Zobrazeno 1 - 10
of 489
pro vyhledávání: '"G. W. Simon"'
Autor:
John Leibacher, R. Wallace, T. Pope, A. M. Title, M. Finch, R. A. Shine, G. W. Simon, R. Rehse, R. Reeves, H. Ramsey, Z. Frank, T. D. Tarbell, W. Livingston, S. H. Ferguson, R. Lindgren, G. A. Kelly, H. Zirin, J. W. Harvey, L. November, M. Morrill, D. Duncan, Loren W. Acton, N. Ogle, K. Topka
Publikováno v:
Solar System Plasma Physics
The solar surface is the astrophysicist's best laboratory for the study of magnetoconvection. There exists equipartition of magnetic and kinetic energy. Higher up in the thin atmosphere of the solar corona, the gas is 'frozen' into the magnetic field
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::3320e27f2c2017bc9561989956f64d24
https://doi.org/10.1029/gm054p0053
https://doi.org/10.1029/gm054p0053
Autor:
J. C. Kasher, David H. Hathaway, J. A. Pintar, John Leibacher, G. W. Simon, Robert Howard, Frank Hill, Harrison P. Jones, Peter A. Gilman, J. W. Harvey
Publikováno v:
Science. 272:1306-1309
Doppler velocity observations obtained by the Global Oscillation Network Group (GONG) instruments directly measure the nearly steady flows in the solar photosphere. The sun's differential rotation is accurately determined from single observations. Th
Publikováno v:
Solar Physics. 191:227-229
Autor:
G. W. Simon, Nigel Weiss
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 252:1P-5P
Observed patterns of motion at the solar surface reflect the structure of subphotospheric convection, which controls the distribution of angular momentum and magnetic fields. Mesogranules are interpreted as secondary features associated with supergra
Publikováno v:
Solar and Stellar Physics ISBN: 3540186786
The Solar Optical Universal Polarimeter (SOUP) on Spacelab 2 collected time sequences of diffraction limited (0.5 are second) granulation images with excellent pointing (.003 arc seconds) and freedom from the distortion that plagues groundbased image
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::fc21ce076dea273d844a2ce91bf3323b
https://doi.org/10.1007/bfb0032318
https://doi.org/10.1007/bfb0032318
Publikováno v:
Frontiers in Astronomy & Space Sciences. 2024, p01-28. 28p.
Autor:
Routh, Srinjana, Jha, Bibhuti Kumar, Mishra, Dibya Kirti, Van Doorsselaere, Tom, Pant, Vaibhav, Chatterjee, Subhamoy, Banerjee, Dipankar
Publikováno v:
Astrophysical Journal; 11/10/2024, Vol. 975 Issue 2, p1-13, 13p
Autor:
Guo, Yang, Guo, Jinhan, Ni, Yiwei, Xia, Chun, Zhong, Ze, Ding, Mingde, Chen, Pengfei, Keppens, Rony
Publikováno v:
Reviews of Modern Plasma Physics; 9/5/2024, Vol. 8 Issue 1, p1-40, 40p
Autor:
J. B. Zirker, G. W. Simon
Publikováno v:
Solar Physics. 35:331-342
High-resolution measurements of magnetic fields have been made in quiet and active regions in order to determine whether the photospheric fine-structures (‘crinkles’), recently photographed by Dunn (1972), coincide with the footpoints of strong,
Autor:
S. P. Worden, G. W. Simon
Publikováno v:
Symposium - International Astronomical Union. 71:121-134
The evolution of the velocity and magnetic fields associated with supergranulation has been investigated using the Sacramento Peak Observatory Diode Array Magnetograph. The observations consist of time sequences of simultaneous velocity, magnetic fie