Rowswap(), Rplcpic, Rref() – Texas Instruments TITANIUM TI-89 User Manual

Page 867: Sec()

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Appendix A: Functions and Instructions

867

rowSwap()

MATH/Matrix/Row ops menu

rowSwap(

matrix1

,

rIndex1

,

rIndex2

)

matrix

Returns

matrix1

with rows

rIndex1

and

rIndex2

exchanged.

[1,2;3,4;5,6]! Mat

¸

1 2

3 4

5 6

rowSwap(Mat,1,3)

¸

5 6

3 4

1 2

RplcPic

CATALOG

RplcPic

picVar

[,

row

][,

column

]

Clears the Graph screen and places picture

picVar

at pixel coordinates (

row

,

column

). If you do not

want to clear the screen, use

RclPic

.

picVar

must be a picture data type variable.

row

and

column

, if included, specify the pixel

coordinates of the upper left corner of the picture.
Default coordinates are (0, 0).

Note: For less than full-screen pictures, only the
area affected by the new picture is cleared.

rref()

MATH/Matrix menu

rref(

matrix1

[,

tol

])

matrix

Returns the reduced row echelon form of

matrix1

.

rref([л2,л2,0,л6;1,л1,9,л9;
л

5,2,4,л4])

¸

1 0 0 66/71

0 1 0

147

71

0 0 1 л 62/71

Optionally, any matrix element is treated as zero
if its absolute value is less than

tol

. This tolerance

is used only if the matrix has floating-point
entries and does not contain any symbolic
variables that have not been assigned a value.
Otherwise,

tol

is ignored.

If you use ¥ ¸ or set the mode to

Exact/Approx=APPROXIMATE

, computations

are done using floating-point arithmetic.

If

tol

is omitted or not used, the default

tolerance is calculated as:

5

E

л 14 щ max(dim(

matrix1

))

ù rowNorm(

matrix1

)

Note: See also

ref()

.

rref([a,b,x;c,d,y])

¸

1 0

dø x-bø y
aø d-bø c

0 1

ë

(cø x-aø y)

aø d-bø c

sec()

MATH/Trig menu

sec(

expression1

)

expression

sec(

list1

)

list

Returns the secant of

expression1

or returns a list

containing the secants of all elements in

list1

.

Note: The result is returned as a degree, gradian
or radian angle, according to the current angle
mode setting.

In Degree angle mode:

sec(45) ¸

(2)

sec({1,2.3,4}) ¸

{

1

cos(1)

1.000…

1

cos(4)}

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