Results 211 to 220 of about 30,680 (264)

Touching with torque enables human-level robotic dexterity. [PDF]

Sci Adv
Wang L, Sun Y, Yang L, Sun Y, Guo Q, Liu Y, Chen X, Shen Y.   +7 more
europepmc   +1 more source

Ferromagnet-like binary switching of a Stoner-Wohlfarth antiferromagnet. [PDF]

Nature
Wang Z, Xiang Y, Chen R, Sun Z, Hong C, Chen X, Gao J, Wu S, Guo Z, Chen Y, Mi Q, Liu Z, Yan S, Lei H, Ruan W, Zhang Y, Yu W, Liu WT, Yuan Z, Wu S.   +19 more
europepmc   +1 more source

Magnetic-Dielectric Synergy in One-Dimensional Metal Heterostructures for Enhanced Low-Frequency Microwave Absorption. [PDF]

Nanomicro Lett
Hu F, Zhang P, Ding P, Zhang S, Fan B, Shamshirgar AS, Zheng W, Sun W, Cai L, Xie H, Shao Q, Rosen J, Sun Z.   +12 more
europepmc   +1 more source

Magnetic fields on the quiet Sun [PDF]

Central European Astrophysical Bulletin, 2011
openaire  

Magnetic fields in the sun

Journal of the Franklin Institute, 1974
The observed properties of solar magnetic fields are reviewed, with particular reference to the complexities imposed on the field by motions of the highly conducting gas. Turbulent interactions between gas and field lead to heating or cooling of the gas according to whether the field energy density is less or greater than the maximum kinetic energy ...
Mullan, D. J.
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Magnetic fields of the Sun and stars

Uspekhi Fizicheskih Nauk, 1966
CONTENTS Introduction 1 1. Methods and technique of measuring magnetic fields 2 2. General magnetic field of the Sun 7 3. Strong magnetic fields in active regions of the Sun 14 4.
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The Sun's Magnetic Field

Annual Review of Astronomy and Astrophysics, 1963
The techniques and instruments for measuring the solar magnetic field are outlined. The poloidal field and lowlatitude fields are discussed. The magnetic fields associated with sunspots, flares, stable filaments, and granules are considered. The solar magnetic cycle and related phenomena are also discussed. (C.E.S.)
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Imbalance of magnetic fields on the Sun

Bulletin of the Crimean Astrophysical Observatory, 2009
Differences of magnetic field flows of “+” and “−” polarities, i.e. the imbalance of magnetic fields for 26 years—from January 1, 1977, to September 30, 2003—are investigated,. The synoptic maps of the longitudinal vector of Sun’s magnetic field strength obtained at the Kitt Peak National Observatory (United States) and kindly given to us by Dr.
N. N. Stepanian, O. A. Andryeyeva, Ya. I. Zyelyk   +2 more
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