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Using the Dipolar and Quadrupolar Moments to Improve Solar-Cycle Predictions Based on the Polar Magnetic Fields
- Source :
- CONICET Digital (CONICET), Consejo Nacional de Investigaciones Científicas y Técnicas, instacron:CONICET
- Publication Year :
- 2013
- Publisher :
- American Physical Society (APS), 2013.
-
Abstract
- The solar cycle and its associated magnetic activity are the main drivers behind changes in the interplanetary environment and Earth?s upper atmosphere (commonly referred to as space weather and climate). In recent years there has been an effort to develop accurate solar cycle predictions, leading to nearly a hundred widely spread predictions for the amplitude of solar cycle 24. Here we show that cycle predictions can be made more accurate if performed separately for each hemisphere, taking advantage of information about both the dipolar and quadrupolar moments of the solar magnetic field during minimum. Fil: Muñoz-Jaramillo, Andrés. Harvard-Smithsonian Center For Astrophysics; Estados Unidos de América; Fil: Balmaceda, Laura Antonia. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Cientifico Tecnológico - CONICET - San Juan. Instituto de Ciencias Astronómicas de la Tierra y del Espacio; Argentina; Fil: Deluca, Edward. Harvard-Smithsonian Center For Astrophysics; Estados Unidos de América
- Subjects :
- Physics
Meteorology
Otras Ciencias Naturales y Exactas
FOS: Physical sciences
PREDICTIONS
General Physics and Astronomy
SOLAR CYCLE
Solar cycle 24
Space weather
Computational physics
Solar cycle
Magnetic field
purl.org/becyt/ford/1 [https]
Atmosphere
Dipole
Ciencias Naturales y Exactas
Astrophysics - Solar and Stellar Astrophysics
Physics::Space Physics
Astrophysics::Solar and Stellar Astrophysics
Polar
Astrophysics::Earth and Planetary Astrophysics
Interplanetary spaceflight
Solar and Stellar Astrophysics (astro-ph.SR)
Subjects
Details
- ISSN :
- 10797114 and 00319007
- Volume :
- 111
- Database :
- OpenAIRE
- Journal :
- Physical Review Letters
- Accession number :
- edsair.doi.dedup.....872989ab7ce29211807e000dac679a0b
- Full Text :
- https://doi.org/10.1103/physrevlett.111.041106