activity
20242026
collaborators

5 papers

astro-ph.SR2026

Hbeta Spicules, Small-scale Jets, and Hbeta Microflashes: Sub-arcsecond Dynamic Events and their Magnetic Origins in the Lower Solar Chromosphere Observed by DKIST

Navdeep K. Panesar, V. Aparna, Sanjiv K. Tiwari +3

We examine an on-disk solar quiet region of enhanced magnetic network using Hbeta images from Daniel K. Inouye Solar Telescopes (DKISTs) Visible Broadband Imager (VBI) and line-of-…

astro-ph.SR2026

Extreme Ultraviolet Microflashes at Plume Bases: A Candidate for Powering the Corona and Solar Wind?

Navdeep K. Panesar, Sanjiv K. Tiwari, Meng Jin +4

Solar plumes - outflows of bright coronal plasma - are a major component of the open-magnetic-field corona and solar wind, but their driving mechanism remains uncertain. Here we re…

astro-ph.SR2025

Pivot of the Emerging Bipolar Magnetic Region in the Birth of Sigmoidal Solar Active Regions

Ronald L. Moore, Sanjiv K. Tiwari, V. Aparna +3

We present an augmentation to longstanding evidence from observations and MHD modeling that (1) every solar emerging bipolar magnetic region (BMR) is made by an emerging omega-loop…

astro-ph.SR2025

Quantifying Suppression of Solar Surface Magnetic Flux Advection with Increasing Field Strength

V. Aparna, Sanjiv K. Tiwari, Ronald L. Moore +4

One of the main theories for heating of the solar corona is based on the idea that solar convection shuffles and tangles magnetic field lines to make many small-scale current sheet…

astro-ph.SR2024

Stealth Non-standard-model Confined Flare Eruptions: Sudden Reconnection Events in Ostensibly Inert Magnetic Arches from Sunspots

Ronald L. Moore, Sanjiv K. Tiwari, Navdeep K. Panesar +2

We report seven examples of a long-ignored type of confined solar flare eruption that does not fit the standard model for confined flare eruptions. Because they are confined erupti…