1989•Journal of Geophysical Research AtmospheresRequires access

Low‐altitude trapped protons at the geomagnetic equator

T. G. Guzik, Muhammad Adel Miah, John Wesley Mitchell, John P. Wefel

Open publisher page 28 citations

Abstract

Geomagnetically trapped protons in the 0.6‐ to 9‐MeV energy range were measured at latitudes near the geomagnetic equator by the Phoenix 1 experiment on board the S81‐1 mission from May to November 1982. The protons show a distribution in latitude along the line of minimum magnetic field strength with a full width at half maximum of ∼10° but with no appreciable longitudinal variation. Between 170 and 290 km the peak proton flux shows a fifth‐power altitude dependence, in contrast to previous measurements at higher altitudes, possibly demonstrating source attenuation. The efficiency of the telescope is calculated as a function of particle pitch angle and used to investigate the time dependence (1969‐1982) of the intensity.

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What this paper is about

Geomagnetically trapped protons in the 0.6‐ to 9‐MeV energy range were measured at latitudes near the geomagnetic equator by the Phoenix 1 experiment on board the S81‐1 mission from May to November 1982. The protons show a distribution in latitude along the line of minimum magnetic field strength with a full width at half maximum of ∼10° but with no appreciable longitudinal variation. Between 170 and 290 km the peak proton flux shows a fifth‐power altitude dependence, in contrast to previous measurements at higher altitudes, possibly demonstrating source attenuation. The efficiency of the telescope is calculated as a function of particle pitch angle and used to investigate the time dependence (1969‐1982) of the intensity.

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Available abstract

Geomagnetically trapped protons in the 0.6‐ to 9‐MeV energy range were measured at latitudes near the geomagnetic equator by the Phoenix 1 experiment on board the S81‐1 mission from May to November 1982. The protons show a distribution in latitude along the line of minimum magnetic field strength with a full width at half maximum of ∼10° but with no appreciable longitudinal variation. Between 170 and 290 km the peak proton flux shows a fifth‐power altitude dependence, in contrast to previous measurements at higher altitudes, possibly demonstrating source attenuation. The efficiency of the telescope is calculated as a function of particle pitch angle and used to investigate the time dependence (1969‐1982) of the intensity.

Key concepts: Earth's magnetic field, Equator, Altitude (triangle), Magnetic dip, Physics, Latitude, Pitch angle, Geomagnetic latitude

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