Anomalous temporal behaviour of NP 0532
Temporal behavior of NP 0532 in radio and optical bands compared for second derivative of period
Holt, S. S.↗
Engineering topics
Holt, S. S.
Publications and source records attributed to Holt, S. S..
Search for line structure in the X-ray spectrum of Sco X-1
Sco X-1 line spectra search in X ray spectrum by rocket-borne proportional counters, noting iron line emission
Boldt, E. A.↗
2-20 kev X-ray sky background
Spectral index for diffuse X ray sky background within specific band determined from rocket observations with wide angle telescope
Boldt, E. A.↗
Pulsars and X-ray-emitting supernova remnants
Pulsars and X ray emitting supernova remnants
Holt, S. S.↗
Anomalous temporal behavior of NP0532
Apparent discontinuities in temporal behavior of NPO532 by radio and optical bands
Holt, S. S.↗
Search for line structure in the X-ray spectrum of Sco X-1
Search for line structure in X ray spectrum of Sco X-1
Boldt, E. A.↗
Delayed appearance of relativistic electrons 5 days after a solar flare
Inverse velocity dispersion of relativistic electron intensity in interplanetary medium after solar flare
Cline, T. L.↗
Pulsed X-ray emission of NP 0532 in March 1968.
Pulsed X ray emission associated with pulsar NP 0532 in Crab Nebula measured by six element detector on Aerobee 150 rocket
Boldt, E. A.↗
Microwave and hard X-ray bursts from solar flares.
Solar flares microwave and hard X ray bursts, discussing gyrosynchroton plasma, nonthermal electron bremsstrahlung and electron relaxation
Holt, S. S.↗
The possible detection of iron line emission from Sco X-1
Detection of iron line emission from Sco X-1
Boldt, E. A.↗
Pulsed X-ray emission of NP 0532 in March 1968
Pulsed X ray emission of pulsar NP 0532 in Crab Nebula
Boldt, E. A.↗
Two-twenty keV X-ray sky background
X ray spectra of diffuse sky background in 2-20 keV range
Boldt, E. A.↗
2-20 kev spectrum of X-rays from the Crab Nebula and the diffuse background near galactic anticenter.
X ray energy spectrum from Crab Nebula and diffuse background on celestial sphere near galactic anticenter, noting spectral index
Boldt, E. A.↗
Very high energy solar X-rays observed during the proton event of 7 July 1966.
Spectral intensity of high energy solar X rays observed during July 7, 1966 polar event with satellite OGO 3, suggesting nonthermal bremsstrahlung origin
Cline, T. L.↗
Microwave and hard X-ray bursts from solar flares
Microwave and hard X ray bursts from solar flares
Holt, S. S.↗
On the generation of synchrotron and X-ray emission from electrons with energy below mc super 2 in solar flares.
Synchrotron and X ray emission generation from upper chromosphere electrons during solar flares
Cline, T. L.↗
Iron line emission from X-ray sources.
Iron line absence in emission spectrum of thermal X ray sources, constraining proposed thermal models
Boldt, E. A.↗
Two-twenty Kev Spectrum of X-rays from the Crab Nebula and the Diffuse Background near Galactic Anticenter
X ray spectroscopy of Crab nebula and diffuse background by sounding balloons and rockets
Boldt, E. A.↗