Results 271 to 280 of about 4,306,191 (296)

Observing the Solar Magnetic Field

2000
Problems of “weak” magnetic fields diagnostics in the upper solar atmosphere are discussed, where the Zeeman splitting is 3-4 orders of magnitude less than the line width. This corresponds to magnetic observations of chromosphere, prominences and the corona requiring more advanced technique as compared with the photosphere.
openaire   +1 more source

Enhancement of Solar Pond Stability Performance Using an External Magnetic Field

Energy Conversion and Management, 2021
J F Zhang, Z G Qu
exaly  

Optimizing Photothermal Conversion Efficiency in a Parabolic Trough Direct Absorption Solar Collector Through Ferrofluid and Magnetic Field Synergy

Energy Conversion and Management, 2023
Chungen Yin, Dan Zheng
exaly  

Magnetic Fields in the Solar Convection Zone

Living Reviews in Solar Physics, 2009
Yuhong Fan
exaly  

Multiparametric Prostate Magnetic Resonance Imaging in the Evaluation of Prostate Cancer

Ca-A Cancer Journal for Clinicians, 2016
Peter A Pinto, Bradford J. Wood, Sandeep Sankineni   +2 more
exaly  

Solar Magnetic Fields

2018
openaire   +1 more source

Solar Magnetic Fields.

Science (New York, N.Y.), 2010
V, Bumba, R, Howard
openaire   +1 more source

Computational Modeling of Magnetic Fields in Solar Active Regions

Space Science Reviews, 1989
Takashi Sakurai
exaly  

Solar Magnetic Fields

1971
openaire   +1 more source

Solar Vortices and Magnetic Fields.—I

Scientific American, 1910
openaire   +1 more source