Solar-terrestrial response to large extension or long-duration solar gamma ray events
Main Article Content
Abstract
Gamma ray lines (GRL) from the large event of 29 September 1989 were observed from a site about 25 degrees from the flare site. In June 1991, at least three long-duration GRL events were observed by several spacecraft. None of the models put forward to explain these events are convincing. We discuss the plasma and particle data at Earth ́s orbit for these two types of events and we propose that some perturbations in interplanetary space may originate in the solar chromosphere outside active regions.
Publication Facts
Metric
This article
Other articles
Peer reviewers
0
2.4
Reviewer profiles N/A
Author statements
Author statements
This article
Other articles
Data availability
N/A
16%
External funding
N/A
32%
Competing interests
N/A
11%
Metric
This journal
Other journals
Articles accepted
2%
33%
Days to publication
8229
145
- Academic society
- Geofísica Internacional
Article Details
How to Cite
Pérez Enríquez, R., Miroshnichenko, L., Rodríguez Taboada, R. E., & Méndez Berhondo, A. (2000). Solar-terrestrial response to large extension or long-duration solar gamma ray events. Geofisica Internacional, 39(1), 87–92. https://doi.org/10.22201/igeof.00167169p.2000.39.1.301
Section
Article

This work is licensed under a Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International License.