1975
DOI: 10.1029/ja080i016p02152
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Rocket measurement of auroral electron fluxes associated with field-aligned currents

Abstract: A Nike‐Tomahawk rocket was instrumented with a vector magnetometer and an array of particle detectors including an electron and proton energy spectrometer covering the energy range 0.5–20 keV in seven fixed intervals and measuring the pitch angle distribution from 0° to 180° as the rocket spun. The payload was launched from Poker Flat, Alaska, at 0722 UT on February 25, 1972, over a bright auroral band that evidently was the poleward electron aurora, beyond the trapping boundary. An upper limit to the measured… Show more

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Cited by 39 publications
(13 citation statements)
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“…If the electron thermal energy is assumed to be 100 eV, the energy of accelerated electrons reaches to 1 ∼ 10 keV. This is comparable with that of observed auroral energetic electrons [15][16][17][18].…”
Section: Simulation Resultssupporting
confidence: 65%
“…If the electron thermal energy is assumed to be 100 eV, the energy of accelerated electrons reaches to 1 ∼ 10 keV. This is comparable with that of observed auroral energetic electrons [15][16][17][18].…”
Section: Simulation Resultssupporting
confidence: 65%
“…This paper describes the results of a vector magnetometer experiment carried aboard a Nike-Tomahawk sounding rocket payload (NASA 18.112 UE) launched on February 25, 1972, UT. The experiment package also carried an array of charged particle detectors and a neutral hydrogen detector, which are discussed in other papers in this issue [Pazich and Anderson, 1975; $piger and Iglesias and Anderson, 1975]. The magnetometer system and data reduction methods have been described in previous publications [e.g., Park and Cloutlet, 1971], and only a simplified description will be given here.…”
Section: Introductionmentioning
confidence: 99%
“…Anderson and P.A. Cloutier and colleagues have carried out detailed studies of rocket launch data involving passage through a discrete auroral arc in the evening sector (ANDERSON and CLOUTIER, 1975;PAZICH and ANDERSON, 1975;SPIGER and ANDERSON, 1975;CASSERLY and CLOUTIER, 1975). The arc lay near the poleward edge of an eastward electrojet.…”
Section: Currents Into Ionospherementioning
confidence: 99%