Auroral zone dayside precipitation during magnetic storm initial phases

Journal of Atmospheric and Solar-Terrestrial Physics

Volumn 63, Issue 5, 2001, Pages 513-522

  Tsurutani, B T ^a   Zhou, X Y ^a   Arballo, J K ^a   Gonzalez, W D ^b   Lakhina, G S ^c   Vasyliunas, V ^d   Pickett, J S ^e   Araki, T ^f   Yang, H ^g   Rostoker, G ^h   Hughes, T J ^h   Lepping, R P ⁱ   Berdichevsky, D ⁱ  

^a CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^b INSTITUTO NACIONAL DE PESQUISAS ESPACIAIS   (Brazil)

^c INDIAN INSTITUTE OF GEOMAGNETISM   (India)

^d MAX PLANCK INSTITUT FÜR SONNENSYSTEMFORSCHUNG   (Germany)

^e UNIVERSITY OF IOWA   (United States)

^f KYOTO UNIVERSITY   (Japan)

^g NATIONAL INSTITUTE OF POLAR RESEARCH   (Japan)

^h Technical Communication and Services   (Canada)

ⁱ NASA GODDARD SPACE FLIGHT CENTER   (United States)

Author keywords

Aurora; Magnetic storms; Magnetosphere

Indexed keywords

AURORA; GEOMAGNETIC STORM; MAGNETOSPHERE;

EID: 6644227414     PISSN: 13646826     EISSN: None     Source Type: Journal    
DOI: 10.1016/S1364-6826(00)00161-9     Document Type: Article

References (45)

1. Electromagnetic ioncyclotron waves stimulated by modest magnetospheric compressions
2. A physical model of geomagnetic sudden commencement
3. Interplanetary fast shocks and associated drivers observed through the twenty-third solar minimum by WIND over its first 2.5 years
4. The driving of the plasma sheet by the solar wind
5. A dayside auroral energy deposition case study using the Polar Ultraviolet Imager
6. Magnetic loop behind an interplanetary shock: Voyager, Helios and IMP-8 observations
7. Global auroral responses to magnetospheric compressions by shocks in the solar wind: Two case studies
8. Interplanetary magnetic field and the auroral zones
9. Use of FUV auroral emissions as diagnostic indicators
10. ST <-100 nT)
11. Solar wind magnetosphere coupling during intense magnetic storms (1978-1979)
12. Comments on the polarity of magnetic clouds
13. What is a geomagnetic storm?
14. Interplanetary causes of the January 10, 1997 substorm event
15. Current understanding of magnetic storms: Storm-substorm relationships
16. A theory of substorms: Onset and subsidence
17. A quarter century of collisionless shock research
18. A generation mechanism for the polar cap boundary layer broadband plasma waves
19. Broadband plasma waves in the boundary layers
20. VLF chorus emissions observed by POLAR during the January 10, 1997 magnetic cloud
21. Magnetic field structures of interplanetary magnetic clouds at 1 AU
22. The WIND magnetic field investigation
23. High time resolution study of the hemispheric energy flux carried by energetic electrons in the ionosphere during the May 19/20. 1996 auroral activity
24. The response of the dipole magnetosphere to pressure pulses
25. Coupling of the magnetopause to the ionosphere by means of Alfvén waves and field-aligned currents
26. Coordinated observations demonstrating external substorm triggering
27. A statistical survey of auroral solitary waves and weak double-layers 1. Occurrence and net voltage
28. SWE, a comprehensive plasma instrument for the Wind spacecraft
29. PCI wave generation by sudden impulses
30. Relationship between changes in the interplanetary magnetic field and variations in magnetic field at the Earth's surface
31. The relationship of periodic structures in auroral luminosity in the afternoon sector of ULF pulsations
32. The interplanetary shock of September 24, 1998: Arrival at Earth
33. Shocks and storm sudden commencements
34. Initial response and complex polar cap structures of the aurora in response to the January 10, 1997 magnetic cloud
35. A far ultraviolet imager for the international solar-terrestrial physics mission
36. The January 10, 1997 auroral hot spot, horseshoe aurora and first substorm: A CME loop?
37. The interplanetary causes of magnetic storms: A review
38. Interplanetary causes of great and superintense magnetic storms
39. Some basic concepts of wave-particle interactions in collisionless plasmas
40. Acceleration of > 47 keV ions and > 2 keV electrons by interplanetary shocks at 1 AU
41. Rapid intensification and propagation of the dayside aurora: Large scale interplanetary pressure pulses (fast shocks)
42. Substorms, pseudobreakups and quiescent events caused by interplanetary shocks