Zobrazeno 1 - 9
of 9
pro vyhledávání: '"W. P. Aiello"'
Publikováno v:
IEEE Transactions on Nuclear Science. 22:575-581
The Energetic Particle Detector (EP) on the DSP satellites consists of four units designed to measure the electron, proton and alpha particle populations at synchronous altitude. The Lo E and Hi E units are sensitive to electrons in the 30-300 keV an
Publikováno v:
IEEE Transactions on Nuclear Science. 19:626-631
A rocket-borne x-ray spectrometer is described which used cooled lithium-drifted semiconductor detectors to measure the differential x-ray energy spectrum of Sco XR-1 in the range 0.6-20 keV.
Autor:
W. P. Aiello, S. Singer
Publikováno v:
IEEE Transactions on Nuclear Science. 16:283-287
The Vela 5 satellite energetic particle experiment will employ an E-dE/dX particle identifier in which the 2-pulse multiplication is performed by a gated, constant current circuit. The multiplication time is proportional to pulse height and varies be
Publikováno v:
IEEE Transactions on Nuclear Science. 16:336-342
The Vela-4 satellite energetic-particle experiment consists of (a) a pair of diffused-junction semiconductor detectors for electrons in the energy range 30-600 keV, and (b) a garded, four-element, solar particle telescope for detecting protons from 0
Publikováno v:
Review of Scientific Instruments. 28:84-88
The energy of an electrostatic accelerator is modulated over a range of 50 kev by applying an alternating potential of 50‐kv amplitude to an insulated target at a frequency of 10 cps. A sample of the modulating voltage and the signals from a nuclea
Autor:
S. R. Kane, R. H. Weitzmann, K. A. Anderson, W. P. Aiello, R. W. Klebesadel, J. H. Primbsch, W. D. Evans
Publikováno v:
IEEE Transactions on Geoscience Electronics. 16:157-159
This experiment is designed to provide continuous coverage of solar flare X-ray bursts and transient cosmic gamma-ray bursts. A proportional counter and a scintillation detector together cover the energy range from 5 to 228 keV with good sensitivity,
Autor:
J.R. Asbridge, P. R. Higbie, W. P. Aiello, Richard D. Belian, J. G. Laros, Daniel N. Baker, R. W. Klebesadel, E.R. Tech
Publikováno v:
23rd Aerospace Sciences Meeting.
The Los Alamos National Laboratory has provided energetic particle sensors for a variety of spacecraft at the geostationary orbit (36,000 km altitude). The sensor system called the Charged Particle Analyzer (CPA) consists of four separate subsystems.
Satellite instrumentation that would serve as one element of a three-satellite network to provide precise directional information for the recently discovered cosmic gamma-ray bursts is described. The proposed network would be capable of determining s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::0b1986803c7e8a0f0c79f65de02732c6
https://doi.org/10.2172/5209207
https://doi.org/10.2172/5209207
Autor:
M.F. Halbig, E.W. Hones, R. D. Belian, E.R. Tech, D.N. Baker, W. P. Aiello, R. Robinson, S. Kedge, J. B. Payne, P. R. Higbie
Energetic electron (30 to 2000 keV) and proton (145 keV to 150 MeV) measurements made by Los Alamos National Laboratory sensors at geostationary orbit 6.6 R/sub E/ are summarized. The data are plotted in terms of daily average spectra, 3-h local time
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::67900b04312b5e0c87332e4f5c2b024f
https://doi.org/10.2172/5888285
https://doi.org/10.2172/5888285