Results 131 to 140 of about 1,371 (185)

Magnetic Reconnection in Space: An Introduction. [PDF]

Space Sci Rev
Burch JL, Nakamura R.
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Evidence for small-scale torsional Alfvén waves in the solar corona. [PDF]

Nat Astron
Morton RJ, Gao Y, Tajfirouze E, Tian H, Van Doorsselaere T, Schad TA.   +5 more
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Ordinal Spectrum: Mapping Ordinal Patterns into Frequency Domain. [PDF]

Entropy (Basel)
Chavez M, Martínez JH.
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Spectral synthesis techniques for supernovae and kilonovae. [PDF]

Living Rev Comput Astrophys
Jerkstrand A.
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Newly formed dust within the circumstellar environment of SN Ia-CSM 2018evt. [PDF]

Nat Astron
Wang王 L灵, Hu M, Wang L, Yang 杨 Y轶, Yang J, Gomez H, Chen S, Hu L, Chen TW, Mo J, Wang X, Baade D, Hoeflich P, Wheeler JC, Pignata G, Burke J, Hiramatsu D, Howell DA, McCully C, Pellegrino C, Galbany L, Hsiao EY, Sand DJ, Zhang J, Uddin SA, Anderson JP, Ashall C, Cheng C, Gromadzki M, Inserra C, Lin H, Morrell N, Morales-Garoffolo A, Müller-Bravo TE, Nicholl M, Gonzalez EP, Phillips MM, Pineda-García J, Sai H, Smith M, Shahbandeh M, Srivastav S, Stritzinger MD, Yang S, Young DR, Yu L, Zhang X.   +46 more
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The Sunrise Ultraviolet Spectropolarimeter and Imager: Standalone polarimetric calibration

Iglesias FA, Feller A, Gandorfer A, Riethmüller TL, Korpi-Lagg A, Solanki SK, Katsukawa Y, Kubo M, Toledo MS.   +8 more
europepmc   +1 more source

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The photospheric network

Solar Physics, 1968
Spectroheliograms, obtained in certain Fraunhofer lines with the 82-cm solar image at the Kitt Peak National Observatory, show a bright photospheric network having the following properties: (1) It resembles, but does not coincide with, the chromospheric network, the structure of the photospheric network being finer and more delicate than the ...
G. A. Chapman, N. R. Sheeley
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Solar Photosphere

2020
Abstract The Sun is a G2V star with an effective temperature of 5780 K. As the nearest star to Earth and the biggest object in the solar system, it serves as a reference for fundamental astronomical parameters such as stellar mass, luminosity, and elemental abundances. It also serves as a plasma physics laboratory.
L P Chitta, H N Smitha, S K Solanki
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The Photosphere of the Sun

1959
An empirical model of the photosphere rests on observations of: (1) the solar constant—which fixes the temperature scale, (2) limb darkening—from which the variation of temperature with depth throughout the atmosphere is determined, and (3) the energy distribution—which, together with limb darkening, reveals the opacity at each depth and for each ...
Leo Goldberg, A. Keith Pierce
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The Photosphere

1992
© Springer Science+Business Media Dordrecht 1992.
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