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Article
Dynamics of Magnetized Accretion Disks of Young Stars
We investigate the dynamics of the accretion disks of young stars with fossil large-scale magnetic field. The author’s magnetohydrodynamic (MHD) model of the accretion disks is generalized to take into account...
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Article
Effect of Dust Evaporation on the Fossil Magnetic Field of Young Stars and Their Accretion Disks
The theory of the fossil magnetic field of young stars and their accretion disks has been verified by comparing the observational data with the results of numerical simulations of the collapse of protostellar ...
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Article
Physical and Chemical Vertical Structure of Magnetostatic Accretion Disks of Young Stars
The vertical structure of accretion disks of young stars with fossil large-scale magnetic field is studied. The equations of magnetostatic equilibrium of the disk are solved taking into account the stellar gra...
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Article
PRIMARY DISKS AND THEIR OBSERVATIONAL APPEARANCE IN COLLAPSING MAGNETIC ROTATING PROTOSTELLAR CLOUDS
The collapse of the magnetic rotating protostellar cloud 10 \({{M}_{ \odot }}\) ... mass is numerically stud...
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Article
Simulations of the Isothermal Collapse of Magnetic Rotating Protostellar Clouds
We investigate the collapse of magnetic protostellar clouds of mass 10 and \(1\;{{M}_{ \odot }}\) . The collapse is ...
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Article
Open AccessThe Mechanical Properties of Chelyabinsk LL5 Chondrite Under Compression and Tension
The mechanical properties of Chelyabinsk LL5 chondrite (Chelyabinsk meteorite) were studied by uniaxial compression and diametral compression/indirect tension test. Twenty cylindrical samples, 10 for compressi...
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Article
The Rate of Falls of Meteorites and Bolides
We perform a statistical analysis of 926 confirmed falls of meteorites that occurred in the period 1860 to 2017. The distribution of meteorites over masses is approximated with a lognormal law. It has been sho...
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Chapter
Frequency of meteorite falls
Between 10,000 and 100,000 tons of space matter falls to Earth annually [1]. Given that seven billion people now live on Earth, that means each resident of the planet could potentially find about 8 g of space ...
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Chapter
Basalt threads in the dust of the Chelyabinsk bolide: Pele’s hair analog
A systematic collection of dust samples after the explosion of the Chelyabinsk bolide was organized during special expeditions from Chelyabinsk State University (see Chapter 5
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Chapter
Why the stone exploded
Why and how did the Chelyabinsk meteoroid explode at an altitude over 20 km above Earth’s surface? Calculations based on standard approaches used in meteorite research indicate that the abrupt increase in ener...
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Chapter
How to protect Earth from meteoroids, asteroids and comets
Since the fall of the Chelyabinsk meteorite, the problem of protecting Earth’s population and infrastructure from meteoroids has become an extremely important one, because for the first time in recent history ...
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Chapter
Meteorite rush: collection of sky stones
The bolide that exploded above the Southern Urals on February 15, 2013 caused a massive meteorite shower. Residents of Yemanzhelinsk District witnessed a space rain that beat against the roofs of houses and bu...
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Article
Magnetic field buoyancy in accretion disks of young stars
Buoyancy of the fossil magnetic field in the accretion disks of young stars is investigated. It is assumed that the Parker instability leads to the formation of slender flux tubes of toroidal magnetic field in...
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Article
Fossil magnetic field of accretion disks of young stars
We elaborate the model of accretion disks of young stars with the fossil large-scale magnetic field in the frame of Shakura and Sunyaev approximation. Equations of the MHD model include Shakura and Sunyaev equ...
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Article
Fragments of the Chelyabinsk meteorite shower: Distribution of masses and sizes and constraints on the mass of the largest fragment
This paper reports data on the masses of fragments of the Chelyabinsk meteorite shower (fall of 15.02.2013). Assuming a lognormal distribution for the masses of fragments, the logarithm of the mean mass and st...
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Article
Self-similar regimes for the collapse of magnetic protostellar clouds
Self-similar solutions describing the homogeneous, free, isothermal collapse of protostellar clouds are considered. One such solution correponds to the critical case of the propagation of a rarefaction wave ne...
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Article
Evolution of collapse nonuniformity for rotating magnetic interstellar clouds
We investigate the formation and evolution of isothermal collapse nonuniformity for rotating magnetic interstellar clouds. The initial and boundary conditions correspond to the statement of the problem of homo...
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Article
Nonself-similar regimes of isothermal collapse of protostellar clouds
We consider the development of inhomogeneity in the isothermal collapse of protostellar clouds. The initial and boundary conditions correspond to the classical statement of the problem on the contraction of a ...
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Chapter and Conference Paper
Fossil Magnetic Fields and Rotation of Early-Type Stars
Observational data of the last 10 years allow two main conclusions:
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Main sequence stars can be separated in two classes: - mag...
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Chapter and Conference Paper
Dynamo and Fossil Magnetic Field in Young Stars
The theory of fossil magnetic fields shows that new born stars may have internal magnetic fields of more than 1 million gauss. Convection inside young solar type stars will tangle any strong fossil magnetic fi...