- Location
-
Deutsche Nationalbibliothek Frankfurt am Main
- Extent
-
Online-Ressource
- Language
-
Englisch
- Bibliographic citation
-
Tracking heliospheric disturbances by interplanetary scintillation ; volume:13 ; number:3 ; year:2006 ; pages:329-338
Nonlinear processes in geophysics ; 13, Heft 3 (2006), 329-338
- Creator
-
Tokumaru, M.
Kojima, M.
Fujiki, K.
Yamashita, M.
- DOI
-
10.5194/npg-13-329-2006
- URN
-
urn:nbn:de:101:1-201801049998
- Rights
-
Open Access; Der Zugriff auf das Objekt ist unbeschränkt möglich.
- Last update
-
15.08.2025, 7:32 AM CEST
Data provider
This object is provided by:
Deutsche Nationalbibliothek. If you have any questions about the object, please contact the data provider.
Deutsche Nationalbibliothek. If you have any questions about the object, please contact the data provider.
Associated
- Tokumaru, M.
- Kojima, M.
- Fujiki, K.
- Yamashita, M.
Other Objects (12)
Developments in the use of EISCAT for interplanetary scintillation
Interplanetary scintillation observations of interaction regions in the solar wind
Measurements of the direction of the solar wind using interplanetary scintillation
Validation of coronal mass ejection arrival-time forecasts by magnetohydrodynamic simulations based on interplanetary scintillation observations
EISCAT measurements of solar wind velocity and the associated level of interplanetary scintillation
Development of a coronal mass ejection arrival time forecasting system using interplanetary scintillation observations
Estimating random transverse velocities in the fast solar wind from EISCAT Interplanetary Scintillation measurements
Simultaneous interplanetary scintillation and optical measurements of the acceleration of the slow solar wind
How did the solar wind structure change around the solar maximum? From interplanetary scintillation observation
On the solar origin of interplanetary disturbances observed in the vicinity of the Earth
"Interplanetary Plasma"
Changes of dayside auroral distribution caused by a solar wind pressure pulse and associated interplanetary magnetic field disturbances
Developments in the use of EISCAT for interplanetary scintillation
Interplanetary scintillation observations of interaction regions in the solar wind
Measurements of the direction of the solar wind using interplanetary scintillation
Validation of coronal mass ejection arrival-time forecasts by magnetohydrodynamic simulations based on interplanetary scintillation observations
EISCAT measurements of solar wind velocity and the associated level of interplanetary scintillation
Development of a coronal mass ejection arrival time forecasting system using interplanetary scintillation observations
Estimating random transverse velocities in the fast solar wind from EISCAT Interplanetary Scintillation measurements
Simultaneous interplanetary scintillation and optical measurements of the acceleration of the slow solar wind
How did the solar wind structure change around the solar maximum? From interplanetary scintillation observation
On the solar origin of interplanetary disturbances observed in the vicinity of the Earth
"Interplanetary Plasma"
Changes of dayside auroral distribution caused by a solar wind pressure pulse and associated interplanetary magnetic field disturbances
Developments in the use of EISCAT for interplanetary scintillation
Interplanetary scintillation observations of interaction regions in the solar wind
Measurements of the direction of the solar wind using interplanetary scintillation
Validation of coronal mass ejection arrival-time forecasts by magnetohydrodynamic simulations based on interplanetary scintillation observations
EISCAT measurements of solar wind velocity and the associated level of interplanetary scintillation
Development of a coronal mass ejection arrival time forecasting system using interplanetary scintillation observations
Estimating random transverse velocities in the fast solar wind from EISCAT Interplanetary Scintillation measurements
Simultaneous interplanetary scintillation and optical measurements of the acceleration of the slow solar wind
How did the solar wind structure change around the solar maximum? From interplanetary scintillation observation
On the solar origin of interplanetary disturbances observed in the vicinity of the Earth
"Interplanetary Plasma"