Results 151 to 160 of about 3,094 (200)

Gonystylones A-E, Antiproliferative 5,6-Dihydro-α-pyrones from the Plant <i>Gonystylus borneensis</i>. [PDF]

J Nat Prod
Kim CK, Freire VF, Dey S, Woldemichael GM, Kim YY, Wen X, Chou HC, Song YK, Wei JS, Akee RK, Orfanoudaki M, Dalilian M, Khan J, Grkovic T, O'Keefe BR.   +14 more
europepmc   +1 more source

The Development of CDC25A-Derived Phosphoseryl Peptides That Bind 14-3-3ε with High Affinities. [PDF]

Int J Mol Sci
Kamayirese S, Maity S, Hansen LA, Lovas S.   +3 more
europepmc   +1 more source

Introduction to Solar Spectropolarimetry.

, 2017
openaire   +1 more source

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Introduction to Spectropolarimetry

2003
Spectropolarimetry embraces the most complete and detailed measurement and analysis of light, as well as its interaction with matter. This book provides an introductory overview of the area, which plays an increasingly important role in modern solar observations.
Jose Carlos del Toro Iniesta
exaly   +2 more sources

Solar spectropolarimetry with THEMIS

EAS Publications Series, 2003
We report spectropolarimetric observations with THEMIS telescope multi-lines operating mode (MTR) during the last campaigns. We demonstrate the very favorable performances of THEMIS for investigations of the magnetic field and we report also observations devoted to the measurement of the scattering polarization.
Molodij, Guillaume, Rayrole, Jean
openaire   +3 more sources

UV Spectropolarimetry With Polstar: Protoplanetary Disks [PDF]

Astrophysics and Space Science, 2022
Polstar is a proposed NASA MIDEX mission that carries a high resolution UV spectropolarimeter capable of measure all four Stokes parameters onboard a 60 cm telescope. The mission has been designed to pioneer the field of time-domain UV spectropolarimetry.
John Wisniewski, Richard Ignace, William C Danchi   +2 more
exaly   +2 more sources

Ultraviolet Spectropolarimetry: On the Origin of Rapidly Rotating B Stars [PDF]

Astrophysics and Space Science, 2022
UV spectroscopy and spectropolarimetry hold the key to understanding certain aspects of massive stars that are largely inaccessible with optical or longer wavelength observations. This is especially true for the rapidly-rotating Be and Bn stars, owing to
Carol E Jones, J P Wisniewski, K G Gayley   +2 more
exaly   +3 more sources

Spectropolarimetry and Magnetic Structures

2019
Kiyoshi Ichimoto
exaly   +2 more sources