Published 2016
| Version v1
Journal article
Solar storms
Creators
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
- Collaborations
- Pereira Cuesta, S.; Pereira Pagan, B.