For improving the UCO qualities, first it was improved the kernel fabrication processes and carbon dispersion method also. In this study, it was evaluated from the reviews on the UO2 and UCO kernel fabrication technologies and its particle characteristics. Furthermore, because the NGNP program have a highly focused goal like UCO kernel, kernel fabrication and coating types varied which made selection of a US reference fabrication process. NGNP program for high specification of HTGR nuclear fuel through the GEN IV study is be progressed. International Nuclear Information System (INIS) NMR and NQR studies of 5f-band metamagnetic UCoAl and UCo with the c-axis parallel to H, which reflects the anisotropy of the spin fluctuations of the system.Īdvanced Fuel UCO Preparation Technology for HTGR (Characteristics of Carbon Black) This system can provide automatic sky level measurement and subtraction to accommodate dynamically changing background levels. On- chip pixel binning and MPP operation are also selectable options. Three different read out speeds allow the astronomer to select between high-speed/high-noise and low-speed/low-noise operation. High speed pixel skipping in both horizontal and vertical directions allows us to quickly access a selected subarea of the detector. Integration times can be varied over a range of 0.1 to 1000 seconds. A thermoelectric device is used to cool the CCD to about -45c. A stand-alone display subsystem is also available. Though fully computer controllable, the camera can be operated as a stand-alone unit with most operating parameters set locally. Various types of CCDs can be used in this system without major modification of the hardware or software. To achieve the desired level of operating flexibility, the design incorporates state-of-the-art technologies such as high density, high speed programmable logic devices and non-volatile static memory. The camera will improve our remote-observing capabilities since it will be easy to control the camera and obtain images over the Observatory computer network. Our goal is a camera which is fully computer controllable, compact in size, versatile enough to provide a wide variety of image acquisition modes, and able to operate with a wide variety of CCD detectors. New design for the UCO/Lick Observatory CCD guide cameraĪ new CCD based field acquisition and telescope guiding camera is being designed and built at UCO/Lick Observatory.
#Prepo id grindr software#
The complete data acquisition software for the Lick CCD camera is running on a variety of PC style computers as well as an HP laptop.
#Prepo id grindr driver#
The necessary device driver software has been written for the Linux operating system which is now widely used at Lick Observatory. No hardware modifications or additions to the computer are needed. Since most computers now support USB 2.0 the Lick interface makes it possible to use the camera on essentially any modern computer that has the supporting software.
#Prepo id grindr serial#
A single USB cable connects to the image acquisition computer and the camera's RS232 serial and fiber optic cables plug into the USB interface.
We present here a simple USB 2.0 interface for the UCO/Lick camera. The fiber optic cable requires either a custom interface board that is plugged into the mainboard of the image acquisition computer to accept the fiber directly or an interface converter that translates the fiber data onto a widely used standard interface. Increasingly RS232 is a legacy interface supported on fewer computers. The new UCO/Lick Observatory CCD camera uses a 200 MHz fiber optic cable to transmit image data and an RS232 serial line for low speed bidirectional command and control. A USB 2.0 computer interface for the UCO/Lick CCD cameras