Comparison between GOES flares, SOHO/LASCO CMEs and RSTN 1.4 GHz solar radio bursts
<|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:'Study 1.4 GHz solar radio bursts as counterparts to coronal mass ejections.For a list of GOES X-ray flares of class M5 or higher, this dataset provides the time integral of their associated 1.4 GHz solar radio burst and compares them with the speed, angular width and kinetic energy of the associated CME, if any' . 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" : ["Coronal mass ejections","Solar flares","Solar radio bursts","Space weather"]} <|eot_id|>
 Here is the Description of a dataset. Description:'Study 1.4 GHz solar radio bursts as counterparts to coronal mass ejections.For a list of GOES X-ray flares of class M5 or higher, this dataset provides the time integral of their associated 1.4 GHz solar radio burst and compares them with the speed, angular width and kinetic energy of the associated CME, if any' . Please return only a json list of at most 3 Keywords corresponding to the Description:.
Study 1.4 GHz solar radio bursts as counterparts to coronal mass ejections.For a list of GOES X-ray flares of class M5 or higher, this dataset provides the time integral of their associated 1.4 GHz solar radio burst and compares them with the speed, angular width and kinetic energy of the associated CME, if any
Coronal mass ejections; Solar flares; Solar radio bursts; Space weather