activity
20072026
most citedKink oscillations of coronal loops

145 citations · 642 across the 22 of their papers we have counts for

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Showing astro-ph.SRShow all

19 papers · 1 filter

astro-ph.SR2026

Machine Learning-Based Characterization of Solar p-Mode Frequency Shifts during Solar Cycle 25

Rekha Jain, Akash Kumar, Sushanta C. Tripathy

The solar interior is probed by the properties of the Sun's acoustic oscillations (p-modes) observed on the solar surface. The frequencies of these p-modes measured in the last thr…

astro-ph.SR2023★ 7 cited

Overstable Convective Modes in a Polytropic Stellar Atmosphere

Bradley W. Hindman, Rekha Jain

Within the convection zone of a rotating star, the presence of the Coriolis force stabilizes long-wavelength convective modes. These modes, which would have been unstable if the st…

astro-ph.SR2022★ 3 cited

Study of transverse oscillations in coronal loops excited by flares and eruptions

Sandra M. Conde C, Rekha Jain, Vera Jatenco-Pereira

We present measurements of periodicity for transverse loop oscillations during the periods of activity of two remote and separated (both temporally and spatially) flares. The oscil…

astro-ph.SR2022★ 1 cited

Radial Trapping of Thermal Rossby Waves within the Convection Zones of Low-Mass Stars

Bradley W. Hindman, Rekha Jain

We explore how thermal Rossby waves propagate within the gravitationally stratified atmosphere of a low-mass star with an outer convective envelope. Under the conditions of slow, r…

astro-ph.SR2021★ 145 cited

Kink oscillations of coronal loops

V. M. Nakariakov, S. A. Anfinogentov, P. Antolin +13

Kink oscillations of coronal loops, i.e., standing kink waves, is one of the most studied dynamic phenomena in the solar corona. The oscillations are excited by impulsive energy re…

astro-ph.SR2021★ 7 cited

Do Coronal Loops Oscillate in Isolation?

Bradley W. Hindman, Rekha Jain

Images of the solar corona by extreme-ultraviolet (EUV) telescopes reveal elegant arches of glowing plasma that trace the corona's magnetic field. Typically, these loops are prefer…

astro-ph.SR2021★ 4 cited

The need for new techniques to identify the high-frequency MHD waves of an oscillating coronal loop

Farhad Allian, Rekha Jain

Magnetic arcades in the solar atmosphere, or coronal loops, are common structures known to host magnetohydrodynamic (MHD) waves and oscillations. Of particular interest are the obs…

astro-ph.SR2020★ 110 cited

Critical Science Plan for the Daniel K. Inouye Solar Telescope (DKIST)

Mark P. Rast, Nazaret Bello González, Luis Bellot Rubio +84

The Daniel K. Inouye Solar Telescope (DKIST) will revolutionize our ability to measure, understand and model the basic physical processes that control the structure and dynamics of…

astro-ph.SR2019★ 11 cited

A New Analysis Procedure for Detecting Periodicities within Complex Solar Coronal Arcades

Farhad Allian, Rekha Jain, B. W Hindman

We study intensity variations, as measured by the Atmospheric Imaging Assembly (AIA) on board the Solar Dynamics Observatory (SDO), in a solar coronal arcade using a newly develope…

astro-ph.SR2018★ 7 cited

A Novel Approach to Resonant Absorption of the Fast MHD Eigenmodes of a Coronal Arcade

Bradley W. Hindman, Rekha Jain

The arched field lines forming coronal arcades are often observed to undulate as magnetohydrodynamic (MHD) waves propagate both across and along the magnetic field. These waves are…

astro-ph.SR2016★ 6 cited

Time-dependent suppression of oscillatory power in evolving solar magnetic fields

S. Krishna Prasad, D. B. Jess, R. Jain +1

Oscillation amplitudes are generally smaller within magnetically active regions like sunspots and plage, when compared to their surroundings. Such magnetic features, when viewed in…

astro-ph.SR2015★ 12 cited

Eigenmodes of three-dimensional magnetic arcades in the Sun's corona

Bradley W. Hindman, Rekha Jain

We develop a model of coronal-loop oscillations that treats the observed bright loops as an integral part of a larger 3-D magnetic structure comprised of the entire magnetic arcade…

astro-ph.SR2015★ 34 cited

Fundamental-Mode Oscillations of Two Coronal Loops within a Solar Magnetic Arcade

Rekha Jain, Ram A. Maurya, B. W. Hindman

We analyse intensity variations, as measured by the Atmospheric Imaging Assembly (AIA) in the 171 Å passband, in two coronal loops embedded within a single coronal magnetic arcade.…

astro-ph.SR2014★ 9 cited

Five-minute oscillation power within magnetic elements in the solar atmosphere

Rekha Jain, Andrew Gascoyne, Bradley W. Hindman +1

It has long been known that magnetic plage and sunspots are regions in which the power of acoustic waves is reduced within the photospheric layers. Recent observations now suggest…

astro-ph.SR2013★ 34 cited

An Interpretation of Flare-Induced and Decayless Coronal-Loop Oscillations as Interference Patterns

Bradley W. Hindman, Rekha Jain

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 f…

astro-ph.SR2013

Equilibrium models of coronal loops that involve curvature and buoyancy

Bradley W. Hindman, Rekha Jain

We construct magnetostatic models of coronal loops in which the thermodynamics of the loop is fully consistent with the shape and geometry of the loop. This is achieved by treating…

astro-ph.SR2012

Kink Oscillations of a Curved, Gravitationally Stratified Coronal Loop

Bradley W. Hindman, Rekha Jain

Loops of magnetic field in the corona are observed to oscillate and these oscillations have been posited to be the superposition of resonant kink waves. To date, most analyses of t…

astro-ph.SR2011★ 22 cited

Axisymmetric Scattering of p Modes by Thin Magnetic Tubes

Bradley W. Hindman, Rekha Jain

We examine the scattering of acoustic p-mode waves from a thin magnetic fibril embedded in a gravitationally stratified atmosphere. The scattering is mediated through the excitatio…

astro-ph.SR2009★ 123 cited

Large Amplitude Oscillations in Prominences

D. Tripathi, H. Isobe, R. Jain

Since the first reports of oscillations in prominences in 1930s there have been major theoretical and observational advances to understand the nature of these oscillatory phenomena…