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Brightness inhomogeneities in the stellar photosphere (dark spots or bright regions) affect the measurements of the planetary transmission spectrum. To investigate the star spots of the M dwarf GJ 1214, we conducted a multicolor photometric…

Solar and Stellar Astrophysics · Physics 2018-06-13 M. Mallonn , E. Herrero , I. G. Juvan , C. von Essen , A. Rosich , I. Ribas , T. Granzer , X. Alexoudi , K. G. Strassmeier

The angular and frequency correlation functions of the transmission coefficient for light propagation through a strongly scattering amplifying medium are considered. It is found that just as in the case of an elastic scattering medium the…

Mesoscale and Nanoscale Physics · Physics 2009-10-31 A. A. Burkov , A. Yu. Zyuzin

Measuring time lags between time-series or lighcurves at different wavelengths from a variable or transient source in astronomy is an essential probe of physical mechanisms causing multiwavelength variability. Time-lags are typically…

Instrumentation and Methods for Astrophysics · Physics 2021-06-17 Nachiketa Chakraborty , Peter Jan van Leeuwen

The Kepler target KIC 5110407, a K-type star, shows strong quasi-periodic light curve fluctuations likely arising from the formation and decay of spots on the stellar surface rotating with a period of 3.4693 days. Using an established…

Solar and Stellar Astrophysics · Physics 2015-06-15 Rachael M. Roettenbacher , John D. Monnier , Robert O. Harmon , Thomas Barclay , Martin Still

Unlocking the full potential of passivating contacts, increasingly popular in the silicon solar cell industry, requires determining the minority carrier lifetime. Minor passivation drops limit the functioning of solar cells, however, they…

Applied Physics · Physics 2021-07-02 Jean Cattin , Jan Haschke , Christophe Ballif , Matthieu Boccard

In this letter we have analyzed the temporal correlations of the angle-of-arrival fluctuations of stellar images. Experimentally measured data were carefully examined by implementing multifractal detrended fluctuation analysis. This…

Atmospheric and Oceanic Physics · Physics 2023-07-19 Luciano Zunino , Damián Gulich , Gustavo Funes , Aziz Ziad

From the previous study (Hiremath 2009b; Hiremath 2010), on the genesis of solar cycle and activity phenomena, it is understood that sunspots are formed at different depths by superposition of Alfven wave perturbations of a strong toroidal…

Solar and Stellar Astrophysics · Physics 2010-12-30 K. M. Hiremath , Lovely , M. R

We study a sample of 21 young and active solar-type stars with spectral types ranging from late F to mid K and characterize the behaviour of their activity. We apply the continuous period search (CPS) time series analysis method on 16 to 27…

Solar and Stellar Astrophysics · Physics 2016-03-21 Jyri Lehtinen , Lauri Jetsu , Thomas Hackman , Perttu Kajatkari , Gregory W. Henry

Using data of fast-rotating active dwarf stars in the Kepler database, we perform time-frequency analysis of the light curves in order to search for signs of activity cycles. We use the phenomenon that the active region latitudes vary with…

Solar and Stellar Astrophysics · Physics 2015-06-16 K. Vida , K. Oláh

We conduct a molecular dynamics simulation of an inelastic gas system utilizing an event-driven algorithm combined with a thermostat mechanism. Initially, the kinetic energy of the system experiences a decay before settling into a…

Computational Physics · Physics 2025-02-03 Rameez Farooq Shah , Shikha Kumari , Syed Rashid Ahmad

Active galactic nuclei (AGN) at the centres of galaxies can cycle between periods of activity and of quiescence. Characterising the duty-cycle of AGN is crucial for understanding their impact on the evolution of the host galaxy. For radio…

We study the influence of reflective boundaries on time-dependent responses of one-dimensional quantum fluids at zero temperature beyond the low-energy approximation. Our analysis is based on an extension of effective mobile impurity models…

Strongly Correlated Electrons · Physics 2016-06-01 I. S. Eliëns , F. B. Ramos , J. C. Xavier , R. G. Pereira

The interacting binary white dwarf (AM CVn) systems HM Cnc and V407 have orbital periods of 5.4 min and 9.5 min, respectively. The two systems are characterized by an "on/off" behaviour in the X-ray light curve, and optical light curves…

Solar and Stellar Astrophysics · Physics 2009-11-13 Matt A. Wood

Stars are changing entities in a constant evolution during their lives. At non-secular time scales (from seconds to years) the effect of dynamical processes such as convection, rotation, and magnetic fields can modify the stellar…

Solar and Stellar Astrophysics · Physics 2019-07-09 S. Mathur , J. Ballot , R. A. Garcia

We investigate the photometric modulation induced by magnetic activity cycles and study the relationship between rotation period and activity cycle(s) in late-type (FGKM) stars. We analyse light-curves spanning up to 9 years of 125 nearby…

Solar and Stellar Astrophysics · Physics 2016-10-26 A. Suárez Mascareño , R. Rebolo , J. I. González Hernández

The CoRoT space telescope observed nearly 160 000 light curves. Among the most outstanding is that of the young, active planet host star CoRoT-2A. In addition to deep planetary transits, the light curve of CoRoT-2A shows strong rotational…

Solar and Stellar Astrophysics · Physics 2016-05-25 Evangelos Nagel , Stefan Czesla , Jürgen H. M. M. Schmitt

The lifetime differences of bottom hadrons are known to be properly explained within the framework of heavy quark effective field theory(HQEFT) of QCD via the inverse expansion of the dressed heavy quark mass. In general, the spectrum…

High Energy Physics - Phenomenology · Physics 2009-11-10 Y. B Zuo , Y. a Yan , Y. L Wu , W. Y Wang

We present an alternative model of coronal-loop oscillations which considers that the waves are trapped in a 2D waveguide formed by the entire arcade of field lines. This differs from the standard 1D model which treats the waves as the…

Solar and Stellar Astrophysics · Physics 2015-06-18 Bradley W. Hindman , Rekha Jain

Optothermal interaction of active colloidal matter can facilitate environmental cues which can influence the dynamics of active soft matter systems. The optically induced thermal effect can be harnessed to study non-equilibrium…

Soft Condensed Matter · Physics 2022-09-07 Diptabrata Paul , Rahul Chand , G V Pavan Kumar

We present an analysis of the starspot evolution, the surface differential rotation (SDR), the correlation between chromospheric activity indicators and the spatial connection between chromospheric and photospheric activities on the active…

Solar and Stellar Astrophysics · Physics 2021-01-11 Fukun Xu , Shenghong Gu , Panogiotis Ioannidis