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Related papers: The April 1, 2471 b.C. eclipse and the end of 4th …

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The solar system has changed dramatically since its birth, and so did our understanding of it. A considerable research effort has been invested in the past decade in an attempt to reconstruct the solar system history, including the earliest…

Earth and Planetary Astrophysics · Physics 2015-07-17 D. Nesvorny , F. Roig

A re-investigation of the parapegma of Euktemon (5th century BC, Athens), based on the assumption that some star observations may in fact have been calculated rather than directly observed. The calculation follows Pliny, Natural History…

History and Philosophy of Physics · Physics 2018-01-19 Robert Hannah

We present a case study of the 13 July 2004 solar event, in which disturbances caused by eruption of a filament from an active region embraced a quarter of the visible solar surface. Remarkable are absorption phenomena observed in the…

Astrophysics · Physics 2008-11-07 V. V. Grechnev , A. M. Uralov , V. A. Slemzin , I. M. Chertok , I. V. Kuzmenko , K. Shibasaki

The earliest written reference in Indian astronomy to a total solar eclipse is in the Rig Veda where Rishi Atri is said to have demolished the asura Swarbhanu to liberate the Sun from a total solar eclipse. The Rig Veda describes the…

History and Philosophy of Physics · Physics 2024-07-30 Mayank Vahia , Misturu Soma

The "extended" solar cycle 24 began in 1999 near 70 degrees latitude, similarly to cycle 23 in 1989 and cycle 22 in 1979. The extended cycle is manifested by persistent Fe XIV coronal emission appearing near 70 degrees latitude and slowly…

Solar and Stellar Astrophysics · Physics 2010-08-20 Richard C. Altrock

Our analysis in Papers I and II (Grechnev et al., 2014, Solar Phys. 289, 289 and 1279) of the 18 November 2003 solar event responsible for the 20 November geomagnetic superstorm has revealed a complex chain of eruptions. In particular, the…

Solar and Stellar Astrophysics · Physics 2014-05-27 A. M. Uralov , V. V. Grechnev , G. V. Rudenko , I. I. Myshyakov , I. M. Chertok , B. P. Filippov , V. A. Slemzin

We report on the 22-23 June 2015 geomagnetic storm. There has been a shortage of intense geomagnetic storms during the current solar cycle 24 in relation to the previous cycle. This situation changed after mid-June 2015 when one of the…

4U 2129+47 was discovered in the early 80's and classified as an accretion disk corona source due to its broad and partial X-ray eclipses. The 5.24 hr binary orbital period was inferred from the X-ray and optical light curve modulation,…

The solar activity in Cycle 23--24 shows differences from the previous cycles that were observed with modern instruments, e.g. long cycle duration and a small number of sunspots. To appreciate the anomalies further, we investigated the…

Solar and Stellar Astrophysics · Physics 2015-06-16 Masumi Shimojo

Although sunspots have been systematically observed on the Sun's surface over the last four centuries, their magnetic properties have been revealed and documented only since the early 1900s. Sunspots typically appear in pairs of opposite…

Solar and Stellar Astrophysics · Physics 2019-09-25 Soumitra Hazra , Dibyendu Nandy

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

Sunspots have been known in the West since Galileo Galilei and Thomas Harriot first used telescopes to observe the Sun nearly four centuries ago; they have been known to the Chinese for more than two thousand years. They appear as…

Solar and Stellar Astrophysics · Physics 2015-05-14 D. O. Gough

On 21 August 2017 a total solar eclipse swept across the contiguous United States providing excellent opportunities for diagnostics of the Sun's corona. The Sun's coronal structure is notoriously difficult to observe except during solar…

Solar and Stellar Astrophysics · Physics 2017-10-03 Dibyendu Nandy , Prantika Bhowmik , Anthony R. Yeates , Suman Panda , Rajashik Tarafder , Soumyaranjan Dash

This work deals with the comparison of different parameters (French/IMCCE and US/JPL ephemerides) used to calculate the extension of the umbral shadow and the location of the centre line in the total solar eclipse that took place on March,…

Solar and Stellar Astrophysics · Physics 2012-02-07 Laura Giannuzzo

This is a historian's view of how modern astronomy data can be used to discuss the shifting historical worldview of Late Antiquity. In this article an attemp is made to construct an approximate model of how the cycles of astronomical…

History and Philosophy of Physics · Physics 2024-03-07 D. N. Starostin

The 8 April 2024 total solar eclipse (TSE) provides a unique opportunity to study the solar corona. This work presents our prediction of the solar corona at the time of the eclipse based on magnetohydrodynamic (MHD) modeling performed with…

Solar radio type IV bursts can sometimes show directivity, so that no burst is observed when the source region in located far from the solar disk center. This has recently been verified also from space observations, at decameter…

Solar and Stellar Astrophysics · Physics 2019-06-19 Silja Pohjolainen , Nasrin Talebpour Sheshvan

The mysterious 3rd magnitude long period eclipsing binary star system epsilon Aurigae is predicted to be starting its 2 year eclipse in the late summer of 2009. While this is when the real excitement starts, much is to be learned before…

Astrophysics · Physics 2008-07-18 J. L. Hopkins , L. Schanne , R. E. Stencel

We report the observations of a moderate but relatively intense geo-effective solar eruption on 2015 November 4 from the peripheral diffusive polarities of active region 12443. We use space-borne Solar Dynamics Observatory and ACE…

Solar and Stellar Astrophysics · Physics 2018-08-22 Rui Wang , Ying D. Liu , Huidong Hu , Xiaowei Zhao

Astronomical observations were used as a marker for time and the Calendar from ancient times. A more subtle calibration of epochs is thrown up by an observation of the position of the solstices and equinoxes, because these points shift in…

General Physics · Physics 2011-02-04 Burra G. Sidharth
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