activity
20102025
most citedMagnetic connectivity of the ecliptic plane within 0.5 AU : PFSS modeling of the first PSP encounter

161 citations · 574 across the 15 of their papers we have counts for

collaborators

15 papers

astro-ph.IM2025

Signal processing and data acquisition system for the BTO detectors onboard COSI

Shunsaku Nagasawa, Tadayuki Takahashi, Kazuhiro Nakazawa +15

The energy range from a few hundred keV to a few MeV includes important probes such as nuclear gamma-rays and the 511 keV annihilation line. However, compared to X-rays and GeV/TeV…

astro-ph.HE2023★ 19 cited

The Compton Spectrometer and Imager

John A. Tomsick, Steven E. Boggs, Andreas Zoglauer +72

The Compton Spectrometer and Imager (COSI) is a NASA Small Explorer (SMEX) satellite mission in development with a planned launch in 2027. COSI is a wide-field gamma-ray telescope…

astro-ph.SR2022★ 4 cited

Observations of Thomson scattering from a loop-prominence system

Juan Carlos Martínez Oliveros, Juan Camilo Guevara Gómez, Pascal Saint-Hilaire +2

We describe observations of the white-light structures in the low corona following the X8.2 flare SOL2017-09-10, as observed in full Stokes parameters by the Helioseismic and Magne…

astro-ph.SR2022★ 22 cited

Tracking a beam of electrons from the low solar corona into interplanetary space with the Low Frequency Array, Parker Solar Probe and 1 au spacecraft

Samuel T. Badman, Eoin P. Carley, Luis Alberto Cañizares +7

Type III radio bursts are the result of plasma emission from mildly relativistic electron beams propagating from the low solar corona into the heliosphere where they can eventually…

astro-ph.SR2020★ 17 cited

Periodicities in an active region correlated with Type III radio bursts observed by Parker Solar Probe

Cynthia Cattell, Lindsay Glesener, Benjamin Leiran +5

Context. Periodicities have frequently been reported across many wavelengths in the solar corona. Correlated periods of ~5 minutes, comparable to solar p-modes, are suggestive of c…

astro-ph.SR2019★ 57 cited

Statistics and Polarization of Type III Radio Bursts Observed in the Inner Heliosphere

Marc Pulupa, Stuart D. Bale, Samuel T. Badman +20

We present initial results from the Radio Frequency Spectrometer (RFS), the high frequency component of the FIELDS experiment on the Parker Solar Probe (PSP). During the first PSP…

astro-ph.SR2019★ 161 cited

Magnetic connectivity of the ecliptic plane within 0.5 AU : PFSS modeling of the first PSP encounter

Samuel T. Badman, Stuart D. Bale, Juan C. Martinez Oliveros +19

We compare magnetic field measurements taken by the FIELDS instrument on Parker Solar Probe (PSP) during its first solar encounter to predictions obtained by Potential Field Source…

astro-ph.SR2019★ 2 cited

An in-situ interplanetary "U-burst": Observation and results

Juan Carlos Martínez-Oliveros, Saida Milena Diaz Castillo, Vratislav Krupar +3

We report and examine the observation of an unusual and rare in-situ electron observation associated with a solar type III radio burst on 24 December 1996. This radio event was acc…

astro-ph.SR2015★ 28 cited

A statistical correlation of sunquakes based on their seismic, white light, and X-ray emission

J. C. Buitrago-Casas, J. C. Martinez Oliveros, C. Lindsey +4

Several mechanisms have been proposed to explain the transient seis- mic emission, i.e., sunquakes, from some solar flares. Some theories associate high-energy electrons and/or whi…

astro-ph.SR2013★ 38 cited

Chromospheric and Coronal Observations of Solar Flares with the Helioseismic and Magnetic Imager

Juan-Carlos Martínez Oliveros, Säm Krucker, Hugh S. Hudson +7

We report observations of white-light ejecta in the low corona, for two X-class flares on the 2013 May 13, using data from the Helioseismic and Magnetic Imager (HMI) of the Solar D…

astro-ph.SR2013★ 10 cited

Transient artifacts in a flare observed by the Helioseismic and Magnetic Imager on the Solar Dynamics Observatory

J. C. Martínez Oliveros, C. Lindsey, H. S. Hudson +1

The Helioseismic and Magnetic Imager (HMI) onboard the Solar Dynamics Observatory (SDO) provides a new tool for the systematic observation of white-light flares, including Doppler…

astro-ph.SR2013★ 8 cited

The Role of Magnetic Fields in Transient Seismic Emission Driven by Atmospheric Heating in Flares

C. Lindsey, A. -C. Donea, J. C. Martinez Oliveros +1

The physics of transient seismic emission in flares remains largely mysterious. Its discoverers proposed that these "sunquakes" are the signature of a shock driven by "thick-target…

astro-ph.SR2012★ 102 cited

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…

astro-ph.SR2012★ 70 cited

The 2010 August 01 type II burst: A CME-CME Interaction, and its radio and white-light manifestations

Juan Carlos Martínez Oliveros, Claire L. Raftery, Hazel M. Bain +4

We present observational results of a type II burst associated with a CME-CME interaction observed in the radio and white-light wavelength range. We applied radio direction-finding…

astro-ph.SR2010★ 36 cited

Imaging Spectroscopy of a White-Light Solar Flare

J. C. Martinez Oliveros, S. Couvidat, J. Schou +4

We report observations of a white-light solar flare (SOL2010-06-12T00:57, M2.0) observed by the Helioseismic Magnetic Imager (HMI) on the Solar Dynamics Observatory (SDO) and the R…