Search results for "Polar cap"

showing 5 items of 5 documents

Observations on a new species of Unicapsula (Myxosporida) in the fish Maena smaris (L.) by conventional and electronmicroscopy

1975

A myxosporidian parasite believed to be congeneric with Unicapsula muscularis Davis (1924), type (and only) species of this genus, was found in the dorsal muscles of the fish Maena smaris (L.) at Banyuls-sur-Mer, France. The spores were tripartite, with corresponding components of the three parts differentially developed. One part consisted of a small shell valve overlying no more than a trace of sporoplasm but covering a polar apparatus with well-developed polar capsule. Each of the other two parts consisted of a long shell valve covering a large sporoplasm and a polar apparatus with only the rudiment of a polar capsule. Electron microscope pictures of the trophozoite showed evidence of pi…

SporoplasmGeneral VeterinaryZoologyGeneral MedicineAnatomyUnicapsulaBiologySporelaw.inventionInfectious DiseaseslawGenusInsect SciencePolar capsuleParasite hostingParasitologyPolar filamentElectron microscopeZeitschrift f�r Parasitenkunde
researchProduct

Absolute kinematics of radio source components in the complete S5 polar cap sample

2004

We observed the thirteen extragalactic radio sources of the complete S5 polar cap sample at 15.4 GHz with the Very Long Baseline Array, on 27 July 1999 (1999.57) and 15 June 2000 (2000.46). We present the maps from those two epochs, along with maps obtained from observations of the 2 cm VLBA survey for some of the sources of the sample, making a total of 40 maps. We discuss the apparent morphological changes displayed by the radio sources between the observing epochs. Our VLBA observations correspond to the first two epochs at 15.4 GHz of a program to study the absolute kinematics of the radio source components of the members of the sample, by means of phase delay astrometry at 8.4 GHz, 15.…

PhysicsSpectral indexInterferometricAstronomy and AstrophysicsAstrometryKinematicsAstrometryAstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICAGalaxies:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]Sample (graphics)Radio continuumSpace and Planetary ScienceBL Lacertae objectsAstrometry ; Interferometric ; Galaxies ; Quasars ; BL Lacertae objects ; Radio continuumUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogoniaPolar capQuasars:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]Very Long Baseline ArrayGroup delay and phase delayAstronomy & Astrophysics
researchProduct

Absolute kinematics of radio source components in the complete S5 polar cap sample I. First and second epoch maps at 8.4 GHz

2001

We observed the thirteen extragalactic radio sources of the S5 polar cap sample at 8.4 GHz with the Very Long Baseline Array, on 1997.93 and 1999.41. We present the maps from those two epochs and briefly discuss the morphological changes experimented by some of the radio sources in the 1.4 yr elapsed. These results correspond to the first two epochs at 8.4 GHz of a program directed to study the absolute kinematics of the radio source components of the members of the sample by means of phase delay astrometry at 8.4, 15 and 43 GHz.

PhysicsInterferometricEpoch (reference date)Astrophysics (astro-ph)AstronomyFOS: Physical sciencesAstronomy and AstrophysicsKinematicsAstrophysicsAstrometryAstrometryUNESCO::ASTRONOMÍA Y ASTROFÍSICAAstrophysicsSample (graphics):ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]Astrometry ; Interferometric ; Quasars ; BL Lacertae objectsSpace and Planetary ScienceBL Lacertae objectsUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogoniaPolar capQuasarsVery Long Baseline Array:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]Group delay and phase delay
researchProduct

Absolute kinematics of radio source components in the complete S5 polar cap sample

2007

We report on the first wide-field, high-precision astrometric analysis of the 13 extragalactic radio sources of the complete S5 polar cap sample at 15.4 GHz. We describe new algorithms developed to enable the use of differenced phase delays in wide-field astrometric observations and discuss the impact of using differenced phase delays on the precision of the wide-field astrometric analysis. From this global fit, we obtained estimates of the relative source positions with precisions ranging from 14 to 200 $\mu$as at 15.4 GHz, depending on the angular separation of the sources (from $\sim$1.6 to $\sim$20.8 degrees). These precisions are $\sim$10 times higher than the achievable precisions usi…

PhysicsAngular distanceAstrophysics (astro-ph)Phase (waves)FOS: Physical sciencesAstronomy and AstrophysicsRangingAstrometryAstrophysicsKinematicsAstrophysicsSample (graphics)Wide fieldSpace and Planetary SciencePolar capAstronomy & Astrophysics
researchProduct

Comparison of the dynamics of the AU and PC indices

1998

The properties of AU and PC data were analyzed with different methods. It is shown that the dynamical behavior of the AU and PC time series, as analyzed by the structure function (SF), are very similar, while the SF of the AL time series shows different behavior. The SF of the AL data has a slope of 0.5 up to about 2 hours, after which it quickly decreases to about 0.1. On the other hand the slope of the SFs of AU and PC data continuously decreases to about 0.2, and in a longer time scale. It is suggested that the dissipative auroral electrojet currents have a characteristic time scale of 2 hours, and this underlies the AL dynamics. In contrast with this, the nondissipative Hall currents th…

PhysicsGeophysicsMeteorologyScale (ratio)Cross-correlationStructure functionDynamics (mechanics)Correlation analysisDissipative systemGeneral Earth and Planetary SciencesElectrojetPolar capMolecular physicsGeophysical Research Letters
researchProduct