'Pitch angle distribution' diaporamas de présentation

Energetic Electrons in a Flaring Loop

Energetic Electrons in a Flaring Loop. H. Nakajima, J. Sato, Y. Hanaoka, M. Shimojo, and A. Asai. ? Microwave & HXR observations of the 2002 Aug 24 flare on or behind the W-limb . ? Showed a clear loop like structure. Observations NoRH: the whole course of the duration.

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Once Upon a Time in the Electron Radiation Belts

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Pitch angle evolution of energetic electrons at geosynchronous orbit during disturbed times

R. Friedel, Y. Chen, G. Reeves, T. Cayton ISR-1, Los Alamos National Laboratory, USA Yuri Shprits University of California, Los Angeles, USA. Pitch angle evolution of energetic electrons at geosynchronous orbit during disturbed times. Contents. Rationale

284 views • 13 slides

Energetic solar particle dynamics during 28 October, 2003 GLE

Energetic solar particle dynamics during 28 October, 2003 GLE. E.V.Vashenyuk a , Yu.V. Balabin a , B.B. Gvozdevsky a , L.I. Miroshnichenko b , K.-L. Klein c , G. Trottet c , and P. Lantos c. (a) Polar Geophysical Institute, Apatity, Murmansk region 184 209, Russia

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Radiation Belt Electron Pitch Angle Measurements from the GOES Satellites

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1. Impulsive flare of March 16, 1999

Fig. 1. 1999/03/16: images in soft X-rays (background), hard X-rays, and microwaves. Fig. 5. 1999/02/16: time profiles of three microwave sources ( I, 17 GHz ) shown in Fig. 4 . Italic digits denote time intervals. Dashed contours: 17 GHz I difference. Color: Yohkoh /SXT.

138 views • 1 slides