data: $integral dT$ [ $partialdiff sub X$ ( NASA LISOTD 0p25 Monthly ) anomalies ]

∫dT [ ∂_X ( NASA LISOTD 0p25 Monthly ) anomalies ]: ∂_X Monthly Flash Density Rate data

Monthly Monthly partial_X partial_X ∂_X Monthly Flash Density Rate from NASA LISOTD 0p25: Satellite monthly flash density rate from TRMM-LIS at 0.25 deg.

Independent Variables (Grids)

Time: grid: /T (days since 1960-01-01) (360) ordered [ (0001 21 Jul 1998) (0001 22 Aug 1998) (0001 20 Sep 1998) ... (0002 14 Sep 2014)] N= 193 pts :grid
Longitude: grid: /X (degree_east) periodic (180W) to (179.75E) by 0.25 N= 1440 pts :grid
Latitud: grid: /Y (degree_north) ordered (37.875S) to (37.875N) by 0.25 N= 304 pts :grid

Other Info

_FillValue_original: -999.98999
bufferwordsize: 8
CE: null
CS: null
datatype: doublearraytype
file_missing_value: -999.98999
missing_value: NaN
units: flashes /km² /day /degree_east days
history: Averaged over T2[16 Dec 1997 - 15 Dec 1998, 16 Dec 2012 - 15 Dec 2013] minimum 0.0% data present

References

Rachel I. Albrecht, Steven J. Goodman, Dennis E. Buechler, Richard J. Blakeslee, and Hugh J. Christian, 0: Where are the lightning hotspots on Earth?. Bull. Amer. Meteor. Soc., doi: 10.1175/BAMS-D-14-00193.1

Last updated: Wed, 02 Nov 2016 03:03:21 GMT

Data Views

	T	X	Y
NASA LISOTD 0p25[Monthly ]
$integral dT$ [ $partialdiff sub X$ ( NASA LISOTD 0p25 Monthly ) anomalies ][ X Y \| T]	M	M	M

Filters

Here are some filters that are useful for manipulating data. There are actually many more available, but they have to be entered manually. See Ingrid Function Documentation for more information.

Monthly Climatology calculates a monthly climatology by averaging over all years.
anomalies calculates the difference between the (above) monthly climatology and the original data.
Integrate along X Y T
Differentiate along X Y T
Take differences along X Y T