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Coronal and loops
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.
Coronal loops are highly radiating sources of plasma and therefore easy to observe by instruments such as TRACE ; they are highly observable laboratories to study phenomena such as solar oscillations, wave activity and nanoflares.
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 magnetic
Coronal arches connecting regions of opposite magnetic polarity ( A ) and the unipolar magnetic field in the coronal hole ( B )
He is best known for his magnetic twisting theory involving the Coronal heating problem of the Sun's atmosphere.
** 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 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 .
* 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.
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.
Image: Gray710. png | Coronal section through mid-brain.
Image: Gray717. png | Coronal section of brain immediately in front of pons.

loops and are
Alkanes ( also known as paraffins or saturated hydrocarbons ) are chemical compounds that consist only of hydrogen and carbon atoms and are bonded exclusively by single bonds ( i. e., they are saturated compounds ) without any cycles ( or loops ; i. e., cyclic structure ).
Saturated hydrocarbons can also combine any of the linear, cyclic ( e. g., polycyclic ) and branching structures, and they are still alkanes ( no general formula ) as long as they are acyclic ( i. e., having no loops ). They also have single covalent bonds between their carbons.
These are generally called " jumps " and facilitate behavior like loops, conditional program execution ( through the use of a conditional jump ), and functions in programs.
Richard Hanley argues that causal loops are not logically, physically, or epistemically impossible: " timed systems, the only possibly objectionable feature that all causal loops share is that coincidence is required to explain them.
Sometimes, the yarns being plied are fed at different rates, so that one yarn loops around the other, as in bouclé.
Stitches are made by pulling one or more loops through each loop of the chain.
Associated with sunspots are coronal loops, loops of magnetic flux, upwelling from the solar interior.
The active regions are ensembles of loop structures connecting points of opposite magnetic polarity in the photosphere, the so called coronal loops.
These loops are the closed-magnetic flux cousins of the open-magnetic flux that can be found in coronal hole ( polar ) regions and the solar wind.
Usually coronal loops lasting for long periods of time are known as steady state or quiescent coronal loops, where there is a balance in loop energy sources and sinks ( example ).
Large-scale structures are very long arcs which can cover over a quarter of the solar disk but contain plasma less dense than in the coronal loops of the active regions.
Larger defects in an ordered structure are usually considered dislocation loops.
The only known mechanisms for the creation of magnetic dipoles are by current loops or quantum-mechanical spin since the existence of magnetic monopoles has never been experimentally demonstrated.
Internal factors not only control ecosystem processes but are also controlled by them and are often subject to feedback loops.
Consequently, they are often subject to feedback loops.

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