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Related papers: The solar eclipse of August 30, 1905 at Alcala de …

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In a recent article by Scafetta, 2010, the author investigates whether or not the decadal and multi-decadal climate oscillations have an astronomical origin. In particular, the author note that several global surface temperature records,…

Data Analysis, Statistics and Probability · Physics 2011-05-20 S. Sello

In Book 8 of his Geographike Hyphegesis Ptolemy gives coordinates for ca. 360 so-called noteworthy cities. These coordinates are the time difference to Alexandria, the length of the longest day, and partly the ecliptic distance from the…

History and Philosophy of Physics · Physics 2015-03-04 Christian Marx

Epsilon Aurigae is a complicated binary star that undergoes optical eclipses every 27 years, including the present year. An update is given here on the array of photometric and spectroscopic observations underway, thanks to the eclipse…

Solar and Stellar Astrophysics · Physics 2010-06-07 Robert E. Stencel

Small radio telescope in 21cm was used for studying the partial solar eclipse, with magnitude 0.89, in Hong Kong on 21st June, 2020. The radio telescope SPIDER 300A was designed and constructed by the Radio2Space Company, Italy. Radio flux…

Instrumentation and Methods for Astrophysics · Physics 2022-07-05 Chun Sing Leung , Thomas K. T. Fok , Kenneith H. K. Hui , K. W. Ng , C. M. Lee , S. H. Chan

A total lunar eclipse is plausible to have an influence on the variation of some environmental physical parameters, specifically on the conditions of the sky brightness, humidity and temperature. During the eclipse on 14$^{th}$-15$^{th}$…

Instrumentation and Methods for Astrophysics · Physics 2021-03-31 C. Góez Therán , S. Vargas Domínguez

The All Sky Automated Survey (ASAS) is monitoring all sky to about 14 mag with a cadence of about 1 day; it has discovered about 10^5 variable stars, most of them new. The instrument used for the survey had aperture of 7 cm. A search for…

Astrophysics · Physics 2009-11-11 Bohdan Paczynski

A striking coincidence of revolution periods of S-stars orbiting a supermassive black hole at the Galactic Center of the Milky Way and oscillation periods of such solar and terrestrial observables as the sunspot number, the geomagnetic…

High Energy Astrophysical Phenomena · Physics 2015-02-03 V. D. Rusov , V. P. Smolyar , M. V. Eingorn

A search for possible radiative decays of solar neutrinos with emission of photons in the visible range was performed during the total solar eclipse of August 11, 1999. Due to very bad weather conditions our two telescopes were unable to…

High Energy Physics - Experiment · Physics 2011-02-21 S. Cecchini , G. Giacomelli , R. Giacomelli , D. Hasegan , O. Maris , V. Popa , R. Serra , M. Serrazanetti , L. Stefanov , L. Tasca , V. Valeanu

We carried out white-light observations of the total solar eclipse on 13 November 2012 at two sites, where the totality occurred 35 minutes apart. We caught an ongoing coronal mass ejection (CME) and a pre-CME loop structure just before the…

Solar and Stellar Astrophysics · Physics 2020-07-29 Yoichiro Hanaoka , Jun Nakazawa , Osamu Ohgoe , Yoshiaki Sakai , Kazuo Shiota

Astrometry, the most ancient branch of astronomy, was facing extinction during much of the 20th century in the competition with astrophysics. The revival of astrometry came with the European astrometry satellite Hipparcos, approved by ESA…

Instrumentation and Methods for Astrophysics · Physics 2014-08-12 Erik Høg

Context. In previous work, we studied a prominence which appeared like a tornado in a movie made from 193 {\AA} filtergrams obtained with the Atmospheric Imaging Assembly (AIA) imager aboard the Solar Dynamics Observatory (SDO). The…

Solar and Stellar Astrophysics · Physics 2019-03-27 M. Zapiór , B. Schmieder , P. Mein , N. Mein , N. Labrosse , M. Luna

We present the XMM-Newton observations obtained during four revolutions in Spring and Summer 2004 of CXOGC J174540.0-290031, a moderately bright transient X-ray source, located at only 2.9" from SgrA*. We report the discovery of sharp and…

Astrophysics · Physics 2009-11-11 D. Porquet , N. Grosso , G. Belanger , A. Goldwurm , F. Yusef-Zadeh , R. S. Warwick , P. Predehl

A rare eclipse of the mysterious object Epsilon Aurigae will occur in 2009-2011. We report an updated single-lined spectroscopic solution for the orbit of the primary star based on 20 years of monitoring at the CfA, combined with historical…

Solar and Stellar Astrophysics · Physics 2015-05-18 Robert P. Stefanik , Guillermo Torres , Justin Lovegrove , Vivian E. Pera , David W. Latham , Joseph Zajac , Tsevi Mazeh

On 12 March 1996 we obtained observations of the quiet Sun with the SUMER instrument. The observa- tions were sequences of 15-20 second exposures of ultraviolet emission line profiles and of the neighboring continua. These data contain…

Astrophysics · Physics 2009-10-30 Mats Carlsson , Philip G. Judge , Klaus Wilhelm

The North-South asymmetry of solar activity has been recognized for different solar phenomena. Following Waldmeier, it is now assumed that solar activity dominates in the Northern solar hemisphere during the ascending part of the secular…

Space Physics · Physics 2007-05-23 K. Georgieva , B. Kirov

On Oct. 29th, 2015, the Earth crossed through a fold in the heliospheric current sheet. This is called a "solar sector boundary crossing". Under this circumstances, a large coronal mass ejection (CME) occurred at 2:24 UT, behind the west…

Solar and Stellar Astrophysics · Physics 2016-03-30 C. R. A. Augusto , C. E. Navia , M. N. de Oliveira , A. A. Nepomuceno , A. C. Fauth

In 1844 Schwabe discovered that the number of sunspots increased and decreased over a period of about 11 years, that variation became known as the sunspot cycle. Almost eighty years later, Hale described the nature of the Sun's magnetic…

This review article summarizes the advancement in the studies of Earth-affecting solar transients in the last decade that encompasses most of solar cycle 24. The Sun Earth is an integrated physical system in which the space environment of…

The value of the eclipse solar radius during the 2017 August 21 total solar eclipse was estimated to be $S_{\odot} = (959.95\pm 0.05)"$ at $1\,au$ with no significant dependence on wavelength. The measurement was obtained from the analysis…

Solar and Stellar Astrophysics · Physics 2021-09-30 Luca Quaglia , John Irwin , Konstantinos Emmanouilidis , Alessandro Pessi

Planets in highly eccentric orbits form a class of objects not seen within our Solar System. The most extreme case known amongst these objects is the planet orbiting HD~20782, with an orbital period of 597~days and an eccentricity of 0.96.…