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Interplanetary Scintillation

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dc.contributor.author Armstrong, John W. en_US
dc.date.accessioned 2004-10-05T05:57:48Z
dc.date.available 2004-10-05T05:57:48Z
dc.date.issued 1995-01-03 en_US
dc.identifier.citation Boulder, CO en_US
dc.identifier.clearanceno 94-1497 en_US
dc.identifier.uri http://hdl.handle.net/2014/33395
dc.description.abstract Interplanetary scintillation (IPS) has been used as a diagnostic of solar wind speed and interplanetary plasma turbulence, allowing inference of speed and electron density power spectrum close to the Sun and out of the ecliptic. In that context, IPS is "signal" and provides scientifically interesting data. IPS is also of interest because amplitude and phase perturbations imposed on radio waves are "noise" for telemetry and precision Doppler tracking of deep space probes and for some radio astronomical observations. This paper briefly reviews the connection between scattering observables and the electron density power spectrum. Interplanetary phase scintillation on time scales of 100 to 10 000 seconds is an important noise in mass determinations of small solar system bodies during space-probe fly-bys and in searches for low-frequency gravitational radiation. en_US
dc.format.extent 10507 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other scintillation interplanetary noise gravity waves solar wind plasma Sun radio waves deep space probes electron density power spectrum diagnostic Doppler tracking radio astronomy en_US
dc.title Interplanetary Scintillation en_US


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