Polar coronal holes and the sunspot cycle. A new method to predict sunspot numbers
- 1 January 1989
- journal article
- research article
- Published by Springer Nature in Solar Physics
- Vol. 122 (2) , 335-343
- https://doi.org/10.1007/bf00913000
Abstract
No abstract availableKeywords
This publication has 19 references indexed in Scilit:
- Prediction of the maximum annual mean sunspot number in the coming solar maximum epochSolar Physics, 1987
- The sources of large-scale heliospheric disturbancesSolar Physics, 1986
- Solar activity cycle variation of the K coronaThe Astrophysical Journal, 1984
- Ten cycles of solar and geomagnetic activitySolar Physics, 1981
- Polar Coronal Holes and Cosmic-Ray ModulationScience, 1980
- Predicted intensity of the solar maximumNature, 1978
- Large-Scale Solar Magnetic FieldsAnnual Review of Astronomy and Astrophysics, 1977
- A coronal hole and its identification as the source of a high velocity solar wind streamSolar Physics, 1973
- Some properties of the day-to-day variability of Sq(H)Planetary and Space Science, 1969
- The Topology of the Sun's Magnetic Field and the 22-YEAR Cycle.The Astrophysical Journal, 1961