Ongoing

History of Antenna and Associated Engineering Technology at the Arecibo Observatory, Arecibo, Puerto Rico

Room: Room 101, Morrison Gallery, Bldg: Madlyn L Hanes Library (Building D), Penn State Harrisburg, 777 West Harrisburg Pike, Middletown, Pennsylvania, United States, 17507

The Arecibo Observatory first opened in 1963, has been named an IEEE Milestone in Electrical Engineering and Computing in 2001, and has been a marvel in engineering ever since. It has been a monumental instrument for scientific research in the fields of astronomy, planetary radar, ionospheric probing and HF heating modification, and optical probing of the atmosphere. While the science and the discoveries are well known to many, the antenna technology and engineering are equally as impressive as the discoveries. The original concept, by Prof. William Gordon in the Electrical Engineering Department at Cornell University, was for a 1000 foot parabolic dish aiming only at zenith, with no tracking capability for studies of the ionosphere with the newly developed technique of incoherent scatter radar (ISR). Fortunately, knowledge of some on-going research with spherical reflectors was suggested where the feed could be moved to slew the beam. This talk will discuss the unique designs over the years of antenna feeds and associated engineering for frequencies from HF well into the microwaves. Many upgrades occurred during these years and will be described in detail in the ways they have provided significant improvements to the Observatory’s capabilities. Most of the 430 MHz 96 foot line feed antenna broke off and fell through the dish in 2017 during Hurricane Maria. Then in December 2020, the platform fell into the dish destroying large sections of the dish and the equipment in the platform. There is so much more to tell about the engineering at Arecibo that will be the subject of this presentation. Dinner will consist of: - Chicken Bruschetta - Garden Salad - Roasted Garlic Mashed Potatoes - Honey Roasted Carrots - Assorted Dinner Rolls - Brownies Parking for the event is free and is in the parking lot south of the library. See the below map of the PSU Harrisburg for an overview on where the building and parking is located. There is a fee for the entire dinner+presentation event. There is no fee for only attending the presentation. Speaker(s): Jim Breakall, Agenda: Dinner: 6:00 - 7:00 PM Presentation: 7:00 - 8:30 PM Room: Room 101, Morrison Gallery, Bldg: Madlyn L Hanes Library (Building D), Penn State Harrisburg, 777 West Harrisburg Pike, Middletown, Pennsylvania, United States, 17507

Robotics and Artificial Intelligence

Pittsburgh 2201 Pennsylvania Furnace Rd, Pennsylvania Furnace

Legislation affecting Robotics and AI and how it impacts engineers working the field Speaker(s): Russ Harrison, Pittsburgh, Pennsylvania, United States

Radiation Resistant Graphene-based photovoltaics for lunar surface applications

Room: 334, Bldg: Loyola Science Center (LSC), 204 Monroe Ave, Physics and Engineering Dept, University of Scranton, Scranton, Pennsylvania, United States, 18510

Radiation resistant photovoltaics (PV) for lunar surface applications has been increasingly important for application on the lunar surface. Graphene-based Schottky diodes with semiconductor various radiation resistant layers is a promising choice for lunar PV due to (i) graphene high photon transparency (ii) and radiation resistant semiconducting layers such as GaN. We propose a G/n-GaN Schottky diode where the metal is replaced by graphene grown on top of a thin oxide layer resting on the semiconductor. Photoexcitation of carriers occurs in both graphene and the semiconductor regions. the oxide layer prevents or reduces recombination of photo-carriers. we propose a model where photo-generated electrons cross the PV device in both directions (from Gr to the semiconductor and vice versa) via two mechanisms by (a) thermionic emission and (b) quantum tunneling. We outline the method of obtaining net current densities (thermionic and tunneling). Tunneling transmission and thermionic carrier escape and current are outlined along with the advantage of high current density generation in the harsh lunar surface environment. Co-sponsored by: EDS Student Branch, Physics & Engineering Dept, University of Scranton Speaker(s): Argyrios Agenda: Professional meeting at the University of Scranton Room: 334, Bldg: Loyola Science Center (LSC), 204 Monroe Ave, Physics and Engineering Dept, University of Scranton, Scranton, Pennsylvania, United States, 18510