interplanetary scintillation

interplanetary scintillation

(IPS) See scattering; interplanetary medium.
References in periodicals archive ?
Remote-sensing observations of the solar wind have been conducted for more than 3 decades at the Solar-Terrestrial Environment Laboratory (STEL) of Nagoya University, using the interplanetary scintillation (IPS) method.
(1995) Multi-station system for solar wind observations using the interplanetary scintillation method.
(1972) Analysis of three-station interplanetary scintillation. J.
(1978) Comparison of 74-MHz interplanetary scintillation and IMP 7 observations of the solar wind during 1973.
(1979) Anisotropic structure of solar wind plasma irregularities observed with interplanetary scintillation. Publ.
(1982) An observation system of interplanetary scintillation at UHF.
(2011) A newly-developed UHF radiotelescope for interplanetary scintillation observations; Solar Wind Imaging Facility.
(1998) Heliospheric tomography using interplanetary scintillation observations, II.
(2001) Latitudinal velocity structures up to the solar poles estimated from interplanetary scintillation tomography analysis.
(2003) MHD tomography using interplanetary scintillation measurement.
(2010) Solar Mass Ejection Imager (SMEI) and interplanetary scintillation (IPS) 3D-reconstructions of the inner heliosphere.
(2006) Tracking heliospheric disturbances by interplanetary scintillation. Nonlinear Process.