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Mixing of inclined dense jetsLai, Chung-kei, Chris. January 2009 (has links)
Thesis (M. Phil.)--University of Hong Kong, 2010. / Includes bibliographical references (p. 111-114). Also available in print.
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Interacting binary jets in L1551 IRS 5 protobinary systemLeung, Ka-wing, 梁家榮 January 2012 (has links)
Rodr??guez et al. (2003b) used Very Large Array (VLA) in addition of Pie Town
antenna (PT antenna) to observe the low mass protostellar system, L1551 IRS 5
at 3.5 cm. Their radio map showed two main results: a number of knots along
the two extend radio jets driven from L1551 IRS 5 and the southern jet shows
a peculiar bend at about 0.006 to the southwest of the driving source. To inves-
tigate how the knots formed and what causes the bend in southern jet, I found
three data sets reliable to make the maps from the VLA online data archive
comprising 1994, 2002 and 2003. The 3.5 cm radio continuum maps of three
epochs showed similar jets structure. I denoted the knots as RK A, B, C, D,
E, F and G. For interpreting the nature of the knots seen in both jets and variations in the intensity/structure of the southern jet, I make the difference
maps for multi-epoch comparison. There are no significant residuals (> 4_) for
above-mentioned knots. We measure the velocities of the RKs relative to RK
A: RK C (19 ± 13 kms?1), RK D (7.5 ± 4.7 kms?1 between epoch 1994 and
2002, 85 ± 20 kms?1 between epoch 2002 and 2003), RK E (72 ± 24 kms?1)
and RK G (24 ± 32 kms?1). And the intrinsic velocity of RK B relative to
southern protostar is 3.8 ± 2.8 kms?1. All of them are insignificant (< 4 _).
However, I detected a positive residual with highly significant (> 6_) in all
difference maps. I denoted it as RK H. And I obtained a significant proper
motion of RK H (128 ± 18 kms?1). RK B, C, D, E, F and G are not likely
formed by enhancement in mass loss or internal shock because their 4_ upper
limit velocities are much slower than jet velocities of their corresponding jet.
They can be interpreted by either the model of interaction of the binary jets or
interaction with ambience cloudlets. Since the flux density of RK H is roughly
constant within 1_ so that it is not likely formed by enhancement in mass loss
but it can be explained by internal shock. / published_or_final_version / Physics / Master / Master of Philosophy
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The influence of electrophilic additives on plasma arc jetsZachariah, Poozhikala Chacko 08 1900 (has links)
No description available.
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A shadowgraph study of intermittent flowBlackshear, Perry Lynnfield 08 1900 (has links)
No description available.
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Turbulent structure and emissions of strongly-pulsed jet diffusion flames /Fregeau, Mathieu. January 2007 (has links)
Thesis (Ph. D.)--University of Washington, 2007. / Vita. Includes bibliographical references (leaves 93-98).
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Jet dispersion studies /Beare, John David. January 1974 (has links) (PDF)
Thesis (M.E.) -- University of Adelaide, Department of Civil Engineering, 1976.
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Mixing and combustion in precessing jet flows /Newbold, Gregory, January 1998 (has links) (PDF)
Thesis (Ph.D.)-- University of Adelaide, Dept. of Mechanical Engineering, 1998. / Bibliography: leaves 173-183.
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The formation of stellar jets /Goodson, Anthony P. January 1998 (has links)
Thesis (Ph. D.)--University of Washington, 1998. / Vita. Includes bibliographical references (p. [143]-151).
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Étude théorique du jet de plasma supersonique à courant continuJodoin, Bertrand. January 1998 (has links)
Thèses (Ph.D.)--Université de Sherbrooke (Canada), 1998. / Titre de l'écran-titre (visionné le 20 juin 2006). Publié aussi en version papier.
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Diagnostic study of low pressure supersonic DC plasma jets by emission spectroscopy and enthalphy probe techniques Diagnostic d'un jet de plasma DC supersonique par les techniques de la spectroscopie d'émission et de la sonde enthalpique.Rajabian, Mahmoud. January 2001 (has links)
Thèses (Ph.D.)--Université de Sherbrooke (Canada), 2001. / Titre de l'écran-titre (visionné le 20 juin 2006). Publié aussi en version papier.
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