solar oscillations

solar oscillations
oscilaciones solares

English-Spanish dictionary of astronomy terms. 2014.

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  • Birmingham Solar Oscillations Network — The Birmingham Solar Oscillations Network (BiSON) consists of a network of six remote solar observatories monitoring low degree solar oscillation modes. It is operated by the High Resolution Optical Spectroscopy group of the School of Physics and …   Wikipedia

  • Solar and Heliospheric Observatory — Pour les articles homonymes, voir Soho. SoHO …   Wikipédia en Français

  • Solar and Heliospheric Observatory — SOHO wird für den Start vorbereitet SOHO steht für „Solar and Heliospheric Observatory“ (Sonnen und Heliosphären Observatorium) und ist eine Raumsonde bzw. ein Weltraumobservatorium von ESA und NASA …   Deutsch Wikipedia

  • Solar sail — Solar sails (also called light sails or photon sails, especially when they use light sources other than the Sun) are a proposed form of spacecraft propulsion using large membrane mirrors. Radiation pressure is about 10 5 Pa at Earth s distance… …   Wikipedia

  • Solar and Heliospheric Observatory — Infobox Space telescope name = Solar and Heliospheric Observatory (SOHO) caption = organization = ESA / NASA alt names = nssdc id = location = L1 orbit type = height = 1.5×106 km (heliocentric) period = 1 Earth year velocity = accel gravity =… …   Wikipedia

  • Solar neutrino problem — The solar neutrino problem was a major discrepancy between measurements of the numbers of neutrinos flowing through the earth and theoretical models of the solar interior, lasting from the mid 1960s to about 2002. The discrepancy has since been… …   Wikipedia

  • Solar-like oscillations — The term solar like oscillations refers to oscillations in other stars that are excited in the same way as those in the Sun, namely by convection in its outer layers.ee also* asteroseismology * helioseismology * variable stars * Procyon * Space… …   Wikipedia

  • Solar mass — Weight of the Sun redirects here. For the song, see Tao of the Dead. Size and mass of very large stars: Most massive example, the blue Pistol Star (150 ). Others are Rho Cassiopeiae (40 …   Wikipedia

  • Timeline of solar astronomy — 9th century * 850 Ahmad ibn Muhammad ibn Kathīr al Farghānī (Alfraganus) gives values for the obliquity of the ecliptic, the precessional movement of the apogees of the Sun 10th century * 900 929 Muhammad ibn Jābir al Harrānī al Battānī… …   Wikipedia

  • Spicule (solar physics) — In solar physics, a spicule is a dynamic jet of about 500km diameter on the Sun. It moves upwards at about 20 km/s from the photosphere. They were discovered in 1877 by Father Angelo Secchi of the Vatican Observatory in Rome. The chromosphere is… …   Wikipedia

  • Neutron-star oscillations — Asteroseismology studies the internal structure of our Sun and other stars using oscillations. These can be studied by interpreting the temporal frequency spectrum acquired through observations [cite journal|… …   Wikipedia

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