Works matching DE "SPHERICAL astronomy"
Results: 599
On the IAU 2000/2006 precession–nutation and comparison with other models and VLBI observations.
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- Celestial Mechanics & Dynamical Astronomy, 2009, v. 103, n. 2, p. 179, doi. 10.1007/s10569-008-9179-9
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Seven-body central configurations: a family of central configurations in the spatial seven-body problem.
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- Celestial Mechanics & Dynamical Astronomy, 2007, v. 99, n. 4, p. 293, doi. 10.1007/s10569-007-9102-9
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Long-term evolution of orbits about a precessing oblate planet: 3. A semianalytical and a purely numerical approach.
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- Celestial Mechanics & Dynamical Astronomy, 2007, v. 99, n. 4, p. 261, doi. 10.1007/s10569-007-9099-0
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A resonant-term-based model including a nascent disk, precession, and oblateness: application to GJ 876.
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- Celestial Mechanics & Dynamical Astronomy, 2007, v. 99, n. 3, p. 197, doi. 10.1007/s10569-007-9097-2
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- Article
How much does latitude modify temperature-mortality relationship in 13 eastern US cities?
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- International Journal of Biometeorology, 2015, v. 59, n. 3, p. 365, doi. 10.1007/s00484-014-0848-y
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Changes in sleep patterns during prolonged stays in Antarctica.
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- International Journal of Biometeorology, 2008, v. 52, n. 8, p. 869
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Coupled G-Mode Intersections and Solar-Cycle Variability.
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- Solar Physics, 2010, v. 262, n. 1, p. 3, doi. 10.1007/s11207-010-9507-6
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Modelling the Longitudinal Asymmetry in Sunspot Emergence: The Role of the Wilson Depression.
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- Solar Physics, 2009, v. 260, n. 1, p. 5, doi. 10.1007/s11207-009-9420-z
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The Rotating Sunspot in AR 10930.
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- Solar Physics, 2009, v. 258, n. 2, p. 203, doi. 10.1007/s11207-009-9425-7
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A Repository of Precision Flat Fields for High-Resolution MDI Continuum Data.
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- Solar Physics, 2009, v. 258, n. 2, p. 343, doi. 10.1007/s11207-009-9408-8
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Baily’s Beads Atlas in 2005 – 2008 Eclipses.
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- Solar Physics, 2009, v. 258, n. 2, p. 191, doi. 10.1007/s11207-009-9400-3
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CME Projection Effects Studied with STEREO/COR and SOHO/LASCO.
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- Solar Physics, 2009, v. 256, n. 1/2, p. 183, doi. 10.1007/s11207-009-9336-7
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Forward Modeling of Coronal Mass Ejections Using STEREO/SECCHI Data.
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- Solar Physics, 2009, v. 256, n. 1/2, p. 111, doi. 10.1007/s11207-009-9346-5
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A Low-Frequency (30 – 110 MHz) Antenna System for Observations of Polarized Radio Emission from the Solar Corona.
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- Solar Physics, 2008, v. 253, n. 1/2, p. 319, doi. 10.1007/s11207-008-9272-y
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Principal Components and Independent Component Analysis of Solar and Space Data.
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- Solar Physics, 2008, v. 248, n. 2, p. 247, doi. 10.1007/s11207-007-9026-2
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The Observed Long- and Short-Term Phase Relation between the Toroidal and Poloidal Magnetic Fields in Cycle 23.
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- Solar Physics, 2008, v. 248, n. 2, p. 339, doi. 10.1007/s11207-007-9109-0
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Visualization of Distributed Solar Data and Metadata with the Solar Weather Browser.
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- Solar Physics, 2008, v. 248, n. 2, p. 225, doi. 10.1007/s11207-007-9105-4
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Multiscale Edge Detection in the Corona.
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- Solar Physics, 2008, v. 248, n. 2, p. 457, doi. 10.1007/s11207-008-9177-9
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A Time-Evolving 3D Method Dedicated to the Reconstruction of Solar Plumes and Results Using Extreme Ultraviolet Data.
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- Solar Physics, 2008, v. 248, n. 2, p. 409, doi. 10.1007/s11207-008-9151-6
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Automatic Detection and Tracking of Coronal Mass Ejections in Coronagraph Time Series.
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- Solar Physics, 2008, v. 248, n. 2, p. 485, doi. 10.1007/s11207-007-9104-5
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Computing Nonlinear Force-Free Coronal Magnetic Fields in Spherical Geometry.
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- Solar Physics, 2007, v. 240, n. 2, p. 227, doi. 10.1007/s11207-006-0266-3
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Temperature of Polar Corona of the Sun According to Kislovodsk Observations During 1957–2002.
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- Solar Physics, 2006, v. 237, n. 1, p. 201, doi. 10.1007/s11207-006-1680-2
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Origin of Coronal Shocks without Mass Ejections.
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- Solar Physics, 2006, v. 233, n. 1, p. 117, doi. 10.1007/s11207-006-2095-9
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A Study of Correlation between Solar Wind Data Observed at Two Points in Interplanetary Space During the Recent Solar Maximum.
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- Solar Physics, 2005, v. 227, n. 2, p. 355, doi. 10.1007/s11207-005-2100-8
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Re-Evaluation of the Flare-Type II-CME Association.
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- Solar Physics, 2004, v. 225, n. 1, p. 141, doi. 10.1007/s11207-004-3514-4
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Principal Component Analysis of the Solar Magnetic Field I: The Axisymmetric Field at the Photosphere.
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- Solar Physics, 2004, v. 225, n. 1, p. 1, doi. 10.1007/s11207-004-3257-2
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Non-Axisymmetric Magnetic Fields and Flip-Flops on the Sun and Cool Stars.
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- Solar Physics, 2004, v. 224, n. 1/2, p. 123, doi. 10.1007/s11207-005-6503-3
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Polar Coronal Structures and the Global Magnetic Field Evolution Through the Cycle.
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- Solar Physics, 2004, v. 224, n. 1/2, p. 277, doi. 10.1007/s11207-005-4280-7
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Long-term longitudinal asymmetries in sunspot activity: Difference between the ascending and descending phase of the solar cycle.
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- Solar Physics, 2004, v. 221, n. 1, p. 151, doi. 10.1023/B:SOLA.0000033367.32977.71
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Oscillations in Sunspots observed in the Near Infrared.
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- Solar Physics, 2003, v. 218, n. 1/2, p. 85, doi. 10.1023/B:SOLA.0000013028.11720.0d
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A New Method for Resolving the 180° Ambiguity in Solar Vector Magnetograms.
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- Solar Physics, 2003, v. 217, n. 1, p. 79, doi. 10.1023/A:1027365413021
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Dark Areas in He I 10 830 Å and Their Relation With Other Effects of Solar Activity.
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- Solar Physics, 2003, v. 216, n. 1/2, p. 21, doi. 10.1023/A:1026110809925
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Energetic Particles and Coronal Mass Ejections: a Case Study From ace and Ulysses.
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- Solar Physics, 2003, v. 213, n. 2, p. 387, doi. 10.1023/A:1023903408107
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Control of parasitic aberrations in multipole optics.
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- Journal of Electron Microscopy, 2009, v. 58, n. 3, p. 123, doi. 10.1093/jmicro/dfp015
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- Article
A method for determination of internal gravity wave parameters from a vertical temperature or density profile measurement in the Earth's atmosphere.
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- Cosmic Research, 2012, v. 50, n. 1, p. 21, doi. 10.1134/S0010952512010029
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Theory of longitude librations of mercury based on the ground radar observations.
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- Cosmic Research, 2011, v. 49, n. 5, p. 452, doi. 10.1134/S0010952511050029
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Solution to the problem of stability of regular precessions of a symmetrical gyrostat in Newtonian field.
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- Cosmic Research, 2011, v. 49, n. 2, p. 175, doi. 10.1134/S001095251102002X
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Relevance of asteroid occultation measurements to determination of characteristics of near-Earth objects.
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- Cosmic Research, 2010, v. 48, n. 5, p. 403, doi. 10.1134/S0010952510050059
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Periodic motions of a nearly dynamically symmetric satellite in the neighborhood of hyperboloidal precession.
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- Cosmic Research, 2009, v. 47, n. 6, p. 525, doi. 10.1134/S0010952509060082
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Design of satellite constellations with continuous coverage on elliptic orbits of Molniya type.
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- Cosmic Research, 2009, v. 47, n. 4, p. 310, doi. 10.1134/S0010952509040066
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Optimization of passive orbit with the use of gravity maneuver.
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- Cosmic Research, 2008, v. 46, n. 5, p. 456, doi. 10.1134/S0010952508050122
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Some peculiarities of changes in characteristics of proper atmosphere of space objects.
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- Cosmic Research, 2008, v. 46, n. 5, p. 408, doi. 10.1134/S0010952508050079
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Specific features of motion of geosynchronous satellites in the neighborhood of unstable stationary points.
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- Cosmic Research, 2008, v. 46, n. 5, p. 425, doi. 10.1134/S0010952508050092
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Change of spacecraft position in a satellite system.
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- Cosmic Research, 2008, v. 46, n. 3, p. 215, doi. 10.1134/S0010952508030040
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A specific case of stability of cylindrical precession of a satellite.
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- Cosmic Research, 2008, v. 46, n. 3, p. 264, doi. 10.1134/S0010952508030106
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Stability of triangle libration points in generalized restricted circular three-body problem.
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- Cosmic Research, 2008, v. 46, n. 1, p. 40, doi. 10.1134/S0010952508010061
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Simulation of penetration of primary protons into the magnetosphere.
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- Cosmic Research, 2006, v. 44, n. 3, p. 197, doi. 10.1134/S0010952506030038
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Approximate Calculation of Required and Available Lateral Range Achieved in a Spacecraft Descent to a Preset Point on the Earth's Surface.
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- Cosmic Research, 2005, v. 43, n. 6, p. 442, doi. 10.1007/s10604-005-0068-7
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Hydrodynamic Analogy for the Solution to the Doubly Averaged Hill Problem Disturbed by Precession of the Orbit Plane of a Disturbing Body.
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- Cosmic Research, 2005, v. 43, n. 5, p. 361, doi. 10.1007/s10604-005-0056-y
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A Three-Component Model of the Solar Wind Structure.
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- Cosmic Research, 2005, v. 43, n. 4, p. 299, doi. 10.1007/s10604-005-0048-y
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