Titlebook: Sun and Planetary System; Proceedings of the S W. Fricke,G. Teleki Conference proceedings 1982 D. Reidel Publishing Company, Dordrecht, Hol

Lumbar-Spine

Nuclear Astrophysics of the SunAn analysis is given of the state of the art and prospects of investigations of high energy processes in solar matter.

群島

N斯巴達(dá)人

狗舍

Subphotospheric Velocity Fields Inferred by Sunspots MotionsThe angular velocity of solar rotation tracers, has been observed to decrease systematically with their age (Godoli et al., 1978); such a decrease is different at different latitudes and results therefore in variations of both faculae (Belvedere et al., 1977) and sunspots (Ternullo et al., 1981) velocity profiles.

MITE

New Impetus to the Exploration of the Solar System (Inaugural Address) to this Meeting. We owe much gratitude to our Yugoslav colleagues for the initiative they have taken in organizing the Meeting in their beautiful country and in particular for having chosen as our meeting place the old cultural centre Dubrovnik. We owe thanks to our Yugoslav friends for their great

緩解

Musket

The Star “Sun” Le Soleil est-il aplati? Recherches et perspectives nouvelles. 2. ., selon les déterminations les plus récentes. Perte de masse séculaire du Soleil. 3. ., et la “constante solaire”. Ses variations rapides et séculaires. Température effective. 4. . R?le de la diffusion; les inhomogénéités de composi

漂亮

The Effect of Personal Equation on Measurements of the Solar Semi-Diameter by Transit Circle Observe84 to 1892 (the only years for which raw observations of the solar limbs were available to us) should probably be attributed to large variations in the personal equation of the individual observers rather than to any real variation of the solar diameter.

逃避現(xiàn)實(shí)

placebo

The Solar Neutrino Puzzlermation about the com-position and temperature in the core of the Sun. Experiments performed by Raymond Davis indicate a significant solar neu-trino flux. but the detection rate is smaller than predicted by the standard solar model. The talk discusses the possible reasons of this discrepancy and the