Lisa Huddleston, William Roeder, David Morabito, Larry D'Addario, Jennifer Morgan, Robert Barbré, Ryan Decker, Barry Geldzahler, Mark Seibert, Michael Miller
This paper provides an overview of ground based operational remote sensing activities that enable a broad range of missions at the Eastern Range (ER), which includes the National Aeronautics and Space Administration (NASA) Kennedy Space Center (KSC) and U.S. Air Force Cape Canaveral Air Force Station (CCAFS). Many types of sensors are in use by KSC and across the ER. We examine remote sensors for winds, lightning and electric fields, precipitation and storm hazards. These sensors provide data that are used in real-time to evaluate launch commit criteria during space launches, major ground processing operations in preparation for space launches, issuing weather warnings/watches/advisories to protect over 25,000 people and facilities worth over $20 billion, and routine weather forecasts. The data from these sensors are archived to focus NASA launch vehicle design studies, to develop forecast techniques, and for incident investigation. The wind sensors include the 50-MHz and 915-MHz Doppler Radar Wind Profilers (DRWP) and the Doppler capability of the weather surveillance radars. The atmospheric electricity sensors include lightning aloft detectors, cloud-to-ground lightning detectors, and surface electric field mills. The precipitation and storm hazards sensors include weather surveillance radars. Next, we discuss a new type of remote sensor that may lead to better tracking of near-Earth asteroids versus current capabilities. The Ka Band Objects Observation and Monitoring (KaBOOM) is a phased array of three 12 meter (m) antennas being built as a technology demonstration for a future radar system that could be used to track deep-space objects such as asteroids. Transmissions in the Ka band allow for wider bandwidth than at lower frequencies, but the signals are also far more susceptible to de-correlation from turbulence in the troposphere, as well as attenuation due to water vapor, which is plentiful in the Central Florida atmosphere. If successful, KaBOOM will have served as the pathfinder for a larger and more capable instrument that will enable tracking 15 m asteroids up to 72 million kilometers (km) away, about half the distance to the Sun and five times further than we can track today. Finally, we explore the use of Site Test Interferometers (STI) as atmospheric sensors. The STI antennas continually observe signals emitted by geostationary satellites and produce measurements of the phase difference between the received signals. STIs are usually located near existing or candidate antenna array sites to statistically characterize atmospheric phase delay fluctuation effects for the site. An STI measures the fluctuations in the difference of atmospheric delay from an extraterrestrial source to two or more points on the Earth. There is a three-element STI located at the KaBOOM site at KSC.
We report the implementation of a novel entanglement-enabled quantum state communication protocol, known as
SuperDense Teleportation, using photons hyperentangled in polarization and orbital angular momentum. We used these
techniques to transmit unimodular ququart states between distant parties with an averaged fidelity of 86.2±3%; almost
twice the classical limit of 44%. We also propose a method to use SuperDense Teleportation to communicate quantum
states from a space platform, such as the International Space Station, to a terrestrial optical telescope. We evaluate
several configurations and investigate the challenges arising from the movement of the space station with respect to the
ground.
With the successful completion of a field demonstration of uplink arraying at 8 GHz (X-band) using real-time
atmospheric compensation enabled by phase transfer rather than time transfer techniques- completion in mid-Aug 2010, NASA is interested in demonstrating a similar capability at 30-31 GHz (Ka band). Such a
demonstration would enable NASA to establish [a] a high power, high resolution, 24 / 7 availability radar system
for characterizing observations of Near Earth Objects, determining the statistics of small [≤10cm] orbital debris,
[ b ] to incorporate the capability into its space communication and navigation tracking stations for emergency
spacecraft commanding in the Ka band era which NASA is entering and [c] to field capabilities of interest to
other US government agencies. We describe a a project of Evolutionary Steps Leading to Revolutionary
Increases in Capability and Capacity
For several years, NASA has been pursuing demonstrations and development of coherent uplink arraying techniques for
the next generation space communications and planetary radar systems. In addition radio science experiments would
benefit with a 1000 times increase in signal to noise over current systems. I shall describe the three methods of uplink
arraying NASA has pursued, all successful, and share the vision for going forward from laboratory demonstrations to the
proposed implementation and deployment of a dedicated multi-purpose facility to infuse an amalgam of these methods
into a system that enhances NASA's missions.
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