Results 161 to 170 of about 10,701,163 (203)

Global meta-analysis of plasma-activated water for improving crop establishment, productivity, and health. [PDF]

Front Plant Sci
Ali N, Dong Y.
europepmc   +1 more source

The Solar Wind Electron (SWE) Instrument for the Interstellar Mapping and Acceleration Probe Mission. [PDF]

Space Sci Rev
Skoug RM, Schultz TB, Venhaus DM, Amaya CE, Choedon T, Christian ER, Crosier RD, De Los Santos A, Fernandes PA, Ford JJ, Gkioulidou M, Hanley JJ, Harvey DS, Hoeper PJ, Kubeczka PW, Liu Y, Martinez JP, McComas DJ, Mohr HD, Nunez C, Pacheco TR, Pope SE, Rodriguez H, Sandoval BF, Schiferl CM, Schwadron NA, Spalsbury LC, Seitz DN, Smith RM, Steinberg JT, Storms SA, Toczynski W, Tyler YD, Vigil VJ.   +33 more
europepmc   +1 more source

The Influence of Applied Voltage on Drying Kinetics, Quality, and Mathematical Modeling of Ginger During Electrohydrodynamic (EHD) Drying. [PDF]

Food Sci Nutr
Ding M, Lu J.
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Mapping the Sun's coronal magnetic field using the Zeeman effect. [PDF]

Sci Adv
Schad TA, Petrie GJD, Kuhn JR, Fehlmann A, Rimmele T, Tritschler A, Woeger F, Scholl I, Williams R, Harrington D, Paraschiv AR, Szente J.   +11 more
europepmc   +1 more source

Measuring the magnetic fields in the chromospheres of low-mass stars

Cang T, Petit P, Donati J, Tian H, Fu J, Li H, Bellotti S, Hu X, Ma X, Ariste AL, Xing K, Morin J, Lu H, Zong W.   +13 more
europepmc   +1 more source

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New possibilities of non-eclipse observations of the solar K-corona with liquid-mirror telescopes

Solar Physics, 1991
Experimental and methodical possibilities of modern observations of the solar K-corona have been analyzed. It is shown that for obtaining information on matter distribution and dynamics in the internal solar corona, it is necessary to measure both its polarization component and its total radiation in the continuum.
Rock, K, Fisher, R, Garcia, C, Seagraves, P, Yasukawa, E   +4 more
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The K-corona under hydrostatic density distribution: Relevance to solar wind

Solar Physics, 1986
An analytical expression is obtained for the K-corona brightness as a function of the distance from the solar limb. The agreement of the theory with the numerous observational data indicates that the density distribution at the levels located at 1.2–2.5 R ⊙ heliocentric distances may be treated as hydrostatic with T = const.
O. G. Badalyan, M. A. Livshits
openaire   +1 more source