213 citations · 996 across the 14 of their papers we have counts for
13 papers
Statistical Properties of Super-hot Solar Flares
Amir Caspi, Säm Krucker, R. P. Lin
We use RHESSI high-resolution imaging and spectroscopy observations from ~6 to 100 keV to determine the statistical relationships between measured parameters (temperature, emission…
Solar Eruptive Events (SEE) 2020 Mission Concept
R. P. Lin, A. Caspi, S. Krucker +20
Major solar eruptive events (SEEs), consisting of both a large flare and a near simultaneous large fast coronal mass ejection (CME), are the most powerful explosions and also the m…
The height of a white-light flare and its hard X-ray sources
Juan-Carlos Martínez Oliveros, Hugh S. Hudson, Gordon J. Hurford +6
We describe observations of a white-light flare (SOL2011-02-24T07:35:00, M3.5) close to the limb of the Sun, from which we obtain estimates of the heights of the optical continuum…
Statistically-derived flaring chromospheric-coronal density structure from non-thermal X-ray observations of the Sun
Pascal Saint-Hilaire, Sam Krucker, Robert P. Lin
For the first time, we have used RHESSI's spatial and energy resolution to determine the combined chromospheric and coronal density profile of the flaring solar atmosphere in a sta…
X-ray emission from the base of a current sheet in the wake of a CME
Pascal Saint-Hilaire, Sam Krucker, Robert P. Lin
Following a CME which started on 2002 November 26, RHESSI, the Ramaty High Energy Solar Spectroscopic Imager, observed for 12 hours an X-ray source above the solar limb, at altitud…
A Statistical Survey of Hard X-ray Spectral Characteristics of Solar Flares with Two Footpoints
Pascal Saint-Hilaire, Sam Krucker, Robert P. Lin
Using RHESSI data, we have analyzed some 172 hard X-ray peaks during 53 solar flares which exhibited a double-footpoint structure. Fitting both footpoints with power-laws, we find…