Large-scale structure of the solar wind from interplanetary scintillation measurements during the rising phase of cycle 23

Advances in Space Research

Volumn 29, Issue 3, 2002, Pages 379-388

  Breen, A R ^a   Canals, A ^a   Fallows, R A ^a   Moran, P J ^a   Kojima, M ^b  

^a ABERYSTWYTH UNIVERSITY   (United Kingdom)

^b NAGOYA UNIVERSITY   (Japan)

Author keywords

[No Author keywords available]

Indexed keywords

GEOMETRY; SCINTILLATION; VELOCITY MEASUREMENT;

SOLAR WINDS;

SOLAR ENERGY;

PLANETARY ATMOSPHERE;

EID: 0036469031     PISSN: 02731177     EISSN: None     Source Type: Journal    
DOI: 10.1016/S0273-1177(01)00600-7     Document Type: Article

References (41)

1. Analysis of three-station interplanetary scintillation data
2. Measurements of solar wind velocity using EISCAT
3. EISCAT measurements of interplanetary scintillation
4. EISCAT measurements of the solar wind
5. EISCAT measurements of interaction regions in the solar wind
6. Interplanetary scintillation measurements of interaction regions in the solar wind
7. Interplanetary scintillation measurements of the solar wind during Whole Sun Month: Linking coronal and insitu observations
8. Interplanetary scintillation measurements of the solar wind above low-latitude coronal holes
9. Measurements of the solar wind over a wide range of heliocentric distances - A comparison of results from the first three Whole Sun Months
10. Structure of a large low-latitude coronal hole
11. The large angle spectroscopic coronagraph (LASCO)
12. Solar wind velocity from IPS observations
13. IPS observations of the solar wind out of the ecliptic
14. Solar cycle changes in the polar solar wind
15. Interplanetary scintillation observations of the high-latitude solar wind
16. The solar wind outside the plane of the ecliptic
17. The high-latitude solar wind in EISCAT interplanetary scintillation data, 1991-1999
18. Rapid acceleration of the polar solar wind
19. Origins of the slow and the ubiquitous fast solar wind
20. Interplanetary scintillation of small-diameter radio sources
21. Heliospheric tomography using interplanetary scintillation observations: 1. Combined Nagoya and Cambridge data
22. Solar wind observed within 0.3 AU with interplanetary scintillation
23. Solar cycle evolution of solar wind speed structure between 1973 and 1985 observed with the interplanetary scintillation method
24. Heliospheric tomography using interplanetary scintillation observations: 2. Latitude and heliocentric distance dependence of solar wind structure at 0.1-1 AU
25. A coronal hole and its identification as the source of a high velocity solar wind stream
26. Magnetohydrodynamic modelling of the solar corona during Whole Sun Month
27. The large-scale structure of the solar corona and inner heliosphere
28. Observations of interplanetary scintillation during the 1998 whole sun month: A comparison between EISCAT, ORT and Nagoya data
29. Coronal holes as sources of recurrent geomagnetic disturbances
30. Ulysses at 50° south: Constant immersion in the high-speed solar wind
31. Very long baseline IPS observations of the solar wind speed in the fast polar streams
32. Evolution of the solar wind over a solar cycle
33. The EISCAT ionospheric radar system - The system and its early results
34. Large-scale structure of the interplanetary medium
35. The latitude and longitude structure of the solar wind from IPS measurements
36. The relation of mariner 2 plasma data to solar phenomena
37. Origin and evolution of coronal streamer structure during the 1996 minimum activity phase
38. SWICS/Ulysses observations: The three-dimensional structure of the heliosphere in the declining/minimum phase of the solar cycle
39. Source regions of the slow solar wind