4 citations · 4 across the 5 of their papers we have counts for
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Cross-Calibration of Chandrayaan-2 XSM with INSPIRESat-1 DAXSS and GOES-16 XRS
N. P. S. Mithun, Santosh V. Vadawale, Asif M. Mandayapuram +9
X-ray spectroscopic observations of the solar corona and flares provide crucial diagnostics of plasma properties and are essential for understanding the physical processes responsi…
Solar Extreme Ultraviolet Spectrograph and High-energy Imager (SEUSHI): Design, Development, and Pre-Flight Calibration
Anant Telikicherla, Thomas N. Woods, Dave Crotser +7
Understanding the initiation of solar flares and coronal mass ejections (CMEs) is essential for improving forecasts of extreme space weather. Soft X-ray (SXR) and Extreme Ultraviol…
Revealing Flare Energetics and Dynamics with SDO EVE Solar Extreme Ultraviolet Spectral Irradiance Observations
Thomas N. Woods, Phillip C. Chamberlin, Andrew Jones +7
NASA's Solar Dynamics Observatory (SDO) Extreme-ultraviolet Variability Experiment (EVE) has been making solar full-disk extreme ultraviolet (EUV) spectral measurements since 2010…
Modelling Stellar Irradiances II: Correlations of solar irradiances with proxies of activity along a cycle
E. Deliporanidou, G. Del Zanna, T. N. Woods +1
There is a pressing need to model X-ray Ultra-Violet (XUV: 1-30 nm) stellar irradiances, given the scarcity of current measurements. One of the measurable effects of a stellar cycl…
The Origin of the EUV Late Phase: A Case Study of the C8.8 Flare on 2010 May 5
R. A. Hock, T. N. Woods, J. A. Klimchuk +2
Since the launch of NASA's Solar Dynamics Observatory on 2010 February 11, the Extreme ultraviolet Variability Experiment (EVE) has observed numerous flares. One interesting featur…