Search Results - "Ruffolo, David"
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1
Variation in Path Lengths of Turbulent Magnetic Field Lines and Solar Energetic Particles
Published in The Astrophysical journal (01-06-2024)“…Abstract Modeling of time profiles of solar energetic particle (SEP) observations often considers transport along a large-scale magnetic field with a fixed…”
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2
Scale and Time Dependence of Alfvénicity in the Solar Wind as Observed by the Parker Solar Probe
Published in The Astrophysical journal (01-02-2024)“…Abstract Alfvénicity is a well-known property, common in the solar wind, characterized by a high correlation between magnetic and velocity fluctuations. Data…”
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3
Variations in the Inferred Cosmic-Ray Spectral Index as Measured by Neutron Monitors in Antarctica
Published in The Astrophysical journal (01-10-2024)“…Abstract A technique has recently been developed for tracking short-term spectral variations in Galactic cosmic rays (GCRs) using data from a single neutron…”
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4
Ab initio calculation of high pressure phases and electronic properties of CuInSe2
Published in Solid state communications (01-05-2012)“…We used an ab initio method to calculate the high pressure phases of CuInSe2. By using the experimentally suggested phases, the enthalpy difference showed that…”
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5
Relativistic solar neutrons and protons on 28 October 2003
Published in Geophysical research letters (01-02-2005)“…The solar cosmic ray event associated with the X17.2 class flare of 28 October 2003 was unusual in several respects: (1) Several high‐latitude neutron monitors…”
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6
Queering Child/Hood Policies: Canadian Examples and Perspectives
Published in Contemporary issues in early childhood (01-09-2009)“…This article examines how notions of ‘child’ and ‘childhood’ are produced in relation to recent early childhood policies in Ontario, Canada. It centers on an…”
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7
Extended Cosmic Ray Decreases with Strong Anisotropy after Passage of Interplanetary Shocks
Published in The Astrophysical journal (01-11-2022)“…Abstract The passage of an interplanetary shock and/or interplanetary coronal mass ejection often causes a rapid decrease in the Galactic cosmic-ray (GCR)…”
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8
Role of Parallel Solenoidal Electric Field on Energy Conversion in 2.5D Decaying Turbulence with a Guide Magnetic Field
Published in The Astrophysical journal (01-12-2021)“…Abstract We perform 2.5D particle-in-cell simulations of decaying turbulence in the presence of a guide (out-of-plane) background magnetic field. The…”
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9
Local modulation and trapping of energetic particles by coherent magnetic structures
Published in Geophysical research letters (28-04-2016)“…Recent observational studies show strong statistical associations between features of interplanetary suprathermal energetic particle (EP) data and rapid…”
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10
Random Walk and Trapping of Interplanetary Magnetic Field Lines: Global Simulation, Magnetic Connectivity, and Implications for Solar Energetic Particles
Published in The Astrophysical journal (01-02-2021)“…Abstract The random walk of magnetic field lines is an important ingredient in understanding how the connectivity of the magnetic field affects the spatial…”
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11
Domains of Magnetic Pressure Balance in Parker Solar Probe Observations of the Solar Wind
Published in The Astrophysical journal (01-12-2021)“…Abstract The Parker Solar Probe (PSP) spacecraft is performing the first in situ exploration of the solar wind within 0.2 au of the Sun. Initial observations…”
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12
EFFECT OF COHERENT STRUCTURES ON ENERGETIC PARTICLE INTENSITY IN THE SOLAR WIND AT 1 AU
Published in The Astrophysical journal (10-10-2015)“…ABSTRACT We present results from an analysis of Advanced Composition Explorer (ACE) observations of energetic particles in the 0.047-4.78 MeV range associated…”
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13
The Alfvén transition zone observed by the Parker Solar Probe in young solar wind – global properties and model comparisons
Published in Monthly notices of the Royal Astronomical Society. Letters (14-06-2024)“…ABSTRACT The transition from subAlfvénic to superAlfvénic flow in the solar atmosphere is examined by means of Parker Solar Probe (PSP) measurements during…”
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14
Ion Acceleration in Driven Magnetic Reconnection during High-energy–Density Plasma Interaction
Published in The Astrophysical journal (01-02-2021)“…Abstract Strongly driven magnetic reconnection occurs in astrophysical events and also in laboratory experiments with laser-produced plasma. We have performed…”
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15
Distinct Pattern of Solar Modulation of Galactic Cosmic Rays above a High Geomagnetic Cutoff Rigidity
Published in The Astrophysical journal (01-05-2018)“…Solar modulation refers to Galactic cosmic-ray variations with the ∼11 yr sunspot cycle and ∼22 yr solar magnetic cycle and is relevant to the space radiation…”
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16
Anisotropic Forbush decrease of 24 March 2024: First look
Published in Advances in space research (15-10-2024)“…A strong Forbush decrease, i.e., suppression of the flux of galactic cosmic rays recorded on Earth, was observed by the global network of ground-based neutron…”
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17
Effects of a Guide Field on the Larmor Electric Field and Upstream Electron Temperature Anisotropy in Collisionless Asymmetric Magnetic Reconnection
Published in The Astrophysical journal (20-08-2017)“…We perform the first study of the properties of the Larmor electric field (LEF) in collisionless asymmetric magnetic reconnection in the presence of an…”
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18
Queering the “I” in academic discourse: Re/visioning agency for an equitable future
Published 01-01-2005“…The vision of an equitable, not equal future is a queer ambition. This thesis challenges (hetero)normative ideologies that further minoritize the minoritized…”
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Dissertation -
19
Multi-spectral optical imaging of the spatiotemporal dynamics of ionospheric intermittent turbulence
Published in Scientific reports (12-07-2018)“…Equatorial plasma depletions have significant impact on radio wave propagation in the upper atmosphere, causing rapid fluctuations in the power of radio…”
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20
On the Estimation of Solar Energetic Particle Injection Timing from Onset Times near Earth
Published in The Astrophysical journal (20-06-2005)“…We examine the accuracy of a common technique for estimating the start time of solar energetic particle injection based on a linear fit to the observed onset…”
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