Longitudinal distribution of PCA sources on the sun

✍ Scribed by L. Fritzová-Svestková; Z. Švestka

• Publisher: Springer
• Year: 1971
• Tongue: English
• Weight: 313 KB
• Volume: 17
• Category: Article
• ISSN: 0038-0938
• DOI: 10.1007/bf00152873

✦ Synopsis

For 181 PCA's recorded during the years 1956-1969 the association with flares is studied. Both the number of events which cannot be associated with any flare on the visible hemisphere, as well as the longitude distribution of identified proton flares:, lead to the conclusion that 25-30~ of PCA's are caused by flares behind the western solar limb. PCA's of this kind are mostly small. During the investigated years no PCA> 13 dB and possibly no PCA> 8.5 dB were caused by flares behind the limb, while hardly 60 ~ of PCA's < 1 dB had their origin on the visible hemisphere.

While the sources of GLE's and of PCA's in general, are centered around 50 ~ W which corresponds to the average curvature of the magnetic field lines in interplanetary space, the strongest PCA's (> 8.5 dB) show an anomalous longitude distribution centered around N 20~ It is suggested that this anomaly may be a consequence of the fact that in strong PCA events the kinetic energy density of protons below 100 MeV becomes comparable to the magnetic energy density in space, thus leading to a 'straightening' of the magnetic field lines.