Search Results - "Popecki, M. A."
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Time‐of‐flight mass spectrographs—From ions to neutral atoms
Published in Journal of geophysical research. Space physics (01-12-2016)“…After their introduction to space physics in the mid 1980s time‐of‐flight (TOF) spectrographs have become a main staple in spaceborne mass spectrometry. They…”
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A statistical analysis of heliospheric plasma sheets, heliospheric current sheets, and sector boundaries observed in situ by STEREO
Published in Journal of geophysical research. Space physics (01-11-2014)“…The heliocentric orbits of STEREO A and B with a separation in longitude increasing by about 45° per year provide the unique opportunity to study the evolution…”
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3
Ionic charge states of solar energetic particles : A clue to the source
Published in Space science reviews (01-06-2007)“…Issue Title: The Composition of Matter The ionic charge of solar energetic particles (SEP) as observed in interplanetary space is an important parameter for…”
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Microchannel plate fabrication using glass capillary arrays with Atomic Layer Deposition films for resistance and gain
Published in Journal of geophysical research. Space physics (01-08-2016)“…Microchannel plates (MCPs) have been used for many years in space flight instrumentation as fast, lightweight electron multipliers. A new MCP fabrication…”
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Solar energetic particle charge states : An overview
Published in Space science reviews (01-06-2006)“…Issue Title: Solar Dynamics and its Effects on the Heliosphere and Earth The ionic charge distributions of solar energetic particles (SEP) as observed in…”
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Conference Proceeding Journal Article -
6
In situ observations from STEREO/PLASTIC: a test for L5 space weather monitors
Published in Annales geophysicae (1988) (07-10-2009)“…Stream interaction regions (SIRs) that corotate with the Sun (corotating interaction regions, or CIRs) are known to cause recurrent geomagnetic storms. The…”
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Escape of O+ through the distant tail plasma sheet
Published in Geophysical research letters (01-11-2010)“…In February 2007, the STEREO‐B spacecraft encountered the magnetosheath, plasma sheet and plasma sheet boundary layer from about 200 RE to 300 RE downtail…”
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The Heliospheric Plasma Sheet Observed in situ by Three Spacecraft over Four Solar Rotations
Published in Solar physics (01-11-2012)“…In this paper we present in situ observations of the heliospheric plasma sheet (HPS) from STEREO-A, Wind , and STEREO-B over four solar rotations in the…”
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On the source and acceleration of energetic He+: A long-term observation with ACE/SEPICA
Published in Journal of Geophysical Research - Space Physics (01-10-2003)“…We report on a systematic study of the He+/He2+ abundance ratio in the energetic population during the years 1998–2000. For the investigation we have used data…”
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Solar wind ion trends and signatures: STEREO PLASTIC observations approaching solar minimum
Published in Annales geophysicae (1988) (13-10-2009)“…STEREO has now completed the first two years of its mission, moving from close proximity to Earth in 2006/2007 to more than 50 degrees longitudinal separation…”
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In Situ Observations of Solar Wind Stream Interface Evolution
Published in Solar physics (01-10-2009)“…The heliocentric orbits of the two STEREO satellites are similar in radius and ecliptic latitude, with separation in longitude increasing by about 45° per…”
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Energetic Particle Observations: Report of Working Group C
Published in Space science reviews (01-03-2006)“…Issue Title: Special Issue: Coronal Mass Ejections The characteristics of solar energetic particles (SEP) as observed in interplanetary space provide…”
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Charge states of energetic (≈0.5 MeV/n) ions in corotating interaction regions at 1 AU and implications on source populations
Published in Geophysical research letters (01-01-2002)“…The ionic charge states of He, C, O, Ne, Mg and Fe at ≈0.5 MeV/n have been obtained in several corotating interaction regions (CIRs) in 1999 and 2000 with the…”
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14
Diagnostics of corotating interaction regions with the kinetic properties of iron ions as determined with STEREO/PLASTIC
Published in Annales geophysicae (1988) (09-02-2010)“…STEREO/PLASTIC determines three-dimensional distributions of solar wind iron ions with unprecedented time resolution. Typically 300 to 1000 counts are…”
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Energetic Particle Observations
Published in Space science reviews (01-03-2006)“…The characteristics of solar energetic particles (SEP) as observed in interplanetary space provide fundamental information about the origin of these particles,…”
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16
Observations of the spatial and temporal structure of field-aligned beam and gyrating ring distributions at the quasi-perpendicular bow shock with Cluster CIS
Published in Annales geophysicae (1988) (01-10-2001)“…During the early orbit phase, the Cluster spacecraft have repeatedly crossed the perpendicular Earth’s bow shock and provided the first multi-spacecraft…”
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Measurement of the Parametrized Single-Photon Response Function of a Large Area Picosecond Photodetector for Time-of-Flight PET Applications
Published in IEEE transactions on radiation and plasma medical sciences (01-09-2021)“…We have used a subpicosecond laser with an output trigger synched to a 4-GHz oscilloscope sampling at 25 GSa/s to characterize the temporally resolved response…”
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OBSERVATION OF HIGH IRON CHARGE STATES AT LOW ENERGIES IN SOLAR ENERGETIC PARTICLE EVENTS
Published in The Astrophysical journal (10-04-2014)“…The ionic charge states of solar energetic particles (SEPs) provide direct information about the source plasma, the acceleration environment, and their…”
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Equator-S observations of He+ energization by EMIC waves in the dawnside equatorial magnetosphere
Published in Geophysical research letters (15-05-2002)“…We present Equator‐S observations of He+ energization by electromagnetic ion cyclotron (EMIC) waves in the dawn side equatorial magnetosphere at L > 7. The He+…”
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Testing electric field models using ring current ion energy spectra from the Equator-S ion composition (ESIC) instrument
Published in Annales geophysicae (1988) (1999)“…During the main and early recovery phase of a geomagnetic storm on February 18, 1998, the Equator-S ion composition instrument (ESIC) observed spectral…”
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