Works matching IS 17439213 AND DT 2011 AND VI 7 AND IP S286
Results: 68
IAU volume 7 issue S286 Cover and Back matter.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S286, p. b1, doi. 10.1017/S1743921312006473
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- Article
IAU volume 7 issue S286 Cover and Front matter.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S286, p. f1, doi. 10.1017/S1743921312006461
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- Article
A solar station in Ica - Mutsumi Ishitsuka: a research center to improve education at the university and schools.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S286, p. 454, doi. 10.1017/S1743921312005273
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Creating a sunspot database at the Solar Observatory of Ica National University in Perú.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S286, p. 452, doi. 10.1017/S1743921312005261
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Seeing measurement on Sasahuine mountain, Moquegua, Perú.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S286, p. 448, doi. 10.1017/S174392131200525X
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The LAGO (Large Aperture GRB Observatory) in Peru.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S286, p. 445, doi. 10.1017/S1743921312005248
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TTVs study in southern stars.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S286, p. 441, doi. 10.1017/S1743921312005236
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Magneto-seismology of solar atmospheric loops by means of longitudinal oscillations.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S286, p. 437, doi. 10.1017/S1743921312005224
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A cellular automaton model for coronal heating.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S286, p. 433, doi. 10.1017/S1743921312005212
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Climate interaction mechanism between solar activity and terrestrial biota.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S286, p. 427, doi. 10.1017/S1743921312005194
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Parallels among the “music scores” of solar cycles, space weather and Earth's climate.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S286, p. 423, doi. 10.1017/S1743921312005182
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Long term relation between solar activity and surface temperature at different geographical regions.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S286, p. 418, doi. 10.1017/S1743921312005170
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A new imminent grand minimum?
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S286, p. 414, doi. 10.1017/S1743921312005169
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Potential energy stored by planets and grand minima events.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S286, p. 410, doi. 10.1017/S1743921312005157
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- Article
Flares and habitability.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S286, p. 405, doi. 10.1017/S1743921312005145
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Effects of solar variability on planetary plasma environments and habitability.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S286, p. 393, doi. 10.1017/S1743921312005133
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Historical records of solar grand minima: a review.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S286, p. 383, doi. 10.1017/S1743921312005121
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Grand minima of solar activity during the last millennia.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S286, p. 372, doi. 10.1017/S174392131200511X
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Is meridional circulation important in modelling irregularities of the solar cycle?
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S286, p. 367, doi. 10.1017/S1743921312005108
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A model for grand minima and geomagnetic reversals.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S286, p. 360, doi. 10.1017/S1743921312005091
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Dynamo models of grand minima.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S286, p. 350, doi. 10.1017/S174392131200508X
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Soft X-ray emission as diagnostics for Maunder minimum stars.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S286, p. 346, doi. 10.1017/S1743921312005078
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Stars in magnetic grand minima: where are they and what are they like?
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S286, p. 335, doi. 10.1017/S1743921312005066
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Precise effective temperatures of solar analog stars.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S286, p. 328, doi. 10.1017/S1743921312005042
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A statistical analysis of Hα-Ca II relation for solar-type stars of different activity levels.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S286, p. 324, doi. 10.1017/S1743921312005030
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12 years of stellar activity observations in Argentina.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S286, p. 317, doi. 10.1017/S1743921312005029
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Semi-empirical modelling of stellar magnetic activity.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S286, p. 307, doi. 10.1017/S1743921312005017
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Magnetic activity of cool stars in the Hertzsprung-Russell diagram.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S286, p. 296, doi. 10.1017/S1743921312005005
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Stellar activity cycles in a model for magnetic flux generation and transport.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S286, p. 291, doi. 10.1017/S1743921312004991
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The solar wind in time.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S286, p. 286, doi. 10.1017/S174392131200498X
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Modulated stellar and solar cycles: parallels and differences.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S286, p. 279, doi. 10.1017/S1743921312004978
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Investigating stellar surface rotation using observations of starspots.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S286, p. 268, doi. 10.1017/S1743921312004966
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Stellar cycles: general properties and future directions.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S286, p. 257, doi. 10.1017/S1743921312004954
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Very intense geomagnetic storms: solar sources, characteristics and cycle distribution.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S286, p. 250, doi. 10.1017/S1743921312004930
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Evolution of a very complex active region during the decay phase of Cycle 23.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S286, p. 246, doi. 10.1017/S1743921312004929
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Earth–directed coronal mass ejections and their geoeffectiveness during the 2007–2010 interval.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S286, p. 242, doi. 10.1017/S1743921312004917
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The 3D solar corona Cycle 24 rising phase from SDO/AIA tomography.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S286, p. 238, doi. 10.1017/S1743921312004905
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Geomagnetic effects on cosmic ray propagation for different conditions.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S286, p. 234, doi. 10.1017/S1743921312004899
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High-speed streams in the solar wind during the last solar minimum.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S286, p. 229, doi. 10.1017/S1743921312004887
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Coronal Mass Ejection deflection in the corona during the two last solar minima.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S286, p. 225, doi. 10.1017/S1743921312004875
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Modeling of the atmospheric response to a strong decrease of the solar activity.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S286, p. 215, doi. 10.1017/S1743921312004863
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A porcupine Sun? Implications for the solar wind and Earth.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S286, p. 210, doi. 10.1017/S1743921312004851
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Extremely low geomagnetic activity during the recent deep solar cycle minimum.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S286, p. 200, doi. 10.1017/S174392131200484X
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Search for solar energetic particle signals in the Mexico City neutron monitor database.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S286, p. 195, doi. 10.1017/S1743921312004838
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Probing the heliosphere with the directional anisotropy of galactic cosmic-ray intensity.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S286, p. 185, doi. 10.1017/S1743921312004826
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The floor in the solar wind: status report.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S286, p. 179, doi. 10.1017/S1743921312004814
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Interplanetary conditions: lessons from this minimum.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S286, p. 168, doi. 10.1017/S1743921312004802
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Dynamical evolution of anisotropies of the solar wind magnetic turbulent outer scale.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S286, p. 164, doi. 10.1017/S1743921312004796
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Dynamic evolution of interplanetary shock waves driven by CMEs.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S286, p. 159, doi. 10.1017/S1743921312004784
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Coronal ejections from convective spherical shell dynamos.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S286, p. 154, doi. 10.1017/S1743921312004772
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