VLF wave-wave interaction experiments in the magnetosphere

VLF wave-wave interaction experiments were carried out by injecting various forms of VLF pulses into the magnetosphere from a 21.2 km dipole antenna at Siple, Antarctica. The injected signals propagate along a geomagnetic field line and often interact strongly with energetic electrons trapped in the...

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Main Author: Chang, D. C. D.
Format: Other/Unknown Material
Language:unknown
Published: 1978
Subjects:
Online Access:http://hdl.handle.net/2060/19790005053
id ftnasantrs:oai:casi.ntrs.nasa.gov:19790005053
record_format openpolar
spelling ftnasantrs:oai:casi.ntrs.nasa.gov:19790005053 2023-05-15T13:40:32+02:00 VLF wave-wave interaction experiments in the magnetosphere Chang, D. C. D. Unclassified, Unlimited, Publicly available May 1, 1978 application/pdf http://hdl.handle.net/2060/19790005053 unknown Document ID: 19790005053 Accession ID: 79N13224 http://hdl.handle.net/2060/19790005053 No Copyright CASI COMMUNICATIONS AND RADAR NASA-CR-157954 SU-SEL-78-017 SU-TR-3458-1 1978 ftnasantrs 2019-07-21T10:45:56Z VLF wave-wave interaction experiments were carried out by injecting various forms of VLF pulses into the magnetosphere from a 21.2 km dipole antenna at Siple, Antarctica. The injected signals propagate along a geomagnetic field line and often interact strongly with energetic electrons trapped in the radiation belts near the equator. Signals may be amplified and trigger emissions. These signals may then interact with one another through these energetic electrons. This report is divided into three parts. In the first part, simulations of VLF pulses propagating in the magnetosphere are carried out. In the second part, it is found for the first time that a 10 ms gap in a triggering wave can induce emission, which may then interact with the post-gap signals. In the third part, sideband triggering is reported for the first time. Other/Unknown Material Antarc* Antarctica NASA Technical Reports Server (NTRS) Siple ENVELOPE(-83.917,-83.917,-75.917,-75.917)
institution Open Polar
collection NASA Technical Reports Server (NTRS)
op_collection_id ftnasantrs
language unknown
topic COMMUNICATIONS AND RADAR
spellingShingle COMMUNICATIONS AND RADAR
Chang, D. C. D.
VLF wave-wave interaction experiments in the magnetosphere
topic_facet COMMUNICATIONS AND RADAR
description VLF wave-wave interaction experiments were carried out by injecting various forms of VLF pulses into the magnetosphere from a 21.2 km dipole antenna at Siple, Antarctica. The injected signals propagate along a geomagnetic field line and often interact strongly with energetic electrons trapped in the radiation belts near the equator. Signals may be amplified and trigger emissions. These signals may then interact with one another through these energetic electrons. This report is divided into three parts. In the first part, simulations of VLF pulses propagating in the magnetosphere are carried out. In the second part, it is found for the first time that a 10 ms gap in a triggering wave can induce emission, which may then interact with the post-gap signals. In the third part, sideband triggering is reported for the first time.
format Other/Unknown Material
author Chang, D. C. D.
author_facet Chang, D. C. D.
author_sort Chang, D. C. D.
title VLF wave-wave interaction experiments in the magnetosphere
title_short VLF wave-wave interaction experiments in the magnetosphere
title_full VLF wave-wave interaction experiments in the magnetosphere
title_fullStr VLF wave-wave interaction experiments in the magnetosphere
title_full_unstemmed VLF wave-wave interaction experiments in the magnetosphere
title_sort vlf wave-wave interaction experiments in the magnetosphere
publishDate 1978
url http://hdl.handle.net/2060/19790005053
op_coverage Unclassified, Unlimited, Publicly available
long_lat ENVELOPE(-83.917,-83.917,-75.917,-75.917)
geographic Siple
geographic_facet Siple
genre Antarc*
Antarctica
genre_facet Antarc*
Antarctica
op_source CASI
op_relation Document ID: 19790005053
Accession ID: 79N13224
http://hdl.handle.net/2060/19790005053
op_rights No Copyright
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