926 resultados para Magic the Gathering
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Hermann Pick
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Leipzig, Univ., Diss., 1897
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Nighttime satellite imagery from the Defense Meteorological Satellite Program (DMSP) Operational Linescan System (OLS) has a unique capability to observe nocturnal light emissions from sources including cities, wild fires, and gas flares. Data from the DMSP OLS is used in a wide range of studies including mapping urban areas, estimating informal economies, and estimating urban populations. Given the extensive and increasing list of applications a repeatable method for assessing geolocation accuracy, performing inter-calibration, and defining the minimum detectable brightness would be beneficial. An array of portable lights was designed and taken to multiple field sites known to have no other light sources. The lights were operated during nighttime overpasses by the DMSP OLS and observed in the imagery. A first estimate of the minimum detectable brightness is presented based on the field experiments conducted. An assessment of the geolocation accuracy was performed by measuring the distance between the GPS measured location of the lights and the observed location in the imagery. A systematic shift was observed and the mean distance was measured at 2.9km. A method for in situ radiance calibration of the DMSP OLS using a ground based light source as an active target is presented. The wattage of light used by the active target strongly correlates with the signal measured by the DMSP OLS. This approach can be used to enhance our ability to make inter-temporal and inter-satellite comparisons of DMSP OLS imagery. Exploring the possibility of establishing a permanent active target for the calibration of nocturnal imaging systems is recommended. The methods used to assess the minimum detectable brightness, assess the geolocation accuracy, and build inter-calibration models lay the ground work for assessing the energy expended on light emitted into the sky at night. An estimate of the total energy consumed to light the night sky globally is presented.
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Clusters of galaxies are expected to be reservoirs of cosmic rays (CRs) that should produce diffuse γ-ray emission due to their hadronic interactions with the intra-cluster medium. The nearby Perseus cool-core cluster, identified as the most promising target to search for such an emission, has been observed with the MAGIC telescopes at very-high energies (VHE, E ≥ 100 GeV) for a total of 253 hr from 2009 to 2014. The active nuclei of NGC 1275, the central dominant galaxy of the cluster, and IC 310, lying at about 0.6º from the centre, have been detected as point-like VHE γ-ray emitters during the first phase of this campaign. We report an updated measurement of the NGC 1275 spectrum, which is described well by a power law with a photon index Γ = 3.6 ± 0.2_(stat) ± 0.2_(syst) between 90 GeV and 1200 GeV. We do not detect any diffuse γ-ray emission from the cluster and so set stringent constraints on its CR population. To bracket the uncertainties over the CR spatial and spectral distributions, we adopt different spatial templates and power-law spectral indexes α. For α = 2.2, the CR-to-thermal pressure within the cluster virial radius is constrained to be ≤ 1 − 2%, except if CRs can propagate out of the cluster core, generating a flatter radial distribution and releasing the CR-to-thermal pressure constraint to ≤ 20%. Assuming that the observed radio mini-halo of Perseus is generated by secondary electrons from CR hadronic interactions, we can derive lower limits on the central magnetic field, B_(0), that depend on the CR distribution. For α = 2.2, B_(0) ≥ 5 − 8 µG, which is below the ∼25 µG inferred from Faraday rotation measurements, whereas for α ≤ 2.1, the hadronic interpretation of the diffuse radio emission contrasts with our γ-ray flux upper limits independently of the magnetic field strength.
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The last month has seen a public confrontation between Igor Sechin, the president of Rosneft, and Arkady Dvorkovich, the deputy prime minister, concerning the consolidation of the energy sector. This is the latest in a series of disputes between the Kremlin & businessmen from Putin’s inner circle on one side, and the government & Prime Minister Medvedev on the other. These disputes have been wide-ranging in nature, concerning economic policy, the scope of competency of individual members of the elite, but also the ‘tough line’ adopted by the Kremlin since Vladimir Putin’s return to the presidency. The Kremlin, which is still the main decision-making centre in Russia, has been effectively forcing its opinions through in its short-term disputes with the government. However, a new element in the ongoing conflicts, which is unfavourable to President Putin, is their exceptional strength, their much more public nature, and their wide range (which has included criticism of the president himself) and ever-changing context, especially the worsening socio-economic situation. These conflicts have been overlapping with signs of dissent among Putin’s business supporters, and their declining political willingness to support the leader unconditionally. The Kremlin’s response to the unrest consists of intensifying efforts to discipline the elite and weakening those groups in which Vladimir Putin has limited confidence. The elite’s support is crucial to the stability of his government; to maintain this support, the Kremlin is ready to introduce restrictive and repressive actions against both parliamentarians and government officials. In the short term, such a policy will force the Kremlin’s supporters back into obedience, but fears of a further increase in repression are also starting to be expressed on the sidelines.
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Mode of access: Internet.
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Bibliographical foot-notes.
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Advertisement for "The 'Shaker and Shakeress' monthly" on verso of title page (p. [2]).
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Mode of access: Internet.
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Shipping list no.: 98-0027-P.
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Bibliography: p. 71-72.
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Mode of access: Internet.