Results 151 to 160 of about 429,319 (205)
Application of chirp stimuli in Kalman-weighted auditory brainstem response testing. [PDF]
Sci ProgYang J +8 more
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Fu's Subcutaneous Needling treatment for migraine without aura: a randomized controlled trial protocol. [PDF]
Front NeurolGuo W, Yang Y, Sun J.
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Systematic rise in flight cancellations during space weather events. [PDF]
Sci RepLuo RD +17 more
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Exploring the relationship between mental health and urban green space soundscapes: A scoping review. [PDF]
PLoS OneAhmadi E +8 more
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Impact of hearing loss on brain signal variability in older adults under different auditory load conditions. [PDF]
Front Aging NeurosciWang S +7 more
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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
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
AIP Conference Proceedings, 2003
The seemingly un‐magnetized part of the solar surface is not really un‐magnetized. It is occupied by magnetic structures producing low polarization which, therefore, escape detection in traditional measurements. Since most of the solar surface belongs to this category, the quiet Sun magnetic fields can easily carry most of the magnetic flux and energy ...
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The seemingly un‐magnetized part of the solar surface is not really un‐magnetized. It is occupied by magnetic structures producing low polarization which, therefore, escape detection in traditional measurements. Since most of the solar surface belongs to this category, the quiet Sun magnetic fields can easily carry most of the magnetic flux and energy ...
openaire +1 more source