Calculating the CME Time-of-Arrival and Speed-on-Arrival using observations from HI-1 using drag force and elliptical front model
<|begin_of_text|><|start_header_id|>system<|end_header_id|> You are a research archivist expert in dataset metadata. Answer the question truthfully.  <|eot_id|><|start_header_id|>user<|end_header_id|> Here is the Description of a dataset. Description:'This are the IDL codes and their input files used on this study. Using this software and opening the .sav files require IDL (tested with 8.0 or higher) and SolarSoft (SECCHI, NRL, SOHO packages, among others)' . Please return only a json list of at most 3 Keywords corresponding to the Description:.<|eot_id|><|start_header_id|>assistant<|end_header_id|> {"Answer" : ["solar physics: coronal mass ejections"]} <|eot_id|>
 Here is the Description of a dataset. Description:'This are the IDL codes and their input files used on this study. Using this software and opening the .sav files require IDL (tested with 8.0 or higher) and SolarSoft (SECCHI, NRL, SOHO packages, among others)' . Please return only a json list of at most 3 Keywords corresponding to the Description:.
This are the IDL codes and their input files used on this study. Using this software and opening the .sav files require IDL (tested with 8.0 or higher) and SolarSoft (SECCHI, NRL, SOHO packages, among others)
solar physics: coronal mass ejections