN AX*SR*T IS CALLED
# MORE THAN ONCE, PROVIDED THE ANGLES HAVE NOT CHANGED.  NOTE THAT SINCE
# IT CLOBBERS BUF2 (IN THE SINE AND COSINE ROUTINES) CD*TR*GS CANNOT BE
# CALLED USING BANKCALL.  SORRY.
#
# CD*TR*G IS LIKE CD*TR*GS EXCEPT THAT IT CAN BE CALLED IN
# INTERPRETIVE.

CDUTRIG		EXIT
		TC	CDUTRIGS
		TC	INTPRET
		RVQ

CD*TR*G		EXIT
		TC	CD*TR*GS
		TC	INTPRET
		RVQ

CDUTRIGS	CA	CDUX
		TS	CDUSPOT +4
		CA	CDUY
		TS	CDUSPOT
## Page 1366
		CA	CDUZ
		TS	CDUSPOT +2

CD*TR*GS	EXTEND
		QXCH	TEM2
		CAF	FOUR
TR*GL**P	MASK	SIX		# MAKE IT EVEN AND SMALLER
		TS	TEM3
		INDEX	TEM3
		CA	CDUSPOT
		DXCH	MPAC		# STORING 2'S COMP ANGLE, LOADING MPAC
		DXCH	VBUF +4		# STORING MPAC FOR LATER RESTORATION
		TC	USPRCADR
		CADR	CDULOGIC
		EXTEND
		DCA	MPAC
		INDEX	TEM3
		DXCH	CDUSPOT		# STORING 1'S COMPLEMENT ANGLE
		TC	USPRCADR
		CADR	COSINE
		DXCH	MPAC
		INDEX	TEM3
		DXCH	COSCDU		# STORING COSINE
		EXTEND
		INDEX	TEM3
		DCA	CDUSPOT		# LOADING 1'S COMPLEMENT ANGLE
		TC	USPRCADR
		CADR	SINE +1		# SINE +1 EXPECTS ARGUMENT IN A AND L
		DXCH	VBUF +4		# BRINGING UP PRIOR MPAC TO BE RESTORED
		DXCH	MPAC
		INDEX	TEM3
		DXCH	SINCDU
		CCS	TEM3
		TCF	TR*GL**P
		TC	TEM2
## Page 1367
# ****************************************************************************************************************
# QUICTRIG, INTENDED FOR GUIDANCE CYCLE USE WHERE TIME IS CRITICAL, IS A MUCH FASTER VERSION OF CD*TR*GS.
# QUICTRIG COMPUTES AND STORES THE SINES AND COSINES OF THE 2'S COMPLEMENT ANGLES AT CDUSPOT, CDUSPOT +2,
# AND CDUSPOT +4.  UNLIKE CD*TR*GS, QUICTRIG DOES NOT LEAVE THE 1'S COMPLEMENT VERSIONS OF THE ANGLES IN
# CDUSPOT.  QUICTRIG'S EXECUTION TIME IS 4.1 MS;    THIS IS 10 TIMES AS FAST AS CD*TR*GS.    QUICTRIG MAY BE
# CALLED FROM INTERPRETIVE AS AN RTB OP-CODE, OR FROM BASIC VIA BANKCALL OR IBNKCALL.

QUICTRIG	INHINT			# INHINT SINCE DAP USES THE SAME TEMPS
		EXTEND
		QXCH	ITEMP1
		CAF	FOUR
 +4		MASK	SIX
		TS	ITEMP2
		INDEX	ITEMP2
		CA	CDUSPOT
		TC	SPSIN
		EXTEND
		MP	BIT14		# SCALE DOWN TO MATCH INTERPRETER OUTPUTS
		INDEX	ITEMP2
		DXCH	SINCDU
		INDEX	ITEMP2
		CA	CDUSPOT
		TC	SPCOS
		EXTEND
		MP	BIT14
		INDEX	ITEMP2
		DXCH	COSCDU
		CCS	ITEMP2
		TCF	QUICTRIG +4
		CA	ITEMP1
		RELINT
		TC	A
## Page 1368
#****************************************************************************************************************
# THESE INTERFACE ROUTINES MAKE IT POSSIBLE TO CALL AX*SR*T, ETC., IN
# INTERPRETIVE.  LATER, WHERE POSSIBLE, THEY WILL BE ELIMINATED.
#
# NBSM WILL BE THE FIRST TO GO.  IT SHOULD NOT BE USED.

NBSM		STQ
			X2
		LXC,1	VLOAD*	
			S1		# BASE ADDRESS OF THE CDU ANGLES IS IN S1
			0,1
		STOVL	CDUSPOT
			32D		# VECTOR TO BE TRANSFORMED IS IN 32D
		CALL
			TRG*NBSM
		STCALL	32D		# SINCE THERE'S NO STGOTO
			X2

# THESE INTERFACE ROUTINES ARE PERMANENT.  ALL RESTORE USER'S EBANK
# SETTING. ALL ARE STRICT INTERPRETIVE SUBROUTINES, CALLED USING "CALL",
# RETURNING VIA QPRET.  ALL EXPECT AND RETURN THE VECTOR TO BE TRANSFOR-
# MED INTERPRETER-STYLE IN MPAC; COMPONENTS AT MPAC, MPAC +3, AND MPAC +5.
#
# TRG*SMNB AND TRG*NBSM BOTH EXPECT TO SEE THE 2'S COMPLEMENT ANGLES
# AT CDUSPOT (ORDER Y Z X, AT CDUSPOT, CDUSPOT +2, AND CDUSPOT +4; ODD
# LOCATIONS NEED NOT BE ZEROED).  TRG*NBSM DOES THE NB TO SM TRANSFOR-
# MATION; TRG*SMNB, VICE VERSA.
#
# CDU*NBSM DOES ITS TRANSFORMATION USING THE PRESENT CONTENTS OF
# THE CDU COUNTERS.  OTHERWISE IT IS LIKE TRG*NBSM.
#
# CDU*SMNB IS THE COMPLEMENT OF CDU*NBSM.

CDU*SMNB	EXIT
		TC	CDUTRIGS
		TCF	C*MM*N1

TRG*SMNB	EXIT
		TC	CD*TR*GS
C*MM*N1		TC	MPACVBUF	# AX*SR*T EXPECTS VECTOR IN VBUF
		CS	THREE		# SIGNAL FOR SM TO NB TRANSFORMATION
C*MM*N2		TC	AX*SR*T
		TC	INTPRET
		VLOAD	RVQ
			VBUF

CDU*NBSM	EXIT
		TC	CDUTRIGS

## Page 1369

		TCF	C*MM*N3

TRG*NBSM	EXIT
		TC	CD*TR*GS
C*MM*N3		TC	MPACVBUF	# FOR AX*SR*T
		CA	THREE		# SIGNAL FOR NB TO SM TRANSFORMATION
		TCF	C*MM*N2

# *NBSM* AND *SMNB* EXPECT TO SEE THE SINES AND COSINES (AT SINCDU
# AND COSCDU) RATHER THAN THE ANGLES THEMSELVES.  OTHERWISE THEY ARE
# LIKE TRG*NBSM AND TRG*SMNB.
#
# NOTE THAT JUST AS CD*TR*GS NEED BE CALLED ONLY ONCE FOR EACH SERIES
# OF TRANSFORMATIONS USING THE SAME ANGLES, SO TOO ONLY ONE OF TRG*NBSM
# AND TRG*SMNB NEED BE CALLED FOR EACH SERIES.  FOR SUBSEQUENT TRANSFOR-
# MATIONS USE *NBSM* AND *SMNB*.

*SMNB*		EXIT
		TCF	C*MM*N1

*NBSM*		EXIT
		TCF	C*MM*N3

# AX*SR*T COMBINES THE OLD SMNB AND NBSM.  FOR THE NB TO SM
# TRANSFORMATION, ENTER WITH +3 IN A.  FOR SM TO NB, ENTER WITH -3.
# THE VECTOR TO BE TRANSFORMED ARRIVES, AND IS RETURNED, IN VBUF.
# AX*SR*T EXPECTS TO FIND THE SINES AND COSINES OF THE ANGLES OF ROTATION
# AT SINCDU AND COSCDU, IN THE ORDER Y Z X.  A CALL TO CD*TR*GS, WITH
# THE 2'S COMPLEMENT ANGLES (ORDER Y Z X) AT CDUSPOT, WILL TAKE CARE OF
# THIS.  HERE IS A SAMPLE CALLING SEQUENCE:-
#		TC	CDUTRIGS
#		CS	THREE		("CA THREE" FOR NBSM)
#		TC	AX*SR*T
# THE CALL TO CD*TR*GS NEED NOT BE REPEATED, WHEN AX*SR*T IS CALLED MORE
# THAN ONCE, UNLESS THE ANGLES HAVE CHANGED.
#
# AX*SR*T IS GUARANTEED SAFE ONLY FOR VECTORS OF MAGNITUDE LESS THAN
# UNITY.  A LOOK AT THE CASE IN WHICH A VECTOR OF GREATER MAGNITUDE
# HAPPENS TO LIE ALONG AN AXIS OF THE SYSTEM TO WHICH IT IS TO BE TRANS-
# FORMED CONVINCES ONE THAT THIS IS A RESTRICTION WHICH MUST BE ACCEPTED.

AX*SR*T		TS	DEXDEX		# WHERE IT BECOMES THE INDEX OF INDEXES
		EXTEND
		QXCH	RTNSAVER

R*TL**P		CCS	DEXDEX		#       	+3 --> 0	-3 --> 2
		CS	DEXDEX		# THUS:		+2 --> 1	-2 --> 1
		AD	THREE		#		+1 --> 2	-1 --> 0
## Page 1370
		EXTEND
		INDEX	A
		DCA	INDEXI
		DXCH	DEXI

		CA	ONE
		TS	BUF
		EXTEND
		INDEX	DEX1
		DCS	VBUF
		TCF	LOOP1		# REALLY BE A SUBTRACT, AND VICE VERSA

LOOP2		DXCH	BUF		# LOADING VECTOR COMPONENT, STORING INDEX

LOOP1		DXCH	MPAC
		CA	SINESLOC
		AD	DEX1
		TS	ADDRWD

		TC	DMPSUB		# MULTIPLY BY SIN(CDUANGLE)
		CCS	DEXDEX
		DXCH	MPAC		# NBSM CASE
		TCF	+3
		EXTEND			# SMNB CASE
		DCS	MPAC
		DXCH	TERM1TMP

		CA	SIX		# SINCDU AND COSCDU (EACH 6 WORDS) MUST
		ADS	ADDRWD		#	BE CONSECUTIVE AND IN THAT ORDER

		EXTEND
		INDEX	BUF
		INDEX	DEX1
		DCA	VBUF
		DXCH	MPAC
		TC	DMPSUB		# MULTIPLY BY COS(CDUANGLE)
		DXCH	MPAC
		DAS	TERM1TMP
		DXCH	TERM1TMP
		DDOUBL
		INDEX	BUF
		INDEX	DEX1
		DXCH	VBUF
		DXCH	BUF		# LOADING INDEX, STORING VECTOR COMPONENT
		CCS	A		# 'CAUSE THAT'S WHERE THE INDEX NOW IS
		TCF	LOOP2

		EXTEND
		DIM	DEXDEX		# DECREMENT MAGNITUDE PRESERVING SIGN

## Page 1371
TSTPOINT	CCS	DEXDEX		# ONLY THE BRANCHING FUNCTION IS USED
		TCF	R*TL**P
		TC	RTNSAVER
		TCF	R*TL**P
		TC	RTNSAVER

SINESLOC	ADRES	SINCDU		# FOR USE IN SETTING ADDRWD

INDEXI		DEC	4		# **********   DON'T   **********
		DEC	2		# **********   TOUCH   **********
		DEC	0		# **********   THESE   **********
		DEC	4		# ********** CONSTANTS **********

# ****************************************************************************************************************
## Page 1372
# THIS SUBROUTINE COMPUTES INCREMENTAL CHANGES IN CDU(GIMBAL) ANGLES FROM INCREMENTAL CHANGES ABOUT SM AXES.  IT
# REQUIRES SM INCREMENTS AS A DP VECTOR SCALED AT ONE REVOLUTION(DTHETASM,+2,+4).  SIN,COS(CDUY,Z,X) ARE IN
# SINCDU,+2,+4 AND COSCDU,+2,+4 RESPECTIVELY, SCALED TO ONE HALF.  CDU INCREENTS ARE PLACED IN DCDU,+2,+4 SCALED TO
# ONE REVOLUTION.
#
#	*  COS(IGA)SEC(MGA)		0		-SIN(IGA)SEC(MGA) *
#	*								  *
#	* -COS(IGA)TAN(MGA)		1		 SIN(IGA)TAN(MGA) *
#	*								  *
#	*      SIN(IGA)			0		     COS(IGA)     *

		BANK	14
		SETLOC	POWFLIT1
		BANK
		
SMCDURES	DLOAD	DMP
			DTHETASM
			COSCDUY
			
		PDDL	DMP
			DTHETASM +4
			SINCDUY
			
		BDSU
		DDV
			COSCDUZ
		STORE	DCDU
		
		DMP	SL1		# SCALE
			SINCDUZ
		BDSU
		
			DTHETASM +2
		STODL	DCDU +2
			DTHETASM
			
		DMP	PDDL
			SINCDUY
			DTHETASM +4
			
		DMP	DAD
			COSCDUY
		SL1
		STORE	DCDU +4
		RVQ

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