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Solar proton monitoring system

Author: G W Adams; Lawrence R Megill; Space Disturbances Laboratory (U.S.),
Publisher: Boulder, Colo. : U.S. Department of Commerce, Environmental Science Services Administration, Space Disturbances Laboratory, 1969.
Series: ESSA technical report ERL., SDL ;, 10.; ESSA technical report ERL, 119.
Edition/Format:   Print book : National government publication : EnglishView all editions and formats
Summary:
A real-time solar-proton monitoring system with ground-based sensors is located in Alaska and other parts of the United States, Greenland, and Canada. A computer in Anchorage, Alaska, interrogates the sensors, processes the data, and transmits the information via teletype to the Solar Forecast Center in Boulder, Colorado. This report describes the physics of the system, i.e., the characteristics of the events  Read more...
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Details

Additional Physical Format: Online version:
Adams, G. W. (Gene W.)
Solar proton monitoring system.
Boulder, Colo. : Space Disturbances Laboratory, 1969
(OCoLC)890596006
Material Type: Government publication, National government publication, Internet resource
Document Type: Book, Internet Resource
All Authors / Contributors: G W Adams; Lawrence R Megill; Space Disturbances Laboratory (U.S.),
OCLC Number: 9396483
Notes: "August 1969."
Description: iv, 43 pages : illustrations ; 27 cm.
Series Title: ESSA technical report ERL., SDL ;, 10.; ESSA technical report ERL, 119.
Responsibility: G.W. Adams and L.R. Megill.

Abstract:

A real-time solar-proton monitoring system with ground-based sensors is located in Alaska and other parts of the United States, Greenland, and Canada. A computer in Anchorage, Alaska, interrogates the sensors, processes the data, and transmits the information via teletype to the Solar Forecast Center in Boulder, Colorado. This report describes the physics of the system, i.e., the characteristics of the events (PCA's, auroras, SID's, REP's, and solar noise bursts), how the sensors (riometers, VLF phase and amplitude, forward scatter, neutron monitors, and magnetometers) respond to these events, how these characteristics are programmed to detect the different events, and how the sensor readings are used to obtain information about solar protons. A second report will give details on a set of rocket experiments to be fired into PCA events.

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