Zobrazeno 1 - 10
of 88
pro vyhledávání: '"R. A. Shine"'
Autor:
R. Krishnan, Raji, Prasad, E., Boniface Fernandez, Francis, Johnson, Elizabath, R. Chandran, Shine, Nishad, K.V, Prema, K.H.
Publikováno v:
In Chemical Physics Letters August 2024 848
Autor:
P. J. MacNeice, Ester Antonucci, G. M. Simnett, Helen E. Mason, Brian R. Dennis, C. Jordan, R. A. Shine, David M. Rust, R. Pallavicini
We describe and analyse observations of an M1.4 flare which began at 17: 00 UT on 12 November, 1980. Ground based Hα and magnetogram data have been combined with EUV, soft and hard X-ray observations made with instruments on-board the Solar Maximum
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7d7be63df1321f5108187c7df67bf2c0
https://doi.org/10.1007/bf00157307
https://doi.org/10.1007/bf00157307
Publikováno v:
Journal of Materials Engineering and Performance. 10:371-377
This study investigated stress corrosion cracking (SCC) of A588 steel welds as determined by U-bend immersion tests and slow strain rate tensile (SSRT) tests to evaluate the steel’s cracking susceptibility in various regions of the weldments. The i
Autor:
Takenori J. Okamoto, Z. Frank, R. A. Shine, A. M. Title, Thomas E. Berger, M. Kubo, T. D. Tarbell, Bruce W. Lites, Kenichi Otsuji
Publikováno v:
The Astrophysical Journal. 718:474-487
We present comprehensive observations of the formation and evolution of a filament channel within NOAA Active Region (AR) 10978 from Hinode/Solar Optical Telescope and TRACE. We employ sequences of Hinode spectro-polarimeter maps of the AR, accompany
Autor:
R. A. Shine, T. D. Tarbell, M. Nagase, Kazuhide Kodeki, Shin Nagata, Yoshinori Suematsu, Christopher G. Edwards, Kiyoshi Ichimoto, E. Thomas, Toshifumi Shimizu, Osamu Ito, K. Kobayashi, S. Sour, Masaki Tabata, Saku Tsuneta, Yasuhiro Kashiwagi, R. Rehse, K. Matsuzaki, C. Hoffmann
Publikováno v:
Solar Physics. 249:221-232
The Hinode Solar Optical Telescope (SOT) is the first space-borne visible-light telescope that enables us to observe magnetic-field dynamics in the solar lower atmosphere with 0.2 – 0.3 arcsec spatial resolution under extremely stable (seeing-free)
Publikováno v:
Astronomy & Astrophysics. 379:1052-1082
We analyze oscillations in the solar atmosphere using image sequences from the Transition Region and Coronal Explorer (TRACE) in three ultraviolet passbands which sample the upper solar photosphere and low chromosphere. We exploit the absence of atmo
Autor:
Jay A. Bookbinder, Harry P. Warren, R. A. McMullen, R.W. Nightingale, B. De Pontieu, R. A. Shine, J. Wolfson, B. N. Handy, Lyndsay Fletcher, T. D. Tarbell, Leon Golub, A. M. Title, Charles C. Kankelborg, Neal E. Hurlburt, Edward E. DeLuca, Carolus J. Schrijver, Thomas E. Berger
Publikováno v:
Solar Physics. 187:261-302
The Transition Region and Coronal Explorer (TRACE) – described in the companion paper by Handy et al. (1999) – provides an unprecedented view of the solar outer atmosphere. In this overview, we discuss the initial impressions gained from, and int
Autor:
J. E. Wiik, L. van Driel-Gesztelyi, B. Schmieder, Z. Frank, T. D. Tarbell, Jean-Marie Malherbe, R. A. Shine
Publikováno v:
The Astrophysical Journal. 482:535-540
The main objective of this paper is to present a quantitative study of the dynamics of the evolution of Hα postflare loops developed after a large solar flare and the processed videos produced from the observations. The high spatial resolution of th
Publikováno v:
Marine pollution bulletin. 75(1-2)
Polonium-210 activity concentration was analysed in the whole body tissue of periwinkle Littorina undulata collected from intertidal rocky shore along Kudankulam coast. We carried out the study for a period of 12 months (2011-2012) focusing on three
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