Search Results - "JACKEL, B"
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1
Using Mutual Information to Determine Geoeffectiveness of Solar Wind Phase Fronts With Different Front Orientations
Published in Journal of geophysical research. Space physics (01-03-2019)“…The geoeffectiveness of solar wind shocks depends on angle with respect to the Sun‐Earth line, with highly angled solar wind shocks being less geoeffective…”
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2
Optical Spectra and Emission Altitudes of Double‐Layer STEVE: A Case Study
Published in Geophysical research letters (16-12-2019)“…We report an event study of STEVE on 17 July 2018, with focus on the optical spectra and emission altitudes of STEVE. We find that the STEVE comprises two…”
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The THEMIS Array of Ground-based Observatories for the Study of Auroral Substorms
Published in Space science reviews (01-12-2008)“…The NASA Time History of Events and Macroscale Interactions during Substorms (THEMIS) project is intended to investigate magnetospheric substorm phenomena,…”
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On the 630 nm red‐line pulsating aurora: Red‐line Emission Geospace Observatory observations and model simulations
Published in Journal of geophysical research. Space physics (01-08-2016)“…In this study, we present observations of red‐line (630 nm) pulsating auroras using the camera system of Red‐line Emission Geospace Observatory (REGO), during…”
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5
Nitriding model for zirconium based fuel cladding in severe accident codes
Published in Journal of nuclear materials (15-08-2023)“…•Model developed for reactions of nitrogen during air oxidation of Zr-cladding.•Data from separate effect tests used to develop the model.•Decisive importance…”
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6
Identifying the 630 nm auroral arc emission height: A comparison of the triangulation, FAC profile, and electron density methods
Published in Journal of geophysical research. Space physics (01-08-2017)“…We present a comprehensive survey of 630 nm (red‐line) emission discrete auroral arcs using the newly deployed Redline Emission Geospace Observatory. In this…”
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7
Intensification of preexisting auroral arc at substorm expansion phase onset: Wave-like disruption during the first tens of seconds
Published in Geophysical research letters (01-09-2008)“…With the deployment of the all‐sky imager array of the THEMIS mission, we were able to construct a preliminary database of auroral substorm expansion phase…”
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8
Birkeland current boundary flows
Published in Journal of geophysical research. Space physics (01-04-2017)“…Intense zonal ion velocity jets in the northern nightside auroral zone are measured during quiet geomagnetic conditions by the Swarm satellites around 500 km…”
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9
Simultaneous THEMIS in situ and auroral observations of a small substorm
Published in Geophysical research letters (01-09-2008)“…We present ground‐based and in situ observations from March 13, 2007. The THEMIS satellites were in the evening sector conjugate to THEMIS ground‐based…”
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10
Severe accident code-to-code comparison for two accident scenarios in a spent fuel pool
Published in Annals of nuclear energy (01-10-2018)“…•Benchmark of 6 SA codes (14 participants) for two accident scenarios in a Spent Fuel Pool.•Differences in draining velocity induced scattering in the onset of…”
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11
Ground-based optical determination of the b2i boundary: A basis for an optical MT-index
Published in Journal of Geophysical Research - Space Physics (01-03-2003)“…The equatorward boundary of the proton aurora corresponds to a transition from strong pitch angle scattering to bounce trapped particles. This transition has…”
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12
The predicted effects of selected Phebus FPT1 sump constituents on iodine volatility
Published in Nuclear engineering and design (01-06-2014)“…The analytical results of containment sump samples in the Phebus FP1Test show the presence of Cd, Sn, U, Ag, Re (destroyed thermocouples) as well as Ag at…”
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13
Timing and location of substorm onsets from THEMIS satellite and ground based observations
Published in Annales geophysicae (1988) (15-07-2009)“…The unprecedented coverage of the THEMIS GBO station network coupled with high temporal and spatial resolution allowed us to determine the various stages of…”
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14
Auroral spectral estimation with wide-band color mosaic CCDs
Published in Geoscientific instrumentation, methods and data systems (11-06-2014)“…Optical aurora can be structured over a wide range of spatial and temporal scales with spectral features that depend on the energy of precipitating particles…”
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Determination of substorm onset timing and location using the THEMIS ground based observatories
Published in Geophysical research letters (01-09-2007)“…The NASA THEMIS mission is studying substorms by timing the substorm signatures at multiple satellite locations in the magnetosphere and in the aurora using 20…”
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16
Width and structure of mesoscale optical auroral arcs
Published in Geophysical research letters (15-02-2001)“…Arc widths were calculated for 3126 stable auroral arcs observed by an all‐sky camera located in Gillam, Manitoba. The camera is filtered to accept 5577‐Å…”
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17
Global observations of substorm injection region evolution: 27 August 2001
Published in Annales geophysicae (1988) (04-05-2009)“…We present riometer and in situ observations of a substorm electron injection on 27 August 2001. The event is seen at more than 20 separate locations…”
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Observation of isolated high-speed auroral streamers and their interpretation as optical signatures of Alfvén waves generated by bursty bulk flows
Published in Geophysical research letters (01-02-2008)“…The THEMIS All‐Sky Imager at Fort Smith, Canada observed a sudden appearance and subsequent evolution of auroral streamers on April 15, 2006. The event took…”
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Large-scale vortex dynamics in the evening and midnight auroral zone: Observations and simulations
Published in Journal of Geophysical Research, Washington, DC (01-08-2000)“…We use Canadian Auroral Network for the OPEN Program Unified Study All‐Sky Imager (ASI) and Meridional Scanning Photometer (MSP) data as the basis for a study…”
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20
THEMIS Ground Based Observatory System Design
Published in Space science reviews (01-12-2008)“…The comprehensive THEMIS approach to solving the substorm problem calls for monitoring the nightside auroral oval with low-cost, robust white-light imagers and…”
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