Mapping the solar corona in X-ray lines of O VII and Ne IX.
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Engineering topics
Publications and source records attributed to Meyerott, A. J..
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Results of a rocket experiment flown on Apr. 29, 1971, in which a survey of the solar corona was carried out with a pair of collimated Bragg spectrometers to study the resonance, intersystem, and forbidden line emission from the helium-like ions O vii (22 A) and Ne ix (13 A). The observed X-ray emission came from the general corona, seven plage regions, and one dynamic feature - the late stage of a small flare. From the intensity of the O vii and Ne ix resonance lines the electron temperature and emission measure of the individual emitting regions are derived on the basis of two models, one in which the region is assumed to be isothermal and another in which the emission measure decreases exponentially with increasing temperature. The latter model, which is the most adequate of the two, yields for the electron temperature of the time-varying feature 2,000,000 to 3,000,000 K, for the other active regions 1,500,000 to 2,500,000 K, and for the general corona 1,300,000 to 1,700,000 K. The Ne ix emitting regions are about 1.5 times as hot as the O vii regions.
The X-ray optical detection system flown on Aerobee 17.08 is described in detail, and the preliminary results of the 24 June 1971 flight are discussed. The optical design, fabrication and parabolic nature of the mirrors, effective aperture of mirror array, and X-ray detectors are considered. Preliminary analysis of data from the flight confirms the extended nature and complex structure of the X-ray source in Virgo. A core of X-ray emission is indicated which is approximately 0.5 deg in diameter and surrounded by an emitting region at least 2 deg across. The Virgo source spectrum is observed to have few low energy photons.
Solar corona O VII and Ne IX helium line triplets observations, examining electron density limits
Night sky X ray sources at low galactic latitudes, describing rocket survey experiment
Galactic X ray sources survey at low galactic altitudes from rocket-borne instruments data, obtaining sources location on celestial sphere
X-ray spectral distributions and fluxes in low kev range of five cosmic sources at low galactic latitude and longitude, noting effective temperature
Celestial X-ray sources at low galactic longitude located by rocket observation
High sensitivity detectors for low-kev cosmic X-ray sources, noting aperture construction from ganging of gas counter outputs
Eight discrete cosmic X-ray sources observed by rocket techniques
Night sky sources for soft X-rays, examining data obtained by Aerobee 4.70 detectors
Upper limit to X-ray flux from Jupiter on September 30, 1962
Night sky sources for soft X-rays, examining data obtained by Aerobee 4.70 detectors