Kevin Genestreti
| Kevin Genestreti | |
| Known for | Magnetic reconnection research |
|---|---|
| Education | University of New Hampshire (B.S.) University of Texas at San Antonio (Ph.D.) |
Kevin Genestreti is a space physicist affiliated with the University of New Hampshire, where he has worked at the Space Science Center.[1] His research concerns magnetic reconnection, including its rate, structure, and electron-scale dynamics as observed by spacecraft missions.[2]
Education
Genestreti earned a B.S. from the University of New Hampshire between 2008 and 2012, and a Ph.D. from the University of Texas at San Antonio between 2012 and 2016.[3]
Career
Genestreti worked as a Doctoral Researcher in the Space Science and Engineering Division at Southwest Research Institute from 2012 to 2016.[4] He then served as a postdoctoral researcher at the Space Research Institute of the Austrian Academy of Sciences from 2016 to 2018.[5] In 2018, he joined the Space Science Center at the University of New Hampshire as a Research Scientist.[6] In 2019, he took a position as a Research Scientist in the Earth, Oceans and Space division of Southwest Research Institute.[7]
Research
Genestreti has published 126 papers that have collectively received 2,156 citations, with an h-index of 29 according to Semantic Scholar.[8] His work centers on magnetic reconnection in space plasmas, including studies using data from the Magnetospheric Multiscale (MMS) mission on the electron-scale structure of the diffusion region, the reconnection rate, and the effects of guide fields on energy conversion during reconnection.[9]
Selected publications
- "Electron-scale dynamics of the diffusion region during symmetric magnetic reconnection in space" (2018), Science[10]
- "Magnetic Reconnection, Turbulence, and Particle Acceleration: Observations in the Earth's Magnetotail" (2018)[11]
- "How Accurately Can We Measure the Reconnection Rate E M for the MMS Diffusion Region Event of 11 July 2017?" (2018), Journal of Geophysical Research - Space Physics[12]
- "First-principles theory of the rate of magnetic reconnection in magnetospheric and solar plasmas" (2022), Communications Physics[13]
- "Measurement of the Magnetic Reconnection Rate in the Earth's Magnetotail" (2018), Journal of Geophysical Research - Space Physics[14]
- "The Effect of a Guide Field on Local Energy Conversion During Asymmetric Magnetic Reconnection: MMS Observations" (2017)[15]
- "Polynomial Reconstruction of the Reconnection Magnetic Field Observed by Multiple Spacecraft" (2020), Journal of Geophysical Research - Space Physics[16]
- "Signatures of Nonideal Plasma Evolution During Substorms Obtained by Mining Multimission Magnetometer Data" (2019), Journal of Geophysical Research: Space Physics[17]
- "Localized Oscillatory Energy Conversion in Magnetopause Reconnection" (2017)[18]
- "Electron Diffusion Regions in Magnetotail Reconnection Under Varying Guide Fields" (2019), Geophysical Research Letters[19]
External links
- ↑ ORCID 0000-0001-6890-2973
- ↑ Semantic Scholar publication metrics for Kevin Genestreti
- ↑ ORCID 0000-0001-6890-2973
- ↑ ORCID 0000-0001-6890-2973
- ↑ ORCID 0000-0001-6890-2973
- ↑ ORCID 0000-0001-6890-2973
- ↑ ORCID 0000-0001-6890-2973
- ↑ Semantic Scholar publication metrics for Kevin Genestreti
- ↑ Semantic Scholar publication metrics for Kevin Genestreti
- ↑ Semantic Scholar publication metrics for Kevin Genestreti
- ↑ Semantic Scholar publication metrics for Kevin Genestreti
- ↑ Semantic Scholar publication metrics for Kevin Genestreti
- ↑ Semantic Scholar publication metrics for Kevin Genestreti
- ↑ Semantic Scholar publication metrics for Kevin Genestreti
- ↑ Semantic Scholar publication metrics for Kevin Genestreti
- ↑ Semantic Scholar publication metrics for Kevin Genestreti
- ↑ Semantic Scholar publication metrics for Kevin Genestreti
- ↑ Semantic Scholar publication metrics for Kevin Genestreti
- ↑ Semantic Scholar publication metrics for Kevin Genestreti