Search NASA⌕ Search

Engineering topics

Murphy, J. A.

Publications and source records attributed to Murphy, J. A..

8 records
All sourcesNASA NTRSDOE OSTI
DOE OSTI2022

QUBIC II: Spectral polarimetry with bolometric interferometry

Bolometric interferometry is a novel technique that has the ability to perform spectral imaging. A bolometric interferometer observes the sky in a wide frequency band and can reconstruct sky maps in several sub-bands within the physical band in post-processing of the data. This provides a powerful spectral method to discriminate between the cosmic microwave background (CMB) and astrophysical foregrounds. In this paper, the methodology is illustrated with examples based on the Q & U Bolometric Interferometer for Cosmology (QUBIC) which is a ground-based instrument designed to measure the B-mode polarization of the sky at millimeter wavelengths. We consider the specific cases of point source reconstruction and Galactic dust mapping and we characterize the point spread function as a function of frequency. We study the noise properties of spectral imaging, especially the correlations between sub-bands, using end-to-end simulations together with a fast noise simulator. Finally, we conclude showing that spectral imaging performance are nearly optimal up to five sub-bands in the case of QUBIC.

79 ASTRONOMY AND ASTROPHYSICS↗
NASA NTRS1986

Implications of the relationships between electromagnetic drift components at mid and low latitudes

A number of relationships between the meridional and longitudinal ion drifts at low and midlatitudes that are enforced by the condition of a curl-free electric field is derived. The application of these relationships to observations from the Jicamarca radar allow additional properties of the observations to be exposed. The results of including and excluding these properties in plasma distribution calculations are discussed. Some possible alternatives to an electrostatic potential model for the ion drifts, which allow extreme features to be included in the conditions of a curl-free electric field, are also discussed.

Murphy, J. A.↗
NASA NTRS1984

The influence of neutral winds on He(+) distributions in the equatorial ionospshere

The effects of F-region neutral winds on the distribution of He(+) in the equatorial ionosphere have been examined using a theoretical model and an observational data set. It is shown by the model that components of neutral wind in the magnetic meridian up to only 50 m/s can produce He(+) gradients in the northern and southern sectors of a flux tube that differ by more than 80 percent. This is associated with interhemisphere transport velocities of He(+) as large as 15 m/s at 800 km. A substantial latitude gradient in the He(+) distribution across the dip equator also results from the redistribution of He(+). The changes in the He(+) concentration at the dip equator and the latitude distribution of H(+) in response to different neutral wind components is determined from the model and used to construct longitude distributions of He(+) to compare with observations made at equinox. Good agreement between the calculations and observations is obtained both at the geographic and geomagnetic equators using the relationship between neutral winds, interhemispheric transport velocity and He(+) concentration derived from the model. If these relationships can be extrapolated to accommodate the different conditions expected during solstice, the He(+) distributions expected during this season can also be discussed.

Murphy, J. A.↗
NASA NTRS1982

Civil helicopter propulsion system reliability and engine monitoring technology assessments

A study to reduce operating costs of helicopters, particularly directed at the maintenance of the propulsion subsystem, is presented. The tasks of the study consisted of problem definition refinement, technology solutions, diagnostic system concepts, and emergency power augmentation. Quantifiable benefits (reduced fuel consumption, on-condition engine maintenance, extended drive system overhaul periods, and longer oil change intervals) would increase the initial cost by $43,000, but the benefit of $24.46 per hour would result in breakeven at 1758 hours. Other benefits not capable of being quantified but perhaps more important include improved aircraft avilability due to reduced maintenance time, potential for increased operating limits due to continuous automatic monitoring of gages, and less time and fuel required to make engine power checks. The most important improvement is the on-condition maintenance program, which will require the development of algorithms, equipment, and procedures compatible with all operating environments.

Murphy, J. A.↗
NASA NTRS1981

Light ion velocities in the polar ionosphere

High-speed flow of light ions along magnetic field lines is not simply a consequence of those field lines having an open topology. It is pointed out that the magnitude of the H(+) flow velocity in the polar wind is not predicted by theoretical models, but rather is imposed as a boundary condition. Thermal diffusion, the electron temperature profile, and a diverging magnetic field can be shown to have important effects on the H(+) flow velocity, which need not be supersonic even when the pressure at large distances from the earth is low.

Murphy, J. A.↗
NASA NTRS1981

Helicopter propulsion system reliability and engine monitoring assessments

The major short life, unreliable, and high maintenance engine and power components and subsystems in current civil helicopters were identified. Categories included both reciprocating and turbine engines, single and multiple engine configurations, single and tandem trotor vehicles, and light, medium, and heavy helicopters. The major focus was on the following parameters: accident rate data; maintenance rate data; and direct operator input.

Murphy, J. A.↗
NASA NTRS1981

A feature of the behavior of He/+/ in the nightside high-latitude ionosphere during equinox

Observations of a hole of ionization in the nightside high-latitude ionosphere during equinox in which He(+) plays an important role in the relative abundance of the ionic constituents are reported. Ion abundance data were obtained during a period of very low magnetic activity from the retarding potential analyzer and magnetic ion mass spectrometer on board AE-D as the satellite passed across the polar region near midnight. Significant decreases in O(+) and H(+) concentrations are observed in the region between 1544 and 1547 UT within the polar cap, accompanied by the rise and dominance of He(+) ions to low altitudes. The dominance of He(+) is attributed to effects on photoproduction of changes in solar zenith angle as the plasma moves from the dayside to the nightside, where it stagnates or resides for periods greater than about 3 hours just poleward of the auroral zone. Model calculations of the physical processes involved in this mechanism are presented which in general tend to fit the observations.

Heelis, R. A.↗