This site will be out of service for maintenance on Monday, May 6 from 7:30 to 8:00.

Structure of the 5-minute solar oscillations - 1976-1980

Bibcode
1981SoPh...74...51C
DOI
10.1007/BF00151273
Claverie, A.; Isaak, G. R.; McLeod, C. P.; van der Raay, H. B.; Roca-Cortés, T.
Bibliographical reference

(ESA and European Physical Society, ESLAB Symposium on Physics of Solar Variations, 14th, Scheveningen, Netherlands, Sept. 16-19, 1980.) Solar Physics, vol. 74, Nov. 1981, p. 51-57. Research supported by the Science Research Council.

Advertised on:
11
1981
Number of authors
5
IAC number of authors
1
Citations
24
Refereed citations
22
Description
The discrete structure in the 5 min velocity oscillations of the solar surface has been confirmed by a re-analysis of data obtained between 1976 and 1979, and in addition a preliminary analysis of 1980 data show excellent consistency of the determined frequencies over the five year period. It is further shown that atmospheric transparency, as measured by the power in the solar intensity fluctuations, shows no correlation with the measured amplitude of the velocity fluctuations, over 2 orders of magnitude.
Type
Refereed
Solar oscillations

It may interest you

  • Refereed
    Nonlinear Wave Damping by Kelvin–Helmholtz Instability-induced Turbulence
    Magnetohydrodynamic kink waves naturally form as a consequence of perturbations to a structured medium, for example, transverse oscillations of coronal loops. Linear theory has provided many insights into the evolution of linear oscillations, and results from these models are often applied to infer information about the solar corona from observed
    Hillier, Andrew et al.

    Advertised on:

    5
    2024
    Bibcode
    2024ApJ...966...68H
    Citations
    0
  • Refereed
    Apparent correlation between extrinsic and intrinsic flux variations in the first gravitationally lensed quasar
    To better understand which sources contribute to optical passband fluxes of Q0957+561, we present and analyse light curves of the doubly imaged gravitationally lensed quasar from its discovery to 2023. After an early microlensing event, the difference light curves (describing delay-corrected flux ratios between the two quasar images) only show
    Goicoechea, L. J. et al.

    Advertised on:

    5
    2024
    Bibcode
    2024MNRAS.530.2273G
    Citations
    0
  • Refereed
    Identification of the Top TESS Objects of Interest for Atmospheric Characterization of Transiting Exoplanets with JWST
    JWST has ushered in an era of unprecedented ability to characterize exoplanetary atmospheres. While there are over 5000 confirmed planets, more than 4000 Transiting Exoplanet Survey Satellite (TESS) planet candidates are still unconfirmed and many of the best planets for atmospheric characterization may remain to be identified. We present a sample
    Hord, Benjamin J. et al.

    Advertised on:

    5
    2024
    Bibcode
    2024AJ....167..233H
    Citations
    0