PERSONAL DATA
Developed software and selected hardware that would be used in monitor and control of the Submillimeter Array(SMA) interferometer. Along with my duties as a software engineer and developer I was involved in making purchases for the group(ordering Workstations(WS), and other Central Processing Units (CPU) needed for VME hardware controllers and other hardware). My duties also involved designing and writing code for the TMS320C40 DSP chips which are part of the correlator board designed for real-time(RT) data collection. Other computers, software packages, and hardware were evaluated as to there use in the overall SMA interferometer project.
I also managed three(3) Sparc Workstations(two(2) Sparc10, one(1) IPX(with a uPower chip which I installed for better preformance), two(2) printers, two(2) DAT drives, one(1) CD-ROM, two(2) PC's, three(3) Motorola 680x0 boards.
Smithsonian Astrophysical Observatory(SAO)
Harvard-Smithsonian Center for Astrophysics(CfA)
Harvard-Smithsonian Center for Astrophysics(CfA)
National Radio Astronomy Observatory(NRAO)
Very Large Baseline Array(VLBA)
National Radio Astronomy Observatory(NRAO)
Very Large Baseline Array(VLBA)
National Radio Astronomy Observatory(NRAO)
Very Large Array(VLA)
Created and worked on existing user interfaces for monitor and control for hardware in a Real Time Environment(RTE). I conferred with personnel to resolve problems of intent, inaccuracy, feasibility, or computer processes. Review results of radio data with interested personnel. Developed new designs and analysis of software and hardware interactions still in use today.
I developed software to control one of the most critical, and arduous part of the VLBA(Very Long Baseline Array) correlator system, the 24 (one inch) Playback tape Drives(PBD). The 24 PBDs are connected to the 24 signal processing engines via a crossbar. The extra 4 PBDs enable tape staging; in full operation the average interval between tape changes are about 1/2 hour. A task was used to coordinate and synchronize crossbar reconfigurations; the design is intended to enable a tape task to switch from one PBD to the other without stopping and restarting. The operator were given windows and a various other ways of monitoring the progress. Some software was developed to manage the large amounts of data coming from the tape(PBDs) drives. Many of the software and hardware purchases were recommended by me for this project(VLBA correlator project). I continued to develop other packages after discussions with the engineering, and scientific staff.
Other projects were the Voyager-Neptune flyby, where many discussion sometimes lead by me and sometimes by others as to how the VLA(Very Large Array) in Socorro would be used in the project. I worked closely with NASA/Jet Propulsion Laboratory(JPL) operations staff to develop procedures and knowledge for efficient VLA/JPL operations and rapid diagnosis and correction of VLA failures. Working with others I enhanced reliability and minimized down time at the VLA and VLBA.
I worked with many operating systems which are mentioned on the cover, and had to meet many deadlines of which were imposed by me or management.
I also had to install and work with Data Base Systems(DBS) such as Ingres, and other DBSs. Worked extensively with AIPS in data reduction and analysis for calibration of the VLA and other instruments, as well as acquiring observations and using AIPS analysis package to study the spatial and temporal characteristics of macrospicules found on the solar surface. I also was and still involved in long term coordianted observations with other observatories to determine solar wind parameters, such as density, temperature, flow speeds and magnetic field strength, along a given solar stream.
National Radio Astronomy Observatory(NRAO)
Very Large Array(VLA)
Mainly to work and solve many of the known functions to be published in a text book "Elliptic Integrals of the third kind" by David Giri.
Science Applications
- THESIS -
Used a special complex variable procedure for the electromagnetic field
distribution of the TEM mode of a symmetrical two-parallel-plate transmission
line. Also investigated the right formula to obtain and produce a
parametric set of plots and tables for the appropriately normalized TEM field
components and magnitudes, as well as potentials.
Kirtland AFB