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Frequencies and splittings of low-degree acoustic modes: a comparison between MDI and GOLF observations |
iacweb |
Hace 2 years 3 months |
Publicación |
Frequencies and splittings of low-degree acoustic modes: a comparison between MDI and GOLF observations. |
iacweb |
Hace 2 years 3 months |
Publicación |
Excitation of Solar Acoustic Modes |
iacweb |
Hace 2 years 3 months |
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The p-mode spectrum measured in intensity: from 1996 to 2000 |
iacweb |
Hace 2 years 3 months |
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Comparison of parameters of low l solar p-modes at maximum and minimum activity |
iacweb |
Hace 2 years 3 months |
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Is turbulent convection the only excitation mechanism for solar p-modes? |
iacweb |
Hace 2 years 3 months |
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XRF 040916, optical follow-up. |
iacweb |
Hace 2 years 3 months |
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The Ionization Structure of a Sample of Wind-Driven Nebulae |
iacweb |
Hace 2 years 3 months |
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Star-forming galaxies in a nearby group: Abell 634 |
iacweb |
Hace 2 years 3 months |
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GRB 030227, possible optical counterpart of XMM-newton source. |
iacweb |
Hace 2 years 3 months |
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GRB 030227 optical afterglow. |
iacweb |
Hace 2 years 3 months |
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Two Extremely Compact Starbursts Inhabiting Clusters of Galaxies: Abell 539 and Abell 634 |
iacweb |
Hace 2 years 3 months |
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Time Variations of Solar Acoustical Mode Frequencies Radius and Neutrino Counting Rate |
iacweb |
Hace 2 years 3 months |
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GOLF results: today's view on the solar modes |
iacweb |
Hace 2 years 3 months |
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The Solar Acoustic Spectrum as Seen by GOLF. I. The Difficult Case: Modes With n<10 |
iacweb |
Hace 2 years 3 months |
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The Solar Acoustic Spectrum as Seen by GOLF. II. Noise Statistics Background and Methods of Analysis |
iacweb |
Hace 2 years 3 months |
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Is the Turbulent Covection the Only Source of the Excitation of p-Modes? (CD-ROM Directory: contribs/perez) |
iacweb |
Hace 2 years 3 months |
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Noise Reduction in GOLF Spectra Using Wavelets (CD-ROM Directory: contribs/regulo) |
iacweb |
Hace 2 years 3 months |
Publicación |
A method to extract p-modes frequencies from solar like stars acoustic spectra with S/N = 1/100 |
iacweb |
Hace 2 years 3 months |
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The analysis of MONS simulation data on α Cen A+B |
iacweb |
Hace 2 years 3 months |
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Background solar velocity spectrum at high and low phases of solar activity cycle |
iacweb |
Hace 2 years 3 months |
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Background solar irradiance spectrum at high and low phases of the solar activity cycle |
iacweb |
Hace 2 years 3 months |
Publicación |
An Attempt to Observe Stellar Convection via Power Spectrum |
iacweb |
Hace 2 years 3 months |
Publicación |
An approach to Eddington science using OMC integral data |
iacweb |
Hace 2 years 3 months |
Publicación |
On the Observation of Convection in Late Type Stars |
iacweb |
Hace 2 years 3 months |