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Showing 1 to 7 of 7 for “"Solar magnetic field"”.

  1. Measurements of the 2001 April 15 and 2005 January 20 ground -level enhancements by the Milagro water Cerenkov detector

    … Although the accelerating source is tied to the solar magnetic field, the physical process responsible continues to be debated. Essential information about the location and nature of the acceleration mechanism can be obtained from measurements of the highest-energy particles.</p><p>The Milagro …

    unh-thes Repository record for Measurements of the 2001 April 15 and 2005 January 20 ground -level enhancements by the Milagro water Cerenkov detector (opens in a new tab)

  2. Observation and study of giga electron volt solar energetic particles using the Milagrito extensive air shower detector

    <p>Measurements of high energy emission from solar events can lead to an understanding of the solar energetic particle acceleration mechanism(s). Although the energy source of these mechanisms is known to reside in the solar magnetic field, the details of the acceleration process(es) have continued …

    unh-thes Repository record for Observation and study of giga electron volt solar energetic particles using the Milagrito extensive air shower detector (opens in a new tab)

  3. Magnetic reconnection in small and large scales on the sun

    Almost all solar activities observed are related to the solar magnetic field, especially the topological restructuring of magnetic fields, the so-called magnetic reconnection in solar physics. They are occurring at different scales related to various phenomena, during minimum or maximum of the …

    njit Repository record for Magnetic reconnection in small and large scales on the sun (opens in a new tab)

  4. High resolution spectroscopy of photospheric bright points

    … bright points are proxies for small-scale magnetic flux concentrations. <br>These magnetic elements are thought to be the building blocks of the solar magnetic field <br>and are important to understand many physical processes on the Sun, e.g. the variability of the solar irradiance. …

    freiburg-diss Repository record for High resolution spectroscopy of photospheric bright points (opens in a new tab)

  5. The Structure and Dynamic nature of the Solar Atmosphere

    … of dynamic phenomena present throughout the solar atmosphere, from the photosphere to the corona. Above the photosphere, where the plasma fi is small, the emitting plasma structure and dynamics are tied intimately to the solar magnetic field. Firstly, a wavelet analysis is applied to …

    cent-lancashire Repository record for The Structure and Dynamic nature of the Solar Atmosphere (opens in a new tab)

  6. Magnetized models for the formation of the moon

    … collision shortly after the formation of the solar system. The giant impact produces liquid and vapor debris, drawn from the proto-Earth and impactor. The debris either escapes the system, falls back to Earth, or enters circumterrestrial orbits forming a “protolunar disk.” The Moon is thought …

    uiuc Repository record for Magnetized models for the formation of the moon (opens in a new tab)

  7. Automatic prediction of solar flares and super geomagnetic storms

    … on space system, satellite-based services. A geomagnetic storm, a disturbance in Earth's magnetosphere, may produce many harmful effects on Earth. Solar flares and Coronal Mass Ejections (CMEs) are believed to be the major causes of geomagnetic storms. Thus, establishing a real time forecasting …

    njit Repository record for Automatic prediction of solar flares and super geomagnetic storms (opens in a new tab)