Role of equatorial electron cyclotron harmonic ( ECH) waves in the generation of diffuse auroras. Contribution of the GEOS IMS spacecraft.

P. Canu; G. Belmont; D. Fontaine

Role of equatorial electron cyclotron harmonic ( ECH) waves in the generation of diffuse auroras. Contribution of the GEOS IMS spacecraft.

P. Canu
, G. Belmont
, D. Fontaine

Research output: Contribution to journal › Article › peer-review

2 Citations (Scopus)

Abstract

A morphology of these emissions is presented. Results reveal high latitudinal confinement of ECH waves (1 deg) at the magnetic equator. The strongest waves are observed in the dayside magnetosphere. In the nightside, 3/2 Fce waves observed are not intense enough to put plasmasheet electrons in strong pitch-angle diffusion and cause the diffuse aurora.-from STAR, 23(14), 1985

Original language	English
Pages (from-to)	581-584
Number of pages	4
Journal	Achievements of the International Magnetospheric Study (IMS)
Publication status	Published - 1 Jan 1984

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title = "Role of equatorial electron cyclotron harmonic ( ECH) waves in the generation of diffuse auroras. Contribution of the GEOS IMS spacecraft.",

abstract = "A morphology of these emissions is presented. Results reveal high latitudinal confinement of ECH waves (1 deg) at the magnetic equator. The strongest waves are observed in the dayside magnetosphere. In the nightside, 3/2 Fce waves observed are not intense enough to put plasmasheet electrons in strong pitch-angle diffusion and cause the diffuse aurora.-from STAR, 23(14), 1985",

author = "P. Canu and G. Belmont and D. Fontaine",

year = "1984",

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language = "English",

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T1 - Role of equatorial electron cyclotron harmonic ( ECH) waves in the generation of diffuse auroras. Contribution of the GEOS IMS spacecraft.

AU - Canu, P.

AU - Belmont, G.

AU - Fontaine, D.

PY - 1984/1/1

Y1 - 1984/1/1

N2 - A morphology of these emissions is presented. Results reveal high latitudinal confinement of ECH waves (1 deg) at the magnetic equator. The strongest waves are observed in the dayside magnetosphere. In the nightside, 3/2 Fce waves observed are not intense enough to put plasmasheet electrons in strong pitch-angle diffusion and cause the diffuse aurora.-from STAR, 23(14), 1985

AB - A morphology of these emissions is presented. Results reveal high latitudinal confinement of ECH waves (1 deg) at the magnetic equator. The strongest waves are observed in the dayside magnetosphere. In the nightside, 3/2 Fce waves observed are not intense enough to put plasmasheet electrons in strong pitch-angle diffusion and cause the diffuse aurora.-from STAR, 23(14), 1985

M3 - Article

AN - SCOPUS:0021568460

SP - 581

EP - 584

JO - Achievements of the International Magnetospheric Study (IMS)

JF - Achievements of the International Magnetospheric Study (IMS)

ER -

Role of equatorial electron cyclotron harmonic ( ECH) waves in the generation of diffuse auroras. Contribution of the GEOS IMS spacecraft.

Abstract

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