activity
20062025
most citedInternetwork chromospheric bright grains observed with IRIS

48 citations · 79 across the 8 of their papers we have counts for

collaborators

9 papers

astro-ph.SR2025

A sudden fine-scale bright kernel captured by Hi-C Flare in 11 MK emission during an M1.6-class solar flare's post-maximum phase

Sanjiv K. Tiwari, Navdeep K. Panesar, Ronald L. Moore +17

On April 17, 2024, the third successful Hi-C sounding rocket flight, Hi-C Flare, recorded coronal images in Fe XXI 129 A emission from 11 MK plasma during the post-maximum phase of…

physics.ao-ph2023

A Spherical Shells Model of Atmospheric Absorption for Instrument Calibration

Nicolas Donders, Genevieve Vigil, Adam Kobelski +4

We present a model for atmospheric absorption of solar ultraviolet (UV) radiation. The initial motivation for this work is to predict this effect and correct it in Sounding Rocket…

astro-ph.SR2021

A new view of the solar interface region from the Interface Region Imaging Spectrograph (IRIS)

B. De Pontieu, V. Polito, V. Hansteen +11

The Interface Region Imaging Spectrograph (IRIS) has been obtaining near- and far-ultraviolet images and spectra of the solar atmosphere since July 2013. The unique combination of…

astro-ph.SR2015★ 48 cited

Internetwork chromospheric bright grains observed with IRIS

Juan Martínez-Sykora, Luc Rouppe van der Voort, Mats Carlsson +18

The Interface Region Imaging Spectrograph (IRIS) reveals small-scale rapid brightenings in the form of bright grains all over coronal holes and the quiet sun. These bright grains a…

astro-ph.SR2010★ 3 cited

Science Objectives for an X-Ray Microcalorimeter Observing the Sun

J. Martin Laming, J. Adams, D. Alexander +57

We present the science case for a broadband X-ray imager with high-resolution spectroscopy, including simulations of X-ray spectral diagnostics of both active regions and solar fla…

astro-ph.SR2009★ 14 cited

Coronal Loop Expansion Properties Explained Using Separators

Joseph E. Plowman, Charles C. Kankelborg, Dana W. Longcope

One puzzling observed property of coronal loops is that they are of roughly constant thickness along their length. Various studies have found no consistent pattern of width variati…