Interplanetary shock detection algorithm
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378289%3A_____%2F12%3A00426535" target="_blank" >RIV/68378289:_____/12:00426535 - isvavai.cz</a>
Result on the web
—
DOI - Digital Object Identifier
—
Alternative languages
Result language
angličtina
Original language name
Interplanetary shock detection algorithm
Original language description
Investigation of the interplanetary (IP) shock formation may clarify our understanding of energy transfer on dierent spatial scales in space plasmas and particle acceleration at shock waves. We present an automated detection algorithm that is able to identify an IP shock arrival in real-time data stream. This algorithm may be implemented onboard the future Solar Orbiter space mission for triggering the transmission of the high resolution data during the IP shock crossings.
Czech name
—
Czech description
—
Classification
Type
O - Miscellaneous
CEP classification
DG - Atmospheric sciences, meteorology
OECD FORD branch
—
Result continuities
Project
<a href="/en/project/LG11032" target="_blank" >LG11032: COSPAR 2011-2013</a><br>
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Others
Publication year
2012
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů