Drew Smith - Instructor, School of Library and Information Science, University of South Florida, Tampa has accumulated 1020 points.
Points on this battle were won as follows:
First, convert mm to inches. Since you're scanning at 1200 * 1200 dpi,
multiply by 1200.
length: 35 mm * (1 in / 25.4 mm) * (1200 pixels / 1 inch) = 1654 pixels
width: (2 / 3) 35 mm * (1 in / 25.4 mm) * (1200 pixels / 1 inch) = 1103
pixels
Since it's in 24 bit color, each pixel takes 3 bytes of memory.
number of pixels = 1654 * 1103 = 1824362
1824362 * 3 = 5,473,086 bytes
The size of the picture when you print it at 300 dpi is the length and width
in pixels divided by 300 (or simply the original size multiplied by 4.)
length: 1654 pixels * (1 inch / 300 pixels) = 5.51 inches width: 1103 pixels
* (1 inch / 300 pixels) = 3.68 inches
The typical 35mm slide is actually 36mm by 24mm, or about 1.4in by 0.94in. At
1200 dpi scanning, this results in about 1700x1134 pixels. At 300 dpi
printing, this results in an image about 5.67in by 3.78in. The amount of hard
drive space taken up by such an image is 1700 times 1134 times 3 (3 bytes are
equivalent to 24 bits), or approximately 5.8 meg of space.
War VIII - battle 13
Points on this battle were won as follows:
War VIII - battle 12
Points on this battle were won as follows:
War VIII - battle 11
Points on this battle were won as follows:
War VIII - battle 10
Points on this battle were won as follows:
War VIII - battle 9
Points on this battle were won as follows:
War VIII - battle 8
Points on this battle were won as follows:
War VIII - battle 7
A$="SUPERCALIFRAGILISTICEXPEALIDOCIUS"
B$=SPACE$(40)
FOR Z=1 TO LEN(A$)
MID$(A$,Z,1)=CHR$(ASC(MID$(A$,Z,1))+ASC(MID$(B$,Z,1)))
NEXT
PRINT A$
Points on this battle were won as follows:
War VIII - battle 6
FOR Z=1 TO 10
A%(Z)=RND*1000+.5
NEXT
N=1
WHILE N>0
N=0
FOR Z=1 TO 9
IF A%(Z)<A%(Z+1) THEN SWAP A%(Z),A%(Z+1):N=N+1
NEXT
WEND
FOR Z=1 TO 10
PRINT A%(Z)
NEXT
Where the old Flotilla lay:
..................
Where the flyin'-fishes play,
An' the dawn comes up like thunder outer China 'crost the Bay!
Points on this battle were won as follows:
"THE HISTORY OF VELOCITY OF LIGHT" GALILEO In 1667, Galileo suggested a method for actually measuring the speed of light. The method was to take two people A and B, covered lanterns to the tops of hills that are separeted by a distance of about a mile. First A uncovers her latern. As soon as B sees A's light, she uncovers her own lantern. By measuring the time from when A uncovers her lantern until A sees B's light, then dividing this time by time by twice the distance between the hill tops, the speed of light can be determined. Galileo was able to determine only that the speed of light was far greater than could be measured using his procedure. Althougt Galileo was unable to provide even an approximate value for the speed of light, his experiment set the stage for later attempts. ROMER The first successfull measurement of the velocity of light was provided by the Danish astronomer Olaf Romer in 1675. He based in measurement on observations of the eclipses of one of the moons of Jupiter. As this moon orbits Jupiter, there is a period of time when Jupiter lies between it and the earth, and blocks it from view. Romer noticed that the duration of these eclipses was shorter when the Earth was moving toward Jupiter than when the Earth was moving away. He correctlly interpreted this phenomena as resulting form the finite speed of light. Geometrically the moon is always behind Jupiter for the same period of time drign each eclipse. Suppose, however, that the Earth is moving away from Jupiter. An astronomer on Earth catches his last glimpse of the moon, not at the instant the moon moves behind Jupiter, but only after the last bit of unblocked light form the moon reaches his eyes. There is a similar delay as the moon moves out form behind Jupiter but, since the Earth has moved father away, the light must now travel a longer distance to reach the astronomer. The astronomer, therefore sees an eclipse that ,lasts longer the actual geometrical eclipse. Similarly, when the Earth is moving toward Jupiter, the astronomer sees and eclipse that lasts a shorter interval of time. From observations of these eclipses over many years, Romer calculated the speed of light to be 2.1*10^8 m/sec. This value is approximately 1/3 too slow due to inaccurate knowledge at at that time of the distances involved. Nevertheless, Romer's method provided clear evidence that the velocity of light was not infinite, and gave a reasonable estimate of its true value-not bad for 1675. FIZEAU The French scientist Fizeau, in 1849, developed an ingenious mehod for measuring the speed of light over terrestrial distances. He used a rapidly revolving cogwheel in front of a light source to deliver the light to a distant mirror in discrete pulses. The mirror reflected these pulses back toward the cogwheel. Depending on the position of the cogwheel a pulse returned, it would either block the pulse of light or pass it through to an observer. He measured the rates of cogwheel rotation that allowed observation of the returning pulses for carefully measured distance between the cogwheel and the mirror. Using the method, Fizeau measurd the speed of light to be 3.15*10^8 m/sec. This is within a few percent of the currently accepted value. FOUCALT Foucalt improved Fizeau's method, using a rotating mirror instead of a rotating cogwheel. Micelson used Foulcalt's method to produce some accurate measurements of the velocity of light. The best of these measurements gave a velocity of 2.99774*10^8 m/sec. This may be compared to the presently accepted value of 2.99792458*10^8 m/sec.also see: http://www.phys.virginia.edu/classes/109N/lectures/spedlite.html
Where the old Flotilla lay: O[n] the road to Mandalay Where the flyin'-fishes play, An' the dawn comes up like thunder outer China 'crost the Bay!by Rudyard Kipling (1865-1936)
War VIII - battle 5
Points on this battle were won as follows:
AT - gets the modems attention. Tells it commands follow. &F - recalls the factory default settings L3 - Selects high speaker volume E1 - Enables the command echo V1 - Selects result codes in WORD format (e.g., modem returns "OK" instead of "0") &C1 - DCD(Data Carrier Detect) will track the state of the data carrier from the remote modem &D2 - controls the modem response to the serial port's Data Terminal Ready (DTR) X4 - Extended Result Code. With the 4, if dial tone is not detected within 5 seconds, NO DIALTONE result code is returned. If a busy signal is detected, BUSY result code is returned. The modem returns CONNECT XXXX result code reflecting the serial port speed when a connection is established.See http://www.modems.com/general/extendat.html
War VIII - battle 4
Points on this battle were won as follows:
War VIII - battle 3
Points on this battle were won as follows:
War VIII - battle 2
21AA:0100 B409 MOV AH,09 ;display string of characters 21AA:0102 BA1701 MOV DX,0117 ;point to string 21AA:0105 CD21 INT 21 ;do it 21AA:0107 B401 MOV AH,01 ;keyboard input function 21AA:0109 CD21 INT 21 ;do it 21AA:010B B44C MOV AH,4C ;exit function 21AA:010D 2C30 SUB AL,30 ;convert to number 21AA:010F 7EF6 JLE 0107 ;jump to 107 if < "1" 21AA:0111 3C09 CMP AL,09 ;compare to "9" 21AA:0113 7FF2 JG 0107 ;jump to 107 if greater 21AA:0115 CD21 INT 21 ;do exit
A law was made a distant moon ago here July and August cannot be too hot And there's a legal limit to the snow here The winter is forbidden till December And exits March the second on the dot By order summer lingers through September The rain may never fall till after sundown By eight the morning fog must disappear The snow may never slush upon the hillside By nine PM the moonlight must appear
Points on this battle were won as follows:
War VIII - battle 1
Points on this battle were won as follows:
Last revised November 18, 2000.
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