90 citations
- Physical Research LaboratoryIN37 papers
- Indian Institute of Technology GandhinagarIN19 papers
- University of GrazAT15 papers
- Indian Institute of AstrophysicsIN8 papers
- University of Alabama in HuntsvilleUS7 papers
- Korea Astronomy and Space Science InstituteKR6 papers
- Kumaun UniversityIN6 papers
- Centre National de la Recherche ScientifiqueFR5 papers
- Max Planck Institute for Solar System ResearchDE5 papers
- Patna UniversityIN5 papers
- Goddard Space Flight CenterUS4 papers
- Gujarat UniversityIN4 papers
7 papers · 1 filter
An Observationally Constrained Analytical Model for Predicting the Magnetic Field Vectors of ICMEs at 1 AU
Ranadeep Sarkar, Nat Gopalswamy, Nandita Srivastava
We report on an observationally constrained analytical model, the INterplanetary Flux ROpe Simulator (INFROS), for predicting the magnetic-field vectors of coronal mass ejections (…
A Hot Cusp-Shaped Confined Solar Flare
Aaron Hernandez-Perez, Yang Su, Julia K. Thalmann +5
We analyze a confined flare that developed a hot cusp-like structure high in the corona (H ~ 66 Mm). A growing cusp-shaped flare arcade is a typical feature in the standard model o…
Lorentz Force Evolution Reveals the Energy Buildup Processes during Recurrent Eruptive Solar Flares
Ranadeep Sarkar, Nandita Srivastava, Astrid M. Veronig
The energy release and build-up processes in the solar corona have significant implications in particular for the case of large recurrent flares, which pose challenging questions a…
Investigation of a confined C-class flare in an arch filament system close to a regular sunspot
Rohan Eugene Louis
A moderate C1.1 class confined flare is investigated here, which occurred on 2013 September 24 at 22:56~UT, in an arch filament system close to a regular, unipolar sunspot. Spectro…
Exploring the damping of Alfvén waves along a long off-limb coronal loop, up to 1.4 R
Girjesh R. Gupta, G. Del Zanna, H. E. Mason
The Alfvén wave energy flux in the corona can be explored using the electron density and velocity amplitude of the waves. The velocity amplitude of Alfvén waves can be obtained fro…
Mass Loss via Solar Wind and Coronal Mass Ejections During Solar Cycle 23 and 24
Wageesh Mishra, Nandita Srivastava, Yuming Wang +3
Similar to the Sun, other stars shed mass and magnetic flux via ubiquitous quasi-steady wind and episodic stellar coronal mass ejections (CMEs). We investigate the mass loss rate v…