• 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
Mars Express - The Scientific Investigations: ASPERA-3
Mars Express - The Scientific Investigations: ASPERA-3

... ions protrude all the way down to pericentre (here 300 km). At the same time we observe energisation of planetary (heavy) ions. The Electron Spectrometer (ELS) has demonstrated a unique capability to resolve the fine structure in electron spectra, such as the CO2 photoelectron peaks (Frahm et al., 2 ...
Stellar Evolution
Stellar Evolution

Electron-ion recombination of the open-4f
Electron-ion recombination of the open-4f

... The experiment was carried out by employing the electron-ion merged-beams technique at the heavy-ion storage ring TSR of the Max-PlanckInstitute for Nuclear Physics in Heidelberg, Germany. As in the previous cases of W18+ and W20+ , an extremely large W19+ recombination rate coefficient has been obs ...
The role of black holes in galaxy formation and evolution
The role of black holes in galaxy formation and evolution

Computational Study Of Molecular Hydrogen In Zeolite Na
Computational Study Of Molecular Hydrogen In Zeolite Na

... probes of adsorption sites in zeolites, on account of its small size and weak interaction with the host. H2, as well as other diatomics, have been used as probes of catalytic acid sites,7 and H2 may probe dual acid-base sites as well.8 One of the applications of zeolites in the area of separation ha ...
Theory of pulsar winds and nebulae - Max-Planck
Theory of pulsar winds and nebulae - Max-Planck

... According to conventional wisdom, an enormous electric field is induced by the rotation of a magnetised neutron star. This field tears particles from the stellar surface and accelerates them up to high energies. As a result, these “primary” particles initiate an electron-positron cascade, which popu ...
Lecture 3 Radiative and Convective Energy Transport I
Lecture 3 Radiative and Convective Energy Transport I

... that the result fails to accord with observation. The proper course is to find the spectral distribution of the emergent radiation by treating each wavelength separately using its own proper values of j and κ.“ ...
The chemical case for no winds in dwarf irregular galaxies
The chemical case for no winds in dwarf irregular galaxies

... gas-rich dwarf galaxies, not affected by external environmental processes. One of the agents that may regulate the star formation history of these objects is the presence of strong galactic winds. If they have a low mass and a high star formation rate (SFR), the energy injected by supernova (SN) exp ...
Low-Energy Electron-Induced Chemistry of
Low-Energy Electron-Induced Chemistry of

... which methanol, a precursor of several prebiotic species, is the most abundant organic species. Using post-irradiation temperature-programmed desorption, we have investigated the radiolysis initiated by low-energy (7 eV and 20 eV) electrons in condensed methanol at ~ 85 K under ultrahigh vacuum (5×1 ...
Protogalaxies Encyclopedia of Astronomy & Astrophysics eaa.iop.org S G Djorgovski
Protogalaxies Encyclopedia of Astronomy & Astrophysics eaa.iop.org S G Djorgovski

Cosmology, Thermodynamics and Time
Cosmology, Thermodynamics and Time

The difficulty of forming large disk galaxies with small bulges
The difficulty of forming large disk galaxies with small bulges

... Binney, Fraternali, Marinacci et al (2006 ff) propose that SN-driven fountain gas entrains hot halo material which returns to the disk. Star formation sustains itself from the hot halo, with accretion rate ~ 2 M yr-1 in the Milky Way. (Deposition rate is smaller than the overall rate of interchang ...
Powerpoint
Powerpoint

Protogalaxies
Protogalaxies

PoS(ICRC2015)509
PoS(ICRC2015)509

Death - Wayne State University Physics and Astronomy
Death - Wayne State University Physics and Astronomy

Paper
Paper

PX211-0406 The following questions were randomly selected for
PX211-0406 The following questions were randomly selected for

... 29. Which of the following statements is least likely to be true of a sample of nitrogen gas at STP? A) Collisions between the gaseous molecules are elastic. B) The intermolecular forces between nitrogen molecules are not negligible. C) Molecules of gaseous nitrogen are in constant random motion. D) ...
No Slide Title
No Slide Title

幻灯片 1
幻灯片 1

Final published version
Final published version

... additional heating elements, temperature controllers, and signal processing elements on a single electronic platform. Besides, operating the device at high temperature reduces its durability. Therefore, an alternative to the thermal activation mechanism is preferable. A number of successful attempts ...
Slide 1
Slide 1

Thermal emission and internal heating processes in millisecond
Thermal emission and internal heating processes in millisecond

... • Gravitochemical heating happens if dG/dt  0 • Both lead to a stationary state of nearly constant temperature that can be probed with old enough pulsars (e.g., MSPs) ...
co2 removal from natural gas by hydrate formation
co2 removal from natural gas by hydrate formation

... Figure 2 shows the variation with elapsed time of the cell temperature, pressure and gas phase composition in a typical experiment, together with selected images (snapshots) through the sapphire window. During the first 30 min, the pressure and the CO2 content in the vapor phase decrease quickly, du ...
L129 DISCOVERY OF A NEW 89 SECOND X
L129 DISCOVERY OF A NEW 89 SECOND X

< 1 ... 16 17 18 19 20 21 22 23 24 ... 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