Classifier Instance:

Anchor text: photometry
Target Entity: Photometry_\u0028astronomy\u0029
Preceding Context: Another problem with wave heating has been the complete absence, until the late 1990s, of any direct evidence of waves propagating through the solar corona. The first direct observation of waves propagating into and through the solar corona was made in 1997 with the SOHO space-borne solar observatory, the first platform capable of observing the Sun in the extreme ultraviolet (EUV) for long periods of time with stable
Succeeding Context: . Those were magneto-acoustic waves with a frequency of about 1 millihertz (mHz, corresponding to a 1,000 second wave period), that carry only about 10% of the energy required to heat the corona. Many observations exist of localized wave phenomena, such as Alfvén waves launched by solar flares, but those events are transient and cannot explain the uniform coronal heat.
Paragraph Title: null
Source Page: Corona

Ground Truth Types:

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|  |---wordnet_artifact_100021939
|  |  |---wordnet_instrumentality_103575240
|  |  |  |---wordnet_system_104377057

Predicted Types:

TypeConfidenceDecision
wordnet_artifact_100021939-0.05729544475002712 0
wordnet_event_100029378-0.9706480368363882 0
wordnet_organization_108008335-1.7504694859208394 0
wordnet_person_100007846-1.6016862785681112 0
yagoGeoEntity-1.7361219218050281 0
|---wordnet_entity_100001740
|  |---wordnet_artifact_100021939
|  |---wordnet_event_100029378
|  |---wordnet_organization_108008335
|  |---wordnet_person_100007846
|  |---yagoGeoEntity