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Beauty in the Sky Lantern

Beauty in the Sky Lantern

Most of the people look at the sky at night because of the wonderful scenery like numbers of stars forming figure and the moon the gives bright

By winniekun
(113 views)

Some BM@N results vs detector strip pitch

Some BM@N results vs detector strip pitch

Some BM@N results vs detector strip pitch. A.Zinchenko, V.Vasendina VBLHEP, JINR, Dubna, Russia. Detector configuration: detector station position along Z. A.Zinchenko. 2. Single Λ. A.Zinchenko. 3. True Λ in minimum bias events. A.Zinchenko. 4.

By rolf
(92 views)

Direction-detection spectrometer concepts the CCAT

Direction-detection spectrometer concepts the CCAT

Direction-detection spectrometer concepts the CCAT. Matt Bradford + others 24 October 2006, in progress. 850 micron counts (stolen from A. Benson talk). Recall: modified IMF and star formation timescale included to reproduce 850 micron counts.

By diamond
(93 views)

PHENIX Status

PHENIX Status

PHENIX Status. Time Meeting, 2/2/2010 Stefan Bathe. Sampled Integrated Luminosity. 0.375 / 1.4 ( nb ^-1) = 26 % of goal (for sampled int. lumi .). 23/70 (days) = 33 % of time. DAQ Performance.  if rate had been > 5 kHz at all times:

By archer
(123 views)

Paper Tower

Paper Tower

Paper Tower. 8 th Grade Physical Science August 30, 2013. Definition of Tower. tow·er ˈ tou (ə)r/ noun a tall narrow building, either freestanding or forming part of a building such as a church or castle. Famous Towers. Famous Towers. Tools. 8 ½” x 11” (21.5 cm x 28 cm) paper

By huey
(188 views)

SMT Assembly & Rates, Take 2 (or 3?)

SMT Assembly & Rates, Take 2 (or 3?)

SMT Assembly & Rates, Take 2 (or 3?). Changes Limited tents to Barrels 1&6, layers 1&3 (of 4) Used Yuri’s tent numbers in addition to nominal tolerance Calculated for s z = 22 cm as well as s z = 30 cm Will show pass rate for nominal tolerance efficiency at fixed rate (nominal)

By emery
(55 views)

Warm up

Warm up

Warm up. Find the area of the irregular figure below. 69 cm 720 cm 2 900 cm 2 1080 cm 2. 15 cm. 30 cm. 24 cm. Problem Solving: Sample for Analysis.

By makani
(58 views)

Ex. 26.2 A concave mirror has a 30 cm radius of curvature.

Ex. 26.2 A concave mirror has a 30 cm radius of curvature.

Ex. 26.2 A concave mirror has a 30 cm radius of curvature. If an object is placed 10 cm from the mirror, where will the image be found?. Case 5: p < f. f = R/2 = 15 cm, p = 10 cm 1/p + 1/q = 1/f  1/10 + 1/q = 1/15 3/30 + 1/q = 2/30 1/q = -1/30 q = -30 cm. q < 0. Real or Virtual

By jara
(120 views)

Ex. 26.2 A concave mirror has a 30 cm radius of curvature.

Ex. 26.2 A concave mirror has a 30 cm radius of curvature.

Ex. 26.2 A concave mirror has a 30 cm radius of curvature. If an object is placed 10 cm from the mirror, where will the image be found?. Case 5: p < f. f = R/2 = 15 cm, p = 10 cm 1/p + 1/q = 1/f  1/10 + 1/q = 1/15 3/30 + 1/q = 2/30 1/q = -1/30 q = -30 cm. q < 0. Real or Virtual

By umed
(123 views)

THE PANORAMIC RADIOGRAPH

THE PANORAMIC RADIOGRAPH

THE PANORAMIC RADIOGRAPH. The panoramic technique is used to show a continuous view of the lower half of the face. This includes the teeth, jaws and some soft tissue anatomy. ADVANTAGES & DISADVANTAGES OF THE PANORAMIC RADIOGRAPH. The principal advantages of the panoramic radiograph are:

By celina
(386 views)

The Pre-Sidedress Nitrate Test PSNT

The Pre-Sidedress Nitrate Test PSNT

The Pre-Sidedress Nitrate Test PSNT. Fred Magdoff Plant & Soil Science University of Vermont fmagdoff@uvm.edu. The Nitrogen Challenge. Needed in large amounts A very dynamic nutrient.

By mei
(97 views)

Yang Yang Underground Lab in Korea (Y2L)

Yang Yang Underground Lab in Korea (Y2L)

Yang Yang Underground Lab in Korea (Y2L). Li Jin IHEP/ Tsinghua Beijing , China. OCPA 2008 , HongKong. Outline. Yang Yang Underground Lab Detector for dark matter search Physics results Other issues in Y2L Summary.

By scott
(373 views)

AP Physics IV.B

AP Physics IV.B

AP Physics IV.B. Physical Optics. 27.1 Linear Superposition. 27.2 Young’s Double Slit Experiment and Wave Properties of light. First, what is diffraction of light?. Bright and dark fringes. Position of the fringes. “Order in the fringe!”. Intensity of the fringes.

By landis
(137 views)

778.534709 HAR

778.534709 HAR

778.534709 HAR A century of model animation : from m‚liŠs to aardman/ by Ray Harryhausen and Tony Dalton. London: Aurum Press Ltd., Y 2008. 240p. ; bib., ind. : 29 cm x 25 cm ISBN : 978-1-84513-567-2 Price : Rs. 1995.00

By eliot
(123 views)

L.U.N.A.R. Eggs-Prize Landing Unique Navigable Astronaut-Controlled Rovers

L.U.N.A.R. Eggs-Prize Landing Unique Navigable Astronaut-Controlled Rovers

L.U.N.A.R. Eggs-Prize Landing Unique Navigable Astronaut-Controlled Rovers. AMY BARTLETT NASA MESSENGER FELLOW RAYMOND S. KELLIS H.S. MARE GILMORE, M.Ed. LIED CHILDREN’S MUSEUM. Payload Protection. Payload = anything in the spacecraft Astronauts Food Medical equipment

By mac
(111 views)

659.1 SAN Life in a rectangle/ by Sujit Sanyal. New Delhi: Fingerprint, Y 2012.

659.1 SAN Life in a rectangle/ by Sujit Sanyal. New Delhi: Fingerprint, Y 2012.

659.1 SAN Life in a rectangle/ by Sujit Sanyal. New Delhi: Fingerprint, Y 2012. 260p. ; 19 cm x 13 cm ISBN : 978-81-7234-398-9 Price : Rs. 395.00 Keywords: advertising; agency Acc. No : 11251

By ray
(90 views)

M. S. Tillack

M. S. Tillack

Final Optic Research – Progress and Plans. M. S. Tillack. with contributions from :. Z. Dragojlovic, F. Hegeler, E. Hsieh, J. Mar, F. Najmabadi, J. Pulsifer, K. Sequoia, M. Wolford. HAPL Project Meeting, PPPL 27-28 October 2004. Overview. Final optic program summary

By shino
(91 views)

X-ray Interferometer Mirror Module ISAL Study

X-ray Interferometer Mirror Module ISAL Study

X-ray Interferometer Mirror Module ISAL Study. Pre-work Overview. Science Team. Webster Cash - University of Colorado 303-492-4056 Ann Shipley - University of Colorado 303-492-1875 Keith Gendreau - NASA/GSFC Code 662 6-6188. Science Driver for MAXIM.

By ronni
(107 views)

 Basic concept with wide aperture NbTi quadrupoles.

 Basic concept with wide aperture NbTi quadrupoles.

Optics limitations and solutions for the Phase-I LHC IR upgrade Project S. Fartoukh BE-AP with contributions from B. Holzer, E. Laface, J. Miles, F. Schmidt, R. Tomas.  Basic concept with wide aperture NbTi quadrupoles.  Optics & Performance limitations … a simplified overview

By tarala
(123 views)

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