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Search indexed NASA NTRS and DOE OSTI research on propulsion, heat transfer, battery materials and energy systems. Follow report and document links to the original sources.

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At least 649 records · Page 36
All sourcesNASA NTRSDOE OSTI
DOE OSTI2025

Origin of Pulsed Radio Emission from Magnetars

Extended periods of radio pulsations have been observed for six magnetars, displaying characteristics different from those of ordinary pulsars. In this Letter, we argue that radio emission is generated in a closed, twisted magnetic flux bundle originating near the magnetic pole and extending beyond 100 km from the magnetar. The electron–positron flow in the twisted bundle has to carry electric current and, at the same time, experiences a strong drag from the radiation field of the magnetar. This combination forces the plasma into a “radiatively locked” state with a sustained two-stream instability, generating radio emission. We demonstrate this mechanism using novel first-principles simulations that follow the plasma behavior by solving the relativistic Vlasov equation with the discontinuous Galerkin method. First, using one-dimensional simulations, we demonstrate how radiative drag induces the two-stream instability, sustaining turbulent electric fields. When extended to two dimensions, the system produces electromagnetic waves, including superluminal modes capable of escaping the magnetosphere. We measure their frequency and emitted power and incorporate the local simulation results into a global magnetospheric model. The model explains key features of the observed radio emission from magnetars: its appearance after an X-ray outburst, wide pulse profiles, luminosities ∼10 30 erg s −1 , and a broad range of frequencies extending up to ∼100 GHz.

Astronomical simulations↗
NASA NTRS1969

Dynamical models of novae.

Nova outburst dynamics investigation by time dependent hydrodynamics computer program including energy transport by radiation and convection

Sparks, W. M.↗
NASA NTRS1971

The appearance of the Gum nebula

The dimensions of the Gum nebula complex appear to be overestimated. The distance of 460 parsecs to the central pulsar is rather on the large side, and likely contributions from gamma Velorum and zeta Puppis were underestimated. The multiorigin character of the Gum nebula is reaffirmed. The parts produced by traditional ultraviolet thermal radiation and by processes directly related to the supernova outburst must be defined.

Bok, B. J.↗
NASA NTRS1972

Ultraviolet photometry of Nova Serpentis 1970

The appearance of the bright nova, Nova Serpentis 1970, provided the first opportunity to obtain spectrophotometric observations of a nova in the vacuum ultraviolet. OAO-2 carried out systematic measurements from shortly after outburst on through the first sixty days of nova activity. This data consist of filter photometry and spectral scans. General characteristics of the light and spectral variations in the ultraviolet exhibited by this set of data are described.

Code, A. D.↗
NASA NTRS1972

Jupiter - Its Red Spot and disturbances in 1970-1971.

Photographic observations of Jupiter and its Red Spot between Dec. 11, 1970, and Oct. 12, 1971, are reported. The Red Spot had a mean rotation period of 9 hr 55 min 38.5 sec, the shortest to be observed since the apparition of 1931-1932. The outstanding event of the apparition was an outburst of activity in the South Equatorial Belt which was similar in many ways to the great disturbance of 1928.

Reese, E. J.↗
NASA NTRS1973

Cas A X-ray spectrum: Evidence for iron line emission

A sensitive measurement by rocket borne detectors of the X-ray flux from Cas A has revealed a steep continuum and a broad spectral feature in the region where line radiation from iron nuclei would be expected. The flux in this feature is .0122 plus or minus .0017 photons/sq cm/s: the total energy flux from 2 to 10 KeV is 1.02 x 10 to the minus 9th power ergs/sq cm/s. The presence of broad iron lines is consistent with a model in which approximately 13 MeV/nucleon iron nuclei charge exchange with surrounding interstellar oxygen and other heavy atoms. The model suggests that a substantial fraction of the energy from the outburst has gone into low energy cosmic rays which produce the observed HII region surrounding the remnant.

Serlemitsos, P. J.↗
NASA NTRS1973

X-ray spectrum of Cassiopeia A - Evidence for iron line emission.

A sensitive measurement by rocket-borne detectors of the X-ray flux from Cas A has revealed a steep continuum and a broad spectral feature in the region where line radiation from iron nuclei would be expected. The flux in this feature is 0.0122 plus or minus 0.0017 photons per sq cm per sec. The presence of broad iron lines is consistent with a model in which about 13 MeV-per-nucleon iron nuclei charge exchange with surrounding interstellar oxygen and other heavy atoms. The model suggests that a substantial fraction of the energy from the outburst has gone into low-energy cosmic rays which produce the observed H II region surrounding the remnant.

Serlemitsos, P. J.↗
NASA NTRS1973

Are the recently observed soft gamma-ray bursts from stellar superflares.

The gamma-ray bursts reported by Klebesadel et al. (1973) are considered. It is suggested that these outbursts are simply giant versions of the X-ray bursts typically seen in solar flares. The time scale, mean photon energy, and energy spectrum shape for both the solar and nonsolar bursts are found to be strikingly similar. However, the nonsolar bursts that have been observed have a much greater intrinsic intensity than their solar counterparts.

Stecker, F. W.↗
NASA NTRS1973

On the non-spherical structure of the nova nebulosity

The observed nonspherical structure of the material ejected during a nova outburst is explained by considering a component of the cataclysmic binaries ignored in previous theories - the ring of material which lies in the equatorial plane and surrounds the white dwarf. When the expanding shell collides with the ring, a shock is formed which heats the material in the ring and in the portion of the shell striking the ring. There is enough energy and density in the expanding shell for it to sweep the ring along, but with a final velocity somewhat lower than the shell moving perpendicular to the ring. The result is a prolate ellipsoid with the long axis perpendicular to the plane of the binary orbit. As the nebulosity evolves, the density remains greater in the equatorial plane than at the polar axis. This hypothesis is supported by calculations of the forbidden emission line ratios which also imply a higher equatorial density.

Sparks, W. M.↗
NASA NTRS1974

Statistical time-dependent model for the interstellar gas

We present models for temperature and ionization structure of low, uniform-density (approximately 0.3 per cu cm) interstellar gas in a galactic disk which is exposed to soft X rays from supernova outbursts occurring randomly in space and time. The structure was calculated by computing the time record of temperature and ionization at a given point by Monte Carlo simulation. The calculation yields probability distribution functions for ionized fraction, temperature, and their various observable moments. These time-dependent models predict a bimodal temperature distribution of the gas that agrees with various observations. Cold regions in the low-density gas may have the appearance of clouds in 21-cm absorption. The time-dependent model, in contrast to the steady-state model, predicts large fluctuations in ionization rate and the existence of cold (approximately 30 K), ionized (ionized fraction equal to about 0.1) regions.

Gerola, H.↗
NASA NTRS1975

Coronagraph particulate measurements. Skylab flight experiment T025

Major results of the Skylab T025 Coronagraph experiment designed to monitor the particulate contamination about the spacecraft and to study the earth's atmospheric aerosol distribution are presented. A model for comet outbursts based on the properties of amorphous ice and ground based narrow-band and white light photography of comet Kohoutek ten days to perihelion are included. The effect of atmospheric refraction on the analysis of the T025 atmospheric data was also investigated.

Greenberg, J. M.↗
NASA NTRS1974

Infrared, radio, and X-ray observations of Cygnus X-3

Infrared observations of Cyg X-3 are presented along with X-ray and radio data. A study of the data shows evidence for several types of behavior in the infrared flux variations of Cyg X-3. It is pointed out that a lack of periodic variations observed can be due either to a real absence of these variations or to a masking by an outburst preceding the observation time. There is no simple radio-infrared correlation, although both radio and infrared emissions were observed during the same period of time.

Becklin, E. E.↗