ライフサイエンスコーパス: coronal

1 The number of apical, coronal 2 mm thick slices with no fat was 2.9 +/- 0.9 in

2 The coronal 21%-22% 2D RL and the 26%-28% 3D RSA bone loss a

3 The coronal 30%-31% 2D RL and the 41%-42% 3D RSA bone loss c

4 of 0.2 arc seconds, of magnetic braids in a coronal active region that are reconnecting, relaxing an

5 f an elliptical mucosal excision followed by coronal advancement of the flap.

6 Figure 1c: (a) Coronal and (b, c) axial fast spin-echo T2-weighted MR i

7 Figure 1a: (a) Coronal and (b, c) axial fast spin-echo T2-weighted MR i

8 Figure 1b: (a) Coronal and (b, c) axial fast spin-echo T2-weighted MR i

9 Coronal and apical deviations of <2 mm were observed in

10 Lateral (coronal and apical) and angular deviations between virtu

11 iofemoral ligament was best evaluated in the coronal and axial oblique planes, and it serves a restri

12 Pulmonary vein diameter was measured in a coronal and axial view at 3 levels (A, ostium; B, 1 cm m

13 gingival margin (GM) 1.7 mm (P = 0.01) more coronal and KT 3.3 mm (P <0.001) wider than untreated si

14 ies have the highest correlation between the coronal and sagittal images from the Allen Mouse Brain A

15 The term three-plane-assembled means that coronal and sagittal images were generated by reformatti

16 ic confidence, and the benefit of additional coronal and sagittal imaging planes in cePET/CT, PET/MR

17 The width of the SAF was measured on coronal and sagittal MR images.

18 e-foot orthoses exert significant effects on coronal and sagittal plane ankle rotation; and both sagi

19 2000 ms; TE-200 ms] fast spin echo study in coronal and sagittal planes.

20 Secondary coronal and sagittal reconstructions were generated.

21 ) and 60% and 80% ASIR techniques, with 3-mm coronal and sagittal reformations.

22 In all patients, coronal and sagittal reformatted images showed herniatio

23 Coronal and sagittal reformatted images were also formed

24 m in-plane resolution (0.05-mm(3) pixels) in coronal and sagittal slabs (17 sections at 1 mm thick) o

25 The mean +/- SD angular, coronal, and apical deviations were 6.53 degrees +/- 4.3

26 linded, independent readers evaluated axial, coronal, and sagittal CT reformations for overall image

27 irrespective of directionality (transverse, coronal, and sagittal planes) and force direction (compr

28 econstructed with and without MARS in axial, coronal, and sagittal planes.

29 ncluding transverse T1-weighted; transverse, coronal, and sagittal T2-weighted; diffusion-weighted; a

30 This was also true for the 3D TEE and CT coronal annular diameters (P<0.01).

31 wound defect between the bone crest and the coronal aspect of the implant has a positive effect on m

32 oxide surface implants coated in their most coronal aspect with rhBMP-2 (coronal-load, six animals),

33 s in ridge width were most pronounced on the coronal aspect, 1.8 mm for CM and 2.0 mm for ECM, wherea

34 st enhancement were subject to assessment in coronal, axial and sagittal planes.

35 In coronal BF slices from GAD67-GFP knock-in or PV-tdTomato

36 zer in full scan mode was performed on 6 mum coronal brain sections from rats that were administered

37 troposterior nucleus (VP) were visualized in coronal brain sections from two macaque monkeys, two owl

38 hrelin to visualize ghrelin binding sites in coronal brain sections of amygdala.

39 Expression of eGFP in coronal brain sections was compared with GHSR mRNA expre

40 Coronal brain sections were incubated with anti-Nrf2 pri

41 Moreover, in acute coronal brain slices of control mice, Abeta25-35 peptide

42 of high-latitude magnetic activity, such as coronal bright points and ephemeral regions, until the t

43 Flossers showed less coronal caries compared to nonflossers (P = 0.02).

44 Coronal cavities are large low-density regions formed by

45 gh-latitude 'polar crown' prominences within coronal cavities reveal dark, low-density 'bubbles' that

46 es to form dark plumes rising into overlying coronal cavities.

47 oncepts of prominences and their relation to coronal cavities.

48 bservations offered a possible mechanism for coronal cavity evolution, although the nature of the bub

49 ource of the buoyancy, and suggests that the coronal cavity-prominence system supports a novel form o

50 ution of the cylinders with ca. 10% residual coronal chains led to the formation of branched rather t

51 concentric rectangular patches with distinct coronal chemistries.

52 The density, length, and coronal chemistry of the micellar brushes can be precise

53 mity and photocrosslinked through controlled coronal chemistry to generate linear oligomeric arrays.

54 uding rhizomelia, chondrodysplasia punctata, coronal clefts, cervical dysplasia, congenital cataracts

55 into the nature of any relationship between coronal composition and fixed stellar properties.

56 Sun is observed as a star, the variation of coronal composition is highly correlated with a proxy fo

57 is observed as a star, then the variation of coronal composition is highly correlated with the F10.7c

58 Figure 2b: (a) Axial and (b) coronal contrast-enhanced CT images of the upper abdomen

59 Figure 2a: (a) Axial and (b) coronal contrast-enhanced CT images of the upper abdomen

60 S) is a dysmorphic syndrome characterized by coronal craniosynostosis and severe midface hypoplasia,

61 of affected individuals range from syndromic coronal craniosynostosis to severe growth restriction, f

62 Coronal cross-linking followed by nanocrystal dissolutio

63 btained 2 months prior to admission.Figure 3:Coronal CT image of the abdomen acquired 60 seconds afte

64 Preoperative coronal CT scans of 13 patients with and without DON who

65 es resistance potential of acid-etched human coronal dentin bonded using augmented pressure adhesive

66 Beams of coronal dentin were obtained from unrestored 3(rd) molar

67 lated with patient age and with sagittal and coronal diameters of the thorax by using the Student t t

68 are identified unambiguously with conjugate coronal dimmings completely enclosed by irregular bright

69 Sites treated with GAPs resulted in coronal displacement of GM with RecRed up to complete ro

70 aracterization in that the OsO4-stained PMVS coronal domains were observed by TEM, whereas the brush

71 olar phenomena, as well as chromospheric and coronal emission at ultraviolet to X-ray wavelengths.

72 l appearing much less severely affected than coronal enamel.

73 cal P-H-P triblock comicelles with polar (P) coronal ends and a hydrophobic (H) central periphery in

74 Furthermore, the horizontal + coronal ([Formula: see text]) freezing orientation facil

75 However, the coronal heating mechanism remains unknown.

76 hese observations provide constraints on the coronal heating mechanism(s) and highlight the importanc

77 d the corona that is highly sensitive to the coronal heating mechanism.

78 ction sheds light on a critical piece of the coronal heating puzzle.

79 with the potential to meet chromospheric and coronal heating requirements.

80 aps even down to smaller jets that may power coronal heating.

81 for the suggested mechanism(s) for quiescent coronal heating.

82 and the ratio of vertebral coronal width to coronal height (W/H).

83 ssion, while patient sex, age, and the apico-coronal height of the gingiva were related to buccal bon

84 Post-mortem MRI was performed on non-fixed coronal hemispheric brain slices of 23 patients with pro

85 of the optic tract was measured in archived coronal histological sections of the brain of every hemi

86 ers(5,6), from interchange reconnection near coronal hole boundaries(7,8), or within coronal holes wi

87 solar wind emerging from a small equatorial coronal hole.

88 ng in active regions, quiet Sun regions, and coronal holes alike.

89 g, and we provide evidence that low-latitude coronal holes are a key source of the slow solar wind.

90 20 randomly selected X-ray jets that form in coronal holes at the Sun's poles.

91 near coronal hole boundaries(7,8), or within coronal holes with highly diverging magnetic fields(9,10

92 ind is known to emanate primarily from polar coronal holes, the source of the slow wind remains unkno

93 tream of plasma originating from deep within coronal holes.

94 Using whole cell recordings in coronal hypothalamic slices from adult female rats, we d

95 tal imaging included fat-saturated axial and coronal images and high-resolution axial T2-weighted ima

96 ents with staphyloma had larger ARs in quasi-coronal images than in myopic subjects without staphylom

97 y post TBI followed by whole brain axial and coronal images using a wide-field fluorescence microscop

98 y in the lumbosacral spine; however, on STIR coronal images, a right perianal abscess with air pocket

99 ssessment showed preserved sagittal balance, coronal imbalance and valgus knee deformity.

100 y results exist regarding influence of apico-coronal implant placement on crestal bone levels.

101 nd the alveolar crest was significantly more coronal in the SIM group (P = 0.038).

102 mpared two measurement techniques (axial and coronal) in patients with suspected high intracranial pr

103 observe a decrease in the intensity of the F-coronal intensity, which is suggestive of the long-sough

104 Here we report simulations of a coronal jet driven by filament ejection, whereby a regio

105 tly concluded from new observations that all coronal jets are driven by filament ejection, just like

106 gy, as in the kink or torus instability; and coronal jets from a resistive process involving magnetic

107 ichiometric coupling of a polymer surfactant coronal layer (2) produces a highly concentrated, solven

108 We show that the coronal layer structure is responsive to the dielectric

109 which depends on the charge of the copolymer coronal layer, serves to trigger enzymatic dephosphoryla

110 and 2.3 +/- 0.5 versus 2.6 +/- 0.8 mm(2) for coronal-load and soak-load implants, respectively (P >0.

111 ant bone density averaged 72.2% +/- 2.1% for coronal-load versus 60.6% +/- 4.7% for soak-load implant

112 d in their most coronal aspect with rhBMP-2 (coronal-load, six animals), or by immersion of the entir

113 ow-up visit, the papilla index and the apico-coronal location of mid-buccal soft tissue positions wer

114 system, in which we see a large, persistent coronal loop approximately one subgiant diameter in heig

115 meters) at the footpoints of hot and dynamic coronal loops.

116 ng perfusion, determined as the average of 6 coronal lung slices through the anterior, mid, and poste

117 ll infiltrates in tissue blocks and/or whole coronal macrosections encompassing a wide array of brain

118 ns of the Sun is related to the evolution of coronal magnetic field activity.

119 te the capability of imaging spectroscopy in coronal magnetic field diagnostics.

120 Our model simulates the coronal magnetic field following a long-duration quasi-s

121 s not yet been resolved because of a lack of coronal magnetic field measurements and the limitations

122 , thought to be produced by the decay of the coronal magnetic field strength.

123 showing spatial and temporal changes in the coronal magnetic field.

124 map the plane-of-sky component of the global coronal magnetic field.

125 ter-propagating Alfvenic waves exist in open coronal magnetic fields and reveal key observational ins

126 ntz-force change due to the back reaction of coronal magnetic restructuring and is accompanied by a d

127 d, was significantly smaller on sagittal and coronal MARS-reconstructed images than on standard recon

128 ii, similar to values observed during recent coronal mass ejection events.

129 Sun and solar wind during an interplanetary coronal mass ejection impact in March 2015.

130 tabilizes, it can either erupt and produce a coronal mass ejection or fail and collapse back towards

131 tion near the Sun, and an event related to a coronal mass ejection.

132 Coronal mass ejections (CMEs) are episodic eruptions of

133 evere geomagnetic effects of solar storms or coronal mass ejections (CMEs) are to a large degree dete

134 We conclude that if coronal mass ejections and jets are indeed of physically

135 tly reported in Nature, eruptive events like coronal mass ejections and solar flares, are organized i

136 Although coronal mass ejections are common and can significantly

137 Coronal mass ejections are solar eruptions driven by a s

138 sion of the filament eruptions that initiate coronal mass ejections drives the jet-producing reconnec

139 to arise through very different mechanisms: coronal mass ejections from an ideal (non-dissipative) p

140 sit interaction between two closely launched coronal mass ejections resulted in the extreme enhanceme

141 ven eruptions on the Sun, from stellar-scale coronal mass ejections to small-scale coronal X-ray and

142 structures, both observed (solar flares and coronal mass ejections) and predicted (the inner heliosh

143 -annual variability in the number of flares, coronal mass ejections, the radiative and particulate en

144 me, eventually erupting as the dark cores of coronal mass ejections.

145 solar physics mission to reveal a ubiquitous coronal mass supply in which chromospheric plasma in fou

146 ), which are typically associated with large coronal-mass-ejection-driven shocks and compressions mov

147 tion due to interaction with the surrounding coronal material; the EUV absorption by the comet and th

148 Coronal maximum intensity projection (MIP) images of bot

149 ekuboyina et al, which works on sagittal and coronal maximum intensity projections (MIPs) and augment

150 Coronal measurements showed less variability between eac

151 of the mechanisms that create the turbulent coronal medium through which the emitted radiation propa

152 the MALDI-MSI analysis of fine structures in coronal mouse brain slices.

153 At a single institution, surface coil coronal MRI was obtained at 312 mum resolution in quasi-

154 Surface coil coronal MRI was obtained in target-controlled central ga

155 Using observations with the Coronal Multi-channel Polarimeter, we have determined th

156 rad/s) head rotation in the sagittal (n=13), coronal (n=7), or axial (n=31) planes.

157 ed on a statistical model indicated that the coronal nanodomains detected likely result from a segmen

158 icelles of controllable length with "patchy" coronal nanodomains were accessible.

159 s, similar30 seconds) heating events called "coronal nanoflares." The accelerated electrons deposit a

160 .80, respectively; all P values < .0001) and coronal oblique acquisitions (mean values of 0.81, 1.09,

161 vrfSSFSE and conventional SSFSE sagittal and coronal oblique acquisitions were performed in 54 consec

162 l acquisitions and from 1494 to 621 msec for coronal oblique acquisitions.

163 ferior transverse ligament were best seen in coronal oblique planes.

164 their IONs were imaged individually using a coronal-oblique T2-weighted fast multidynamic image acqu

165 led architecture of cells and myelin, within coronal olfactory bulb and cortical sections, and from s

166 ver, evidence of a mechanosensory organ (the coronal organ) employing hair cells in the mouth of tuni

167 th P. atlanticum and D. nationalis possess a coronal organ, in addition to sensory structures contain

168 -planar DT imaging sequence was performed in coronal orientation by using five b values (0, 200, 400,

169 contrast to the sagittal orientation, in the coronal orientation the organization of Purkinje cell re

170 e micelles upon enzyme-triggered cleavage of coronal peptide sidechains.

171 FAN-derived ventilation images on the coronal plane and volumes of interest were compared with

172 WB DWI was performed in the coronal plane using a 1.5-T scanner and a body coil.

173 cal problem, simplified NMR (T1,T2, STIR; in coronal plane) was conducted with a 1.5 Tesla magnet.

174 t tangentially to the pial surface or in the coronal plane, were stained for CTb immunocytochemistry

175 ons involved 0.625 to 0.8-mm sections in the coronal plane, with or without axial planes, through the

176 n which the cortical tissues were cut in the coronal plane.

177 e arborized asymmetrically, primarily in the coronal plane.

178 e less distinct but still symmetrical in the coronal plane.

179 nal planes and with T2 SPACE sequence in the coronal plane.

180 l the brains were fixed and sectioned in the coronal plane; Nissl-stained sections were used for esti

181 was obtained at 312 mum resolution in quasi-coronal planes 2 mm thick throughout the orbit in 20 nor

182 atory triggered HASTE technique in axial and coronal planes and with T2 SPACE sequence in the coronal

183 MRI in quasi-coronal planes was analyzed during target-controlled cen

184 and T2 mapping of cartilage in the axial and coronal planes were performed.

185 nually segmented in the axial, sagittal, and coronal planes.

186 are unknown, though theory predicts that the coronal plasma should be confined in a magnetic loop str

187 PAP) or scaling and root planing followed by coronal polishing (SRP).

188 from the analysis due to the exposure of the coronal portion of the fixture.

189 vere abnormal surface pitting in the tooth's coronal portion.

190 The molars migrated to a more coronal position in ENAM(-/-) mice and mice on HC.

191 mplant-abutment junction provided for a more coronal position of the first point of bone-implant cont

192 A, B, and C, respectively (P<0.01 for all); coronal pulmonary vein diameter decreased by a median of

193 the immediate location of the damage in the coronal pulp tissue with no drug action detected in the

194 lare ribbon propagating across the sunspots, coronal rain (made of condensing plasma) streaming down

195 the chromosphere's response to the impact of coronal rain, showing fine-scale brightenings at the foo

196 (b) Portal venous phase coronal reformatted CT image shows the upper abdomen.

197 ment of soft tissue was observed both in the coronal region due to high fluid velocity, and on the ve

198 nt buildup and final preparation: A) >50% of coronal residual structure or B) equal to or <50% of cor

199 residual structure or B) equal to or <50% of coronal residual structure.

200 l properties of a new calcium-silicate-based coronal restorative material (Biodentine) and a glass-io

201 The largest diameter on the axial plane; coronal, sagittal, and maximal diameter perpendicular to

202 l regions by cytoarchitectonic boundaries in coronal, sagittal, and tangential sections processed for

203 dividing the lung field with equally spaced coronal, sagittal, and transverse planes, perpendicular

204 nization imaging MS data sets of a rat brain coronal section and human larynx carcinoma and discussed

205 even anatomical regions of an MSI image of a coronal section of mouse brain were modeled.

206 Coronal sectioning of e13.5 and e14.5 heads revealed tha

207 scent tracer, and subsequently immunoreacted coronal sections for ZII.

208 ges of metal distribution with corresponding coronal sections from the Allen Mouse Brain Reference At

209 nstrated by blunted STAT3 phosphorylation in coronal sections in response to an intracerebral ventric

210 -silver and peroxidase detection approach in coronal sections in the dorsolateral segment of the stri

211 The pubococcygeal muscles were analyzed on coronal sections obtained through the middle part of the

212 The puborectalis muscles were analyzed on coronal sections obtained through the perineal body.

213 The iliococcygeal muscles were analyzed on coronal sections obtained through the rectum.

214 In individual coronal sections of the brains of seven artiodactyl ungu

215 amined its anatomical organization in serial coronal sections stained alternately with Nissl and Gall

216 Coronal sections through the dorsal hippocampus were pro

217 profile within the cytoplasm, on all serial coronal sections under a confocal microscope, a total of

218 Coronal sections were analyzed utilizing in situ hybridi

219 t rats), their brains were dissected out and coronal sections were immunolabeled for calbindin, calre

220 Serial coronal sections were prepared from a rostrocaudal direc

221 In coronal sections, the different retrogradly labeled habe

222 In the same series of coronal sections, we then determined the total volume of

223 ges from MALDI-TOF IMS datasets of rat brain coronal sections.

224 , few VNNE cells are OMP reactive as view in coronal sections.

225 allizable core-forming blocks and functional coronal segments were coassembled into low-dispersity, o

226 magnetic resonance images (T2-weighted HASTE coronal sequences) from patients with ADPKD to train the

227 Coronal short tau inversion-recovery (STIR)-warp and tra

228 ated for pancreatic cysts by using axial and coronal single-shot fast spin-echo T2-weighted images ob

229 tively activate LGN terminal fields in acute coronal slices containing V1, and recorded monosynaptic

230 However, in coronal slices of the striatum, potentiation of M5 with

231 maging of the brain, which includes thin-cut coronal slices to determine risk of recurrence and the n

232 Tracer influx assessed in coronal slices was increased in agreement with previous

233 0 mum isotropic image volume composed of 256 coronal slices with 71 manually delineated structures an

234 tically treated teeth with CHX placed in the coronal space (test).

235 hrough the central H segment length, L1) and coronal steric effects (via the PtBA corona chain length

236 By manipulation of several factors, namely coronal steric effects (via the PtBA corona chain) and a

237 eafter, T1-warp) images, as well as standard coronal STIR and transverse T1-weighted sequence images

238 Our observations of the coronal streamer evolution confirm the large-scale topol

239 hetic restoration and the amount of residual coronal structure ( P = 0.024; HR, 1.372; 95% CI for HR,

240 nalysis revealed that the amount of residual coronal structure ( P = 0.041; hazard ratio [HR], 2.026;

241 penile cells from 2 anatomical sites (glans/coronal sulcus and shaft) at baseline.

242 Penile lavage samples collected from the coronal sulcus at baseline and 4 weekly visits after MC

243 ith oncogenic types, was slower in the glans/coronal sulcus of the penis of uncircumcised men than ci

244 1.8%-5.6%] among men with HPV-negative glans/coronal sulcus specimens (P = .01).

245 infection among men with HPV-positive glans/coronal sulcus specimens was 1.8 (95% CI, 1.1-2.9), comp

246 3.6%-7.9%) among men with HPV-positive glans/coronal sulcus specimens, versus 3.7% [95% CI, 1.8%-5.6%

247 ), compared with men with HPV-negative glans/coronal sulcus specimens.

248 edian duration of HPV infection of the glans/coronal sulcus was significantly longer in uncircumcised

249 e triangle between the ansate, diagonal, and coronal sulcus were identified in all animals.

250 We found that penile (glans, foreskin, coronal sulcus) T cells and, to a lesser extent, macroph

251 Specimens from the coronal sulcus, glans penis, shaft, and scrotum were obt

252 ng advanced cavitated carious lesions on any coronal surface (moderate to high certainty).

253 on cumulative caries increments on root and coronal surfaces and, among coronal surfaces, on smooth

254 We digitized the coronal surfaces before and 10 min after restoration to

255 ents on root and coronal surfaces and, among coronal surfaces, on smooth (buccal and lingual), occlus

256 f supraorbital mesenchymal cells to form the coronal suture between E11.0 and E13.5.

257 2-TWIST1 heterodimers is critical for normal coronal suture development.

258 NeuC/Mes lineage boundary positioning during coronal suture formation.

259 d mesoderm-derived parietal bone accompanies coronal suture fusion during embryonic development.

260 We show in mouse that coronal suture progenitors originate from hedgehog-respo

261 substitution (p.R3S), in a male patient with coronal suture synostosis.

262 the mesenchymal precursors that generate the coronal suture, an important structural boundary in mamm

263 t these mice exhibit craniosynostosis of the coronal suture, as well as other cranial sutures.

264 to be critical for positioning of the murine coronal suture.

265 rbital regulatory center, which patterns the coronal suture.

266 genic and non-osteogenic compartments at the coronal suture.

267 Nearly all vertebrates have a prominent 'coronal' suture that separates the front and back of the

268 craniosynostosis, specifically involving the coronal sutures, and variable learning disability are th

269 ads to expansion of cartilage underlying the coronal sutures, which contribute to suture closure thro

270 ts were examined with standard MR-sequences, coronal SWMR and radiographs in anteroposterior pelvic v

271 put-collum-diaphyseal angle were measured on coronal SWMR MIP-images, T1weighted MIP-images and radio

272 s predominantly occurred in individuals with coronal synostosis and accounted for 32% and 10% of subj

273 ommend genetic testing when common causes of coronal synostosis have been excluded.

274 -Chotzen syndrome, typically associated with coronal synostosis.

275 on mutations in Tcf12 and Twist1 have severe coronal synostosis.

276 Coronal T1 maps of the lungs were acquired with the pati

277 for attenuation correction and an unenhanced coronal T1-weighted turbo spin-echo (TSE) sequence for b

278 ences that were performed included axial and coronal T2 half-Fourier acquisition single-shot turbo sp

279 Figure 2a: (a) Coronal T2-weighted (repetition time msec/echo time msec

280 Figure 2b: (a) Coronal T2-weighted (repetition time msec/echo time msec

281 Figure 3a: (a) Coronal T2-weighted fat-saturated fast spin-echo (repeti

282 Figure 3c: (a) Coronal T2-weighted fat-saturated fast spin-echo (repeti

283 Figure 3b: (a) Coronal T2-weighted fat-saturated fast spin-echo (repeti

284 Additional axial and coronal T2-weighted images were used to visualize the an

285 d renal sinus fat invasion on transverse and coronal T2-weighted MR images.

286 tario) during the current admission.Figure 2:Coronal T2-weighted MRI (repetition time msec/echo time

287 mygdalar volumetry were performed on oblique coronal T2W and T1W MP-RAGE images respectively.

288 A coronal technique has been studied on healthy volunteers

289 the levator ani muscle complex are noted at coronal thin-section MR imaging with double opacificatio

290 implants from the apical portion to the most coronal thread.

291 Two breath-hold, coronal, three-dimensional, ultrashort-echo-time, gradie

292 n = 30) according to the amount of residual coronal tissues after abutment buildup and final prepara

293 Decreasing biochemical gradients from coronal to apical zones, specifically biomolecules that

294 or bone metastasis screening, which included coronal two-dimensional (2D) whole-body T1-weighted MR i

295 (b) Coronal unenhanced CT image of the mass at the level of

296 igher than those of nonisotropic images with coronal views (median, 3 vs 2, respectively [25th and 75

297 ments of the optic nerve sheath in axial and coronal views either averaged between eyes or the highes

298 (c) Coronal volume-rendering image shows an anterior view of

299 its height (A/H), and the ratio of vertebral coronal width to coronal height (W/H).

300 -scale coronal mass ejections to small-scale coronal X-ray and extreme-ultraviolet jets, have frequen