Works matching IS 00380938 AND DT 2006 AND VI 239 AND IP 1/2
Results: 27
X-Ray Polarization of Solar Flares Measured with Rhessi.
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- Solar Physics, 2006, v. 239, n. 1/2, p. 149, doi. 10.1007/s11207-006-0268-1
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The Periodicity of High-Latitude Solar Activity.
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- Solar Physics, 2006, v. 239, n. 1/2, p. 493, doi. 10.1007/s11207-006-0008-6
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Cosmic Ray Intensity Variations in Relation with Solar Flare Index and Sunspot Numbers.
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- Solar Physics, 2006, v. 239, n. 1/2, p. 475, doi. 10.1007/s11207-006-0138-x
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A Radio Burst and Its Associated CME on March 17, 2002.
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- Solar Physics, 2006, v. 239, n. 1/2, p. 277, doi. 10.1007/s11207-006-0202-6
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The Evaporation Regime in a Confined Flare.
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- Solar Physics, 2006, v. 239, n. 1/2, p. 193, doi. 10.1007/s11207-006-0273-4
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The Trace Telescope Point Spread Function for the 171 Å Filter.
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- Solar Physics, 2006, v. 239, n. 1/2, p. 531, doi. 10.1007/s11207-006-1994-0
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Do Quasi-Regular Structures Really Exist in the Solar Photosphere? I. Observational Evidence.
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- Solar Physics, 2006, v. 239, n. 1/2, p. 93, doi. 10.1007/s11207-006-0231-1
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Properties of Interplanetary Coronal Mass Ejections at One AU During 1995 – 2004.
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- Solar Physics, 2006, v. 239, n. 1/2, p. 393, doi. 10.1007/s11207-006-0133-2
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Seismic Emission from A M9.5-Class Solar Flare.
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- Solar Physics, 2006, v. 239, n. 1/2, p. 113, doi. 10.1007/s11207-006-0108-3
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Evolution of Electric Currents Associated with Two M-Class Flares.
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- Solar Physics, 2006, v. 239, n. 1/2, p. 137, doi. 10.1007/s11207-006-0120-7
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The Gradual Phase of the X17 Flare on October 28, 2003.
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- Solar Physics, 2006, v. 239, n. 1/2, p. 173, doi. 10.1007/s11207-006-0184-4
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The Citation Impact of Digital Preprint Archives for Solar Physics Papers.
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- Solar Physics, 2006, v. 239, n. 1/2, p. 549, doi. 10.1007/s11207-006-0262-7
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Comparative Analysis of Super-Kamiokande and SNO Solar-Neutrino Data and the Photospheric Magnetic Field.
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- Solar Physics, 2006, v. 239, n. 1/2, p. 1, doi. 10.1007/s11207-006-0304-1
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The May 13, 2005 Eruption: Observations, Data Analysis and Interpretation.
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- Solar Physics, 2006, v. 239, n. 1/2, p. 317, doi. 10.1007/s11207-006-0177-3
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Field-Line Draping Around ICMES.
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- Solar Physics, 2006, v. 239, n. 1/2, p. 437, doi. 10.1007/s11207-006-0308-x
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Spatial and Temporal Scales of Coronal Magnetic Restructuring in the Development of Coronal Mass Ejections.
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- Solar Physics, 2006, v. 239, n. 1/2, p. 257, doi. 10.1007/s11207-006-0181-7
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Fast Segmentation of Solar Extreme Ultraviolet Images.
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- Solar Physics, 2006, v. 239, n. 1/2, p. 519, doi. 10.1007/s11207-006-0140-3
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On Magnetic Coupling Between the Two Hemispheres in Solar Dynamo Models.
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- Solar Physics, 2006, v. 239, n. 1/2, p. 29, doi. 10.1007/s11207-006-0201-6
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Spectral Line Selection for HMI: A Comparison of Fe I 6173 Å and Ni I 6768 Å.
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- Solar Physics, 2006, v. 239, n. 1/2, p. 69, doi. 10.1007/s11207-006-0279-y
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Initial-Condition Influences on CME Expansion and Propagation.
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- Solar Physics, 2006, v. 239, n. 1/2, p. 293, doi. 10.1007/s11207-006-0302-3
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The Effects of Atmospheric Dispersion on High-Resolution Solar Spectroscopy.
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- Solar Physics, 2006, v. 239, n. 1/2, p. 503, doi. 10.1007/s11207-006-0283-2
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Relationships Among Magnetic Clouds, CMES, and Geomagnetic Storms.
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- Solar Physics, 2006, v. 239, n. 1/2, p. 449, doi. 10.1007/s11207-006-0037-1
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The Fe-Line Feature in the X-Ray Spectrum of Solar Flares: First Results from the SOXS Mission.
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- Solar Physics, 2006, v. 239, n. 1/2, p. 217, doi. 10.1007/s11207-006-0066-9
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Energetics and Dynamics of an Impulsive Flare on March 10, 2001.
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- Solar Physics, 2006, v. 239, n. 1/2, p. 239, doi. 10.1007/s11207-006-0098-1
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On the Near-One-Year Variation of the Sun’s Mean Magnetic Field.
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- Solar Physics, 2006, v. 239, n. 1/2, p. 461, doi. 10.1007/s11207-006-0146-x
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Sunspots with the Strongest Magnetic Fields.
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- Solar Physics, 2006, v. 239, n. 1/2, p. 41, doi. 10.1007/s11207-006-0265-4
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Properties of Stream Interactions at One AU During 1995 – 2004.
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- Solar Physics, 2006, v. 239, n. 1/2, p. 337, doi. 10.1007/s11207-006-0132-3
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