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VERSION:2.0
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X-WR-CALNAME:Planetary Science and Exploration Seminar\, Megan Seritan: "Ma
 gnetic field morphology correlated with surface slopes at the Gerasimovich
  lunar magnetic anomaly"
X-WR-TIMEZONE:Pacific Time (US & Canada)
BEGIN:VEVENT
DTSTAMP:20260616T062326Z
UID:tag:localist.com\,2008:EventInstance_52154025904006
DTSTART:20260225T203000Z
DTEND:20260225T212000Z
DESCRIPTION:The crustal magnetic anomalies near the lunar crater Gerasimovi
 ch are among the highest-magnitude anomalies on the Moon. Previous work ha
 s suggested they formed from the deposition and magnetization of ejecta fr
 om the Crisium basin\, which is antipodal to the region. In this talk\, I 
 will describe the correlation between topographic slope and magnetic field
  morphology in this region\, present a predictive model of magnetic field 
 strength based on slope that reproduces key features of the observed field
 \, estimate the source body magnetization of the fill deposit thickness in
 side of Gerasimovich crater\, and describe the implications of the varying
  magnetization directions within the group of Gerasimovich anomalies.\n\n 
 \n\nDr. Megan R. K. Seritan received her B.S. in Physics from UC Santa Bar
 bara in 2016\, and her Ph.D. in Planetary Science from UC Santa Cruz in 20
 22. During her Ph.D.\, her advisor was Ian Garrick-Bethell\, who is the co
 llaborator for the work presented in this talk. In 2023\, Megan joined the
  SETI Institute\, where she is the Deputy Manager of the Ring Moon Systems
  Node of NASA's Planetary Data System archive.
GEO:37.426402;-122.172635
LOCATION:Mitchell Earth Sciences\, 350/372
SUMMARY:Planetary Science and Exploration Seminar\, Megan Seritan: "Magneti
 c field morphology correlated with surface slopes at the Gerasimovich luna
 r magnetic anomaly"
URL;VALUE=URI:https://events.stanford.edu/event/planetary-science-and-explo
 ration-seminar-megan-seritan-magnetic-field-morphology-correlated-with-sur
 face-slopes-at-the-gerasimovich-lunar-magnetic-anomaly
CATEGORIES:Class/Seminar
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