Works matching IS 00380938 AND DT 2007 AND VI 245 AND IP 2
Results: 14
Solar Cycle Variation of the Interplanetary Forward Shock Drivers Observed at 1 AU.
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- Solar Physics, 2007, v. 245, n. 2, p. 391, doi. 10.1007/s11207-007-9042-2
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- Article
Two-Dimensional Spectroscopy of Photospheric Shear Flows in a Small δ Spot.
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- Solar Physics, 2007, v. 245, n. 2, p. 219, doi. 10.1007/s11207-007-9039-x
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- Article
Magnetofrictional Extrapolations of Low and Lou’s Force-Free Equilibria.
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- Solar Physics, 2007, v. 245, n. 2, p. 263, doi. 10.1007/s11207-007-9046-y
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- Article
Did the Sun’s Prairie Ever Stop Burning?
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- Solar Physics, 2007, v. 245, n. 2, p. 247, doi. 10.1007/s11207-007-9057-8
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- Article
Enhanced Joule Heating in Umbral Dots.
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- Solar Physics, 2007, v. 245, n. 2, p. 239, doi. 10.1007/s11207-007-9052-0
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- Article
Calculating and Testing Nonlinear Force-Free Fields.
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- Solar Physics, 2007, v. 245, n. 2, p. 251, doi. 10.1007/s11207-007-9054-y
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- Article
Latitude Dependence of the “Gnevyshev” Peaks and Gaps.
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- Solar Physics, 2007, v. 245, n. 2, p. 415, doi. 10.1007/s11207-007-9031-5
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- Article
On Solar Intermediate Drift Radio Bursts at Decimeter and Meter Wavelength.
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- Solar Physics, 2007, v. 245, n. 2, p. 327, doi. 10.1007/s11207-007-9036-0
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Thousand-Year Cycle Signals in Solar Activity.
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- Solar Physics, 2007, v. 245, n. 2, p. 411, doi. 10.1007/s11207-007-9048-9
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- Article
Cosmic-Ray Modulation: An Empirical Relation with Solar and Heliospheric Parameters.
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- Solar Physics, 2007, v. 245, n. 2, p. 369, doi. 10.1007/s11207-007-9043-1
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- Article
Diagnostics of Near-Solar Plasma Turbulence Parameters Using the Radio Sounding Technique at Small Heliocentric Distances.
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- Solar Physics, 2007, v. 245, n. 2, p. 355, doi. 10.1007/s11207-007-9051-1
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- Article
Absorption in Burst Emission.
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- Solar Physics, 2007, v. 245, n. 2, p. 345, doi. 10.1007/s11207-007-9049-8
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- Article
Filament Kinking and Its Implications for Eruption and Re-formation.
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- Solar Physics, 2007, v. 245, n. 2, p. 287, doi. 10.1007/s11207-007-9045-z
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- Article
Evidence that Synchrotron Emission from Nonthermal Electrons Produces the Increasing Submillimeter Spectral Component in Solar Flares.
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- Solar Physics, 2007, v. 245, n. 2, p. 311, doi. 10.1007/s11207-007-9044-0
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- Article