'230 ghz' presentation slideshows

Start by initializing a particle in the left well and see if it can flow to the right well.

We would like to use the concepts of eigenstates to think about transport through a device, like a FET. Assume that the 3 wells are a very simple model for a FET. If we can determine I1 and I2, we know the current flow through the devices.

708 views • 61 slides

Case Western Reserve University May 19, 2009

Case Western Reserve University May 19, 2009. Imaging Black Holes. Testing theory of gas accretion: disks, jets Testing General Relativity: strong field gravity. Avi Loeb Institute for Theory & Computation Harvard University.

507 views • 36 slides

322 views • 29 slides

SMA Observations of Sgr A*

SMA Observations of Sgr A*. Dan P. Marrone, Ram Rao, Jim Moran, Jun-Hui Zhao Harvard-Smithsonian Center for Astrophysics. Sgr A * at 337 GHz 2004 May 25. Outline. Introduction to Sgr A*, submm perspective SMA Capabilities Observations of Sgr A* 2004: Polarimetry at 880 ? m ( 340 GHz)

290 views • 20 slides

SMA Observations of Sgr A*

SMA Observations of Sgr A*. Dan P. Marrone, Ram Rao, Jim Moran, Jun-Hui Zhao Harvard-Smithsonian Center for Astrophysics. Sgr A * at 337 GHz 2004 May 25. Outline. Introduction to Sgr A*, submm perspective SMA Capabilities Observations of Sgr A* 2004: Polarimetry at 880 ? m ( 340 GHz)

204 views • 20 slides

Prospects for High-Frequency Calibration with the SMA Dual-IF/Receiver System

298 views • 17 slides

Prospects for High-Frequency Calibration with the SMA Dual-IF/Receiver System

181 views • 17 slides

Strumentazione sub-mm/mm pre-ALMA

Strumentazione sub-mm/mm pre-ALMA. APEX SCUBA & SCUBA-2 IRAM SMA CSO OVRO, BIMA ? CARMA NMA. APEX : A tacama P athfinder EX periment. Location: Llano de Chajnantor (Chile, 5000 m) Antenna modified copy of US ALMA prototype MPIfR=50% Onsala Sp. Obs=23% ESO=27%

332 views • 16 slides