The cause of high-intensity long-duration continuous AE activity (HILDCAAs): Interplanetary Alfvén wave trains

Planetary and Space Science

Volumn 35, Issue 4, 1987, Pages 405-412

  Tsurutani, Bruce T ^a   Gonzalez, Walter D ^a  

^a CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0001450242     PISSN: 00320633     EISSN: None     Source Type: Journal    
DOI: 10.1016/0032-0633(87)90097-3     Document Type: Article

References (28)

1. Solar wind variations and geomagnetic storms a study of individual storms based on high time resolution ISEE-3 data
2. Signatures in the interplanetary medium for substorms
3. An ISEE-3 high time resolution study of interplanetary parameter correlations with magnetospheric activity
4. p
5. Transverse fluctuations in the interplanetary magnetic field a requisite for geomagnetic variability
6. Hydromagnetic waves and turbulence in the solar wind
7. Subcritical and supercritical interplanetary shocks magnetic field and energetic particle observations
8. Large amplitude Alfvén wave in the interplanetary medium 2
9. Hydromagnetic waves in the interplanetary plasma
10. Wave-like phenomena in the interplanetary plasma: Mariner 2
11. Interplanetary magnetic field and the auroral zones
12. Influence of solar wind variability on geomagnetic activity
13. The propagation direction of interplanetary Alfvén waves
14. ST < −100 nT)
15. Noncompressive density enhancements in the solar wind
16. Some physical processes in the solar wind
17. Interplanetary magnetic clouds at 1 AU
18. A reexamination of rotational and tangential discontinuities in the solar wind
19. A study of geomagnetic storms
20. Response time of the magnetosphere to the interplanetary electric field
21. Shocks and storm sudden commencements
22. Magnetic fields on the sun and the North-South component of transient variations of the interplanetary magnetic field at 1 AU
23. Substorm warnings an ISEE-3 real time data system
24. Acceleration of 〉 47keV ions and 〉 2keV electrons by interplanetary shocks at 1 AU
25. Interplanetary magnetic field variations and substorm activity
26. A kinky heliospheric current sheet: cause of CDAW-6 substorms
27. Coupling between the solar wind and the magnetosphere CDAW-6
28. Convective nature of transient solar wind phenomena observed by ISEE-3 and ISEE-1 (abstract)