• Study Resource
  • Explore
    • Arts & Humanities
    • Business
    • Engineering & Technology
    • Foreign Language
    • History
    • Math
    • Science
    • Social Science

    Top subcategories

    • Advanced Math
    • Algebra
    • Basic Math
    • Calculus
    • Geometry
    • Linear Algebra
    • Pre-Algebra
    • Pre-Calculus
    • Statistics And Probability
    • Trigonometry
    • other →

    Top subcategories

    • Astronomy
    • Astrophysics
    • Biology
    • Chemistry
    • Earth Science
    • Environmental Science
    • Health Science
    • Physics
    • other →

    Top subcategories

    • Anthropology
    • Law
    • Political Science
    • Psychology
    • Sociology
    • other →

    Top subcategories

    • Accounting
    • Economics
    • Finance
    • Management
    • other →

    Top subcategories

    • Aerospace Engineering
    • Bioengineering
    • Chemical Engineering
    • Civil Engineering
    • Computer Science
    • Electrical Engineering
    • Industrial Engineering
    • Mechanical Engineering
    • Web Design
    • other →

    Top subcategories

    • Architecture
    • Communications
    • English
    • Gender Studies
    • Music
    • Performing Arts
    • Philosophy
    • Religious Studies
    • Writing
    • other →

    Top subcategories

    • Ancient History
    • European History
    • US History
    • World History
    • other →

    Top subcategories

    • Croatian
    • Czech
    • Finnish
    • Greek
    • Hindi
    • Japanese
    • Korean
    • Persian
    • Swedish
    • Turkish
    • other →
 
Profile Documents Logout
Upload
Modeling of Intense Laser Driven High Energy Density Plasmas
Modeling of Intense Laser Driven High Energy Density Plasmas

PETAL: A Research Pathway to Fossil
PETAL: A Research Pathway to Fossil

... measured for PETAL's altitudinal tracking motion. In order to provide a precise characterization of PETAL’s tracking accuracy, use was again made of a CCD camera rigidly attached to the dish surface. This time the camera was aligned parallel to the optical axis of the dish so that it could view the ...
Formation and Disruption of Cosmological Low Mass Objects
Formation and Disruption of Cosmological Low Mass Objects

... luminous objects such as galaxies and QSOs. On the other hand, the reionization of the intergalactic medium and the presence of heavy elements at high-z suggest that there are other population of luminous objects, which precedes normal galaxies. Thus, theoretical approach to reveal the formation mec ...
High-Energy Emission from the PSR B1259
High-Energy Emission from the PSR B1259

Star formation bursts in isolated spiral galaxies
Star formation bursts in isolated spiral galaxies

THE DYNAMICAL STRUCTURE AND EVOLUTION OF GIANT
THE DYNAMICAL STRUCTURE AND EVOLUTION OF GIANT

The Nature of Earth:
The Nature of Earth:

... "primeval atom." Because of the conditions of temperature and pressure that would have existed in such a sphere, matter as we know it could not exist. What existed within the sphere were basic atomic particles called quarks and leptons. B. Another theory proposes that the entire universe was contain ...
Year Long Plan: School Name
Year Long Plan: School Name

(1965)
(1965)

... nature but is also more difficult to apply than the much simpler "energy balance method". It is shown that the "energy balance method" gives very good results for the conditions of interest in this work. The theory becomes completely determinate with the "cylindrical growth and instability break-up ...
Accretion and radial disk structure
Accretion and radial disk structure

The Origin of Life from Primordial Planets
The Origin of Life from Primordial Planets

Document
Document

Studying explosive phenomena in astrophysics by the example of
Studying explosive phenomena in astrophysics by the example of

... Necessary instruments of studying stellar explosion were developed as a part of doctoral research: code for solving systems of nuclear reaction equations was incorporated into hydrodynamical code. These tools were applied for supernovae simulations in order to find possible connection with GRBs. Bas ...
Modeling non-thermal emission from stellar bow shocks
Modeling non-thermal emission from stellar bow shocks

... (2012), where different non-thermal processes are proposed to explain the origin of the emission in these shocks. Further details on the non-thermal processes are also found in Adams (1980), Kelner et al. (2006), Longair (2011) or Rybicki & Lightman (1979), and other contributions to the explanation ...
Chandra HETGS Multiphase Spectroscopy Of The Young
Chandra HETGS Multiphase Spectroscopy Of The Young

... Feldmeier et al. 1997b), in which shocks form from interactions between wind streams that are flowing radially away from the star at moderately different speeds. What makes the MCWS shocks more efficient than instabilitydriven wind shocks is the velocity contrast experienced in the shocks. The magne ...
An exceptionally bright flare from SGR 1806–20 and the origins of
An exceptionally bright flare from SGR 1806–20 and the origins of

... neutron star interior (density r1015 r15 g cm23 ) is Dt < 2R=V A < 0:2B21 p15 s: Thus the 27 December event could have been a crustal instability that drove helicity from the star19,26. The unwinding of a toroidal magnetic field embedded in the crust is strongly impeded by the stable stratification ...
Superconductive bolometers and calorimeters
Superconductive bolometers and calorimeters

... a poor charge meter! The transfer function is UA = I RF if there is no parasitic capacitance Cp . Such Cp , however, is in practice always present and this applies especially to the bolometer, where the parasitic capacitance is the heat capacity of the absorber. The transfer function of a current me ...
STAR FORMATION IN ISOLATED DISK GALAXIES. II. SCHMIDT
STAR FORMATION IN ISOLATED DISK GALAXIES. II. SCHMIDT

III Ionized Hydrogen (HII) Regions
III Ionized Hydrogen (HII) Regions

11.6 Protoplanetary disks
11.6 Protoplanetary disks

Master`s thesis: On the investigation of dark matter haloes
Master`s thesis: On the investigation of dark matter haloes

... sense that, faint stars have large positive magnitudes and bright stars have low even negative magnitudes. The Greeks not only gave us the magnitude system but also one of the first rational models of the Universe. They believed in the perfection of geometry and that this (divine) geometry also gove ...
Presentation in PDF format.
Presentation in PDF format.

... Allow to expand adiabatically until pressure within is equal to pressure outside. Release the element. If it continues to move upwards, the layer is convectively unstable. If it remains stationary or sinks, the layer is stable against convection. It may be shown that the condition for convective equ ...
Detailed modeling of the evaporation and thermal decomposition of
Detailed modeling of the evaporation and thermal decomposition of

... [1, 2]. Urea is typically being used as an aqueous solution at its eutectic composition (32.5% wt. urea, marketed as Adblue®). In a typical SCR system, urea-water-solution (UWS) is sprayed into the hot engine exhaust upstream of the SCR catalyst. It is commonly believed that water evaporates first ...
d+p 3He
d+p 3He

... • 1920 Aston measures mass defect of helium (!= 4p’s) • 1920 Nuclear Astrophysics is born with Sir Arthur Eddington remarks in his presidential address to the British Association for the Advancement of Science: “Certain physical investigations in the past year make it probable to my mind that some p ...
pp-chain
pp-chain

... • 1920 Aston measures mass defect of helium (!= 4p’s) • 1920 Nuclear Astrophysics is born with Sir Arthur Eddington remarks in his presidential address to the British Association for the Advancement of Science: “Certain physical investigations in the past year make it probable to my mind that some p ...
< 1 ... 5 6 7 8 9 10 11 12 13 ... 85 >

Microplasma



Microplasmas are plasmas of small dimensions, ranging from tens to thousands of micrometers. They can be generated at a variety of temperatures and pressures, existing as either thermal or non-thermal plasmas. Non-thermal microplasmas that can maintain their state at standard temperatures and pressures are readily available and accessible to scientists as they can be easily sustained and manipulated under standard conditions. Therefore, they can be employed for commercial, industrial, and medical applications, giving rise to the evolving field of microplasmas.
  • studyres.com © 2025
  • DMCA
  • Privacy
  • Terms
  • Report