ELF Sferic Occurrences in the Antarctic during a Solar Proton Event: Case Study of Occurrences at Byrd Station during the Event of 9 June 1968.

Electromagnetic waves with frequencies above the extremely-low-frequency range (ELF; frequencies in the range 5 Hz-3KHz) are susceptible to a variety of solar proton event (SPE) effects when propagating through a polar region in the earth-ionosphere waveguide. These effects appear to become less sev...

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Bibliographic Details
Main Authors: Fraser-Smith ,A C, Helliwell,R A
Other Authors: STANFORD UNIV CALIF STANFORD ELECTRONICS LABS
Format: Text
Language:English
Published: 1979
Subjects:
Online Access:http://www.dtic.mil/docs/citations/ADA078923
http://oai.dtic.mil/oai/oai?&verb=getRecord&metadataPrefix=html&identifier=ADA078923
id ftdtic:ADA078923
record_format openpolar
spelling ftdtic:ADA078923 2023-05-15T14:00:45+02:00 ELF Sferic Occurrences in the Antarctic during a Solar Proton Event: Case Study of Occurrences at Byrd Station during the Event of 9 June 1968. Fraser-Smith ,A C Helliwell,R A STANFORD UNIV CALIF STANFORD ELECTRONICS LABS 1979-09-19 text/html http://www.dtic.mil/docs/citations/ADA078923 http://oai.dtic.mil/oai/oai?&verb=getRecord&metadataPrefix=html&identifier=ADA078923 en eng http://www.dtic.mil/docs/citations/ADA078923 APPROVED FOR PUBLIC RELEASE DTIC AND NTIS Atmospheric Physics Radiofrequency Wave Propagation *IONOSPHERIC PROPAGATION *EXTREMELY LOW FREQUENCY *ATMOSPHERICS POLAR REGIONS PROTONS IONIZATION ATTENUATION SOLAR ACTIVITY RADIOFREQUENCY INTERFERENCE ANTARCTIC REGIONS ELECTROMAGNETIC SUSCEPTIBILITY IONOSPHERIC DISTURBANCES POLAR CAP ABSORPTION SOLAR COSMIC RAYS D REGION Seafarer project Sanguine project Solar proton events PE62710H WU49 Text 1979 ftdtic 2016-02-20T17:25:41Z Electromagnetic waves with frequencies above the extremely-low-frequency range (ELF; frequencies in the range 5 Hz-3KHz) are susceptible to a variety of solar proton event (SPE) effects when propagating through a polar region in the earth-ionosphere waveguide. These effects appear to become less severe as the frequency of the waves becomes smaller and approaches the ELF range. Although measurements have been lacking, it would be expected that ELF wave propagation through the polar regions would be comparatively stable. To investigate polar ELF wave propagation during an SPE, we have carried out a series of measurements of the properties of ELF sferics (75 Hz) at a polar location (Byrd Station, Antarctica) during a moderately-large SPE. These measurements suggest that an SPE can significantly alter the characteristics of ELF signals propagating through the polar regions; during the first 24 hours of the SPE there was a reduction of about 50% in the median amplitudes of the sferics, compared with their amplitudes before the SPE, and there were substantial changes in their rates of occurrence. Text Antarc* Antarctic Antarctica Defense Technical Information Center: DTIC Technical Reports database Antarctic Byrd Byrd Station ENVELOPE(-119.533,-119.533,-80.017,-80.017) The Antarctic
institution Open Polar
collection Defense Technical Information Center: DTIC Technical Reports database
op_collection_id ftdtic
language English
topic Atmospheric Physics
Radiofrequency Wave Propagation
*IONOSPHERIC PROPAGATION
*EXTREMELY LOW FREQUENCY
*ATMOSPHERICS
POLAR REGIONS
PROTONS
IONIZATION
ATTENUATION
SOLAR ACTIVITY
RADIOFREQUENCY INTERFERENCE
ANTARCTIC REGIONS
ELECTROMAGNETIC SUSCEPTIBILITY
IONOSPHERIC DISTURBANCES
POLAR CAP ABSORPTION
SOLAR COSMIC RAYS
D REGION
Seafarer project
Sanguine project
Solar proton events
PE62710H
WU49
spellingShingle Atmospheric Physics
Radiofrequency Wave Propagation
*IONOSPHERIC PROPAGATION
*EXTREMELY LOW FREQUENCY
*ATMOSPHERICS
POLAR REGIONS
PROTONS
IONIZATION
ATTENUATION
SOLAR ACTIVITY
RADIOFREQUENCY INTERFERENCE
ANTARCTIC REGIONS
ELECTROMAGNETIC SUSCEPTIBILITY
IONOSPHERIC DISTURBANCES
POLAR CAP ABSORPTION
SOLAR COSMIC RAYS
D REGION
Seafarer project
Sanguine project
Solar proton events
PE62710H
WU49
Fraser-Smith ,A C
Helliwell,R A
ELF Sferic Occurrences in the Antarctic during a Solar Proton Event: Case Study of Occurrences at Byrd Station during the Event of 9 June 1968.
topic_facet Atmospheric Physics
Radiofrequency Wave Propagation
*IONOSPHERIC PROPAGATION
*EXTREMELY LOW FREQUENCY
*ATMOSPHERICS
POLAR REGIONS
PROTONS
IONIZATION
ATTENUATION
SOLAR ACTIVITY
RADIOFREQUENCY INTERFERENCE
ANTARCTIC REGIONS
ELECTROMAGNETIC SUSCEPTIBILITY
IONOSPHERIC DISTURBANCES
POLAR CAP ABSORPTION
SOLAR COSMIC RAYS
D REGION
Seafarer project
Sanguine project
Solar proton events
PE62710H
WU49
description Electromagnetic waves with frequencies above the extremely-low-frequency range (ELF; frequencies in the range 5 Hz-3KHz) are susceptible to a variety of solar proton event (SPE) effects when propagating through a polar region in the earth-ionosphere waveguide. These effects appear to become less severe as the frequency of the waves becomes smaller and approaches the ELF range. Although measurements have been lacking, it would be expected that ELF wave propagation through the polar regions would be comparatively stable. To investigate polar ELF wave propagation during an SPE, we have carried out a series of measurements of the properties of ELF sferics (75 Hz) at a polar location (Byrd Station, Antarctica) during a moderately-large SPE. These measurements suggest that an SPE can significantly alter the characteristics of ELF signals propagating through the polar regions; during the first 24 hours of the SPE there was a reduction of about 50% in the median amplitudes of the sferics, compared with their amplitudes before the SPE, and there were substantial changes in their rates of occurrence.
author2 STANFORD UNIV CALIF STANFORD ELECTRONICS LABS
format Text
author Fraser-Smith ,A C
Helliwell,R A
author_facet Fraser-Smith ,A C
Helliwell,R A
author_sort Fraser-Smith ,A C
title ELF Sferic Occurrences in the Antarctic during a Solar Proton Event: Case Study of Occurrences at Byrd Station during the Event of 9 June 1968.
title_short ELF Sferic Occurrences in the Antarctic during a Solar Proton Event: Case Study of Occurrences at Byrd Station during the Event of 9 June 1968.
title_full ELF Sferic Occurrences in the Antarctic during a Solar Proton Event: Case Study of Occurrences at Byrd Station during the Event of 9 June 1968.
title_fullStr ELF Sferic Occurrences in the Antarctic during a Solar Proton Event: Case Study of Occurrences at Byrd Station during the Event of 9 June 1968.
title_full_unstemmed ELF Sferic Occurrences in the Antarctic during a Solar Proton Event: Case Study of Occurrences at Byrd Station during the Event of 9 June 1968.
title_sort elf sferic occurrences in the antarctic during a solar proton event: case study of occurrences at byrd station during the event of 9 june 1968.
publishDate 1979
url http://www.dtic.mil/docs/citations/ADA078923
http://oai.dtic.mil/oai/oai?&verb=getRecord&metadataPrefix=html&identifier=ADA078923
long_lat ENVELOPE(-119.533,-119.533,-80.017,-80.017)
geographic Antarctic
Byrd
Byrd Station
The Antarctic
geographic_facet Antarctic
Byrd
Byrd Station
The Antarctic
genre Antarc*
Antarctic
Antarctica
genre_facet Antarc*
Antarctic
Antarctica
op_source DTIC AND NTIS
op_relation http://www.dtic.mil/docs/citations/ADA078923
op_rights APPROVED FOR PUBLIC RELEASE
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