Tao SW Venus / Input DSCOVR

SPASE resource : spase://CNES/NumericalOutput/CDPP-AMDA/TAO/Venus/tao-venus-dsc

Last Updated

2024-03-24T22:20:29Z

Description

DSCOVR FC solar wind 1-min data is used as model input. Calculation : IRAP.

Information links

Model Description

Model Article

Caveats

Note an important parameter - angle Venus-Sun-Earth - which could be considered as quality flag.

Temporal description

Time range: 2016/08/01 00:00:00 — 2024/03/23 00:00:00

Sampling: 1h

Acknowledgement

TBD

Thank you for acknowledging the use of AMDA in publications with wording like "Data analysis was performed with the AMDA science analysis system provided by the Centre de Données de la Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and Université Paul Sabatier, Toulouse". See the Rules of the road at https://amda.cdpp.eu/help/policy.html . Please acknowledge the Data Providers.

Contacts

Principal Investigator:

Dr. Chihiro Tao

chihiro.tao@nict.go.jp - National Institute of Information and Communications Technology

SPASE resource : spase://CNES/Person/CDPP-AMDA/Chihiro.Tao

Technical Contact:

Elena Budnik

elena.budnik@irap.omp.eu - Noveltis

SPASE resource : spase://SMWG/Person/Elena.Budnik