Interplanetary scintillation observations of interaction regions in the solar wind
- Location
-
Deutsche Nationalbibliothek Frankfurt am Main
- Extent
-
Online-Ressource
- Language
-
Englisch
- Bibliographic citation
-
Interplanetary scintillation observations of interaction regions in the solar wind ; volume:16 ; number:10 ; year:1998 ; pages:1265-1282
Annales geophysicae ; 16, Heft 10 (1998), 1265-1282
- Creator
-
Breen, A. R.
Moran, P. J.
Varley, C. A.
Wilkinson, W. P.
Williams, P. J. S.
Coles, W. A.
Lecinski, A.
Markkanen, J.
- DOI
-
10.1007/s00585-998-1265-5
- URN
-
urn:nbn:de:101:1-201712208449
- Rights
-
Open Access; Der Zugriff auf das Objekt ist unbeschränkt möglich.
- Last update
-
15.08.2025, 7:36 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
- Breen, A. R.
- Moran, P. J.
- Varley, C. A.
- Wilkinson, W. P.
- Williams, P. J. S.
- Coles, W. A.
- Lecinski, A.
- Markkanen, J.
Other Objects (12)
Measurements of the direction of the solar wind using interplanetary scintillation
How did the solar wind structure change around the solar maximum? From interplanetary scintillation observation
EISCAT measurements of solar wind velocity and the associated level of interplanetary scintillation
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
Tracking heliospheric disturbances by interplanetary scintillation
Developments in the use of EISCAT for interplanetary scintillation
Forecasting Heliospheric CME Solar-Wind Parameters Using the UCSD Time-Dependent Tomography and ISEE Interplanetary Scintillation Data: The 10 March 2022 CME
High-latitude GPS phase scintillation and cycle slips during high-speed solar wind streams and interplanetary coronal mass ejections: a superposed epoch analysis
Solar Wind and Heavy Ion Properties of Interplanetary Coronal Mass Ejections
Development of a coronal mass ejection arrival time forecasting system using interplanetary scintillation observations
Non-radial solar wind flows induced by the motion of interplanetary coronal mass ejections
Measurements of the direction of the solar wind using interplanetary scintillation
How did the solar wind structure change around the solar maximum? From interplanetary scintillation observation
EISCAT measurements of solar wind velocity and the associated level of interplanetary scintillation
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
Tracking heliospheric disturbances by interplanetary scintillation
Developments in the use of EISCAT for interplanetary scintillation
Forecasting Heliospheric CME Solar-Wind Parameters Using the UCSD Time-Dependent Tomography and ISEE Interplanetary Scintillation Data: The 10 March 2022 CME
High-latitude GPS phase scintillation and cycle slips during high-speed solar wind streams and interplanetary coronal mass ejections: a superposed epoch analysis
Solar Wind and Heavy Ion Properties of Interplanetary Coronal Mass Ejections
Development of a coronal mass ejection arrival time forecasting system using interplanetary scintillation observations
Non-radial solar wind flows induced by the motion of interplanetary coronal mass ejections
Measurements of the direction of the solar wind using interplanetary scintillation
How did the solar wind structure change around the solar maximum? From interplanetary scintillation observation
EISCAT measurements of solar wind velocity and the associated level of interplanetary scintillation
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
Tracking heliospheric disturbances by interplanetary scintillation
Developments in the use of EISCAT for interplanetary scintillation
Forecasting Heliospheric CME Solar-Wind Parameters Using the UCSD Time-Dependent Tomography and ISEE Interplanetary Scintillation Data: The 10 March 2022 CME
High-latitude GPS phase scintillation and cycle slips during high-speed solar wind streams and interplanetary coronal mass ejections: a superposed epoch analysis
Solar Wind and Heavy Ion Properties of Interplanetary Coronal Mass Ejections
Development of a coronal mass ejection arrival time forecasting system using interplanetary scintillation observations