Works matching IS 00380938 AND DT 2009 AND VI 259 AND IP 1/2
Results: 23
Numerical Heliospheric Simulations as Assisting Tool for Interpretation of Observations by STEREO Heliospheric Imagers.
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- Solar Physics, 2009, v. 259, n. 1/2, p. 297, doi. 10.1007/s11207-009-9449-z
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3D Evolution of a Filament Disappearance Event Observed by STEREO.
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- Solar Physics, 2009, v. 259, n. 1/2, p. 13, doi. 10.1007/s11207-009-9448-0
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On 3D Reconstruction of Coronal Mass Ejections: I. Method Description and Application to SECCHI-COR Data.
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- Solar Physics, 2009, v. 259, n. 1/2, p. 123, doi. 10.1007/s11207-009-9416-8
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3D Reconstruction of the Leading Edge of the 20 May 2007 Partial Halo CME.
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- Solar Physics, 2009, v. 259, n. 1/2, p. 213, doi. 10.1007/s11207-009-9423-9
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The Apparent Layered Structure of the Heliospheric Current Sheet: Multi-Spacecraft Observations.
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- Solar Physics, 2009, v. 259, n. 1/2, p. 389, doi. 10.1007/s11207-009-9452-4
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On the Tomographic Reconstruction of the 3D Electron Density for the Solar Corona from STEREO COR1 Data.
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- Solar Physics, 2009, v. 259, n. 1/2, p. 109, doi. 10.1007/s11207-009-9401-2
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On the Temporal Variability of the “Strahl” and Its Relationship with Solar Wind Characteristics: STEREO SWEA Observations.
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- Solar Physics, 2009, v. 259, n. 1/2, p. 311, doi. 10.1007/s11207-009-9402-1
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The Impact of Geometry on Observations of CME Brightness and Propagation.
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- Solar Physics, 2009, v. 259, n. 1/2, p. 179, doi. 10.1007/s11207-009-9403-0
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Multipoint Observations of Solar Type III Radio Bursts from STEREO and Wind.
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- Solar Physics, 2009, v. 259, n. 1/2, p. 255, doi. 10.1007/s11207-009-9404-z
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The Solar Wind Quasi-Invariant Observed by STEREO A and B at Solar Minimum 2007 and Comparison with Two Other Minima.
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- Solar Physics, 2009, v. 259, n. 1/2, p. 381, doi. 10.1007/s11207-009-9412-z
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Hybrid Reconstruction to Derive 3D Height – Time Evolution for Coronal Mass Ejections.
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- Solar Physics, 2009, v. 259, n. 1/2, p. 199, doi. 10.1007/s11207-009-9409-7
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STEREO Observations of Energetic Ions in Corotating Interaction Regions During the May 2007 Solar Events.
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- Solar Physics, 2009, v. 259, n. 1/2, p. 361, doi. 10.1007/s11207-009-9415-9
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Characteristics of EUV Coronal Jets Observed with STEREO/SECCHI.
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- Solar Physics, 2009, v. 259, n. 1/2, p. 87, doi. 10.1007/s11207-009-9424-8
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Pre-CME Onset Fuses – Do the STEREO Heliospheric Imagers Hold the Clues to the CME Onset Process?
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- Solar Physics, 2009, v. 259, n. 1/2, p. 277, doi. 10.1007/s11207-009-9417-7
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STEREO/SECCHI Observations on 8 December 2007: Evidence Against the Wave Hypothesis of the EIT Wave Origin.
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- Solar Physics, 2009, v. 259, n. 1/2, p. 73, doi. 10.1007/s11207-009-9375-0
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Comparison of STEREO/EUVI Loops with Potential Magnetic Field Models.
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- Solar Physics, 2009, v. 259, n. 1/2, p. 1, doi. 10.1007/s11207-009-9383-0
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Reconstructing the 3D Morphology of the 17 May 2008 CME.
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- Solar Physics, 2009, v. 259, n. 1/2, p. 163, doi. 10.1007/s11207-009-9391-0
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Relation Between Type II Bursts and CMEs Inferred from STEREO Observations.
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- Solar Physics, 2009, v. 259, n. 1/2, p. 227, doi. 10.1007/s11207-009-9382-1
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In Situ Observations of Solar Wind Stream Interface Evolution.
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- Solar Physics, 2009, v. 259, n. 1/2, p. 323, doi. 10.1007/s11207-009-9393-y
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What Is the Nature of EUV Waves? First STEREO 3D Observations and Comparison with Theoretical Models.
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- Solar Physics, 2009, v. 259, n. 1/2, p. 49, doi. 10.1007/s11207-009-9386-x
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On the Origin, 3D Structure and Dynamic Evolution of CMEs Near Solar Minimum.
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- Solar Physics, 2009, v. 259, n. 1/2, p. 143, doi. 10.1007/s11207-009-9422-x
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Formation, Interaction and Merger of an Active Region and a Quiescent Filament Prior to Their Eruption on 19 May 2007.
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- Solar Physics, 2009, v. 259, n. 1/2, p. 31, doi. 10.1007/s11207-009-9427-5
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Multi-Spacecraft Observations: Stream Interactions and Associated Structures.
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- Solar Physics, 2009, v. 259, n. 1/2, p. 345, doi. 10.1007/s11207-009-9445-3
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- Article