CMB Telescopes and Optical Systems

The cosmic microwave background radiation (CMB) is now firmly established as a fundamental and essential probe of the geometry, constituents, and birth of the Universe. The CMB is a potent observable because it can be measured with precision and accuracy. Just as importantly, theoretical models of the Universe can predict the characteristics of the CMB to high accuracy, and those predictions can be directly compared to observations. There are multiple aspects associated with making a precise measurement. In this review, we focus on optical components for the instrumentation used to measure the CMB polarization and temperature anisotropy. We begin with an overview of general considerations for CMB observations and discuss common concepts used in the community. We next consider a variety of alternatives available for a designer of a CMB telescope. Our discussion is guided by the ground and balloon-based instruments that have been implemented over the years. In the same vein, we compare the arc-minute resolution Atacama Cosmology Telescope (ACT) and the South Pole Telescope (SPT). CMB interferometers are presented briefly. We conclude with a comparison of the four CMB satellites, Relikt, COBE, WMAP, and Planck, to demonstrate a remarkable evolution in design, sensitivity, resolution, and complexity over the past thirty years.Comment: To appear in: Planets, Stars and Stellar Systems (PSSS), Volume 1: Telescopes and Instrumentatio

The Pioneer Anomaly

Radio-metric Doppler tracking data received from the Pioneer 10 and 11 spacecraft from heliocentric distances of 20-70 AU has consistently indicated the presence of a small, anomalous, blue-shifted frequency drift uniformly changing with a rate of ~6 x 10^{-9} Hz/s. Ultimately, the drift was interpreted as a constant sunward deceleration of each particular spacecraft at the level of a_P = (8.74 +/- 1.33) x 10^{-10} m/s^2. This apparent violation of the Newton's gravitational inverse-square law has become known as the Pioneer anomaly; the nature of this anomaly remains unexplained. In this review, we summarize the current knowledge of the physical properties of the anomaly and the conditions that led to its detection and characterization. We review various mechanisms proposed to explain the anomaly and discuss the current state of efforts to determine its nature. A comprehensive new investigation of the anomalous behavior of the two Pioneers has begun recently. The new efforts rely on the much-extended set of radio-metric Doppler data for both spacecraft in conjunction with the newly available complete record of their telemetry files and a large archive of original project documentation. As the new study is yet to report its findings, this review provides the necessary background for the new results to appear in the near future. In particular, we provide a significant amount of information on the design, operations and behavior of the two Pioneers during their entire missions, including descriptions of various data formats and techniques used for their navigation and radio-science data analysis. As most of this information was recovered relatively recently, it was not used in the previous studies of the Pioneer anomaly, but it is critical for the new investigation.Comment: 165 pages, 40 figures, 16 tables; accepted for publication in Living Reviews in Relativit

Hypoxia: From molecular responses to ecosystem responses

Hypoxia affects thousands of km 2 of marine waters all over the world, and has caused mass mortality of marine animals, benthic defaunation and decline in fisheries production in many places. The severity, frequency occurrence and spatial scale of hypoxia have increased in the last few decades. Due to rapid human population growth and global warming, the problem of hypoxia is likely to become worse in the coming years. Molecular responses of marine animals to hypoxia are poorly known. In many animals, a haem protein probably serves as the cellular sensor for oxygen, and reactive oxygen species are generated as signaling molecules. In mammal and fish, a heterodimeric transcription factor, hypoxia-inducible factor 1 (HIF-1) has been identified. HIF-1 receives signals from the molecular oxygen senor through redox reactions and/or phosphorylation, and in turn, regulates the transcription of a number of hypoxia-inducible genes, including genes involved in erythropoiesis, angiogenesis and glycolysis. These molecular responses then cascade into a series of biochemical and physiological adjustments, enabling the animal to survive better under hypoxic conditions. Marine animals respond to hypoxia by first attempting to maintain oxygen delivery (e.g. increases in respiration rate, number of red blood cells, or oxygen binding capacity of hemoglobin), then by conserving energy (e.g. metabolic depression, down regulation of protein synthesis and down regulation/modification of certain regulatory enzymes). Upon exposure to prolonged hypoxia, animals must eventually resort to anaerobic respiration. Hypoxia reduces growth and feeding, which may eventually affect individual fitness. Effects of hypoxia on reproduction and development of marine animals, albeit important in affecting species survival, remain almost unknown. Many fish and marine organisms can detect, and actively avoid hypoxia. Some benthos may leave their burrows and move to sediment surface during hypoxia. These behaviorial changes may render the animals more vulnerable to predation. Hypoxia may eliminate sensitive species, thereby causing major changes in species composition of benthic, fish and phytoplankton communities. Decreases in species diversity and species richness are well documented, and changes in trophodynamics and functional groups have also been reported. Under hypoxic conditions, there is a general tendency for suspended feeders to be replaced by deposit feeders; demersal fish by pelagic fish; and macrobenthos by meiobenthos. Microflagellates and nanoplankton also tend to dominate in the phytoplankton community in hypoxic environments. Existing evidence suggest that recovery of benthic communities in temperate region take two to several years. Recovery however, appears to be much quicker in subtropical environments. In natural conditions, hypoxia is often associated with increases in ammonia, hydrogen sulphide and particulate organic materials. The inability to isolate effects of hypoxia from interactions of these compounding factors makes it difficult to attribute many of the observed ecological effects to hypoxia. © 2002 Elsevier Science Ltd. All rights reserved.link_to_subscribed_fulltex