activity
20152025
most citedThe High-Resolution Coronal Imager, Flight 2.1

69 citations · 160 across the 10 of their papers we have counts for

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Showing astro-ph.SRShow all

9 papers · 1 filter

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…

astro-ph.SR2024

Determining the nanoflare heating frequency of an X-ray Bright Point observed by MaGIXS

Biswajit Mondal, P. S. Athiray, Amy R. Winebarger +18

Nanoflares are thought to be one of the prime candidates that can heat the solar corona to its multi-million kelvin temperature. Individual nanoflares are difficult to detect with…

astro-ph.SR2022★ 19 cited

The First Flight of the Marshall Grazing Incidence X-ray Spectrometer (MaGIXS)

Sabrina L. Savage, Amy R. Winebarger, Ken Kobayashi +34

The Marshall Grazing Incidence X-ray Spectrometer (MaGIXS) sounding rocket experiment launched on July 30, 2021 from the White Sands Missile Range in New Mexico. MaGIXS is a unique…

astro-ph.SR2019★ 69 cited

The High-Resolution Coronal Imager, Flight 2.1

Laurel A. Rachmeler, Amy R. Winebarger, Sabrina L. Savage +49

The third flight of the High-Resolution Coronal Imager (Hi-C 2.1) occurred on May 29, 2018, the Sounding Rocket was launched from White Sands Missile Range in New Mexico. The instr…

astro-ph.SR2019★ 16 cited

Solar Active Region Heating Diagnostics from High Temperature Emission using the Marshall Grazing Incidence X-ray Spectrometer (MaGIXS)

P. S. Athiray, Amy R. Winebarger, Will T. Barnes +7

The relative amount of high temperature plasma has been found to be a useful diagnostic to determine the frequency of coronal heating on sub-resolution structures. When the loops a…

astro-ph.SR2018★ 31 cited

CLASP Constraints on the Magnetization and Geometrical Complexity of the Chromosphere-Corona Transition Region

J. Trujillo Bueno, J. Štěpán, L. Belluzzi +25

The Chromospheric Lyman-Alpha Spectro-Polarimeter (CLASP) is a suborbital rocket experiment that on 3rd September 2015 measured the linear polarization produced by scattering proce…

astro-ph.SR2018★ 3 cited

A Statistical Inference Method for Interpreting the CLASP Observations

J. Stepan, J. Trujillo Bueno, L. Belluzzi +25

On 3rd September 2015, the Chromospheric Lyman-Alpha SpectroPolarimeter (CLASP) successfully measured the linear polarization produced by scattering processes in the hydrogen Lyman…

astro-ph.SR2015★ 11 cited

Temporal Pointing Variations of The Solar Dynamics Observatory's HMI and AIA Instruments on Sub-Weekly Time Scales

N. Brice Orange, Hakeem M. Oluseyi, David L. Chesny +5

Achieving sub-arcsecond co-registration across varying time-lines of multi-wavelength and instrument images is not trivial, and requires accurate characterization of instrument poi…

astro-ph.SR2015★ 8 cited

Direct Observations of Plasma Upflows and Condensation in a Catastrophically Cooling Solar Transition Region Loop

N. B. Orange, D. L. Chesny, H. M. Oluseyi +3

Minimal observational evidence exists for fast transition region (TR) upflows in the presence of cool loops. Observations of such occurrences challenge notions of standard solar at…