Evolution of the Sun's large-scale magnetic field since the Maunder minimum

Nature

Volumn 408, Issue 6811, 2000, Pages 445-447

  Solanki, S K ^a   Schussler M ^a   Fligge, M ^b  

^a MAX PLANCK INSTITUT FÜR SONNENSYSTEMFORSCHUNG   (Germany)

^b ETH ZURICH   (Switzerland)

Author keywords

[No Author keywords available]

Indexed keywords

ARTICLE; ASTRONOMY; MAGNETIC FIELD; MATHEMATICAL ANALYSIS; MATHEMATICAL MODEL; MATHEMATICAL PARAMETERS; MODEL; PRIORITY JOURNAL;

EID: 0034707073     PISSN: 00280836     EISSN: None     Source Type: Journal    
DOI: 10.1038/35044027     Document Type: Article

References (24)

1. The solar sunspot cyle in the Maunder minimum AD1645 to AD1715
2. 10Be in polar ice to trace the 11-year cycle of solar activity
3. A doubling of the Sun's coronal magnetic field during the past 100 years
4. Properties and emergence of bipolar active regions
5. The rotation of photospheric magnetic fields: A random walk transport model
6. The long-term variation of the Sun's open magnetic flux
7. Understanding the evolution of the Sun's open magnetic flux
8. Large-scale coronal heating by the small-scale magnetic field of the Sun
9. Surface magnetic fields during the solar activity cycle
10. Solar magnetograph employing integrated diode arrays
11. The photospheric magnetic flux budget
12. Solar variability and the relation of facular to sunspot areas during solar cycle 22
13. A model of solar total and spectral irradiance variations
14. Solar luminosity and the sunspot cycle
15. Is the solar cycle timed by a clock?
16. Solar implications of ULYSSES interplanetary field measurements
17. The extended solar activity cycle
18. Length of the solar cycle: An indicator of solar activity closely associated with climate
19. Variation of cosmic ray flux and global cloud coverage - A missing link in solar-climate relationships
20. Influence of cosmic rays on Earth's climate
21. The Solar Oscillations Investigation - Michelson Doppler Imager