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Noisy galvanic vestibular stimulation improves postural stability under virtual reality perturbation by enhancing vestibular processing and multisensory integration. [PDF]
J Neuroeng RehabilXie H +5 more
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Accuracy and time efficiency of an automated commercial audiometer in the evaluation of hearing in quiet and noisy environments. [PDF]
Sci ProgYi Y, Wang XR, Xiong Q, Xiong GX.
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Acute effects of Tai Chi with different practice emphasis on autonomic activity. [PDF]
Front Sports Act LivingDuan D, Huang H, Li W, Xiao C, Wang D.
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The fine structure of the quiet Sun
Solar Physics, 1985The observed properties of the small-scale features visible in the quiet photosphere — the granulation, of convective origin, and the network bright points, associated with kG magnetic fields — are described. The known properties of the magnetic flux tubes associated with network bright points are also presented.
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Scientific American, 2010
The article discusses the solar cycle which is an eleven-year period in which the Sun's activity fluctuates. According to the author, sunspots, which are magnetic markers on the Sun's surface, provide helioseismologists with visual cues to the cycle's evolution.
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The article discusses the solar cycle which is an eleven-year period in which the Sun's activity fluctuates. According to the author, sunspots, which are magnetic markers on the Sun's surface, provide helioseismologists with visual cues to the cycle's evolution.
openaire +1 more source
Solar Physics, 1979
Macrospicules have been observed in Hα and He i D3, on the disk and above the limb. In 1975, a rate of 1400 (A⊙day)−1 is inferred, and the ratio of equatorial to polar rates ≲ 2. D3 intensities are a few × 10−3 of the disk center, and do not decrease in coronal holes. The ratio of Hα to D3 intensities is ≈ 10.
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Macrospicules have been observed in Hα and He i D3, on the disk and above the limb. In 1975, a rate of 1400 (A⊙day)−1 is inferred, and the ratio of equatorial to polar rates ≲ 2. D3 intensities are a few × 10−3 of the disk center, and do not decrease in coronal holes. The ratio of Hα to D3 intensities is ≈ 10.
openaire +1 more source
2019
Total solar eclipses provide a unique view of the faint solar corona, without the bright over-powering emission from the solar disk, enabling us to explore the electron density, temperature, thermodynamics, and related fundamental physics (Habbal et al. 2010a, 2011, 2013).
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Total solar eclipses provide a unique view of the faint solar corona, without the bright over-powering emission from the solar disk, enabling us to explore the electron density, temperature, thermodynamics, and related fundamental physics (Habbal et al. 2010a, 2011, 2013).
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Radio Observations of the Quiet Sun
2004While radio observations of the Sun have mostly focused on active region phenomena, they also contribute unique data to our knowledge of the quiet Sun, in particular through accurate measurements of the temperature as a function of height in the atmosphere and through the measurement of nonthermal emissions from chromospheric and coronal heating events.
Christoph U. Keller, Säam Krucker
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Physics Today, 1974
An up-to-date textbook of solar physics is presented. The solar structure and processes, and the interior are described along with the photosphere, the chromosphere, and the corona. The strongest Fraunhofer lines, visible coronal lines, and coronal UV, XUV, and X-ray lines are listed.
Edward G. Gibson, Robert D. Chapman
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An up-to-date textbook of solar physics is presented. The solar structure and processes, and the interior are described along with the photosphere, the chromosphere, and the corona. The strongest Fraunhofer lines, visible coronal lines, and coronal UV, XUV, and X-ray lines are listed.
Edward G. Gibson, Robert D. Chapman
openaire +1 more source