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The wind speed decreased and reached minimum 35 min after the last contact. The eclipse -induced decrease of PBL height was about m, with minimum reached 20 min after the eclipse maximum. Although dependent on UV radiation, surface ozone concentration did not show the expected decrease, possibly due to less significant influence of photochemical reactions at the measurement site and decline of PBL height.

Air-ion concentration decreased during the solar eclipse , with minimum almost coinciding with the eclipse maximum. Perturbation of the receiving signal level RSL was observed on March 20, probably induced by the solar eclipse. Eclipse -related perturbations in ionospheric D-region were detected. Full Text Available Transiting exoplanets provide access to data to study the mass-radius relation and internal structure of extrasolar planets. Long-period transiting planets allow insight into planetary environments similar to the Solar System where, in contrast to hot Jupiters, planets are not constantly exposed to the intense radiation of their parent stars.

Observations of secondary eclipses additionally permit studies of exoplanet temperatures and large-scale exo-atmospheric properties. We show how transit and eclipse probabilities are related to planet-star system geometries, particularly for long-period, eccentric orbits. The resulting target selection and observational strategies represent the principal ingredients of our photometric survey of known radial-velocity planets with the aim of detecting transit signatures TERMS. During World War II, the archive was moved to the University of Pennsylvania, which was one of the world centers for Eclipsing Binary research, consequently, the contributions to the catalog during this time were immense.

The catalog has been kept in storage since then. The objective of this project is to digitize this archive and create a fully functional online catalog that contains the information available on the cards, along with the scan of the actual cards. Our group has built a database using a python-powered infrastructure to contain the collected data. The team also built a prototype web-based searchable interface as a front-end to the catalog. Following the data-entry process, information like the Right Ascension and Declination will be run against SIMBAD and any differences between values will be noted as part of the catalog.

Information published online from the card catalog and even discrepancies in information for a star, could be a catalyst for new studies on these Eclipsing Binaries. Once completed, the database-driven interface will be made available to astronomers worldwide. The group will also acquire, from the database, a list of referenced articles that have yet to be found online in order to further pursue their digitization.

This list will be comprised of references in the cards that were neither found on ADS nor online during the data-entry process. Pursuing the integration of these references to online queries such as ADS will be an ongoing process that will contribute and further facilitate studies on Eclipsing Binaries. Relativistic apsidal motion in eccentric eclipsing binaries. Wolf, M. Radial Velocities of 41 Kepler Eclipsing Binaries. Eclipsing binaries are vital for directly determining stellar parameters without reliance on models or scaling relations.

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Spectroscopically derived parameters of detached and semi-detached binaries allow us to determine component masses that can inform theories of stellar and binary evolution. We obtain radial velocities and spectroscopic orbits for five single-lined and 35 double-lined systems, and confirm one false positive eclipsing binary. Finally, we constrain the mass of the tertiary component for five double-lined binaries with previously detected companions. Eclipse Megamovie How did we do? The Eclipse Megamovie program, as set up for the Great American Eclipse of 21 August , achived a massive volunteer participation, making maximal use existing equipment but with coordinated training.

Everything worked fine, and the archive entered the public domain on Friday, October 6. An additional GB of data were obtained by smartphone cameras operating a dedicated free app. The massive oversampling made possible by the many about volunteer observers has opened new parameter space for tracking coronal and chromospheric time development.

Fortuitously some solar activity appeared during the minute period of totality, including a C-class flare and an ongoing CME. At the smartphone level, with the advantage of precise GPS timing, we have data on solar structure via the timing of Baily's Beads at the 2nd and 3rd contacts.

The Megamovie archive is an historical first, and we hope that it has already been a springboard for citizen-science projects. We discuss the execution of the program, presenting some of the science plans and results. We expect that the eclipse of will be better still. Fourier analysis of the light curves of eclipsing variables. The aim of the present paper is to introduce a new definition of the loss of light suffered by mutual eclipses of the components of close binary systems: namely, as a cross-correlation of two apertures representing the eclipsing and eclipsed discs.

The advantages of such a strategy over the more conventional geometrical approach are a greater symmetry of the respective expressions; b greater affinity of expressions arising from distortion with those expressing the light changes due to eclipses of spherical stars; and c greater freedom in dealing with the effects of particular distribution of brightness over the disc of the star undergoing eclipse generalized limb-darkening , as well as of possible semi-transparency of the eclipsing component Wolf-Rayet stars.

In point of fact, none of these tasks could be handled with equal ease by any other technique; nor could the corresponding loss of light be so automated by any other approach. Secondary eclipses in the CoRoT light curves. Full Text Available We identify and characterize secondary eclipses in the original light curves of published CoRoT planets using uniform detection and evaluation criteria.

Our analysis is based on a Bayesian statistics: the eclipse search is carried out using Bayesian model selection, and the characterization of the plausible eclipse candidates using Bayesian parameter estimation. We also find marginally significant eclipse events passing our plausibility criteria for CoRoT-3b, 13b, 18b, and 21b, and confirm the previously published CoRoT-1b and CoRoT-2b eclipses.

More than three years ahead of the "Great American Eclipse " of August , the American Astronomical Society formed the AAS Solar Eclipse Task Force to function as a think tank, coordinating body, and communication gateway to the vast resources available about the eclipse and solar eclipses more generally. The task force included professional and amateur astronomers, formal and informal educators, and science journalists; many had experienced total solar eclipses before, and others would experience their first totality in August These resources were used mainly for three purposes: 1 to build a website that contains basic information about solar eclipses , safe viewing practices, and eclipse imaging and video, along with resources for educators and the media and a searchable map of eclipse -related events and activities, with links to other authoritative websites with more detailed information; 2 to solicit, receive, evaluate, and fund proposals for mini-grants to support eclipse -related education and public outreach to underrepresented groups both inside and outside the path of totality; and 3 to organize a series of multidisciplinary workshops across the country to prepare communities for the eclipse and to facilitate collaborations between astronomers, meteorologists, school administrators, and transporation and emergency-management professionals.

In the weeks immediately preceding the eclipse , it became clear that the marketplace was being flooded by counterfeit eclipse glasses and solar viewers, leading to a last minute change in our communication strategy. In this talk, we'll review the. Impact of perioperative blood pressure variability on health resource utilization after cardiac surgery: an analysis of the ECLIPSE trials.

Sixty-one medical centers in the United States. Patients 18 years or older undergoing cardiac surgery. Clevidipine was compared with nitroglycerin, sodium nitroprusside, and nicardipine. The ECLIPSE trials included 3 individual randomized open-label studies comparing clevidipine to nitroglycerin, sodium nitroprusside, and nicardipine. Blood pressure control was assessed as the integral of the cumulative area under the curve AUC outside specified systolic blood pressure ranges, such that lower AUC represents less variability.

All rights reserved. Educating the Public about the Total Solar Eclipse. On behalf of the International Astronomical Union's Working Group on Solar Eclipses , I have long worked to bring knowledge about eclipses and how to observe the safely to the people of the various countries from which partial, annular, or total solar eclipses are visible. We link to important mapping sites at Eclipse Wise. We are working to disseminate accurate information about how and why to observe the total solar eclipse , trying among other things to head off common misinformation about the hazards of looking at the sun at eclipses or otherwise.

Lunar eclipses : Probing the atmosphere of an inhabited planet. The Moon's brightness during a lunar eclipse is indicative of the composition, cloudiness and aerosol loading of the Earth's atmosphere. The idea of using lunar eclipse observations to characterize the Earth's atmosphere is not new, but the interest raised by the prospects of discovering Earth-like exoplanets transiting their host stars has brought renewed attention to the method. We review some recent efforts made in the prediction and interpretation of lunar eclipses. We also comment on the contribution of the lunar eclipse theory to the refractive theory of planetary transits.

Full Text Available The Moon's brightness during a lunar eclipse is indicative of the composition, cloudiness and aerosol loading of the Earth's atmosphere. Seeing a total solar eclipse is often described as a once-in-a-lifetime experience. However, for many who have experienced totality, once-in-a-lifetime is simply not enough.

They want more, and are willing to go to great lengths often at great expense to repeat the experience. What is it like to experience totality? What is it about the experience that motivates these eclipse chasers? Is there an eclipse chaser personality? Can eclipse chasing actually be described as an addiction? This book describes the people who dedicate their lives to chasing their dream. Kepler eclipsing binary stars.

Synonyms and antonyms of eclipse in the Spanish dictionary of synonyms

Precise eclipse times for close binaries and identification of candidate three-body systems. Conroy, Kyle E. We present a catalog of precise eclipse times and analysis of third-body signals among close binaries in the latest Kepler Eclipsing Binary Catalog. For these short-period binaries, Kepler's 30 minute exposure time causes significant smearing of light curves. In addition, common astrophysical phenomena such as chromospheric activity, as well as imperfections in the light curve detrending process, can create systematic artifacts that may produce fictitious signals in the eclipse timings.

We present a method to measure precise eclipse times in the presence of distorted light curves, such as in contact and near-contact binaries which exhibit continuously changing light levels in and out of eclipse. We identify systems for which we find a timing variation signal compatible with the presence of a third body. These are modeled for the light travel time effect and the basic properties of the third body are derived.

This study complements J. Orosz et al. Together, these two papers provide comprehensive eclipse timings for all binaries in the Kepler Eclipsing Binary Catalog, as an ongoing resource freely accessible online to the community.

Eclipse / Spanish Edition

Continuous photometry from the K2 mission on Campaign Two has revealed the presence of additional eclipses due to the presence of a third star in the system. These are explained by a system composed of the two previously known members of the eclipsing system Ba and Bb with a period of 1.

The timing of the eclipses of Ba and Bb reveals the same Here we combine radial velocities and analytical approximations for the timing of the eclipses to derive masses and radii for the three components of the system. We obtain a mass of 1. HD is the first triply eclipsing system for which radial velocities of all components could be measured. This paper includes data collected by the Kepler mission. The total solar eclipse of was a high-profile opportunity for nationwide public education.

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Astronomy experts suddenly became vital sources of information for a lay population whose interest in the eclipse greatly surpassed expectations. At the National Air and Space Museum, we leveraged our relatively accessible location and particularly diverse audience to help thousands of people, from novices to enthusiasts, prepare to view the eclipse safely.

The goal was to empower all people so they could experience this unique astronomical event, understand what was happening, and observe the Sun safely. Over the course of two years spent talking with the public about the eclipse , we encountered common misconceptions, worries about safety or liability, and people experiencing confusion or information overload.

Eclipse (Spanish Edition)

We developed guidelines for handling these challenges, from correcting misinformation to managing the sudden spike in demand for glasses just before August In particular, we helped people understand the following essential points:- The total phase of the eclipse is only visible from a limited path. Public education about the eclipse appears to have been successful, as evidenced by the large number of people who saw their first total solar eclipse and the absence of reported eye damage cases.

Amidst the excitement, photographs, and stories that. White dwarfs in the WTS: Eclipsing binaries. Full Text Available We have identified photometric white dwarf candidates in the WFCAM transit survey through a reduced proper motion versus colour approach. We have also performed a simple sensitivity analysis in order to assess the ability of the survey to detect companions to white dwarfs via the transit method.

Birkby, J. The WTS is an ongoing photometric monitoring campaign that operates on the 3. The survey began on August 5, and the eclipsing systems presented in this paper are all found in just one of the four WTS fields. Photometric follow-up observations to help test and refine our light-curve models were obtained in the Sloan i band using the Wide-Field Camera WFC on the 2. Zimbabwe's total solar eclipse June 21st Unknown The research was developed to observe and record the effects of the total solar eclipse on the behaviour of wildlife in the park, and covered a period of 3 days in order to provide comparisons between normal and eclipse conditions.

The data is still undergoing comparative analysis, and the results will be submitted to the Visual damage following direct sighting of solar eclipse in Ghana Advanced techniques, such as scanning laser Ophthalmoscopy and the multifocal electroretinography ERG offer the possibility of detailed examination of small retina lesions in Ghana after an eclipse of the sun.

African Journal of Health Sciences Vol. Statistical analysis of geomagnetic field variations during solar eclipses. Though it is generally considered that the geomagnetic field can be modulated during solar eclipses , the effect of the solar eclipse on the observed geomagnetic field has proved subtle to be detected. Instead of exploring the geomagnetic field as a case study, we analyze geomagnetic manifestations acquired by geomagnetic observatories during 39 solar eclipses occurring from to As a result of examining a pattern of the geomagnetic field variation on average, we confirm that the effect can be seen over an interval of min centered at the time of maximum eclipse on a site of a geomagnetic observatory.

That is, demonstrate an increase in the Y component of the geomagnetic field and decreases in the X component and the total strength of the geomagnetic field. We have demonstrated it by dividing the whole data set into subsets based on parameters of the geomagnetic field, solar activity, and solar eclipses. It is suggested, therefore, that an evidence of the solar eclipse effect can be revealed even at the solar maximum, as long as the day of the solar eclipse is magnetically quiet.

Dusenbery, P. More than two million pairs of eclipse glasses were distributed free through public libraries in the U. About 7, organizations, including public library branches, bookmobiles, tribal libraries, library consortia, and state libraries took part in the celestial event of the century. Many organizations received a package of free safe-viewing glasses, plus a page information booklet about eclipse viewing and suggested program ideas. An educational video was also produced on how best to do public outreach programs about the eclipse. This presentation will provide an overview of the extensive collaboration that made this program possible as well as highlight the national impact that public libraries made in their communities.

V tauri. Preparing a Nation for the Eclipse of a Generation -. On August 21st , there was a total solar eclipse visible from a vast swath of the US. In preparation for that event, the American Astronomical society created a taskforce charged with planning for the eclipse for the entire nation. The preparations included interfacing with the public, the media, non-profit organizations and governmental organizations. Moreover, there were no major problems associated with the event, in spite of valiant attempts from, e.

The eclipse offered opportunities for many scientific experiments within and ebyond astronomy. Here we present on the work of the taskforce, and the lessons learned as well as lesser known science experiments undertaken during the eclipse. Local creativity and artistry is a powerful resource that enhances education programs and helps us generate excitement for science within our communities.

With the help of the Maui Economic Development Board and the University of Hawai'is Institute for Astronomy, we solicited art entries from all K schools in Maui County approximately 6 months prior to the eclipse. Along with divisional prizes, a grand prize was selected by a panel of local judges, which was subsequently printed on 25, solar eclipse viewing glasses and distributed to all Maui students. We found that the impact of a locally-sourced glasses design cannot be understated.

Overall, the success of this program relied upon reaching out to individual teachers, supplying educational flyers to all schools, and visiting classrooms. This eclipse art contest was integral to making local connections to help promote science education on Maui, and we suggest that it could be adapted to the solar community's EPO activities for the upcoming Great American Solar Eclipse. The August 21, total solar eclipse across America was, by all accounts, the biggest science education program ever carried out by NASA, significantly larger than the Curiosity Mars landing and the New Horizons Pluto flyby.

Initial accounting estimates over two billion people reached and website hits exceeding five billion. The NASA Science Mission Directorate spent over two years planning and developing this enormous public education program, establishing over 30 official NASA sites along the path of totality, providing imagery from 11 NASA space assets, two high altitude aircraft, and over 50 high altitude balloons.

In addition, a special four focal plane ground based solar telescope was developed in partnership with Lunt Solar Systems that observed and processed the eclipse in 6K resolution. This talk will discuss NASA's strategy, results, and lessons learned; and preview some of the big events we plan to feature in the near future. Eclipses of cataclysmic variables. U Geminorum. U Gem is an eclipsing dwarf nova with an orbital period of 4 h 15 m. High-speed, multicolor photometric observations of U Gem in its quiescent state were obtained. A program was used that synthesizes the light curves of cataclysmic variables to derive the properties of U Gem from its eclipses.

The model also reproduces the published infrared light curves and ultraviolet spectral distributions of U Gem. A mass transfer rate of 7. The structure of the ring around the white dwarf is consistent with the current theories of accretion disk instabilities in dwarf novae. We report eclipse depths of 0. WASPb is one of the hottest planets yet discovered—as hot as an M-class star. The planet's pressure-temperature profile most likely features a thermal inversion. The observations also require WASPb to have near-zero albedo and almost no redistribution of energy from the day side to the night side of the planet.

Eclipse journeys to the dark side of the Moon. On August 21st, over one hundred million people will gather across the USA to witness the most-watched total solar eclipse in history. Eclipse : Journeys to the Dark Side of the Moon, by popular science author Frank Close, describes the spellbinding allure of this beautiful natural phenomenon. The book explains why eclipses happen, reveals their role in history, literature and myth, and introduces us to eclipse chasers, who travel with ecstatic fervor to some of the most inaccessible places on the globe.

The book also includes the author's quest to solve a year-old mystery: how did the moon move backward during a total solar eclipse , as claimed in the Book of Joshua? Eclipse is also the story of how a teacher inspired the author, aged eight, to pursue a career in science and a love affair with eclipses that has taken him to a war zone in the Western Sahara, the South Pacific, and the African bush. The tale comes full circle with another eight-year old boy - the author's grandson - at the great Americ Values of Teff, v sin I, and metallicity for the stars have been derived from medium-resolution spectroscopy.

The stellar pulsation, atmospheric and fundamental parameters e. Relationships between the pulsation periods, amplitudes and stellar parameters in our list have been examined. Significant correlations between the pulsation periods and the orbital periods, Teff, log g, radius, mass ratio, v sin I and the filling factor have been found. A comprehensive catalog of galactic eclipsing binary EB systems with eccentric orbits is presented with more than times of minima determined from the archived photometric data by various sky-survey projects and new photometric measurements.

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  • The systems are divided into two groups according to whether the individual system has a GCVS name or not. Some important statistics for the AM parameters are discussed and compared with those derived for the eccentric EB systems in the Large and Small Magellanic Clouds. Coordinated weather balloon solar radiation measurements during a solar eclipse.

    Solar eclipses provide a rapidly changing solar radiation environment. These changes can be studied using simple photodiode sensors, if the radiation reaching the sensors is unaffected by cloud. Transporting the sensors aloft using standard meteorological instrument packages modified to carry extra sensors, provides one promising but hitherto unexploited possibility for making solar eclipse radiation measurements. For the 20 March solar eclipse , a coordinated campaign of balloon-carried solar radiation measurements was undertaken from Reading The balloons reached sufficient altitude at the eclipse time for eclipse -induced variations in solar radiation and solar limb darkening to be measured above cloud.

    Because the sensor platforms were free to swing, techniques have been evaluated to correct the measurements for their changing orientation. In the swing-averaged technique, the mean value across a set of swings was used to approximate the radiation falling on a horizontal surface; in the swing-maximum technique, the direct beam was estimated by assuming that the maximum solar radiation during a swing occurs when the photodiode sensing surface becomes normal to the direction of the solar beam.

    Both approaches, essentially independent, give values that agree with theoretical expectations for the eclipse -induced radiation changes. This article is part of the themed issue 'Atmospheric effects of solar eclipses stimulated by the UK eclipse '. The anticipation and excitement surrounding the total solar eclipse of provided astronomy educators with an incredible platform to share space science with huge audiences.

    In order to increase our reach, we found success in partnerships. These partnerships proved fruitful for both parties. While MiLB is a national organization, each team is deeply rooted in its community. With this tactic, a handful of NASA representatives were able to reach nearly 30, people. In turn, LRO provided engaging educational content relevant to the context, SMEs to guide the eclipse viewing experience, eclipse glasses, and safety information.

    Our participation drew in an audience who would not typically attend baseball games while we were able to reach individuals who would not normally attend a science event. In addition, the eclipse inspired one team, the Salem-Keizer Volcanoes from Salem, OR, to make baseball history by holding the first ever eclipse delay in professional sports.

    In this talk, we will present on the benefits of the partnership, offer lessons learned, and suggest ways to get involved for the eclipse — and all the baseball seasons in between. Eclipse effects on field crops and marine zooplankton: the 29 March total solar eclipse. Full Text Available Some effects in the biosphere from the Total Solar Eclipse of 29 March were investigated in field crops and marine zooplankton.

    Taking into account the decisive role of light on plant life and productivity, measurements of photosynthesis and stomatal behaviour were conducted on seven important field-grown cereal and leguminous crops. A drop in photosynthetic rates, by more than a factor of 5 in some cases, was observed, and the minimum values of photosynthetic rates ranged between 3.

    The drop in solar irradiance and the increase in mesophyll CO 2 -concentration during the eclipse did not induce stomatal closure thus not blocking CO 2 uptake by plants. Light effects on the photochemical phase of photosynthesis may be responsible for the observed depression in photosynthetic rates. Field studies addressing the migratory responses of marine zooplankton micro-zooplankton ciliates, and meso-zooplankton due to the rapid changes in underwater light intensity were also performed.

    The light intensity attenuation was simulated with the use of accurate underwater radiative transfer modeling techniques. Ciliates, responded to the rapid decrease in light intensity during the eclipse adopting night-time behaviour. From the meso-zooplankton assemblage, various vertical migratory behaviours were adopted by different species. Economou, G.

    Some effects in the biosphere from the Total Solar Eclipse of 29 March were investigated in field crops and marine zooplankton. The drop in solar irradiance and the increase in mesophyll CO2-concentration during the eclipse did not induce stomatal closure thus not blocking CO2 uptake by plants. Field studies addressing the migratory responses of marine zooplankton micro-zooplankton ciliates , and meso-zooplankton due to the rapid changes in underwater light intensity were also performed.

    An Outreach Project to Provide 2. It appears that this project was the single largest program to provide glasses and eclipse information to the public in the U. We were able to get glasses to a diverse set of institutions, including urban, rural, Native American, small town and large city libraries. In this poster, we will summarize the history of the project, the various components and how they worked together, and the results of a post survey of the librarians, which provided numbers, photographs, and impressions from the many libraries and their patrons.

    A map of the libraries involved is at www. All planned activities will engage Space Campers and local high school students in the application of the scientific method as they seek to explore a wide range of observations during the eclipse. Ancient Chinese observations of physical phenomena attending solar eclipses.

    The realization that solar activity probably undergoes changes in qualitative character on time scales greater than the 11 or 22 year cycle but short compared to the duration of recorded history gives renewed importance to historical documents describing the state of solar activity. Modern eclipse observation reveal the presence of solar acitivity through the appearance of coronal structures and prominences. It has been widely remarked that eclipse records prior to the 18th century are uniformly silent on these conspicuous solar eclipse features, raising the possibility, however unlikely, that a change in solar activity has occurred which rendered them only recently noticeable.

    We present here material from ancient Chinese sources, primarily astrological, that describe phenomena attending solar eclipses that are almost certainly coronal structures and prominences. Thus, these aspects of the present character of solar activity have apparently occurred at other times in history, if not continuously. Chronic obstructive pulmonary disease COPD is a complex condition with pulmonary and extra-pulmonary manifestations.

    In preparation for the August 21 total solar eclipse across the continental United States, a multifaceted effort encouraged safe public observation of this spectacular event. However, we experienced mixed results distributing free ISO compliant eclipse glasses. On the positive side, we successfully dispensed several hundred in Virginia through in-school programs about the eclipse.

    We created a eclipse information sheet to accompany a safe-viewing handout. To facilitate sending glasses home in student backpacks, we wrapped each pair in a double-sided flyer and sealed the bundle in an individual envelope. We also passed out glasses during evening and weekend activities at a planetarium. Religious, business, and educational groups were all excited to receive them as were co-workers, family, and friends.

    On the negative side, planetarium staff declined to give eclipse glasses to students without a parent due to safety and liability concerns. Then, a day camp returned pairs less than 72 hours before the event for the same reasons. However, we also received several requests from groups that had waited until too late to be accommodated easily. While many people were well prepared, the recalls and reported counterfeiting made others suspicious. The experiences of the total solar eclipse , both good and bad, will not completely fade before preparations for begin.

    We look forward enthusiastically to sharing that event with as many people as possible and hope that the overall distribution of eclipse glasses goes more smoothly. Physics Of Eclipsing Binaries. Towards the Increased Model Fidelity. The precision of photometric and spectroscopic observations has been systematically improved in the last decade, mostly thanks to space-borne photometric missions and ground-based spectrographs dedicated to finding exoplanets. The field of eclipsing binary stars strongly benefited from this development.

    Eclipsing binaries serve as critical tools for determining fundamental stellar properties masses, radii, temperatures and luminosities , yet the models are not capable of reproducing observed Hot spot manifestation in eclipsing dwarf nova HT Cassiopeiae. We report the detection of the hot spot in light curves of the eclipsing dwarf nova HT Cassiopeiae during its superoutburst in November.

    Analysis of eight reconstructed light curves of the hot spot eclipses showed directly that the brightness of the hot spot was changing significantly during the superoutburst. Thereby, detected hot spot manifestation in HT Cas is the newest observational evidence for the EMT model for dwarf novae.

    A new general expression for the theoretical moments Asub 2m of the light curves of eclipsing systems has been presented in the form of infinite series expansion. In this expansion, the terms have been given as the product of two different polynomials which satisfy certain three-term recursion formulae, and the coefficients diminish rapidly with increasing number of terms. Thus, the numerical values of the theoretical moments Asub 2m can be generated recursively up to four significant figures for any given set of eclipse elements.

    This can be utilized to solve the eclipse elements in two ways: i with an indirect method, ii with a direct method as minimization to the observational moments Asub 2m area fitting. The procedures for obtaining the elements of any eclipsing system consisting of spherical stars have been automated by making use of the new expression for the moments Asub 2m of the light curves. The theoretical functions f 0 , f 2 , f 4 , f 6 , g 2 and g 4 which are the functions of a and c 0 , have been used to solve the eclipse elements from the observed photometric data. The closed-form expressions for the functions f 2 , f 4 and f 6 have also been derived in terms of Kopal's I-integrals.

    The automated methods for obtaining the eclipse elements from one minimum alone have been tested on the light curves of YZ 21 Cassiopeiae under the spherical model assumptions. The results of these applications are given. Hudson, H. Our intention is to have used this opportunity as a trial run for the eclipse in , which features 1.

    Conceived first and foremost as an education and public outreach activity, the plan is to engage the public in solar science and technology by providing a way for them to include images they have taken of the solar eclipse , into a movie representation of coronal evolution in time. This project will assimilate as much eclipse photography as possible from the public.

    Eclipse / Spanish Edition by Stephenie Meyer, Paperback | Barnes & Noble®

    She used to work for the U. And when they decided she was a liability, they came for her without warning. Now, she rarely stays in the same place or uses the same name for long. They want her dead, and soon. But it means taking one last job for her ex-employers. To her horror, the information she acquires only makes her situation more dangerous. Resolving to meet the threat head on, she prepares for the toughest fight of her life, but finds herself falling for a man who can only complicate her likelihood of survival. As she sees her choices being rapidly whittled down, she must apply her unique talents in ways she never dreamed of.

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