Filters
Results 1 - 1 of 1
Results 1 - 1 of 1.
Search took: 0.016 seconds
AbstractAbstract
[en] All the existing observations which did resolve low energy deuterons and He3's appear to form a self-consistent set with a hysteresis type of variation over the solar cycle of the ratio PHI(d)/PHI(He4*), where PHI(He4*) is the He4 flux corrected for the ''anomalous'' low energy component. This hysteresis can be understood if one accepts an interplanetary deceleration which is weak during the rising phase, and strong during the recovery phase of the solar cycle, and a continued increase of the escape length from the galaxy below a few GeV/n
[fr]
Toutes les observations existantes qui resoudraient les deuterons et He3 de faible energie apparaissent former un ensemble auto-consistant avec une variation de type hysteresis sur le cycle solaire du rapport PHI(d)/PHI(He4x), ou PHI(He4*) est le flux de He4 corrige de la composante basse energie anormale. Cette hysteresis peut etre comprise si on accepte: une deceleration interplanetaire qui est faible pendant la phase de lever et forte durant la phase de retour du cycle solaire et une augmentation continue de la longueur d'echappement de la galaxie au dessous de quelques GeV/nPrimary Subject
Source
1975; 6 p; 14. International cosmic ray conference; Garching, near Muenchen, F.R. Germany; 15 Aug 1975
Record Type
Report
Literature Type
Conference
Report Number
Country of publication
Reference NumberReference Number
INIS VolumeINIS Volume
INIS IssueINIS Issue