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Journal ArticleDOI

The general pattern of auroral particle precipitation

T.R. Hartz, +1 more
- 01 Feb 1967 - 
- Vol. 15, Iss: 2, pp 301-329
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TLDR
In this article, the authors examined statistical data on optical and radio-auroral phenomena to establish the latitude-versus-time pattern for the causal particle precipitation and found that two distinct particle populations are involved on the average.
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This article is published in Planetary and Space Science.The article was published on 1967-02-01. It has received 190 citations till now. The article focuses on the topics: Precipitation types & Drizzle.

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Citations
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Journal ArticleDOI

Postmidnight chorus: A substorm phenomenon

TL;DR: In this paper, the post-midnight chorus was detected in the midnight sector of the magnetosphere in conjunction with magnetospheric substorms and the characteristics of these emissions such as their frequency time structure, emission frequency with respect to the local equatorial electron gyrofrequency, intensity-time variation, and the average intensity were investigated.
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Global morphology of ionospheric scintillations

TL;DR: In this article, a review of the available amplitude and phase scintillation data is presented, where the effect of magnetic activity, solar sunspot cycle, and time of day is shown for each three latitudinal sectors.
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Two types of magnetospheric ELF chorus and their substorm dependences

TL;DR: In this paper, the distribution of extremely low frequency (10-1500 Hz) magnetospheric chorus to all local times and latitudes is investigated in order to determine dependence on substorms, and to evaluate the conditions under which chorus is generated.
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Bulk motion of the magnetosphere

TL;DR: In this article, an upper atmosphere geophysical measurements are surveyed to determine to what extent the available data support the concept of bulk motion of the magnetosphere (convection) and the associated electric field.
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Magnetospheric chorus - Occurrence patterns and normalized frequency

TL;DR: In this paper, the authors analyzed 400 hours of continuous broadband data obtained by the OGO 3 satellite to provide a statistically accurate description of band-limited (magnetospheric) chorus and concluded that most magnetospheric chorus consists of rising emissions which are probably generated by gyroresonant electrons slightly off the equator.
References
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Journal ArticleDOI

Limit on stably trapped particle fluxes

TL;DR: The limit on stably trapped particle fluxes determined theoretically and compared with data from Explorer satellites was first established in this paper, and the limit was later confirmed by the International Journal of Astronautics.
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A unifying theory of high-latitude geophysical phenomena and geomagnetic storms

TL;DR: In this article, the occurrence at high latitudes of a large number of geophysical phenomena, including geomagnetic agitation and bay disturbances, aurorae, and various irregular distri...
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Direct Measurement of Particles Producing Visible Auroras

TL;DR: In this paper, the nature of particles producing two visible auroras at Fort Churchill, Canada, was determined with the aid of rocket-borne detectors, and it was found that a major fraction of the auroral light was produced by electron with energies of less than 10 kev.
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Tail of the magnetosphere

TL;DR: Tangential stress effects on magnetosphere tail with regard to magnetic field intensity and direction, trapped particle fluxes and low energy cosmic ray cut-off were studied in this article, where the authors considered the effect of magnetic field and particle flux on the magnetosphere.