Comment on "a new method of forecasting geomagnetic activity and proton showers" by A. Hewish and P.J. Duffet-Smith

Planetary and Space Science

Volumn 36, Issue 2, 1988, Pages 205-206

  Tsurutani, Bruce T ^a   Goldstein, Bruce E ^a   Gonzalez, Walter D ^b   Tang, Francis ^c  

^a CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^b INSTITUTO NACIONAL DE PESQUISAS ESPACIAIS   (Brazil)

^c CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0001727591     PISSN: 00320633     EISSN: None     Source Type: Journal    
DOI: 10.1016/0032-0633(88)90056-6     Document Type: Article

References (17)

1. Subcritieal and interplanetary shocks magnetic field and energetic particle observations
2. Interplanetary magnetic field and the auroral zones
3. Magnetic storms
4. st < − 100 nT)
5. Field line draping about fast coronal mass ejecta a source of strong out-of- the-ecliptic interplanetary magnetic fields
6. A new method of forecasting geomagnetic activity and proton showers
7. Interplanetary magnetic clouds at 1 AU
8. Comment on “Magnetic fields on the sun and the North-South component of transient variations of the interplanetary magnetic field at 1 AU” by F.Tan
9. The structure and parameters of flare streams
10. The structure of the solar flare stream magnetic field
11. Observation of interaction regions and corotating shocks
12. Magnetic fields on the sun and the North-South component of transient variations of the interplanetary magnetic field at 1 AU
13. Reply
14. Substorm warnings an ISEE-3 real time data system
15. Acceleration of 〉 47 keV ions and 〉 2 keV electrons by interplanetary shocks at 1 AU
16. A kinky heliospheric current sheet: cause of CDAW-6 substorms
17. Plasma properties of driver gas following interplanetary shocks observed by ISEE-3