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Ionosphere Delay Calibration and Calibration Errors for Satellite Navigation of Aircraft
The Federal Aviation Administration (FAA) is implementing a satellite-based navigation system for aircraft using the Global Positioning System (GPS).
LISA laser noise cancellation test using time-delayed interferometry
We describe a laboratory test of TDI with an unequal arm interferometer. The intent is to ascertain the performance limitations and proof-of-concept for 6 orders of magnitude frequency noise suppression.
Comparison of atmospheric delay statistics from Deep Space Network arrays and nearby site test interferometers
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BPv6 and BPv7 Coexistence in Delay Tolerant Networking (DTN)
As DTN has progressed since its inception in 2002, the community stabilized around Bundle Protocol version 6 (BPv6). This protocol was standardized by the RFC 5050’s definition of BPv6 and was later standardized and refined for space operations by the CCSDS Bundle Protocol Specification. After the release of RFC 5050, a variety of implementations and missions used BPv6 and noted several improvements that could be made to the protocol. These improvements culminated in a push to release a new protocol version, BPv7. Unfortunately, the vast improvements and difference in encoding that separates BPv7 from BPv6 also makes the two versions inherently incompatible. Consequently, there is an issue implementing BPv7 in existing systems while continuing support for BPv6 implementations. In response to this issue, two solutions emerge: (1) Bundle-in-Bundle Encapsulation (BIBE), a capability that wraps a bundle in another bundle for shipping between intermediary nodes, and (2) version agnostic DTN implementations. These concepts have been proven out in the MSFC DTN implementation known as DTNME.
Relativistic Shapiro Delay Measurements of an Extremely Massive Millisecond Pulsar
Despite its importance to our understanding of physics at supranuclear densities, the equation of state (EoS) of matter deep within neutron stars remains poorly understood. Millisecond pulsars (MSPs) are among the most useful astrophysical objects in the Universe for testing fundamental physics, and place some of the most stringent constraints on this high-density EoS. Pulsar timing—the process of accounting for every rotation of a pulsar over long time periods—can precisely measure a wide variety of physical phenomena, including those that allow the measurement of the masses of the components of a pulsar binary system1. One of these, called relativistic Shapiro delay2, can yield precise masses for both an MSP and its companion; however, it is only easily observed in a small subset of high-precision, highly inclined (nearly edge-on) binary pulsar systems. By combining data from the North American Nanohertz Observatory for Gravitational Waves (NANOGrav) 12.5-yr data set with recent orbitalphase- specific observations using the Green Bank Telescope, we have measured the mass of the MSP J0740+6620 to be 2.14+0:10-0:09 M⊙ (68.3% credibility interval; the 95.4% credibility interval is 2.14+0:20-0:18 M⊙). It is highly likely to be the most massive neutron star yet observed, and serves as a strong constraint on the neutron star interior EoS.
Alleviating Bundle Throughput Constriction for Delay Tolerant Networking (DTN) Bundles with Software Defined Networking (SDN)
Networks are expanding and becoming more complex. Therefore, they are also increasing bundle packet throughput within the system. IF DTN nodes are constricted in packet throughput, how would the system act? Would it just drop the packet without a flag? What happens IF all DTN node’s send at their limits to the ISS DTN node?
A Zero-order Hold Approach for Fractional-delay Interpolation in Auralization
During the signal processing chain of an auralization simulating the propagation of a sound from a moving source to a stationary receiver, it is often necessary to interpolate between the samples of the source signal in order to arrive at uniformly-spaced samples at the receiver. In some cases, this interpolation is done in the receiver time frame – where the “input” samples of the source have become irregularly spaced due to time dilation effects. Canonical band-limited interpolation methods (i.e., sinc and sinc-derived approaches) cannot be applied in this case as they rely on having a uniformly-spaced input. The use of geometric interpolation methods that can handle irregularly-spaced input may not be grounded in signal processing principles and may produce unwanted artifacts and noise. This presentation outlines the possibility of embedding an irregularly-spaced zero-order hold signal within a highly over-sampled uniformly-spaced signal, and then processing down to the desired sampling rate through successive decimations. Initial distortion and noise characteristics of the approach are shown for some basic propagation geometries. The possible benefits of using such an approach in an auralization scheme with a time-varying Doppler shift are discussed including: the prevention of aliasing, processing time advantages, and the possibility for asynchronous processing.