Electron Firehose instability and acceleration of electrons in solar
... kinetic theory. These thresholds were connected to the pre-flare plasma parameters by assuming an acceleration model acting exclusively in parallel direction. For usually assumed pre-flare plasma conditions the electrons become unstable during the acceleration process and lefthand circularly polariz ...
... kinetic theory. These thresholds were connected to the pre-flare plasma parameters by assuming an acceleration model acting exclusively in parallel direction. For usually assumed pre-flare plasma conditions the electrons become unstable during the acceleration process and lefthand circularly polariz ...
Zettawatt-Exawatt Lasers and Their Applications in Ultrastrong
... level. It has the advantage that it could use KDP as the nonlinear medium. KDP has been produced in large dimensions at a relatively low cost for the NIF and LMJ programs. The working fluence on the crystal will be 1 J/cm2 , leading to a beam diameter of around 10 m2 to accommodate the whole pump ene ...
... level. It has the advantage that it could use KDP as the nonlinear medium. KDP has been produced in large dimensions at a relatively low cost for the NIF and LMJ programs. The working fluence on the crystal will be 1 J/cm2 , leading to a beam diameter of around 10 m2 to accommodate the whole pump ene ...
ssimic - CERN Indico
... • Produce the observed temporal variability of gamma emission • Stochastic process • Put the constraints on the central engine – relativistic flow of well defined collimated shells with random parameters (masses, velocities, …) • Interaction decelerate the shells • Effect of accumulation of ejected ...
... • Produce the observed temporal variability of gamma emission • Stochastic process • Put the constraints on the central engine – relativistic flow of well defined collimated shells with random parameters (masses, velocities, …) • Interaction decelerate the shells • Effect of accumulation of ejected ...
Stellar Evolution
... – This causes the temperature to increase rapidly to 300 million K and there’s a sudden flash when a large part of the Helium gets burned all at once. – We don’t see this flash because it’s buried inside the Sun. ...
... – This causes the temperature to increase rapidly to 300 million K and there’s a sudden flash when a large part of the Helium gets burned all at once. – We don’t see this flash because it’s buried inside the Sun. ...
COIL—Chemical Oxygen Iodine Laser
... power laser, which wavelength 1315 nm is suitable for propagating trough the air or optical fibres. On the COIL device we measured the small signal gain and laser output power and besides also the flows of gases and pressure in the main parts of COIL. Our work should be the contribution to the furth ...
... power laser, which wavelength 1315 nm is suitable for propagating trough the air or optical fibres. On the COIL device we measured the small signal gain and laser output power and besides also the flows of gases and pressure in the main parts of COIL. Our work should be the contribution to the furth ...
Lecture 2
... acts like a prism. Red light is less bent than green light which is less bent than blue light. The image of the Sun in these different colors is therefore separated. When the Sun is low on the horizon, the red Sun sets first, then the green Sun. By then, all the blue light is scattered out so there ...
... acts like a prism. Red light is less bent than green light which is less bent than blue light. The image of the Sun in these different colors is therefore separated. When the Sun is low on the horizon, the red Sun sets first, then the green Sun. By then, all the blue light is scattered out so there ...
Unit 13 Stoichiometry (Theoretical)
... 8. CaC2 (s) + H2O (l) C2H2 (g) + Ca(OH)2 (aq) a. Balance the above equation. b. How many grams of acetylene (C2H2) are produced by adding water to 5.00 grams of CaC2? (ans. 2.03 g C2H2) ...
... 8. CaC2 (s) + H2O (l) C2H2 (g) + Ca(OH)2 (aq) a. Balance the above equation. b. How many grams of acetylene (C2H2) are produced by adding water to 5.00 grams of CaC2? (ans. 2.03 g C2H2) ...
Classification of magnetized star-planet interactions: dynamics and
... Stellar irradiation is believed to drive outflows from the surface of close-in planets, a phenomenon that is supported by transit observations of Hot Jupiters. Assuming planetary magnetospheres similar to those of our solar system, such outflows are expected to be magnetized. On the other hand, the ...
... Stellar irradiation is believed to drive outflows from the surface of close-in planets, a phenomenon that is supported by transit observations of Hot Jupiters. Assuming planetary magnetospheres similar to those of our solar system, such outflows are expected to be magnetized. On the other hand, the ...
RECOMBINATION OF HYDROGEN IN THE HOT MODEL OF THE
... plasma is in equilibrium with radiation. Cooling as a result of expansion leads to recombination. Since in the course of the expansion there is conservation of specific entropy T 3 /n = 3 x 10 6 deg3 cm 3 [ 21 , it can be easily verified 1 > that according to the Saha equilibrium formula a 50% degre ...
... plasma is in equilibrium with radiation. Cooling as a result of expansion leads to recombination. Since in the course of the expansion there is conservation of specific entropy T 3 /n = 3 x 10 6 deg3 cm 3 [ 21 , it can be easily verified 1 > that according to the Saha equilibrium formula a 50% degre ...
m - viXra
... by these impacts and dust clouds are formed. They are dusty plasma clouds * because atoms from the dust grains are ionized by the UV radiation and X-rays from the solar radiation that incides continuously on the lunar surface ...
... by these impacts and dust clouds are formed. They are dusty plasma clouds * because atoms from the dust grains are ionized by the UV radiation and X-rays from the solar radiation that incides continuously on the lunar surface ...
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.