Applicability of Taylor’s hypothesis during Parker Solar Probe perihelia

Parker Solar Probe: Ushering a new frontier in space exploration

Open Access

Table 1

Selected 24 h intervals used in our analysis, one from each of the first four encounters E1 to E4.

Encounter	Interval	r (au)	Plasma instrument
E1	2018-11-05 15:30 to 2018-11-06 15:30	0.166	SPC
E2	2019-04-04 16:00 to 2019-04-05 16:00	0.166	SPC
E3	2019-08-29 12:00 to 2019-08-30 12:00	0.191	SPC
E4	2020-01-28 14:30 to 2020-01-29 14:30	0.131	SPAN-ion

Notes. We note that r represents the average heliocentric distance for each interval. The last column indicates the primary instrument used in the analysis of plasma moments. With the exception of E3, all intervals were selected to be near PSP perihelia.

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