Maqola

Is the solar core rotating faster or slower than the envelope?

M. LazrekLaboratoire d'Astronomie et de Geophysique CNCPRST, BP 8027, Rabat, MarocAustin R. PantelDépartement d'Astrophysique, URA CNRS 709, UNSA, F-06108, Nice, Cedex 2, FranceE. FossatDépartement d'Astrophysique, URA CNRS 709, UNSA, F-06108, Nice, Cedex 2, FranceB. GellyDépartement d'Astrophysique, URA CNRS 709, UNSA, F-06108, Nice, Cedex 2, FranceF. X. SchmiderDépartement d'Astrophysique, URA CNRS 709, UNSA, F-06108, Nice, Cedex 2, FranceD. Fierry-FraillonDépartement d'Astrophysique, URA CNRS 709, UNSA, F-06108, Nice, Cedex 2, FranceG. GrecDépartement Cassini, URA CNRS 1362, Observatoire de la Côte d'Azur, BP229, F-06304, Nice, Cedex 4, FranceS. LoudaghDepartment of Physics, National Tsing Hua University, 30043, Hsinchu, Taiwan, R.O. ChinaSh. A. EhgamberdievAstronomical Institute of Uzbek Academy of Sciences, Astronomicheskaya 33, Tashkent, UzbekistanI. KhamitovAstronomical Institute of Uzbek Academy of Sciences, Astronomicheskaya 33, Tashkent, UzbekistanJ. T. HoeksemaC.S.S.A. Stanford University, 94305, Stanford, CA, U.S.AP. L. Pall�Instituto de Astrofisica de Canarias, La Laguna, Tenerife, EspagneC. R�guloInstituto de Astrofisica de Canarias, La Laguna, Tenerife, Espagne

Solar Physicsjournal1996en

ABI

Annotatsiya

Annotatsiya mavjud emas.

Mavzular

Solar and Space Plasma Dynamics Stellar, planetary, and galactic studies Astro and Planetary Science

Identifikatorlar

DOI: 10.1007/bf00179353

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