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Simultaneous Observations of Electromagnetic Ion Cyclotron (EMIC) Waves and Pitch Angle Scattering During a Van Allen Probes Conjunction
Journal article   Open access   Peer reviewed

Simultaneous Observations of Electromagnetic Ion Cyclotron (EMIC) Waves and Pitch Angle Scattering During a Van Allen Probes Conjunction

K. Sigsbee, C. A. Kletzing, J. B. Faden, A. N. Jaynes, G. D. Reeves and J-M Jahn
Journal of geophysical research. Space physics, Vol.125(4), e2019JA027424
04/2020
DOI: 10.1029/2019JA027424
url
https://www.osti.gov/biblio/1760619View
Open Access

Abstract

On 22 December 2015, the two Van Allen Probes observed two sets of electromagnetic ion cyclotron (EMIC) wave bursts during a close conjunction when both Probe A and Probe B were separated by 0.57 to 0.68 RE. The EMIC waves occurred during an active period in the recovery phase of a coronal mass ejection-driven geomagnetic storm. Both spacecraft observed EMIC wave bursts that had similar spatial structure within a 1-2 min time delay. The EMIC waves occurred outside the plasmasphere, within Delta L approximate to 1-2 of the plasmapause and within a few degrees in magnetic latitude of the equatorial plane. The spatial structure of the EMIC wave bursts may have been related to the proton drift paths outside the plasmasphere and influenced by total magnetic field strength variations associated with solar wind pressure enhancements. The EMIC waves were observed in a narrow L shell region from L approximate to 4.55-5.32 between 10 and 11 magnetic local time (MLT) on the outbound halves of the spacecraft orbits and from L approximate to 4.82-5.51 between 13 and 14 MLT on the inbound halves of the spacecraft orbits. However, Pc1 pulsations were observed on the ground over a broad range of local times. The anisotropy of the proton pitch angle distributions was enhanced when the EMIC waves were observed. Although the overall radiation belt response during this storm was dominated by acceleration and transport processes, the EMIC waves produced local pitch angle scattering of 13-15 keV protons and 2.1-2.6 MeV electrons, consistent with calculations of the expected resonant energies. Plain Language Summary In 1958, James Van Allen discovered Earth was surrounded by rings of electrons and ions, now called the radiation belts. In 2012, NASA launched the twin Van Allen Probes to study the radiation belts. Radiation belt electrons traveling near the speed of light can damage communication and weather satellites and pose a risk to astronauts. Electromagnetic waves from 1-2 cycles every 10 min up to radio frequencies (several thousand cycles per second) are critical to radiation belt physics. Some waves energize the radiation belts, while others decrease their strength. We studied electromagnetic ion cyclotron (EMIC) waves (1-4 cycles per second) during a geomagnetic storm. The Van Allen Probes encountered two EMIC wave activity regions 25,000 km above Earth's surface, one just before local noon and one slightly after local noon. The two satellites were close together and observed the waves in each region simultaneously. The wave activity regions were 2,000-4,000 km wide and 8,000 km across (twice the distance from Washington, DC, to San Francisco). Although this geomagnetic storm increased the global radiation belt strength, EMIC waves ejected electrons and protons from their paths around Earth, temporarily reducing the local radiation belt strength measured by the Van Allen Probes.
 Physical Sciences Astronomy & Astrophysics Science & Technology

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