Pulsar quadrant: Difference between revisions

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|position    = center
|position    = center
|viewerconfig = #C [[ GPS 4 THUMBSIZE 2 ]]
|viewerconfig = #C [[ GPS 4 THUMBSIZE 2 ]]
|apgcode = xp228_178cyfc871xggozwg8g0717y9g8g04461ik871zw1210sgsy9121y13zgs26yf62sg
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Revision as of 02:48, 25 June 2024

Pulsar quadrant
5bo2b$3b3o2b$2bo3b2o$o2bo2bob$o3bobob$o4bo2b2$2b3o! #C [[ THUMBSIZE 2 THEME 6 GRID GRIDMAJOR 0 SUPPRESS THUMBLAUNCH ]] #C [[ AUTOSTART ]] #C [[ THUMBSIZE 2 GPS 2 ]]
Pattern type Oscillator
Number of cells 18
Bounding box 9 × 9
Period 3 (mod: 3)
Heat 8
Volatility 0.46 | 0.46
Kinetic symmetry Unspecified
Rotor type Pulsar
Discovered by David Buckingham
Year of discovery 1973

Pulsar quadrant (or pulse) is a period-3 oscillator that was found by David Buckingham in July 1973.[1] It consists of a quarter of the outer part of a pulsar stabilized by a cis-fuse with two tails.

Commonness

Information on this oscillator's commonness with respect to other naturally-occurring patterns is currently unknown.

LCM oscillators

The smallest known oscillator of period 228 is an LCM oscillator comprised of a pulsar quadrant and a p76 pi-heptomino shuttle.

x = 35, y = 20, rule = B3/S23 8b2o23b2o$9bo23bo$9bobo19bobo$2bo7b2o19b2o$2b3o$2o3bo9bo$bo2bobo7b3o$b obo2b3o5bo2bo$2bo8bo19bo$3b2o5bobo17bobo$4bo5bobo17bobo$4bo6bo19bo$14b o2bo$14b3o$15bo2$10b2o19b2o$9bobo19bobo$9bo23bo$8b2o23b2o! #C [[ THUMBSIZE 2 THEME 6 GRID GRIDMAJOR 0 SUPPRESS THUMBLAUNCH ]] #C [[ GPS 4 THUMBSIZE 2 ]]
(click above to open LifeViewer)
Catagolue: here

See also

References

  1. ↑ Dean Hickerson's oscillator stamp collection. Retrieved on March 14, 2020.