An Empirical Relation Between SEP Proton Flux, CME Linear Speed And Flare Class
Journal Title: International Journal of Engineering and Science Invention - Year 2018, Vol 7, Issue 10
Abstract
The effects of Solar Energetic Particle (SEP) events are well known in terms of the potential damages they can cause for space systems like satellites and space probes, health hazards to astronauts, electronic equipment on ground, the power grids, radio communication and more important to space weather. Earlier studies have indicated that the solar flares and Coronal Mass Ejections (CMEs) play a major role in producing SEP events where in high energy particles are involved. GOES satellites carry instruments to measure the proton flux of these SEPs in many ranges. Efforts were on to predict the SEPs early and give warning in advance so that preventive or protective actions can be initiated before the actual event occurs. A few operating systems are also available for the early prediction of SEPs each having a limited number of short falls in terms of probability of detection and false alarms. There are two aspects of predicting SEPs. One is to predict the occurrence early in time and the second is to predict the proton flux of the SEP event that is going to occur. In this paper an empirical relation is derived between SEP proton flux, CME linear speed and the flare peak intensity given by X-ray class. The first part is listing the associated CMEs and flares and the second part is finding the relation between them finally leading to the derivation of a simple empirical relation.
Authors and Affiliations
V. Koteswara Rao, Dr. K. Ramagopal, Prof. R. Ramakrishna Reddy
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