activity
20072026
most citedLarge-Amplitude Oscillation of an Erupting Filament as Seen in EUV, H-alpha and Microwave Observations

53 citations · 100 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.SR2026

Potential Solar Precursors to Magnetic Switchbacks

Durgesh Tripathi, Maria S. Madjarska, Judy Karpen +9

The origin of magnetic switchbacks-large-amplitude, spherically polarized magnetic-field fluctuations with local polarity inversions shown to be nearly ubiquitous in the inner heli…

astro-ph.SR2026

Near-Sun Switchbacks Show Statistical Signatures of Solar Activity

Sneha Pandit, Thierry Dudok de Wit, Clara Froment +3

The large amplitude, Alfvénic deflections in the solar wind, called magnetic switchbacks, are a ubiquitous feature of the inner heliosphere, yet their origin and variability remain…

astro-ph.SR2026

Energy Evolution from the Chromosphere to the Heliosphere in the 2021 October 28 Solar Eruption

Katharine K. Reeves, Daniel B. Seaton, Cynthia Cattell +20

We perform a detailed study of the energetics for a well-observed solar eruption and flare that occurred on 28 October 2021. This event included a GOES class X1.0 flare, a global E…

astro-ph.SR2026

Magnetic switchback formation: a review of proposed mechanisms

Peter F. Wyper, Jonathan Squire, Etienne Pariat +19

Magnetic switchbacks are large amplitude deflections of the magnetic field within the solar wind. They are Alfvénic in character and so are associated with a spike in velocity and…

astro-ph2008★ 16 cited

The solar wind disappearance event of 11 May 1999: source region evolution

P. Janardhan, D. Tripathi, H. E. Mason

Context. A recent, detailed study of the well-known solar wind disappearance event of 11 May 1999 traced its origin to a coronal hole (CH) lying adjacent to a large active region (…

astro-ph2008★ 31 cited

A bright coronal downflow seen in multi-wavelength observations: evidence of a bifurcating flux-rope?

D. Tripathi, S. K. Solanki, H. E. Mason +1

Aims: To study the origin and characteristics of a bright coronal downflow seen after a coronal mass ejection associated with erupting prominences on 5 March 2000. Methods: This st…