Reproduction data for two figures (4 and 6) which were produced for the review paper 'Dust observations with antenna measurements and its prospects for observations with Parker Solar Probe and Solar Orbiter'. Other figures are previously published.
The work presents a review of dust measurements from spacecraft Cassini, STEREO, MMS, Cluster, Maven and WIND. We also consider the details of dust impacts and charge generation, and how different antenna signals can be generated. We compare observational data to laboratory experiments and simulations and discuss the consequences for dust observation with the new NASA Parker Solar Probe and ESA Solar Orbiter spacecraft.
'Figure 4' has formats TXT and CSV, and each file is name according to which panel (and bias) it represents.
The files are two dimensional an the first column is time in microseconds before impact event, and the second column is recorded voltage.
'Figure 6' is in CDF (common data format) format.
A suitable software must be used to handle the data (See NASA documentation for CDF format v 3.7.1: https://cdf.gsfc.nasa.gov/html/FAQ.html).
'mms1_edp_BURST_SC-POTENTIAL_2016-11.cdf' contains data for panel 3, SC potential.
'mms1_edp_BURST_DC_2016-11.cdf' contains monopole and dipole data.
Both these sets are for burst mode operation.