[1]
|
H. I. Abdussamatov, “Long-term variations of the integral radiation flux and possible temperature changes in the solar core,” Kinematics and Physics of Celestial Bodies, Vol. 21, No. 6, pp. 328–332, 2005.
|
[2]
|
H. I. Abdussamatov, “The time of the end of the current solar cycle and the relationship between duration of 11-year cycles and secular cycle phase,” Kinematics and Physics of Celestial Bodies, Vol. 22, pp. 141–143, 2006.
|
[3]
|
H. I. Abdussamatov, “Optimal prediction of the peak of the next 11-year activity cycle and of the peaks of several succeeding cycles on the basis of long-term variations in the solar radius or solar constant,” Kinematics and Physics of Celestial Bodies, Vol. 23, pp. 97–100, 2007.
|
[4]
|
S. Duhau, “An early prediction of maximum sunspot number in solar cycle 24,” Solar Physics, Vol. 213, pp. 203–212, 2003.
|
[5]
|
C. Fr?hlich, “Solar constant,” 2009. http://www.pmodwrc. ch/pmod.php?topic=tsi/composite/SolarConstant
|
[6]
|
S. Sello, “Solar cycle activity: A preliminary prediction for cycle 24,” Astronomy and Astrophysics, Vol. 401, pp. 691–693, 2003.
|
[7]
|
SIDC (Solar Influences Data Analysis Center), 2009. http://sidc.oma.be/sunspot-data/
|