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Coronal and loops
Coronal loops are the basic structures of the magnetic solar corona.
Coronal loops may have lifetimes in the order of seconds ( in the case of flare events ), minutes, hours or days.
Coronal loops have become very important when trying to understand the current coronal heating problem.
report the detection of damped transverse oscillations of solar coronal loops observed with the EUV imager on board the Transition Region And Coronal Explorer ( TRACE ), interpreted as standing kink ( or " Alfvénic ") oscillations of the loops.

Coronal and are
Coronal streamers are considered as sources of the slow solar wind.
Coronal holes are the polar regions which look dark in the X-rays since they do not emit much radiation.
In addition, Coronal mass ejections from the Sun are highly dangerous, and are fatal within a very short timescale to humans unless they are protected by massive shielding.
Coronal consonants are consonants articulated with the flexible front part of the tongue.
Coronal stars, or stars within a coronal cloud, are ubiquitous among the stars in the cool half of the Hertzsprung-Russell diagram.
Among his best-known early works are the illustrations he produced for The Book of British Ballads ( 1842 ), and a frontispiece he designed for The Kentish Coronal ( 1840 ).
Coronal mass ejections and their associated shock waves are also important drivers of space weather as they can compress the magnetosphere and trigger geomagnetic storms.
Coronal mass ejections are often associated with other forms of solar activity, most notably solar flares, but a causal relationship has not been established.
Coronal mass ejections are usually observed with a white-light coronagraph.
Coronal mass ejections are often associated with other forms of solar activity, most notably:
The Coronal, Pontifex, Lady of the Isle ( of Sleep ), and King of Dreams are all humans as are the bulk of their respective staffs.
Two primary experiments are the Ultraviolet Coronal Spectrometer from the Smithsonian Astrophysical Observatory, and the White Light Coronograph ( WLC ) from the High Altitude Observatory.
Shown are T1-weighted ( a ) pre-contrast and ( b ) post-contrast Coronal plane | coronal images.
* Coronal sounds are articulated with the tip and / or blade of the tongue.

Coronal and highly
The planet is ruled by an unusual tetrarchy: an adoptive Coronal rules in a highly visible and symbolic manner from his palace atop Castle Mount ; the previous Coronal retires to become the Pontifex, the head of the bureaucracy in an underground Labyrinth ; the Coronal's mother becomes the Lady of the Isle of Sleep, promoting the morals of Majipoor by sending dreams to its inhabitants ; while a hereditary King of Dreams on the distant continent of Suvrael punishes wrongdoers by visiting them with nightmares.

Coronal and by
The first detection of a Coronal mass ejection ( CME ) as such was made on December 1, 1971 by R. Tousey of the US Naval Research Laboratory using OSO 7.
** The Coronal Multi-channel Polarimeter ( CoMP ) monitors the magnetic field in the corona by recording the strength and polarization of light received from corona.
* Coronal axis or frontal axis is the axis perpendicular to the coronal plane, i. e., the one formed by the intersection of the sagittal and the transversal planes.

Coronal and instruments
* The Advanced Coronal Observing System ( ACOS ) is a set of instruments for monitoring the chromosphere on a shared mount.

Coronal and TRACE
* TRACE ( Transition Region and Coronal Explorer ), a NASA satellite
* Transition Region and Coronal Explorer ( TRACE ), launched 1998, decommissioned 2010.

Coronal and solar
Coronal mass ejections have been tracked as far out in the solar system as Saturn.
* October 19, 1989, a large solar event included the full array of space weather effects: Solar Energetic Particles, Coronal Mass Ejection, Forbush decrease, ground level enhancement, geomagnetic storm, etc ..
Coronal mass ejections release huge quantities of matter and electromagnetic radiation into space above the sun's surface, either near the corona ( sometimes called a solar prominence ) or farther into the planet system or beyond ( interplanetary CME ).
Coronal mass ejections, along with solar flares of other origin, can disrupt radio transmissions and cause damage to satellites and electrical transmission line facilities, resulting in potentially massive and long-lasting power outages.
* Coronal dimming ( long-term brightness decrease on the solar surface )
* Coronal mass ejection, a massive burst of solar wind and other ejecta from a star
* Coronal mass ejection ( CME ), a massive burst of solar wind, sometimes associated with solar flares
* 2007: Tomczyk, et al., report the detection of Alfvénic waves in images of the solar corona with the Coronal Multi-Channel Polarimeter ( CoMP ) instrument at the National Solar Observatory, New Mexico.
His main interest has been solar physics research, and he was instigator of the first multi-observatory observation of coronal mass ejections, joint leader at the 81. 5 MHz radio array at Cambridge, principal scientists for the first mm observations of the Sun and principal investigator of the Coronal Diagnostic Spectrometer on SOHO.

Coronal and wave
He is best known for his wave heating theory involving the Coronal heating problem of the Sun's atmosphere.

Coronal and .
* Dr. Ignatov ’ s methodic for Color Coronal ( Kirlian ) spectral analysis, Sofia, Bulgaria
Coronal plane.
Image: Gray402. png | Coronal section of pelvis, showing arrangement of fasciæ.
Image: Gray954. png | Coronal section of larynx and upper part of trachea.
Image: Gray744. png | Coronal section of brain through anterior commissure.
The " Dividing Line " as giant stars evolve to become red giants also coincides with the Wind and Coronal Dividing Lines.
Image: Gray710. png | Coronal section through mid-brain.
Image: Gray717. png | Coronal section of brain immediately in front of pons.

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