Biblio

Found 12 results
Filters: Author is McComas, D. J.  [Clear All Filters]
A B C D E F G H I J K L M N O P Q R S T U V W X Y Z 
Van Allen Probes
Authors: Goldstein J, Angelopoulos V, De Pascuale S., Funsten H O, Kurth W S, et al.
Title: Cross-scale observations of the 2015 St. Patrick's day storm: THEMIS, Van Allen Probes, and TWINS
Abstract: We present cross-scale magnetospheric observations of the 17 March 2015 (St. Patrick's Day) storm, by Time History of Events and Macroscale Interactions during Substorms (THEMIS), Van Allen Probes (Radiation Belt Storm Probes), and Two Wide-angle Imaging Neutral-atom Spectrometers (TWINS), plus upstream ACE/Wind solar wind data. THEMIS crossed the bow shock or magnetopause 22 times and observed the magnetospheric compression that initiated the storm. Empirical models reproduce these boundary locations within 0.7 RE. Van Allen Probes crossed the plasmapause 13 times; test particle simulations reproduce these encounters within 0.5 RE. Before the storm, Van Allen Probes measured quiet double-nose proton spectra in the region of corotating cold plasma. About 15 min after a 0605 UT dayside sout. . .
Date: 01/2017 Publisher: Journal of Geophysical Research: Space Physics Pages: 368 - 392 DOI: 10.1002/jgra.v122.110.1002/2016JA023173 Available at: http://onlinelibrary.wiley.com/doi/10.1002/2016JA023173/full
More Details
Authors: Valek P. W., Goldstein J, Jahn J -M, McComas D J, and Spence H E
Title: First joint in situ and global observations of the medium-energy oxygen and hydrogen in the inner magnetosphere
Abstract: We present the first simultaneous observations of the in situ ions and global Energetic Neutral Atom (ENA) images of the composition-separated, medium-energy (~1–50 keV) particle populations of the inner magnetosphere. The ENA emissions are mapped into L shell/magnetic local time space based on the exospheric density along the line of sight (LOS). The ENA measurement can then be scaled to determine an average ion flux along a given LOS. The in situ ion flux tends to be larger than the scaled ENAs at the same local time. This indicates that the ion population is more concentrated in the Van Allen Probes orbital plane than distributed along the Two Wide-angle Imaging Neutral-atom Spectrometers LOS. For the large storm of 14 November 2012, we observe that the concentration of O (in situ i. . .
Date: 09/2015 Publisher: Journal of Geophysical Research: Space Physics Pages: 7615 - 7628 DOI: 10.1002/2015JA021151 Available at: http://doi.wiley.com/10.1002/2015JA021151http://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1002%2F2015JA021151
More Details
TWINS
Authors: Valek P. W., Goldstein J, Jahn J -M, McComas D J, and Spence H E
Title: First joint in situ and global observations of the medium-energy oxygen and hydrogen in the inner magnetosphere
Abstract: We present the first simultaneous observations of the in situ ions and global Energetic Neutral Atom (ENA) images of the composition-separated, medium-energy (~1–50 keV) particle populations of the inner magnetosphere. The ENA emissions are mapped into L shell/magnetic local time space based on the exospheric density along the line of sight (LOS). The ENA measurement can then be scaled to determine an average ion flux along a given LOS. The in situ ion flux tends to be larger than the scaled ENAs at the same local time. This indicates that the ion population is more concentrated in the Van Allen Probes orbital plane than distributed along the Two Wide-angle Imaging Neutral-atom Spectrometers LOS. For the large storm of 14 November 2012, we observe that the concentration of O (in situ i. . .
Date: 09/2015 Publisher: Journal of Geophysical Research: Space Physics Pages: 7615 - 7628 DOI: 10.1002/2015JA021151 Available at: http://doi.wiley.com/10.1002/2015JA021151http://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1002%2F2015JA021151
More Details
Authors: Goldstein J, Angelopoulos V, De Pascuale S., Funsten H O, Kurth W S, et al.
Title: Cross-scale observations of the 2015 St. Patrick's day storm: THEMIS, Van Allen Probes, and TWINS
Abstract: We present cross-scale magnetospheric observations of the 17 March 2015 (St. Patrick's Day) storm, by Time History of Events and Macroscale Interactions during Substorms (THEMIS), Van Allen Probes (Radiation Belt Storm Probes), and Two Wide-angle Imaging Neutral-atom Spectrometers (TWINS), plus upstream ACE/Wind solar wind data. THEMIS crossed the bow shock or magnetopause 22 times and observed the magnetospheric compression that initiated the storm. Empirical models reproduce these boundary locations within 0.7 RE. Van Allen Probes crossed the plasmapause 13 times; test particle simulations reproduce these encounters within 0.5 RE. Before the storm, Van Allen Probes measured quiet double-nose proton spectra in the region of corotating cold plasma. About 15 min after a 0605 UT dayside sout. . .
Date: 01/2017 Publisher: Journal of Geophysical Research: Space Physics Pages: 368 - 392 DOI: 10.1002/jgra.v122.110.1002/2016JA023173 Available at: http://onlinelibrary.wiley.com/doi/10.1002/2016JA023173/full
More Details
THEMIS
Authors: Goldstein J, Angelopoulos V, De Pascuale S., Funsten H O, Kurth W S, et al.
Title: Cross-scale observations of the 2015 St. Patrick's day storm: THEMIS, Van Allen Probes, and TWINS
Abstract: We present cross-scale magnetospheric observations of the 17 March 2015 (St. Patrick's Day) storm, by Time History of Events and Macroscale Interactions during Substorms (THEMIS), Van Allen Probes (Radiation Belt Storm Probes), and Two Wide-angle Imaging Neutral-atom Spectrometers (TWINS), plus upstream ACE/Wind solar wind data. THEMIS crossed the bow shock or magnetopause 22 times and observed the magnetospheric compression that initiated the storm. Empirical models reproduce these boundary locations within 0.7 RE. Van Allen Probes crossed the plasmapause 13 times; test particle simulations reproduce these encounters within 0.5 RE. Before the storm, Van Allen Probes measured quiet double-nose proton spectra in the region of corotating cold plasma. About 15 min after a 0605 UT dayside sout. . .
Date: 01/2017 Publisher: Journal of Geophysical Research: Space Physics Pages: 368 - 392 DOI: 10.1002/jgra.v122.110.1002/2016JA023173 Available at: http://onlinelibrary.wiley.com/doi/10.1002/2016JA023173/full
More Details
Substorm Injections
Authors: Birn J, Thomsen M F, Borovsky J E, Reeves G D, McComas D J, et al.
Title: Substorm electron injections: Geosynchronous observations and test particle simulations
Abstract: We investigate electron acceleration and the flux increases associated with energetic electron injections on the basis of geosynchronous observations and test-electron orbits in the dynamic fields of a three-dimensional MHD simulation of neutral line formation and dipolarization in the magnetotail. This complements an earlier investigation of test protons [Birn et al., 1997b]. In the present paper we consider equatorial orbits only, using the gyrocenter drift approximation. It turns out that this approximation is valid for electrons prior to and during the flux rises observed in the near tail region of the model at all energies considered (∼ 100 eV to 1 MeV). The test particle model reproduces major observed characteristics: a fast flux rise, comparable to that of the ions, and the exist. . .
Date: 05/1998 Publisher: Journal of Geophysical Research Pages: 9235 - 9248 DOI: 10.1029/97JA02635 Available at: http://onlinelibrary.wiley.com/doi/10.1029/97JA02635/abstract
More Details
storms
Authors: Valek P. W., Goldstein J, Jahn J -M, McComas D J, and Spence H E
Title: First joint in situ and global observations of the medium-energy oxygen and hydrogen in the inner magnetosphere
Abstract: We present the first simultaneous observations of the in situ ions and global Energetic Neutral Atom (ENA) images of the composition-separated, medium-energy (~1–50 keV) particle populations of the inner magnetosphere. The ENA emissions are mapped into L shell/magnetic local time space based on the exospheric density along the line of sight (LOS). The ENA measurement can then be scaled to determine an average ion flux along a given LOS. The in situ ion flux tends to be larger than the scaled ENAs at the same local time. This indicates that the ion population is more concentrated in the Van Allen Probes orbital plane than distributed along the Two Wide-angle Imaging Neutral-atom Spectrometers LOS. For the large storm of 14 November 2012, we observe that the concentration of O (in situ i. . .
Date: 09/2015 Publisher: Journal of Geophysical Research: Space Physics Pages: 7615 - 7628 DOI: 10.1002/2015JA021151 Available at: http://doi.wiley.com/10.1002/2015JA021151http://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1002%2F2015JA021151
More Details
oxygen
Authors: Valek P. W., Goldstein J, Jahn J -M, McComas D J, and Spence H E
Title: First joint in situ and global observations of the medium-energy oxygen and hydrogen in the inner magnetosphere
Abstract: We present the first simultaneous observations of the in situ ions and global Energetic Neutral Atom (ENA) images of the composition-separated, medium-energy (~1–50 keV) particle populations of the inner magnetosphere. The ENA emissions are mapped into L shell/magnetic local time space based on the exospheric density along the line of sight (LOS). The ENA measurement can then be scaled to determine an average ion flux along a given LOS. The in situ ion flux tends to be larger than the scaled ENAs at the same local time. This indicates that the ion population is more concentrated in the Van Allen Probes orbital plane than distributed along the Two Wide-angle Imaging Neutral-atom Spectrometers LOS. For the large storm of 14 November 2012, we observe that the concentration of O (in situ i. . .
Date: 09/2015 Publisher: Journal of Geophysical Research: Space Physics Pages: 7615 - 7628 DOI: 10.1002/2015JA021151 Available at: http://doi.wiley.com/10.1002/2015JA021151http://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1002%2F2015JA021151
More Details
multimission
Authors: Goldstein J, Angelopoulos V, De Pascuale S., Funsten H O, Kurth W S, et al.
Title: Cross-scale observations of the 2015 St. Patrick's day storm: THEMIS, Van Allen Probes, and TWINS
Abstract: We present cross-scale magnetospheric observations of the 17 March 2015 (St. Patrick's Day) storm, by Time History of Events and Macroscale Interactions during Substorms (THEMIS), Van Allen Probes (Radiation Belt Storm Probes), and Two Wide-angle Imaging Neutral-atom Spectrometers (TWINS), plus upstream ACE/Wind solar wind data. THEMIS crossed the bow shock or magnetopause 22 times and observed the magnetospheric compression that initiated the storm. Empirical models reproduce these boundary locations within 0.7 RE. Van Allen Probes crossed the plasmapause 13 times; test particle simulations reproduce these encounters within 0.5 RE. Before the storm, Van Allen Probes measured quiet double-nose proton spectra in the region of corotating cold plasma. About 15 min after a 0605 UT dayside sout. . .
Date: 01/2017 Publisher: Journal of Geophysical Research: Space Physics Pages: 368 - 392 DOI: 10.1002/jgra.v122.110.1002/2016JA023173 Available at: http://onlinelibrary.wiley.com/doi/10.1002/2016JA023173/full
More Details
Modeling
Authors: Goldstein J, Angelopoulos V, De Pascuale S., Funsten H O, Kurth W S, et al.
Title: Cross-scale observations of the 2015 St. Patrick's day storm: THEMIS, Van Allen Probes, and TWINS
Abstract: We present cross-scale magnetospheric observations of the 17 March 2015 (St. Patrick's Day) storm, by Time History of Events and Macroscale Interactions during Substorms (THEMIS), Van Allen Probes (Radiation Belt Storm Probes), and Two Wide-angle Imaging Neutral-atom Spectrometers (TWINS), plus upstream ACE/Wind solar wind data. THEMIS crossed the bow shock or magnetopause 22 times and observed the magnetospheric compression that initiated the storm. Empirical models reproduce these boundary locations within 0.7 RE. Van Allen Probes crossed the plasmapause 13 times; test particle simulations reproduce these encounters within 0.5 RE. Before the storm, Van Allen Probes measured quiet double-nose proton spectra in the region of corotating cold plasma. About 15 min after a 0605 UT dayside sout. . .
Date: 01/2017 Publisher: Journal of Geophysical Research: Space Physics Pages: 368 - 392 DOI: 10.1002/jgra.v122.110.1002/2016JA023173 Available at: http://onlinelibrary.wiley.com/doi/10.1002/2016JA023173/full
More Details
Heliophysics System Observatory
Authors: Goldstein J, Angelopoulos V, De Pascuale S., Funsten H O, Kurth W S, et al.
Title: Cross-scale observations of the 2015 St. Patrick's day storm: THEMIS, Van Allen Probes, and TWINS
Abstract: We present cross-scale magnetospheric observations of the 17 March 2015 (St. Patrick's Day) storm, by Time History of Events and Macroscale Interactions during Substorms (THEMIS), Van Allen Probes (Radiation Belt Storm Probes), and Two Wide-angle Imaging Neutral-atom Spectrometers (TWINS), plus upstream ACE/Wind solar wind data. THEMIS crossed the bow shock or magnetopause 22 times and observed the magnetospheric compression that initiated the storm. Empirical models reproduce these boundary locations within 0.7 RE. Van Allen Probes crossed the plasmapause 13 times; test particle simulations reproduce these encounters within 0.5 RE. Before the storm, Van Allen Probes measured quiet double-nose proton spectra in the region of corotating cold plasma. About 15 min after a 0605 UT dayside sout. . .
Date: 01/2017 Publisher: Journal of Geophysical Research: Space Physics Pages: 368 - 392 DOI: 10.1002/jgra.v122.110.1002/2016JA023173 Available at: http://onlinelibrary.wiley.com/doi/10.1002/2016JA023173/full
More Details
ENAs
Authors: Valek P. W., Goldstein J, Jahn J -M, McComas D J, and Spence H E
Title: First joint in situ and global observations of the medium-energy oxygen and hydrogen in the inner magnetosphere
Abstract: We present the first simultaneous observations of the in situ ions and global Energetic Neutral Atom (ENA) images of the composition-separated, medium-energy (~1–50 keV) particle populations of the inner magnetosphere. The ENA emissions are mapped into L shell/magnetic local time space based on the exospheric density along the line of sight (LOS). The ENA measurement can then be scaled to determine an average ion flux along a given LOS. The in situ ion flux tends to be larger than the scaled ENAs at the same local time. This indicates that the ion population is more concentrated in the Van Allen Probes orbital plane than distributed along the Two Wide-angle Imaging Neutral-atom Spectrometers LOS. For the large storm of 14 November 2012, we observe that the concentration of O (in situ i. . .
Date: 09/2015 Publisher: Journal of Geophysical Research: Space Physics Pages: 7615 - 7628 DOI: 10.1002/2015JA021151 Available at: http://doi.wiley.com/10.1002/2015JA021151http://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1002%2F2015JA021151
More Details