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Magnetic reconnection in the solar wind
Enžl, Jakub ; Přech, Lubomír (advisor)
Magnetic reconnection is a fundamental process that changes magnetic field configuration and converts a magnetic energy to flow energy and plasma heating. It can be found in a plasma with frozen magnetic field lines at boundaries where different magnetic field topologies encounter each other and thin current sheets are created as it is typical in the solar wind. In the thesis, we have used spacecraft measurements of solar wind plasma and magnetic field to found magnetic reconnection exhausts. We analyze and compare them with theoretical predictions. The results of the statistical analysis oriented on re-distribution of the magnetic energy in reconnection showed that both a portion of the energy deposited into heat as well as the energy spent on an acceleration of the exhaust plasma increase with the magnetic shear angle in accord with the increase of the magnetic flux available for reconnection. Moreover, we identify unusual events in the solar wind; we found magnetic reconnection exhausts accompanied by one or two side jets and explained their possible causes.
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Magnetic reconnection in the solar wind
Enžl, Jakub ; Přech, Lubomír (advisor) ; Bárta, Miroslav (referee) ; Kulhánek, Petr (referee)
Magnetic reconnection is a fundamental process that changes magnetic field configuration and converts a magnetic energy to flow energy and plasma heating. It can be found in a plasma with frozen magnetic field lines at boundaries where different magnetic field topologies encounter each other and thin current sheets are created as it is typical in the solar wind. In the thesis, we have used spacecraft measurements of solar wind plasma and magnetic field to found magnetic reconnection exhausts. We analyze and compare them with theoretical predictions. The results of the statistical analysis oriented on re-distribution of the magnetic energy in reconnection showed that both a portion of the energy deposited into heat as well as the energy spent on an acceleration of the exhaust plasma increase with the magnetic shear angle in accord with the increase of the magnetic flux available for reconnection. Moreover, we identify unusual events in the solar wind; we found magnetic reconnection exhausts accompanied by one or two side jets and explained their possible causes.
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Turbulence in the solar wind from inertial to kinetic scales
Pitňa, Alexander ; Šafránková, Jana (advisor) ; Hellinger, Petr (referee) ; Kulhánek, Petr (referee)
Solar wind, a stream of supersonic plasma emanating from the solar corona, serves as an ideal laboratory for a study of high Reynolds number plasma flows. Turbulent processes that govern the dynamics of the so-called inertial range, i.e., the spatial scales smaller than energy injection scales but larger than the scales where the dissipation processes set in, have been studied for decades. At present, it is believed that the large-scale free energy in a form of kinetic and magnetic fluctuations is transferred via turbulent cascade into smaller scales, where kinetic effects become dominant and heating takes place. In order to understand dissipation processes, high-cadence measurements of solar wind parameters are necessary. The bright monitor of the solar wind (BMSW) instrument on board the Spektr-R spacecraft provides such data, and in tandem with high-cadence measurements of the magnetic field from the Wind spacecraft, we are able address the nature of the sub-ion scale fluctuations. The thesis focus on three interconnected topics, (a) what changes are induced by the passage of a collisionless IP shock in the framework of turbulence, (b) study of a decay of the turbulent energy downstream an IP shock, and (c) identifying the dominant mode of the sub-ion scale fluctuations.
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Development of UV detector for space applications
Kočiščák, Samuel ; Pavlů, Jiří (advisor) ; Jeřáb, Martin (referee)
Title: Development of UV Detector for Space Applications Author: Samuel Kočiščák Department: Department of Surface and Plasma Science Supervisor: doc. RNDr. Jiří Pavlů, Ph.D., Department of Surface and Plasma Science Abstract: It is not unusual that space measurement is influenced by UV irradia- tion causing photoemission on delicate electronic components. Therefore informa- tion on UV irradiance is very useful. Particularly useful is non-delayed, immediate quantitative information (on a time scales of seconds) identifying unexpected va- riation in the irradiance of such electronic parts. The goal was to construct a prototype, measure basic properties and discuss ca- pabilities of a detector capable of continuous measurement of UV irradiance of a spacecraft, working on the principle of photoemission alone. We have success- fully shown the capabilities of a prototype and established some of its key basic properties, e.g. their stability in cosmic environment. Keywords: VUV, Faraday cup, UV detector, UV transmittance, solar wind
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Investigation of Ionizing Radiation Infuence to the Communication Systems of Satellites
Golubev, Martin ; Kubíček, Michal (referee) ; Katovský, Karel (advisor)
This master thesis discuss about ionizing radiation, interaction with matter and effects on her. In the work is discussed differend types of interactions of directly ionizing radiation and indirectly ionizing radiation. Below is an overview of methods of shielding from all of types of ionizing radiation. Second part of this thesis discuss about single event effects in semiconductors which are cause by ionizing radiation. At the end is described design of measuring instrument included FPGA chips. This design is discused both from point of wiew hardware and software too.
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Empirical modeling of the location of the Earth's magnetopause
Machková, Anna ; Němec, František (advisor) ; Grygorov, Kostiantyn (referee)
This bachelor thesis focuses on suggesting possible improvements of the existing models of the magnetopause stand-off distance, i.e., on identification of the parameters which are not properly (or not at all) included. Magnetopause is a border between the terrestrial and interplanetary magnetic fields, where the pressure of the Earth's magnetic field balances the solar wind dynamic pressure. In order to analyze the parameters, which have an influence on the magnetopause radial distance, we perform a systematic study of an existing database of 16800 magnetopause crossings registered by 8 different satellites. We focus on the effect of the topology of the terrestrial magnetic field, which is not perfectly dipolar, and whose values close to the subsolar point exhibit significant diurnal and annual variations. Another analyzed phenomenon is the magnetospheric ring current and its influence on the magnetic field strength near the magnetopause. Possible changes of this magnetic field have a direct influence on the magnetopause distance from the Earth. Attention is also devoted to the potentially different positions of the magnetopause at the times of fast and slow solar wind. Finally, we discuss complications related to the satellite orbits and the resulting uneven spatial distribution of the used data set.
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Variations of solar wind parameters through solar cycle
Turčičová, Marie ; Šafránková, Jana (advisor) ; Ďurovcová, Tereza (referee)
Statistical analysis of data from satellites that operate in the vicinity of the Sun can partly contribute to the elucidation of complex processes around the Sun. This thesis is devoted to a long-term statistical study of particular parameters of the solar wind. We have used data from the Wind satellite, especially its measurements of the velocity, density and temperature of protons and α- particles. By using standard statistical tools, we explored their behaviour during the 23th and 24th solar cycles, including a comparison of both cycles. Our results are in accordance with other known studies.
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Investigation of Ionizing Radiation Infuence to the Communication Systems of Satellites
Golubev, Martin ; Hobst, Leonard (referee) ; Katovský, Karel (advisor)
This master thesis discuss about ionizing radiation, interaction with matter and effects on her. In the work is discussed differend types of interactions of directly ionizing radiation and indirectly ionizing radiation. Below is an overview of methods of shielding from all of types of ionizing radiation. Second part of this thesis discuss about single event effects in semiconductors which are cause by ionizing radiation. At the end is described design of measuring instrument included FPGA chips. This design is discused both from point of wiew hardware and software too.
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Fast solar wind helium abundance variations and their relations to solar processes
Ďurovcová, Tereza ; Šafránková, Jana (advisor) ; Vandas, Marek (referee)
Helium can significantly influence solar wind dynamics. The changes of its relative abundance are usually associated with crossings of the boundaries between adjacent flux tubes. However, the recent studies of the data from the BMSW instrument onboard the Spektr-R spacecraft show that the relative helium abundance could vary also inside the flux tubes. The differential motion of proton and helium solar wind components was suggested as a source of turbulence inside the flux tube. The thesis is devoted to the long-term statistical study of the fast helium abundance variations with respect to parameters of the solar wind and changes of its source region. For this purpose, the plasma data from the instruments onboard the Wind and the Spektr-R spacecraft and magnetic field measurements from Wind were used. Simultaneous changes of the relative helium abundance and solar wind parameters were investigated in the long-term Wind observations as well as in the observations prior to and behind interplanetary shocks. Finally, the study of differences between proton and helium velocities during solar minima and solar maxima was conducted.
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Selected Wave Phenomena in the Earth's Magnetosphere
Bezděková, Barbora ; Němec, František (advisor) ; Macúšová, Eva (referee)
Electromagnetic waves are crucial for energy transfer in the nearly collision- less plasma of the Earth's inner magnetosphere. The waves in the frequency range 1-8 kHz whose visualisation in the form of frequency-time spectrograms reveals a harmonic frequency modulation of the wave intensity are called magnetospheric line radiation (MLR). Waves characterized by a nearly periodic time modulation of the wave intensity observed at frequencies between about 0.5 and 4 kHz are called quasiperiodic (QP) emissions. Although both types of the events were re- peatedly observed by ground-based instruments and low-altitude satellites, their origin remains still unclear. Between 2004 and 2010 these wave events were me- asured by the DEMETER spacecraft (almost Sun-synchronous orbit, altitude of about 700 km). This thesis presents a systematic study of the properties of the observed events, a comparison of the observations by the spacecraft and ground- based instruments, and an investigation of a relation to solar wind parameters.
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