Solar Orbiter Radio and Plasma Waves - Time Domain Sampler: In-flight performance and first results
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F21%3A00552647" target="_blank" >RIV/67985815:_____/21:00552647 - isvavai.cz</a>
Alternative codes found
RIV/68378289:_____/21:00550709 RIV/00216208:11320/21:10439896
Result on the web
<a href="http://hdl.handle.net/11104/0327764" target="_blank" >http://hdl.handle.net/11104/0327764</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1051/0004-6361/202140948" target="_blank" >10.1051/0004-6361/202140948</a>
Alternative languages
Result language
angličtina
Original language name
Solar Orbiter Radio and Plasma Waves - Time Domain Sampler: In-flight performance and first results
Original language description
This article presents the first data from the RPW-TDS receiver and discusses the in-flight performance of the instrument and, in particular, the on-board wave and dust detection algorithm. We present the TDS data products and its scientific operation. We demonstrate the content of the dataset on several examples. In particular, we study the distribution of solar Langmuir waves in the first year of observations and one Type III burst event. The on-board detection algorithm is described in detail in this article and classifies the observed waveform snapshots, identifying plasma waves and dust impacts based on the ratio of their maximum amplitude to their median and on the spectral bandwidth. The algorithm allows TDS to downlink the most scientifically relevant waveforms and to perform an on-board statistical characterization of the processed data. The detection algorithm of TDS is shown to perform very well in its detection of plasma waves and dust impacts with a high accuracy. The initial analysis of statistical data returned by TDS shows that sporadic Langmuir waves that are not associated with Type III events are routinely observed in the inner heliosphere, with a clear increase in occurrence rate closer to the Sun. We also present an example of RPW observations during an encounter of the source region of a Type III burst, which exploits the on-board calculated histograms data.
Czech name
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Czech description
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Classification
Type
J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database
CEP classification
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OECD FORD branch
10308 - Astronomy (including astrophysics,space science)
Result continuities
Project
—
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Others
Publication year
2021
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Name of the periodical
Astronomy & Astrophysics
ISSN
0004-6361
e-ISSN
1432-0746
Volume of the periodical
656
Issue of the periodical within the volume
December
Country of publishing house
FR - FRANCE
Number of pages
9
Pages from-to
A26
UT code for WoS article
000730246400036
EID of the result in the Scopus database
2-s2.0-85121588410