794 research outputs found
Millimetric Astronomy from the High Antarctic Plateau: site testing at Dome C
Preliminary site testing at Dome C (Antarctica) is presented, using both
Automatic Weather Station (AWS) meteorological data (1986-1993) and
Precipitable Water Vapor (PWV) measurements made by the authors. A comparison
with South Pole and other sites is made. The South Pole is a well established
astrophysical observing site, where extremely good conditions are reported for
a large fraction of time during the year. Dome C, where Italy and France are
building a new scientific station, is a potential observing site in the
millimetric and sub-millimetric range. AWS are operating at both sites and they
have been continuously monitoring temperature, pressure, wind speed and
direction for more than ten years. Site testing instruments are already
operating at the South Pole (AASTO, Automated Astrophysical Site-Testing
Observatory), while ''light'' experiments have been running at Dome C (APACHE,
Antarctic Plateau Anisotropy CHasing Experiment) during summertime. A direct
comparison between the two sites is planned in the near future, using the
AASTO. The present analysis shows that the average wind speed is lower at Dome
C (~1 m/s) than at the South Pole (~2 m/s), while temperature and PWV are
comparable.Comment: 10 pages, 8 figures, se also http://www.atnf.csiro.au/pasa/16_2
Stomach Content Analysis of Recent Snowy Owl (\u3ci\u3eBubo scandiacus\u3c/i\u3e) Specimens from Nebraska
The Snowy Owl (Bubo scandiacus) is a circumpolar bird of prey that breeds in extreme northern latitudes, including Canadian and Alaskan tundra. During winter months, some immature and non-breeding birds disperse south. North American birds may travel to southern Canada and northern parts of the United States, and in some extreme cases as far south as Oklahoma and Texas (Parmelee 1992). Although not fully understood, these irruptive events may be caused by the abundance of prey in northern Canada and Alaska (Parmelee 1992).
Prey typical of Snowy Owls are small mammals (e.g., lemmings and hares) of their home range and an occasional bird from a variety of species including waterfowl (Parmelee, 1992). Research on prey items selected by birds outside of breeding range in North America primarily includes ducks and grebes in southwest British Columbia (Campbell and Maccoll 1978), voles in Montana (Detienne et al. 2008), and mice and voles in southern Alberta and Michigan (Boxall and Lein 1982, Chamberlin 1980, respectively).
Over the past century, several irruptions of Snowy Owls have been recorded in Nebraska, most notably during the winters of 1917-18, 1954-55, and 2011-12 (Jorgensen et al., 2012). The most recent of these irruptions, during the winter of 2011-12, produced the largest number of confirmed Snowy Owl sightings in Kansas and Missouri, possibly explained by the increased ease of communication through the use of mobile technology in the general public (Robbins and Otte 2013).
Once reaching areas as far south as Nebraska, Snowy Owls typically suffer high rates of mortality, possibly due to lack of prey species, disease, or anthropogenic factors (Kerlinger and Lein 1988, Meade 1942). During the 2011-12 irruption, several carcasses were donated to the University of Nebraska State Museum (UNSM) and provided a source for examination of body condition and diet. Also included was one carcass donated to UNSM during the following winter, 2012-13
The Planck Low Frequency Instrument
The Low Frequency Instrument (LFI) of the "Planck Surveyor" ESA mission will
perform high-resolution imaging of the Cosmic Microwave Background anisotropies
at four frequencies in the 30-100 GHz range. We review the LFI main scientific
objectives, the current status of the instrument design and the on-going effort
to develop software simulations of the LFI observations. In particular we
discuss the design status of the PLANCK telescope, which is critical for
reaching adequate effective angular resolution.Comment: 10 pages, Latex (use epsfig.sty); 4 Postscript figures; Astrophys.
Lett & Comm, in press. Proc. of the Conference: "The Cosmic Microwave
Background and the Planck Mission", Santander, Spain, 22-25 June 199
Planck Low Frequency Instrument: Beam Patterns
The Low Frequency Instrument on board the ESA Planck satellite is coupled to
the Planck 1.5 meter off-axis dual reflector telescope by an array of 27
corrugated feed horns operating at 30, 44, 70, and 100 GHz. We briefly present
here a detailed study of the optical interface devoted to optimize the angular
resolution (10 arcmin at 100 GHz as a goal) and at the same time to minimize
all the systematics coming from the sidelobes of the radiation pattern. Through
optical simulations, we provide shapes, locations on the sky, angular
resolutions, and polarization properties of each beam.Comment: On behalf of the Planck collaboration. 3 pages, 1 figure. Article
published in the Proceedings of the 2K1BC Experimental Cosmology at
millimetre wavelength
Dynamic validation of the Planck/LFI thermal model
The Low Frequency Instrument (LFI) is an array of cryogenically cooled
radiometers on board the Planck satellite, designed to measure the temperature
and polarization anisotropies of the cosmic microwave backgrond (CMB) at 30, 44
and 70 GHz. The thermal requirements of the LFI, and in particular the
stringent limits to acceptable thermal fluctuations in the 20 K focal plane,
are a critical element to achieve the instrument scientific performance.
Thermal tests were carried out as part of the on-ground calibration campaign at
various stages of instrument integration. In this paper we describe the results
and analysis of the tests on the LFI flight model (FM) performed at Thales
Laboratories in Milan (Italy) during 2006, with the purpose of experimentally
sampling the thermal transfer functions and consequently validating the
numerical thermal model describing the dynamic response of the LFI focal plane.
This model has been used extensively to assess the ability of LFI to achieve
its scientific goals: its validation is therefore extremely important in the
context of the Planck mission. Our analysis shows that the measured thermal
properties of the instrument show a thermal damping level better than
predicted, therefore further reducing the expected systematic effect induced in
the LFI maps. We then propose an explanation of the increased damping in terms
of non-ideal thermal contacts.Comment: Planck LFI technical papers published by JINST:
http://www.iop.org/EJ/journal/-page=extra.proc5/1748-022
Millimeter and sub-millimeter atmospheric performance at Dome C combining radiosoundings and ATM synthetic spectra
The reliability of astronomical observations at millimeter and sub-millimeter
wavelengths closely depends on a low vertical content of water vapor as well as
on high atmospheric emission stability. Although Concordia station at Dome C
(Antarctica) enjoys good observing conditions in this atmospheric spectral
windows, as shown by preliminary site-testing campaigns at different bands and
in, not always, time overlapped periods, a dedicated instrument able to
continuously determine atmospheric performance for a wide spectral range is not
yet planned. In the absence of such measurements, in this paper we suggest a
semi-empirical approach to perform an analysis of atmospheric transmission and
emission at Dome C to compare the performance for 7 photometric bands ranging
from 100 GHz to 2 THz. Radiosoundings data provided by the Routine
Meteorological Observations (RMO) Research Project at Concordia station are
corrected by temperature and humidity errors and dry biases and then employed
to feed ATM (Atmospheric Transmission at Microwaves) code to generate synthetic
spectra in the wide spectral range from 100 GHz to 2 THz. To quantify the
atmospheric contribution in millimeter and sub-millimeter observations we are
considering several photometric bands in which atmospheric quantities are
integrated. The observational capabilities of this site at all the selected
spectral bands are analyzed considering monthly averaged transmissions joined
to the corresponding fluctuations. Transmission and pwv statistics at Dome C
derived by our semi-empirical approach are consistent with previous works. It
is evident the decreasing of the performance at high frequencies. We propose to
introduce a new parameter to compare the quality of a site at different
spectral bands, in terms of high transmission and emission stability, the Site
Photometric Quality Factor.Comment: accepted to MNRAS with minor revision
The Planck-LFI flight model composite waveguides
The Low Frequency Instrument on board the PLANCK satellite is designed to
give the most accurate map ever of the CMB anisotropy of the whole sky over a
broad frequency band spanning 27 to 77 GHz. It is made of an array of 22
pseudo-correlation radiometers, composed of 11 actively cooled (20 K) Front End
Modules (FEMs), and 11 Back End Modules (BEMs) at 300K. The connection between
the two parts is made with rectangular Wave Guides. Considerations of different
nature (thermal, electromagnetic and mechanical), imposed stringent
requirements on the WGs characteristics and drove their design. From the
thermal point of view, the WG should guarantee good insulation between the FEM
and the BEM sections to avoid overloading the cryocooler. On the other hand it
is essential that the signals do not undergo excessive attenuation through the
WG. Finally, given the different positions of the FEM modules behind the focal
surface and the mechanical constraints given by the surrounding structures,
different mechanical designs were necessary. A composite configuration of
Stainless Steel and Copper was selected to satisfy all the requirements. Given
the complex shape and the considerable length (about 1.5-2 m), manufacturing
and testing the WGs was a challenge. This work deals with the development of
the LFI WGs, including the choice of the final configuration and of the
fabrication process. It also describes the testing procedure adopted to fully
characterize these components from the electromagnetic point of view and the
space qualification process they underwent. Results obtained during the test
campaign are reported and compared with the stringent requirements. The
performance of the LFI WGs is in line with requirements, and the WGs were
successfully space qualified.Comment: this paper is part of the Prelaunch status LFI papers published on
JINST: http://www.iop.org/EJ/journal/-page=extra.proc5/jins
Meteorologic parameters analysis above Dome C made with ECMWF data
In this paper we present the characterization of all the principal
meteorological parameters (wind speed and direction, pressure, absolute and
potential temperature) extended over 25 km from the ground and over two years
(2003 and 2004) above the Antarctic site of Dome C. The data set is composed by
'analyses' provided by the General Circulation Model (GCM) of the European
Center for Medium Weather Forecasts (ECMWF) and they are part of the catalog
MARS. A monthly and seasonal (summer and winter time) statistical analysis of
the results is presented. The Richardson number is calculated for each month of
the year over 25 km to study the stability/instability of the atmosphere. This
permits us to trace a map indicating where and when the optical turbulence has
the highest probability to be triggered on the whole troposphere, tropopause
and stratosphere. We finally try to predict the best expected isoplanatic angle
and wavefront coherence time employing the Richardson number maps, the wind
speed profiles and simple analytical models of CN2 vertical profiles.Comment: 28 pages, 14 figures, pdf file, to be published on July 2006 - PASP,
see also http://www.arcetri.astro.it/~masciad
The Planck Telescope
In this paper we present an overview of the Telescope designed for ESA's
mission dedicated to map the Cosmic Microwave Background Anisotropies and
Polarization. Two instruments, LFI and HFI, operate in an overall frequency
range between 25 and 900 GHz and share the focal region of the 1.5 meter
optimized telescope. The optimization techniques adopted for the optical design
and the telescope characteristic are reported and discussed.Comment: On behalf of the Planck collaboration. 5 pages, 4 figures. The
following article has been submitted for publication in the AIP Proceedings
of the Workshop on "Experimental Cosmology at millimeter wavelengths",
Cervinia, Italy, 9-13 July 200
- …