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This white paper is a call for a concerted effort to support total solar eclipse observations over the next decade, in particular for the 21 August 2017 eclipse which will traverse the US continent. With the recent advances in image…

Solar and Stellar Astrophysics · Physics 2015-03-19 Shadia R. Habbal , John Cooper , Adrian Daw , Adalbert Ding , Miloslav Druckmuller , Ruth Esser , Judd Johnson , Huw Morgan

Snowden and coworkers have presented a model for the 1/4 keV soft X-ray diffuse background in which the observed flux is dominated by a ~ 10^6 K thermal plasma located in a 100-300 pc diameter bubble surrounding the Sun, but has significant…

Astrophysics · Physics 2009-04-13 Eric C. Bellm , John E. Vaillancourt

We searched for a fast moving H$\alpha$ shell around the Crab nebula. Such a shell could account for this supernova remnant's missing mass, and carry enough kinetic energy to make SN 1054 a normal Type II event. Deep H$\alpha$ images were…

Solar and Stellar Astrophysics · Physics 2009-11-13 A. Tziamtzis , M. Schirmer , P. Lundqvist , J. Sollerman

We report the results of polarimetric observations of the total solar eclipse of 21 August 2017 from Rexburg, Idaho (USA). We use three synchronized DSLR cameras with polarization filters oriented at 0{\deg}, 60{\deg}, and 120{\deg} to…

In this article we present examples of a wider study of space-time correlation of electron precipitation event of the Van Allen belts with the position and time of occurrence of strong (M>6.5) earthquakes. The study is based on the analysis…

Geophysics · Physics 2010-12-17 G. Anagnostopoulos , V. Rigas , E. Vassiliadis

In-depth analysis of eclipsing binary (EB) observational data collected for several decades can inform us about a lot of astrophysically interesting processes taking place in the systems. We have developed a wide-ranging method for the…

Instrumentation and Methods for Astrophysics · Physics 2014-03-05 Zdeněk Mikulášek , Miloslav Zejda , Marek Chrastina , ShengBang Qian , LiYing Zhu

Eclipsing, short-period post-common envelope binaries (PCEBs) have been studied for several decades by eclipse timing variations (ETVs) which have been interpreted as being caused by circumbinary bodies. In this paper we report 355 new…

Solar and Stellar Astrophysics · Physics 2025-10-29 D. Pulley , I. D. Sharp , J. Mallett , S. von Harrach

Solar eclipses offer unparalleled opportunities for public engagement in astronomy. Large groups of people often gather to view eclipses, and these events require affordable and easy to use tools to safely observe the Sun. One unique way to…

We report 90 new observations of three post common envelope binaries at primary eclipse spanning between December 2018 to February 2022. We combine recent primary eclipse timing observations with previously published values to search for…

Solar and Stellar Astrophysics · Physics 2022-10-05 Xinyu Mai , Robert L. Mutel

The search for young planets had its first breakthrough with the detection of the accreting planet PDS70b. In this study, we aim to broaden our understanding towards the formation of multi-planet systems such as HR8799 or the Solar System.…

Strong He I 1083 nm atomic line signals have been previously measured during total solar eclipses at coronal heights above the lunar limb. This rather unexpected measurement has kindled a discussion about the hypothesized presence of…

Solar and Stellar Astrophysics · Physics 2025-06-04 M. E. Molnar , R. Casini , P. Bryans , B. Berkey , K. Tyson

At least 50% of the baryons in the local universe are undetected and predicted to be in a hot dilute phase (1E5-1E7 K) in low and moderate overdensity environments. We searched for the predicted diffuse faint emission through shadowing…

Cosmology and Nongalactic Astrophysics · Physics 2009-09-30 Joel N. Bregman , Birgit Otte , Jimmy A. Irwin , Mary E. Putman , Edward J. Lloyd-Davies , Christian Brüns

A significant fraction of debris discs consist of a bright ring beyond which extends a wide halo. Such a halo should be made of small grains produced in the ring of parent bodies (PB) and pushed on high-e orbits by radiation pressure. It…

Earth and Planetary Astrophysics · Physics 2023-07-05 Philippe Thebault , Johan Olofsson , Quentin Kral

We present calculations of the heliospheric SWCX emission spectra and their contributions in the ROSAT 1/4 keV band. We compare our results with the soft X-ray diffuse background (SXRB) emission detected in front of 378 identified shadowing…

Astrophysics · Physics 2011-02-11 D. Koutroumpa , R. Lallement , J. C. Raymond , V. Kharchenko

AX J1745.6-2901 is an eclipsing low mass X-ray binary (LMXB) in the Galactic Centre (GC). It shows significant X-ray excess emission during the eclipse phase, and its eclipse light curve shows an asymmetric shape. We use archival XMM-Newton…

High Energy Astrophysical Phenomena · Physics 2018-04-25 Chichuan Jin , Gabriele Ponti , Frank Haberl , Randall Smith , Lynne Valencic

This work presents possible quasi-periodic oscillations in the Transiting Exoplanet Survey Satellite observations of blazars that are in the 157-month hard X-ray survey done by Swift's Burst Alert Telescope. We report observations from four…

High Energy Astrophysical Phenomena · Physics 2025-12-15 Ashutosh Tripathi , Paul J. Wiita , Krista Lynne Smith

Light pollution, a typically underrecognized environmental issue, has gained attention in recent years. While controlling light pollution requires sustained efforts, Earth Hour offers a unique natural experimental setting to assess…

Instrumentation and Methods for Astrophysics · Physics 2025-07-04 Chu Wing So , Chun Shing Jason Pun , Shengjie Liu , Sze Leung Cheung , Ho Keung Kenneith Hui , Kelly Blumenthal , Constance Elaine Walker

Precise starlight positions near the sun were measured during the 21 August 2017 total solar eclipse in order to measure their gravitational deflections. The equipment, procedures, and analysis are described in detail. A portable refractor,…

Instrumentation and Methods for Astrophysics · Physics 2018-03-28 Donald G. Bruns

We report high precision spectrophotometric observations of four planetary transits of HD 209458, in the region of the sodium resonance doublet at 589.3 nm. We find that the photometric dimming during transit in a bandpass centered on the…

Astrophysics · Physics 2011-07-18 David Charbonneau , Timothy M. Brown , Robert W. Noyes , Ronald L. Gilliland