「coronal」の共起表現一覧(1語右で並び替え)

coronal

1語右で並び替え

該当件数:50件

  • Coronal, a collection of verses (1931)
  • in 1978, she turned her attention to stellar coronal and chromospheric activity.
  • a limited extent as found in studies of near coronal and corona activity.
  • stosis (complete skull-joint closure) of both coronal and lambdoid sutures, facial hypoplasia (unde
  • Main article: Coronal cloud
  • The X-ray luminosity (Lx) of the galactic coronal cloud is 1.5 x 1040 erg s−1.
  • a in the chromosphere, transition region, and coronal cloud rotates at the same rate as the photosp
  • I region of hydrogen, a molecular cloud, or a coronal cloud.
  • I region of hydrogen, a molecular cloud, or a coronal cloud.
  • of the baryons in the universe reside in the coronal clouds that compose the hot intergalactic med
  • onic mass dominated by X-ray emitting plasma ( coronal clouds), which is ten times the mass of the s
  • ere are also accounts from the Vietnam War of coronal cranial impalement.
  • TRACE (Transition Region and Coronal Explorer) was a NASA space telescope designed
  • b in his hand, and smote at the king that his coronal fell to the earth.
  • This coronal gas may be sustained by the galactic fountain
  • Modeling of M dwarfs suggests that the coronal geometry for low-mass dwarfs is dominated by
  • own for his wave heating theory involving the Coronal heating problem of the Sun's atmosphere.
  • an apparent lack of a change in coronal heating efficiency going from stars which hav
  • phenomena, and as an explanation of the solar coronal heating problem.
  • umber of solar phenomena, including sunspots, coronal heating, wave propagation, magnetic instabili
  • Helium-I Imager - Chromosphere ~ 2000 km and coronal holes
  • Polar coronal holes (about north and south poles) shown her
  • ed forecasters to see space phenomena such as coronal holes, whose geomagnetic storms impact power
  • camera for coronal imaging at 2000-3000 A and up to 24 Solar rad
  • g family of dark and wood elves of Miyeritar, Coronal Ivosaar Vyshaan chose to make a claim toward
  • y of the transition to an upper energy level, coronal lines are emission lines produced by metal io
  • the TRACE instrument is the fine structure of coronal loops low in the solar atmosphere.
  • tar could have blown off a volatile layer via coronal mass ejection.
  • Understand the initiation and evolution of coronal mass ejections (CMEs) and interplanetary shoc
  • causing this event was itself the result of a coronal mass ejection on March 9, 1989.
  • ssion for ICE consisting of investigations of coronal mass ejections in coordination with ground-ba
  • The comet was hit by a coronal mass ejection during its pass near the sun; s
  • S 14 for the early detection of solar flares, coronal mass ejections (CME)s and other X-ray generat
  • c outbursts to produce so-called superflares ( coronal mass ejections) that release between 100 and
  • CoMP Coronal Multi-channel Polarimeter - Near IR Coronal P
  • the Sun and the solar system (radioastronomy, coronal plasma, cometary and interplanetary dust), hi
  • Coronal section through mid-brain.
  • Human brain frontal ( coronal) section
  • Coronal section through right talocrural and talocalc
  • Coronal section of brain through intermediate mass of
  • Coronal section of anterior part of pelvis, through t
  • It is a narrow white band, triangular on coronal section, the apex being directed upward.
  • rticularly a green line) were observed in the coronal spectrum during solar eclipses that did not c
  • The coronal stops differ not so much in the location of t
  • he anatomical point on the skull at which the coronal suture is intersected perpendicularly by the
  • bregma is located at the intersection of the coronal suture and the sagittal suture on the superio
  • laced at the junction of the sagittal suture, coronal suture, and frontal suture; it is lozenge-sha
  • rd, and join the galea aponeurotica below the coronal suture.
  • At coronal temperatures, electrons, due to their much sm
  • incidence X-ray telescope designed to record coronal x-ray images in continuous sequence at 1-minu