300 research outputs found
New Research in the Military History of the Late Rome and Early Byzantium
Submitted: 08.07.2020. Accepted: 15.10.2020.ΠΠΎΡΡΡΠΏΠΈΠ»Π° 08.07.2020. ΠΡΠΈΠ½ΡΡΠ° 15.10.2020.A review of: Mekhamadiev, E. A. (2019). Voennaia organizatsiia pozdnei Rimskoi imperii v 253β353 gg.: ot reform imperatora Galliena do perioda Tetrarkhii (253β305) [A Military Organization of the Later Roman Empire in 253β353 AD: From Emperor Gallienusβ Reforms to the Age of the Tetrarchy (253β305)]. St Petersburg: Peterburgskoe Vostokovedenie Publishers. 406 p. This paper states that the monograph published E. A. Mekhamadiev, a researcher from St. Petersburg, is a fundamental study of the Later Roman military organization, with especial attention to the epigraphic and papyrological accounts. The use of these sources allows the author to reconstruct the history of specific military units, their spatial movements, participation in various military campaigns and wars, and changes in their ranks. Important is that Mekhamadiev examined the internal (organizational) structure of all regional armies of the Roman empire from 253 to 305 and not restricted himself to specific and narrow aspects of history of a particular province or country. The author of the book under present review has analysed the data related to both the eastern and the western imperial provinces, discovered close interrelations of the western and eastern provinces, and indicated permanent movements of the military units from the west to east and in the opposite direction depending on the geopolitical and home political situation.Π Π΅ΡΠ΅Π½Π·ΠΈΡ Π½Π° ΠΊΠ½ΠΈΠ³Ρ: ΠΠ΅Ρ
Π°ΠΌΠ°Π΄ΠΈΠ΅Π² Π. Π. ΠΠΎΠ΅Π½Π½Π°Ρ ΠΎΡΠ³Π°Π½ΠΈΠ·Π°ΡΠΈΡ ΠΏΠΎΠ·Π΄Π½Π΅ΠΉ Π ΠΈΠΌΡΠΊΠΎΠΉ ΠΈΠΌΠΏΠ΅ΡΠΈΠΈ Π² 253β353 Π³Π³.: ΠΎΡ ΡΠ΅ΡΠΎΡΠΌ ΠΈΠΌΠΏΠ΅ΡΠ°ΡΠΎΡΠ° ΠΠ°Π»Π»ΠΈΠ΅Π½Π° Π΄ΠΎ ΠΏΠ΅ΡΠΈΠΎΠ΄Π° Π’Π΅ΡΡΠ°ΡΡ
ΠΈΠΈ (253β305). Π‘ΠΠ±. : ΠΠ΅ΡΠ΅ΡΠ±ΡΡΠ³ΡΠΊΠΎΠ΅ Π²ΠΎΡΡΠΎΠΊΠΎΠ²Π΅Π΄Π΅Π½ΠΈΠ΅, 2019. 406 Ρ. Π ΡΡΠ°ΡΡΠ΅ ΠΎΡΠΌΠ΅ΡΠ°Π΅ΡΡΡ, ΡΡΠΎ ΡΠ΅ΡΠ΅Π½Π·ΠΈΡΡΠ΅ΠΌΠ°Ρ ΠΊΠ½ΠΈΠ³Π° ΠΏΠ΅ΡΠ΅ΡΠ±ΡΡΠ³ΡΠΊΠΎΠ³ΠΎ ΠΈΡΡΠ»Π΅Π΄ΠΎΠ²Π°ΡΠ΅Π»Ρ Π. Π. ΠΠ΅Ρ
Π°ΠΌΠ°Π΄ΠΈΠ΅Π²Π° ΡΠ²Π»ΡΠ΅ΡΡΡ ΡΡΠ½Π΄Π°ΠΌΠ΅Π½ΡΠ°Π»ΡΠ½ΡΠΌ ΠΈΡΡΠ»Π΅Π΄ΠΎΠ²Π°Π½ΠΈΠ΅ΠΌ ΠΏΠΎ Π²ΠΎΠ΅Π½Π½ΠΎΠΉ ΠΎΡΠ³Π°Π½ΠΈΠ·Π°ΡΠΈΠΈ ΠΏΠΎΠ·Π΄Π½Π΅Π³ΠΎ Π ΠΈΠΌΠ°, Π² ΠΊΠΎΡΠΎΡΠΎΠΌ ΡΠ΄Π΅Π»Π°Π½ ΠΎΡΠΎΠ±ΡΠΉ Π°ΠΊΡΠ΅Π½Ρ Π½Π° Π΄Π°Π½Π½ΡΠ΅ ΡΠΏΠΈΠ³ΡΠ°ΡΠΈΠΊΠΈ ΠΈ ΠΏΠ°ΠΏΠΈΡΠΎΠ»ΠΎΠ³ΠΈΠΈ. ΠΡ
ΠΏΡΠΈΠ²Π»Π΅ΡΠ΅Π½ΠΈΠ΅ ΠΏΠΎΠ·Π²ΠΎΠ»ΠΈΠ»ΠΈ Π°Π²ΡΠΎΡΡ ΡΠ΅ΠΊΠΎΠ½ΡΡΡΡΠΈΡΠΎΠ²Π°ΡΡ ΠΈΡΡΠΎΡΠΈΡ ΠΎΡΠ΄Π΅Π»ΡΠ½ΡΡ
Π²ΠΎΠΉΡΠΊΠΎΠ²ΡΡ
ΠΏΠΎΠ΄ΡΠ°Π·Π΄Π΅Π»Π΅Π½ΠΈΠΉ, ΠΈΡ
ΡΠ΅ΡΡΠΈΡΠΎΡΠΈΠ°Π»ΡΠ½ΡΠ΅ ΠΏΠ΅ΡΠ΅ΠΌΠ΅ΡΠ΅Π½ΠΈΡ, ΡΡΠ°ΡΡΠΈΠ΅ Π² ΡΠ°Π·Π»ΠΈΡΠ½ΡΡ
Π²ΠΎΠ΅Π½Π½ΡΡ
ΠΊΠ°ΠΌΠΏΠ°Π½ΠΈΡΡ
ΠΈ ΠΏΠΎΡ
ΠΎΠ΄Π°Ρ
, ΠΈΠ·ΠΌΠ΅Π½Π΅Π½ΠΈΡ ΡΠ°Π½Π³ΠΎΠ². Π£ΠΊΠ°Π·ΡΠ²Π°Π΅ΡΡΡ, ΡΡΠΎ Π. Π. ΠΠ΅Ρ
Π°ΠΌΠ°Π΄ΠΈΠ΅Π² ΡΠ°ΡΡΠΌΠΎΡΡΠ΅Π» Π²Π½ΡΡΡΠ΅Π½Π½ΡΡ (ΠΎΡΠ³Π°Π½ΠΈΠ·Π°ΡΠΈΠΎΠ½Π½ΡΡ) ΡΡΡΡΠΊΡΡΡΡ Π²ΡΠ΅Ρ
ΡΠ΅Π³ΠΈΠΎΠ½Π°Π»ΡΠ½ΡΡ
Π°ΡΠΌΠΈΠΉ Π ΠΈΠΌΠ° Ρ 253 ΠΏΠΎ 305 Π³., Π½Π΅ ΠΎΠ³ΡΠ°Π½ΠΈΡΠΈΠ»ΡΡ ΠΈΡΡΠ»Π΅Π΄ΠΎΠ²Π°Π½ΠΈΠ΅ΠΌ ΠΎΡΠ΄Π΅Π»ΡΠ½ΡΡ
ΠΈ ΡΠ·ΠΊΠΈΡ
ΡΡΠΆΠ΅ΡΠΎΠ², ΡΠ²ΡΠ·Π°Π½Π½ΡΡ
Ρ ΠΈΡΡΠΎΡΠΈΠ΅ΠΉ ΠΎΡΠ΄Π΅Π»ΡΠ½ΠΎ Π²Π·ΡΡΠΎΠΉ ΠΈΠΌΠΏΠ΅ΡΡΠΊΠΎΠΉ ΠΏΡΠΎΠ²ΠΈΠ½ΡΠΈΠΈ ΠΈΠ»ΠΈ ΡΠ΅Π³ΠΈΠΎΠ½Π°. ΠΠ²ΡΠΎΡ ΡΠ΅ΡΠ΅Π½Π·ΠΈΡΡΠ΅ΠΌΠΎΠΉ ΠΊΠ½ΠΈΠ³ΠΈ ΠΏΡΠΎΠ°Π½Π°Π»ΠΈΠ·ΠΈΡΠΎΠ²Π°Π» Π΄Π°Π½Π½ΡΠ΅ ΠΊΠ°ΠΊ ΠΏΠΎ Π²ΠΎΡΡΠΎΡΠ½ΡΠΌ, ΡΠ°ΠΊ ΠΈ ΠΏΠΎ Π·Π°ΠΏΠ°Π΄Π½ΡΠΌ ΠΏΡΠΎΠ²ΠΈΠ½ΡΠΈΡΠΌ ΠΈΠΌΠΏΠ΅ΡΠΈΠΈ, Π²ΡΡΠ²ΠΈΠ» ΡΠ΅ΡΠ½ΡΡ Π²Π·Π°ΠΈΠΌΠΎΡΠ²ΡΠ·Ρ Π·Π°ΠΏΠ°Π΄Π½ΡΡ
ΠΈ Π²ΠΎΡΡΠΎΡΠ½ΡΡ
ΠΏΡΠΎΠ²ΠΈΠ½ΡΠΈΠΉ, ΡΠΊΠ°Π·Π°Π» Π½Π° ΠΏΠΎΡΡΠΎΡΠ½Π½ΡΠ΅ ΠΏΠ΅ΡΠ΅ΠΌΠ΅ΡΠ΅Π½ΠΈΡ Π²ΠΎΠΉΡΠΊΠΎΠ²ΡΡ
ΠΏΠΎΠ΄ΡΠ°Π·Π΄Π΅Π»Π΅Π½ΠΈΠΉ Ρ Π·Π°ΠΏΠ°Π΄Π° Π½Π° Π²ΠΎΡΡΠΎΠΊ ΠΈ Π² ΠΎΠ±ΡΠ°ΡΠ½ΡΡ ΡΡΠΎΡΠΎΠ½Ρ Π² Π·Π°Π²ΠΈΡΠΈΠΌΠΎΡΡΠΈ ΠΎΡ Π³Π΅ΠΎΠΏΠΎΠ»ΠΈΡΠΈΡΠ΅ΡΠΊΠΎΠΉ ΠΈ Π²Π½ΡΡΡΠΈΠΏΠΎΠ»ΠΈΡΠΈΡΠ΅ΡΠΊΠΎΠΉ ΡΠΈΡΡΠ°ΡΠΈΠΈ
Ocular Manifestations In COVID-19: Clinical Case Reports And A Literature (Review)
Coronavirus disease 2019 (COVID-19) has affected more than 130 million people as of April 2021. During the current pandemic, SARS-CoV-2 has been found to cause conjunctivitis with anecdotal evidence of a wide range of manifestations from scleritis to retinitis, occlusive vasculitis and optic neuritis. The purpose of this study is to raise awareness about possible COVID-19 related ocular manifestations, including papillophlebitis, anterior ischemic optic neuropathy, uveitis and neuroretinitis. Further detailed analyses will be needed to elucidate the link between SARS-CoV-2 and ocular pathology
Search for a new gauge boson in the Experiment (APEX)
We present a search at Jefferson Laboratory for new forces mediated by
sub-GeV vector bosons with weak coupling to electrons. Such a
particle can be produced in electron-nucleus fixed-target scattering and
then decay to an pair, producing a narrow resonance in the QED trident
spectrum. Using APEX test run data, we searched in the mass range 175--250 MeV,
found no evidence for an reaction, and set an upper limit of
. Our findings demonstrate that fixed-target
searches can explore a new, wide, and important range of masses and couplings
for sub-GeV forces.Comment: 5 pages, 5 figures, references adde
Evidence for proton acceleration up to TeV energies based on VERITAS and Fermi-LAT observations of the Cas A SNR
We present a study of -ray emission from the core-collapse supernova
remnant Cas~A in the energy range from 0.1GeV to 10TeV. We used 65 hours of
VERITAS data to cover 200 GeV - 10 TeV, and 10.8 years of \textit{Fermi}-LAT
data to cover 0.1-500 GeV. The spectral analysis of \textit{Fermi}-LAT data
shows a significant spectral curvature around GeV that is
consistent with the expected spectrum from pion decay. Above this energy, the
joint spectrum from \textit{Fermi}-LAT and VERITAS deviates significantly from
a simple power-law, and is best described by a power-law with spectral index of
with a cut-off energy of TeV. These
results, along with radio, X-ray and -ray data, are interpreted in the
context of leptonic and hadronic models. Assuming a one-zone model, we exclude
a purely leptonic scenario and conclude that proton acceleration up to at least
6 TeV is required to explain the observed -ray spectrum. From modeling
of the entire multi-wavelength spectrum, a minimum magnetic field inside the
remnant of is deduced.Comment: 33 pages, 9 Figures, 6 Table
New Measurements of the Transverse Beam Asymmetry for Elastic Electron Scattering from Selected Nuclei
We have measured the beam-normal single-spin asymmetry An in the elastic scattering of 1-3 GeV transversely polarized electrons from H-1 and for the first time from He-4, C-12, and Pb-208. For H-1, He-4, and C-12, the measurements are in agreement with calculations that relate A(n) to the imaginary part of the two-photon exchange amplitude including inelastic intermediate states. Surprisingly, the Pb-208 result is significantly smaller than the corresponding prediction using the same formalism. These results suggest that a systematic set of new A(n) measurements might emerge as a new and sensitive probe of the structure of heavy nuclei
Direct measurement of stellar angular diameters by the VERITAS Cherenkov Telescopes
The angular size of a star is a critical factor in determining its basic
properties. Direct measurement of stellar angular diameters is difficult: at
interstellar distances stars are generally too small to resolve by any
individual imaging telescope. This fundamental limitation can be overcome by
studying the diffraction pattern in the shadow cast when an asteroid occults a
star, but only when the photometric uncertainty is smaller than the noise added
by atmospheric scintillation. Atmospheric Cherenkov telescopes used for
particle astrophysics observations have not generally been exploited for
optical astronomy due to the modest optical quality of the mirror surface.
However, their large mirror area makes them well suited for such
high-time-resolution precision photometry measurements. Here we report two
occultations of stars observed by the VERITAS Cherenkov telescopes with
millisecond sampling, from which we are able to provide a direct measurement of
the occulted stars' angular diameter at the milliarcsecond scale.
This is a resolution never achieved before with optical measurements and
represents an order of magnitude improvement over the equivalent lunar
occultation method. We compare the resulting stellar radius with empirically
derived estimates from temperature and brightness measurements, confirming the
latter can be biased for stars with ambiguous stellar classifications.Comment: Accepted for publication in Nature Astronom
- β¦