Works matching IS 00380938 AND DT 2014 AND VI 289 AND IP 4
Results: 24
Analysis of Different Solar Spectral Irradiance Reconstructions and Their Impact on Solar Heating Rates.
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- Solar Physics, 2014, v. 289, n. 4, p. 1115, doi. 10.1007/s11207-013-0381-x
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- Article
The Association of Solar Flares with Coronal Mass Ejections During the Extended Solar Minimum.
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- Solar Physics, 2014, v. 289, n. 4, p. 1257, doi. 10.1007/s11207-013-0388-3
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- Article
Detectability of Large-Scale Solar Subsurface Flows.
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- Solar Physics, 2014, v. 289, n. 4, p. 1085, doi. 10.1007/s11207-013-0386-5
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Imaging Observations of X-Ray Quasi-periodic Oscillations at 3 – 6 keV in the 26 December 2002 Solar Flare.
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- Solar Physics, 2014, v. 289, n. 4, p. 1239, doi. 10.1007/s11207-013-0405-6
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- Article
Joint Measurements of Flare Flux Densities at 210 – 212 GHz by Two Different Radio Telescopes.
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- Solar Physics, 2014, v. 289, n. 4, p. 1227, doi. 10.1007/s11207-013-0390-9
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- Article
Automated Detection, Characterization, and Tracking of Sunspots from SoHO/MDI Continuum Images.
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- Solar Physics, 2014, v. 289, n. 4, p. 1413, doi. 10.1007/s11207-013-0393-6
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- Article
Sausage Mode Propagation in a Thick Magnetic Flux Tube.
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- Solar Physics, 2014, v. 289, n. 4, p. 1203, doi. 10.1007/s11207-013-0380-y
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- Article
Time-Series Analysis of Supergranule Characteristics at Solar Minimum.
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- Solar Physics, 2014, v. 289, n. 4, p. 1101, doi. 10.1007/s11207-013-0383-8
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- Article
Meridional-Flow Measurements from <i>Global Oscillation Network Group</i> Data.
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- Solar Physics, 2014, v. 289, n. 4, p. 1077, doi. 10.1007/s11207-013-0394-5
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- Article
On Solar-Wind Electron Heating at Large Solar Distances.
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- Solar Physics, 2014, v. 289, n. 4, p. 1359, doi. 10.1007/s11207-013-0403-8
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- Article
Cycle 23 Variation in Solar Flare Productivity.
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- Solar Physics, 2014, v. 289, n. 4, p. 1341, doi. 10.1007/s11207-013-0384-7
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- Article
Tubes of Magnetic Flux and Electric Current in Space Physics.
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- Solar Physics, 2014, v. 289, n. 4, p. 1173, doi. 10.1007/s11207-013-0399-0
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- Article
Modeling the Relationship Between Neutron Counting Rates and Sunspot Numbers Using the Hysteresis Effect.
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- Solar Physics, 2014, v. 289, n. 4, p. 1387, doi. 10.1007/s11207-013-0391-8
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- Article
Coronal Holes in Solar Cycles 21 to 23.
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- Solar Physics, 2014, v. 289, n. 4, p. 1349, doi. 10.1007/s11207-013-0387-4
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- Article
Nonlinear Force-Free Modeling of the Corona in Spherical Coordinates.
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- Solar Physics, 2014, v. 289, n. 4, p. 1153, doi. 10.1007/s11207-013-0406-5
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- Article
On the Nature of Neutral-Line-Associated Radio Sources.
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- Solar Physics, 2014, v. 289, n. 4, p. 1215, doi. 10.1007/s11207-013-0396-3
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- Article
Automated Processing of LASCO Coronal Images: Spurious Point-Source-Filtering and Missing-Blocks Correction.
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- Solar Physics, 2014, v. 289, n. 4, p. 1433, doi. 10.1007/s11207-013-0402-9
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- Article
A Challenging Solar Eruptive Event of 18 November 2003 and the Causes of the 20 November Geomagnetic Superstorm. II. CMEs, Shock Waves, and Drifting Radio Bursts.
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- Solar Physics, 2014, v. 289, n. 4, p. 1279, doi. 10.1007/s11207-013-0397-2
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- Article
Long-Term Variability of the Polytropic Index of Solar Wind Protons at 1 AU.
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- Solar Physics, 2014, v. 289, n. 4, p. 1371, doi. 10.1007/s11207-013-0401-x
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- Article
One Possible Reason for Double-Peaked Maxima in Solar Cycles: Is a Second Maximum of Solar Cycle 24 Expected?
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- Solar Physics, 2014, v. 289, n. 4, p. 1379, doi. 10.1007/s11207-013-0407-4
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- Article
The Interaction Between Coronal Mass Ejections and Streamers: A Statistical View over 15 Years (1996 – 2010)
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- Solar Physics, 2014, v. 289, n. 4, p. 1313, doi. 10.1007/s11207-013-0379-4
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- Article
Bimodal Distribution of Magnetic Fields and Areas of Sunspots.
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- Solar Physics, 2014, v. 289, n. 4, p. 1143, doi. 10.1007/s11207-013-0382-9
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- Article
Linear MHD Wave Propagation in Time-Dependent Flux Tube: II. Finite Plasma Beta.
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- Solar Physics, 2014, v. 289, n. 4, p. 1193, doi. 10.1007/s11207-013-0400-y
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- Article
Applying an Automatic Image-Processing Method to Synoptic Observations.
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- Solar Physics, 2014, v. 289, n. 4, p. 1403, doi. 10.1007/s11207-013-0404-7
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- Article