Latitude-dependence of a forbush type decrease
The latitude dependence of a cosmic ray intensity decrease is determined. It is shown that the relative amplitude does not flatten beyond the latitude knee. It, rather, keeps increasing far beyond the knee. It is also seen that the relative amplitude is not symmetrical around the geomagnetic equator.
- Research Organization:
- Gulmarg Research Observatory, India
- Sponsoring Organization:
- USDOE
- NSA Number:
- NSA-15-024194
- OSTI ID:
- 4028391
- Journal Information:
- Nuovo Cimento, Journal Name: Nuovo Cimento Journal Issue: 3 Vol. 20; ISSN 0029-6341
- Country of Publication:
- Country unknown/Code not available
- Language:
- English
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