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The Pi2 waves are observed around 1 min later at the onset station at GILL.
Any regions in white are where onset times are the same within the uncertainty and the auroral onset station (GILL) is marked in green to aid the eye since this station first observes both the Pi1-2 onset and the auroral onset at 06:04:20 UT.
A number of features stand out in Fig. 5a, most notably that at the auroral and ULF wave onset station Pi1-2 ULF waves clearly lead Pi2 waves by ~ 1 min and across the majority of latitudes and longitudes the Pi1-2 onset leads the Pi2 onset by ~ 1 2 min.
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Temperature data were logged every minute by the project meteorological station (Onset Microstation, Onset Computer Corporation) at the INCLEN field headquarters in Palwal town, between 5 and 12 km from study villages.
To download the data from the data logger, I used the Hobo® Optic USB Base Station (Onset part #BASE-U-1, US$59) which connects the data loggers to a computer via a USB port.
PAGASA defined Philippine summer monsoon onset using eight stations in the northwestern Philippines (Fig. 1; Cayanan 2010).
Keograms from all-sky imager data showed formation of an arc at onset time at the station showing the earliest pulsation signal.
The maximum error in this fit is of the order of seconds and hence represents the actual onset time at each station within stated errors.
The most distant stations are not used because it was difficult to read the onset precisely at those stations.
The results of the statistical analysis show that 87% of the Pi 2 onsets at a ground station (Kuju, GMLat. = 26.13°, GMLon. = 202.96°) were delayed from the Pi 2 onsets at ETS-VIII, and the average of the delay times was 29 sec.
In order to determine the location of the rupture starting point and rupture time for each SMGA objectively, we read the onset of S1 S4 at stations along the source region.
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