Published 2016 | Version v1
Journal article

Solar storms

Description

Solar storms begin with an explosion, or solar flare, on the surface of the sun. The X-rays and extreme ultraviolet radiation from the flare reach the Earths orbit minutes later-travelling at light speed. The ionization of upper layers of our atmosphere could cause radio blackouts and satellite navigation errors (GPS). Soon after, a wave of energetic particles, electrons and protons accelerated by the explosion crosses the orbit of the Earth, and can cause real and significant damage. (Author)

Additional details

Additional titles

Original title (Spanish)
Tormentas solares

Publishing Information

Journal Title
Nuclear Espana (1996)
Journal Volume
371
Journal Page Range
p. 44-49
ISSN
1137-2885
CODEN
NUESFO

INIS

Country of Publication
Spain
Country of Input or Organization
Spain
INIS RN
47081769
Subject category
S46: INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY;
Descriptors DEI
ATMOSPHERIC PRECIPITATIONS; ELECTRONS; IONIZATION; METEOROLOGY; PROTONS; SOLAR ACTIVITY; STORMS
Descriptors DEC
BARYONS; ELEMENTARY PARTICLES; FERMIONS; HADRONS; LEPTONS; NUCLEONS; STELLAR ACTIVITY

Optional Information