2006
DOI: 10.1186/bf03351999
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Preliminary results of rocket attitude and auroral green line emission rate in the DELTA campaign

Abstract: The attitude of a sounding rocket launched in the DELTA (Dynamics and Energetics of the Lower Thermosphere in Aurora) campaign was determined with IR horizon sensors and geomagnetic sensors. Since the payload was separated into two portions, two sets of attitude sensors were needed. A new IR sensor was developed for the present experiment, and found the zenith-angle of the spin-axis of the rocket with an accuracy of 2• . By combining information obtained by both type of sensors, the absolute attitudes were det… Show more

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Cited by 3 publications
(2 citation statements)
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“…The peak altitude of q p was 115–120 km around the period of the rocket launch and 105–110 km after 01:00 UT. Iwagami et al [2006] estimated the characteristic energy of the precipitating auroral electrons during the rocket flight to be 4 keV, by comparing the observed peak altitude of the green line emission [ Kurihara et al , 2006] with the calculated green line volume emission rate for unit incident flux [ Banks et al , 1974]. The peak altitudes of q p during the rocket flight are consistent with the calculated ionization rate for the characteristic energy of 4 keV that peaks around 120 km [ Banks et al , 1974].…”
Section: Auroral Heating Rate Estimationmentioning
confidence: 77%
“…The peak altitude of q p was 115–120 km around the period of the rocket launch and 105–110 km after 01:00 UT. Iwagami et al [2006] estimated the characteristic energy of the precipitating auroral electrons during the rocket flight to be 4 keV, by comparing the observed peak altitude of the green line emission [ Kurihara et al , 2006] with the calculated green line volume emission rate for unit incident flux [ Banks et al , 1974]. The peak altitudes of q p during the rocket flight are consistent with the calculated ionization rate for the characteristic energy of 4 keV that peaks around 120 km [ Banks et al , 1974].…”
Section: Auroral Heating Rate Estimationmentioning
confidence: 77%
“…For example, it is well known that the ground-based FPI measurements have a problem with the assumption of the auroral emission layer heights, and it is difficult to find a region where the thermospheric wind is measured. A comparison between in-situ measurement of neutral temperature by the NTV on Iwagami et al (2006) the rocket and remote measurements by the FPI from the ground will provide information useful for estimating the effective emission height. Thus, an integrated analysis of the in-situ measurement and the ground based observation enables us to study the thermospheric dynamics or energetics from further insight.…”
Section: Campaign Objectivesmentioning
confidence: 99%