Published 1981
| Version v1
Book
Low energy (>35 keV) proton enhancements associated with co-rotating solar wind streams at 1 AU
Creators
- 1. Imperial Coll. of Science and Technology, London (UK). Blackett Lab.
Description
Analyses of low energy proton data in co-rotating plasma streams at 1 AU show an intensity enhancement for protons < or approximately 200 keV close to the stream interface on the fast plasma flow side. Possible origins for these particles are briefly discussed, also their relationship to the forward, and reverse, shock particle intensity increases observed in CIRs
Additional details
Publishing Information
- Publisher
- Commissariat a l'Energie Atomique.
- Imprint Place
- Paris, France
- ISBN
- 2-7272-0059-5
- Imprint Title
- Conference papers. 17. International cosmic ray conference, Paris, 13-25 July 1981
- Imprint Pagination
- 544 p.
- Journal Page Range
- v. 3 p. 430-433.
Conference
- Title
- 17. International cosmic ray conference.
- Dates
- 13 - 25 Jul 1981.
- Place
- Paris, France.
INIS
- Country of Publication
- France
- Country of Input or Organization
- France
- INIS RN
- 13667282
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- COSMIC RADIATION; KEV RANGE; PROTONS; SOLAR WIND
- Descriptors DEC
- BARYONS; CATIONS; CHARGED PARTICLES; ELEMENTARY PARTICLES; ENERGY RANGE; FERMIONS; HADRONS; HYDROGEN IONS; HYDROGEN IONS 1 PLUS; IONIZING RADIATIONS; IONS; NUCLEONS; RADIATIONS; SOLAR ACTIVITY