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Johns Hopkins HealthCare dmsp data
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Article Title: Position of the Source of Dayside High-Latitude Magnetic Impulses in the Magnetosphere from DMSP Satellite Data
Article Snippet: Dayside high-latitude geophysical phenomena provide a ground-based observer with information about the processes at the dayside magnetopause and/or in the adjacent magnetospheric domains.. It is assumed that these phenomena are initiated by changes in the parameters of the interplanetary medium and can therefore be used as a tool to investigate the ways in which solar wind energy penetrates through the magnetopause.. Such phenomena include magnetic impulses, which are an isolated train of damped oscillations of two to three bursts with a repetition period of 8–12 min.

Article Title: Interhemispheric comparison of GPS phase scintillation at high latitudes during the magnetic-cloud-induced geomagnetic storm of 5–7 April 2010
Article Snippet: The DMSP particle detectors were designed by Dave Hardy of Air Force Research Laboratory, and the data were obtained from Johns Hopkins University Applied Research Laboratory.

Article Title: In Situ Observational Evidence of the Polar Cap Arc at 1500 MLT (15MLT‐PCA) Associated With the Lobe Reconnection
Article Snippet: Data Availability Statement The authors would like to thank Johns Hopkins University Applied Physics Laboratory for providing the DMSP data.



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Johns Hopkins HealthCare dmsp ssusi data products
Composite plot of Swarm and <t>DMSP</t> observations of a polar cap event in the Southern Hemisphere. Presented are field-aligned currents along the Swarm track (top left), where the black curve shows dual-SC FAC and the red and blue curves show results from Swarm A and C, respectively. Auroral images and the Swarm orbit track are illustrated below. Precipitating particle spectrograms with FAC profiles over-plotted are shown to the right, with electrons at the top and ions at the bottom.
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Composite plot of Swarm and DMSP observations of a polar cap event in the Southern Hemisphere. Presented are field-aligned currents along the Swarm track (top left), where the black curve shows dual-SC FAC and the red and blue curves show results from Swarm A and C, respectively. Auroral images and the Swarm orbit track are illustrated below. Precipitating particle spectrograms with FAC profiles over-plotted are shown to the right, with electrons at the top and ions at the bottom.

Journal: Annales geophysicae

Article Title: Filamentary field-aligned currents at the polar cap region during northward interplanetary magnetic field derived with the Swarm constellation

doi: 10.5194/angeo-34-901-2016

Figure Lengend Snippet: Composite plot of Swarm and DMSP observations of a polar cap event in the Southern Hemisphere. Presented are field-aligned currents along the Swarm track (top left), where the black curve shows dual-SC FAC and the red and blue curves show results from Swarm A and C, respectively. Auroral images and the Swarm orbit track are illustrated below. Precipitating particle spectrograms with FAC profiles over-plotted are shown to the right, with electrons at the top and ions at the bottom.

Article Snippet: DMSP SSUSI data products are publicly available at the Johns Hopkins Applied Physics Laboratory (JHU/APL) website http://ssusi.jhuapl.edu/data_products ( ).

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