Solar rotation

Results: 112



#Item
21Large-scale zonal flows during the solar minimum  and the rise of cycle 24 R. Howe1, R. Komm2, F. Hill2, J. Christensen-Dalsgaard3,  T. P. Larson4, J. Schou4, M. J. Thompson5 1 University of Birmingham 2 National Solar O

Large-scale zonal flows during the solar minimum and the rise of cycle 24 R. Howe1, R. Komm2, F. Hill2, J. Christensen-Dalsgaard3, T. P. Larson4, J. Schou4, M. J. Thompson5 1 University of Birmingham 2 National Solar O

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Source URL: gong.nso.edu

Language: English - Date: 2011-06-08 14:33:10
22

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Source URL: www.spaceweathercenter.org

Language: English - Date: 2009-06-18 18:34:29
23The Astrophysical Journal, 585:553–565, 2003 March 1 # 2003. The American Astronomical Society. All rights reserved. Printed in U.S.A. CHANGES IN SOLAR DYNAMICS FROM 1995 TO 2002 Sarbani Basu Astronomy Department, Yale

The Astrophysical Journal, 585:553–565, 2003 March 1 # 2003. The American Astronomical Society. All rights reserved. Printed in U.S.A. CHANGES IN SOLAR DYNAMICS FROM 1995 TO 2002 Sarbani Basu Astronomy Department, Yale

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Source URL: repository.ias.ac.in

Language: English - Date: 2010-11-10 01:13:10
24Earth Planets Space, 62, 525–544, 2010  The influence of the sidereal cosmic-ray anisotropies originated on the tail- and nose-boundaries of the heliomagnetosphere (HMS) upon the solar cosmic-ray anisotropy produced in

Earth Planets Space, 62, 525–544, 2010 The influence of the sidereal cosmic-ray anisotropies originated on the tail- and nose-boundaries of the heliomagnetosphere (HMS) upon the solar cosmic-ray anisotropy produced in

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Source URL: www.terrapub.co.jp

Language: English - Date: 2011-03-15 22:37:58
25Adv.SpaceRer.Vol. 17,No.4/5,pp276, 1996 ~~~~1995COSP~ Printed in Grat B&a&. All rights reserved. K&$9.50+0.00

Adv.SpaceRer.Vol. 17,No.4/5,pp276, 1996 ~~~~1995COSP~ Printed in Grat B&a&. All rights reserved. K&$9.50+0.00

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Source URL: cosray.phys.uoa.gr

Language: English
26Journal of Atmospheric and Solar-Terrestrial Physics – 1033  www.elsevier.com/locate/jastp Time evolution of cosmic-ray intensity and solar &are index at the maximum phase of cycles 21 and 22

Journal of Atmospheric and Solar-Terrestrial Physics – 1033 www.elsevier.com/locate/jastp Time evolution of cosmic-ray intensity and solar &are index at the maximum phase of cycles 21 and 22

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Source URL: cosray.phys.uoa.gr

Language: English
27Measurement of Spin-Orbit Alignment in an Extrasolar Planetary System Mark Richardson  Outline

Measurement of Spin-Orbit Alignment in an Extrasolar Planetary System Mark Richardson Outline

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Source URL: www.asu.edu

Language: English - Date: 2009-10-03 02:41:53
28Lectures 4-6:   Dynamo models of the solar cycle  The solar cycle Basic model setup Mean-field electrodynamics and models  Babcock-Leighton models Models based on MHD instabilities Global 3D MHD simulations

Lectures 4-6: Dynamo models of the solar cycle The solar cycle Basic model setup Mean-field electrodynamics and models Babcock-Leighton models Models based on MHD instabilities Global 3D MHD simulations

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Source URL: www.heliophysics.ucar.edu

Language: English - Date: 2010-12-14 17:05:30
29Adv. Space Res. Vol. 11, No. 1, pp—(1)172, 1991 Printed in Great Britain. All rightsreserved. 0273— $0.00 + .50 Copyright © 1991 COSPAR

Adv. Space Res. Vol. 11, No. 1, pp—(1)172, 1991 Printed in Great Britain. All rightsreserved. 0273— $0.00 + .50 Copyright © 1991 COSPAR

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Source URL: cosray.phys.uoa.gr

Language: English
30Saturn: Diameter, 120,000 km; Mass, 95.2 Earth masses; Density, 0.7 (density of water is 1.0); Rotation Period, 10 hours, 14 minutes; Axis Inclination, 26° 44’; Oblateness, 0.1;

Saturn: Diameter, 120,000 km; Mass, 95.2 Earth masses; Density, 0.7 (density of water is 1.0); Rotation Period, 10 hours, 14 minutes; Axis Inclination, 26° 44’; Oblateness, 0.1;

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Source URL: www.lcse.umn.edu

Language: English - Date: 2015-03-01 19:22:32