1971
DOI: 10.1029/rs006i010p00871
|View full text |Cite
|
Sign up to set email alerts
|

Observed and Predicted VLF Phase Behavior for the Solar Eclipses of September 11, 1969, and March 7, 1970

Abstract: A VLF propagation and a D‐region aeronomy model have been used to predict the effect of two solar eclipses on VLF propagation to Aztec, Arizona. Transmissions at 12.2 kHz from Hawaii were monitored during the eclipse on September 11, 1969; and transmissions at 12.0 kHz from Trinidad, at 24 kHz from transmitter NBA, at 12.5 kHz from Forestport, New York, and at 17.8 kHz from transmitter NAA were monitored during the eclipse on March 7, 1970. The VLF phase predictions were found to agree with measurements except… Show more

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
1

Citation Types

0
1
0

Year Published

1981
1981
2018
2018

Publication Types

Select...
4
1

Relationship

0
5

Authors

Journals

citations
Cited by 9 publications
(1 citation statement)
references
References 12 publications
0
1
0
Order By: Relevance
“…These observations also allowed them to calculate the D-region recombination coefficients during the event. Noonkester and Sailors [1971] used a VLF propagation and D-region aeronomy model to predict VLF phase change due to solar eclipse. However, they managed to accurately predict only one out of two events.…”
Section: Solar Eclipsementioning
confidence: 99%
“…These observations also allowed them to calculate the D-region recombination coefficients during the event. Noonkester and Sailors [1971] used a VLF propagation and D-region aeronomy model to predict VLF phase change due to solar eclipse. However, they managed to accurately predict only one out of two events.…”
Section: Solar Eclipsementioning
confidence: 99%