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heliophysics query scripts
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Review script for paper "2023ApJ...954L..47C" made with predictor "DataLinkerCondenseDetailsWithTemplate" #28

Closed abuonomo closed 5 months ago

abuonomo commented 5 months ago

Created by Paper Data Linking Bot

Please review the download script and instrument details for the paper.

bibcode: 2023ApJ...954L..47C predictor: DataLinkerCondenseDetailsWithTemplate

abuonomo commented 5 months ago

Paper says that HXR emissions only appeared in enegy bands less than 12 keV, but this does not mean they only looked at those energy bands. Additionally the syntax is not valid. We should maybe clue the LLM in to the correct syntax to potential resolve problems like this. 

sunpy.net.attrs.Wavelength(wavemin, wavemax=None)
abuonomo commented 5 months ago

script runs successfully and returns records for all queries. Interestingly, many seem to be capped 595 files, indicating potential pagination. Also, there is only 1 result from GOES. Not sure if this is correct or no.

abuonomo commented 5 months ago

The EUV imaging data from the Sun Earth Connection Coronal and Heliospheric Investigation (SECCHI; Howard et al. 2008) on board the Solar Terrestrial Relations Observatory (STEREO)

I think we should probably only be using the EUVI detector on SECCHI.

UPDATE:

In addition, to inspect the CME generated by the MFR eruption, we also make use of the data from the Large Angle and Spectrometric Coronagraph (LASCO; Brueckner et al. 1995) on board the Solar and Heliospheric Observatory (SOHO) and the SECCHI instrument suite on board STEREO-A. The CME velocity in the higher corona is from the CDAW Data Center1. The Geostationary Operational Environmental Satellite (GOES) provides the soft X-ray (SXR) fluxes of associated flares at two bands of 1-8 ̊A and 0.5-4 ̊A. The Helioseismic and Magnetic Imager (HMI; Schou et al. 2012) also on board SDO provides the photospheric vector magnetic field of the investigated AR with a temporal cadence of 12 minutes and spatial resolution of 1.2 arcsecond.

The quote indicates that COR1 and COR2 may also have been used since they are more relevant for observing CMEs. Therefore, the initial query just asking for all SECCHI detectors is more correct.